0 Assigned ID: 128 ----- Attempting Submission 1 (Wed Apr 05 06:45:37 GMT 2017) ----- HST Phase I Proposal 128 (Cycle25_1-Ph1.apt) successfully submitted. Receipt: # 128-1 ----- Attempting Submission 2 (Thu Apr 06 04:35:46 GMT 2017) ----- HST Phase I Proposal 128 (Cycle25_1-Ph1.apt) successfully submitted. Receipt: # 128-2 ----- Attempting Submission 3 (Fri Apr 07 06:04:31 GMT 2017) ----- HST Phase I Proposal 128 (Cycle25_1-Ph1.apt) successfully submitted. Receipt: # 128-3 ----- Attempting Submission 4 (Fri Apr 07 17:59:21 GMT 2017) ----- HST Phase I Proposal 128 (Cycle25_1-Ph1.apt) successfully submitted. Receipt: # 128-4 ----- Attempting Submission 5 (Fri Apr 07 19:17:39 GMT 2017) ----- HST Phase I Proposal 128 (Cycle25_1-Ph1.apt) successfully submitted. Receipt: # 128-5 For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. typo in abstract "hyrdogen" corrected. 11 Oct 2017: changed all occurrences of cenwave "1223" to "1222," as per new recommendation from STScI; and adjusted NUV acq exp times to accommodate slight "unused time" in each orbit as a result of cenwave shift. 12-Feb-2018: changed ACQ/IMAG exposure times to reflect new threshold S/N=30; exposure "savings" evenly split among the four settings of each visit, with any remaining time (typically 1s, or so) put back into the ACQ. 27-Nov-2018: changed Visit 34 ACQ/IMAG to MIRROR-B because the target has bluer colors than its indicated spectral type, which caused an over-light issue when MIRROR-A was used and a more appropriate earlier spectral type was specified for the ETC simulation. Observed Galex NUV magnitude supports the bluer optical colors. ACQ/IMAG exposure time increased, and the four science exposures were trimmed accordingly (about 20s per exp). -1698436970 ----- Attempting Submission 1 (Thu Jul 06 19:44:36 GMT 2017) ----- HST Phase II Proposal 15300 (GO-15300.apt) successfully submitted. Receipt: # 15300-1 ----- Attempting Submission 2 (Mon Jul 10 02:05:42 GMT 2017) ----- ----- Attempting Submission 3 (Wed Oct 11 23:44:03 GMT 2017) ----- ----- Attempting Submission 4 (Tue Feb 13 07:12:18 GMT 2018) ----- ----- Attempting Submission 5 (Tue Nov 27 15:52:17 GMT 2018) ----- Orbit planner and Visit planner were run; the 49 warnings are not relevant (have to do with FP-POS choices for fixed pattern mitigation; taken care of with two [mostly] overlapping wavelength settings, 2 FP-POS at each). BACKGROUND: Now and in coming years, a number of orbiting observatories will be scanning the skies for astrometry (Gaia), transiting exoplanets (TESS), and high-energy sources (eROSITA). A key characteristic of these surveys is their high degree of exposure in the ecliptic polar regions, north and south; a natural consequence of their preferred scanning orientation. Further, JWST, although not a scanning instrument, also holds the ecliptic poles in special regard because they are accessible at all times ("continuous viewing zones"), a key advantage for exo-planet studies. THIS PROPOSAL: Record FUV spectra, with COS G130M, of a well-defined sample of sunlike dwarfs (F2V-K2V) at the ecliptic poles to take advantage of the enhanced, wholistic information concerning rotation periods, sizes, masses, metallicities, ages, activity levels, and coronal properties that will be available for bright e-polar stars over the next few years. There is a sweet spot at about 8th magnitude where sunlike stars are not too bright for TESS, bright enough for eROSITA, and just right for COS. The G130M channel captures a wide range of ionization states, especially of Si, N, O, and C; the hydrogen Lyman-alpha emission; and also coronal forbidden transitions of Fe XII (124 nm) and Fe XXI (135 nm); altogether reflecting gas temperatures from 10,000 K to 10 MK in the magnetically disturbed stellar outer atmospheres. The combined photometric (starspots), asteroseismic, FUV, and X-ray measurements will inform community-wide efforts to explore stellar activity and its underlying magnetic machine, the Dynamo. This is a unique opportunity, and one -- like a solar eclipse -- too good to pass up. The EclipSS project -- Ecliptic poles Stellar Survey -- aims to collect FUV spectra (115-143 nm), from HST's ultra-sensitive Cosmic Origins Spectrograph (COS), of a sample of 49 F2-K2 dwarf stars in the North and South ecliptic polar regions, to further advance studies of magnetic activity among cool Main sequence stars analogous to the Sun. The ecliptic poles occupy favored places for several current and up-coming astronomical survey satellites, including Gaia (astrometry), TESS (exoplanets and asteroseismology), and eROSITA (coronal X-rays). These instruments scan along lines of ecliptic longitude, and thus accumulate their deepest exposures in the ecliptic polar regions. The 49 EclipSS targets were down-selected from a larger sample of potential candidates to fall in a favorable range of visual magnitudes (not too bright for TESS, but bright enough for eROSITA and COS), ostensibly single stars (a few are known visual binaries of nearly equal components [HD156389, HD22359] with separations smaller than half the COS PSA radius; or with a much fainter secondary [HD144061, HD41004] that likely will not be visible), and not have any other bright star close by (important for 0.5'-resolution eROSITA). The targets are listed in Table 1. TABLE 1. EclipSS Targets =================================================================== # Name RA Dec V SpTp B-V d GAL RASS (hms) (dms) (mag) Lum (mag) (pc) (logLx) ------------------------------------------------------------------- 01 HD156559 17 14 43 +58 23 02 7.89 F2V 0.37 84 Y 28.72 02 HD39755 05 50 18 -62 04 48 7.82 F2V 0.38 79 Y 28.95 03 HD156389 17 14 06 +56 08 01 7.77 F2V 0.45 86 Y -- AB 0.4" PA=319 dHp=0.28 04 HD24636 03 48 11 -74 41 38 7.12 F3V 0.38 57 Y 28.93 05 HD21166 03 18 57 -73 59 10 7.23 F3V 0.39 73 Y -- 06 HD56737 07 14 22 -61 04 11 7.16 F3V 0.41 59 Y -- 07 HD154956 17 05 47 +53 45 03 8.29 F5V 0.46 93 Y -- 08 HD53658 07 01 05 -65 42 23 7.34 F6V 0.41 57 Y -- 09 HD28481 04 26 38 -53 42 15 8.30 F6V 0.44 100 Y -- 10 HD22359 03 32 43 -60 34 27 7.65 F6V 0.46 68 Y -- AB 0.7" PA=85 dHp=0.35 11 HD29255 04 29 58 -72 16 31 8.36 F6V 0.48 86 Y -- 12 HD165700 18 04 00 +55 16 23 7.80 F8V 0.41 89 Y 28.71 13 HD185239 19 34 51 +57 46 21 8.16 F8V 0.41 81 Y 28.49 14 HD168093 18 15 20 +50 58 16 7.66 F8V 0.53 54 Y -- 15 HD20052 03 10 08 -62 21 27 8.34 F8V 0.54 79 Y -- 16 HD180712 19 14 01 +59 33 06 7.99 F8V 0.58 45 Y 28.07 17 HD159329 17 29 44 +63 51 09 7.67 F9V 0.52 46 Y -- 18 HD36767 05 25 19 -75 41 32 7.18 F9V 0.53 36 Y -- 19 HD187876 19 49 12 +57 24 33 7.76 G0V 0.56 47 N -- 20 HD146044 16 10 47 +59 40 31 8.13 G0V 0.68 43 Y -- 21 HD51929 06 55 53 -56 56 32 7.43 G2V 0.59 38 N -- 22 HD28701 04 25 45 -69 59 37 7.87 G2V 0.61 44 Y -- 23 HD172669 18 36 23 +66 54 47 7.60 G3V 0.58 36 Y 28.12 24 HD150706 16 31 17 +79 47 23 7.02 G3V 0.60 28 Y 28.90 25 HD62850 07 42 36 -59 17 50 7.19 G3V 0.64 33 N 29.22 26 HD24293 03 48 01 -64 50 11 7.85 G3V 0.65 43 Y -- 27 HD64184 07 49 26 -59 22 51 7.52 G3V 0.67 33 N -- 28 HD73744 08 32 15 -76 55 43 7.61 G5V 0.60 35 N -- 29 HD147231 16 14 50 +70 55 46 7.90 G5V 0.63 41 Y -- 30 HD28471 04 25 09 -64 04 48 7.91 G5V 0.65 44 Y -- 31 HD144061 15 58 21 +70 53 40 7.29 G5V 0.66 29 N -- AB 2.3" PA=34 dV=5.0 32 HD146868 16 14 57 +60 40 11 7.69 G5V 0.66 30 Y -- 33 HD137826 15 24 04 +66 33 14 8.72 G6V 0.69 49 Y 28.38 34 HD32778 05 02 17 -56 04 49 7.02 G7V 0.63 22 Y -- 35 HD34297 05 06 35 -77 34 02 7.31 G8V 0.66 40 Y -- 36 HD199476 20 51 44 +74 46 49 7.81 G8V 0.70 30 Y -- 37 HD55720 07 11 31 -49 25 27 7.47 G8V 0.77 28 N -- 38 HD63765 07 47 49 -54 15 50 8.10 G9V 0.75 32 N -- 39 HD161897 17 41 06 +72 25 13 7.61 K0V 0.72 30 N 28.26 40 HD201651 21 06 56 +69 40 28 8.20 K0V 0.74 32 N -- 41 HD39194 05 44 31 -70 08 36 8.07 K0V 0.76 26 N -- 42 HD51608 06 54 51 -55 15 33 8.17 K0V 0.77 35 Y -- 43 HD151541 16 42 38 +68 06 07 7.56 K1V 0.76 24 Y -- 44 HD47252 06 31 56 -68 42 35 8.27 K1V 0.79 28 Y -- 45 HD202123 21 08 40 +73 41 48 8.70 K1V 0.82 32 Y -- 46 HD41004 05 59 49 -48 14 22 8.65 K1V 0.84 37 Y 29.24 AB 0.5" dHp=3.7 PA=176 47 HD42286 06 06 03 -59 32 35 8.47 K1V 0.84 25 Y -- 48 HD38459 05 43 26 -47 49 22 8.50 K1V 0.87 37 Y 28.56 49 HD30501 04 45 38 -50 04 27 7.58 K2V 0.88 21 Y 27.98 90 Mjup companion ------------------------------------------------------------------- GAL= Galex; RASS= Rosat all-sky survey; log(Lx) in erg/s The observing plan is similar for all the targets, requiring a single COS orbit each. Following the Guide Star acquisition, an NUV imaging ACQ is carried out, using the BOA and either Mirror A or B depending on the target brightness. The NUV exposure times range from about 10s (Mirror A) to about 200s (Mirror B). The NUV ACQ is followed by exposures with G130M-1223 at FP-POS 3 and 4 (107-121 nm [Segment B], 122-136 nm [A]), then G130M-1291, again at FP-POS 3 and 4 (113-128 nm [B], 129-143 [A]). Each sub-exposure was assigned the same duration, about 520 s for the typical target. The 113-136 nm region is (mostly, except for Ly-alpha) covered by all four exposures, so that fixed pattern noise would be effectively mitigated for that interval. SAFETY ISSUES. Athough the targets have not been observed previously in the FUV (e.g., by IUE), they are optically faint enough that the normal chromospheric (O I 130 nm, C II 133 nm) and "sub-coronal" lines (N V 124 nm, Si IV 139 nm) also will be faint, so that detector safety concerns should not be an issue. To test this, ETC simulations were carried out using an "extreme" FUV reference spectrum. The test spectrum was constructed by first collecting STIS FUV tracings, from the StarCAT catalog, of thirteen representative dwarf stars covering the same spectral type range as the EclipSS targets; interpolating these onto a reference wavelength scale correcting for radial velocities and after adjusting the flux scales to V=0; then taking the average of the top three values at each wavelength. The constituent stars were chosen such that their ROSAT All-Sky Survey (RASS) luminosities were in the same (upper) range as recorded for the 14 EclipSS targets having RASS detections (the rest are upper limits). The final co-added spectrum is dominated by the 3 reference StarCAT dwarfs with log(Lx)>29 (erg/s). The "extreme" FUV spectrum then was adjusted to V=7.2 mag, which is the value of the brightest of the two EclipSS targets with log(Lx)>29 (HD62850: 29.22). The reference spectrum is typical of a moderately active dwarf star, like those of the Hyades cluster (already safely observed by COS) but still far below the most active G dwarfs, such as the young (50 Myr) solar analog EK Draconis (which has log(Lx)>30). Most of the EclipSS targets (i.e., those with only RASS upper limits: log(Lx)<28), will have much fainter FUV energy distributions than that of the test spectrum. Further, the EclipSS targets were specifically drawn from spectral classes (F2-K2) that are not known for large flare events (unlike the early/mid-M dwarfs), and long-term FUV variability (say, due to activity cycles) is observed to be modest in such stars as well. The only potential spectral safety issue identified in the ETC simulations involves the brightest feature in cool-star FUV spectra: H I Ly-alpha. The ETC run (COS.sp.1005139) for the extreme FUV spectrum at Ly-alpha predicts a brightest pixel of 0.28 cps, of which most (60% ) is contributed by the sky geocoronal background assumed by the simulation. This is 4x below the local count rate limit (for the star-alone contribution of 0.11 cps, on top of the 0.17 cps geocoronal), especially considering that the Ly-alpha emission of the generally more distant EclipSS targets likely is more degraded by ISM absorption than the closer StarCAT stars that comprise the reference FUV spectrum. Further, the "extreme" ETC simulation refers to just the most active (in terms of Lx) of the EclipSS stars, HD62850; all the other targets have lower log(Lx), or similar log(Lx) but fainter V magnitude, and thus weaker expected Ly-alpha. If, however, it is deemed that Ly-alpha observations of the most active of the EclipSS targets are too risky, then "Plan B" would be to observe with G130M-1223 A+B, but then turn off side B for the subsequent G130M-1291 exposures. The reconfiguration, however, "costs" about 350s, so would result in a loss of about 16% exposure. Another possibility would be to use segment A exclusively for 1223 and 1291, which would not give up any exposure time, but would lose key diagnostics below Ly-alpha, such as Si III 120 nm and C III 117 nm, so is not preferred. Indeed, recording Ly-alpha would be an important objective in itself, so the program as proposed is the best option scientifically, with essentially no risk. Finally, in terms of background FUV objects that might be included in the COS PSA, most of the targets (38 of the 49) have Galex detections, all with the (low) intensity expected from the cool star itself, which rules out background sources for those cases. Further, some of the "non-Galex" targets have high proper motions. Thus, in the decades separating sky surveys like POSS and 2MASS from the present epoch, the proper motion of the typical EclipSS target would place it at a position that was "uncovered" in the earlier surveys, and thus allow any current close background object to be identified. Also, the ecliptic poles are away from the galactic equator, so the density of, say, background 14th magnitude O-type stars would be small to begin with, and the chances of a high-latitude hot star accidentally falling into the COS aperture is vanishingly small. (The one possible exception is HD39194 [target #41], which happens to be projected against the outskirts of the LMC. Fortunately, this is one of the high proper motion stars, and the target confirmation chart shows that the contemporary position is free of any other objects.) Stellar Physics 0 false false true false false false 0.0 0.0 false SUPPORTED STAR F0-F2 NO J2000 J2000 sptyp= F2V; (B-V)= 0.37 mag; dist= 84 pc STAR F0-F2 NO J2000 J2000 sptyp= F2V; (B-V)= 0.38 mag; dist= 79 pc STAR F0-F2 NO J2000 J2000 sptyp= F2V; (B-V)= 0.45 mag; dist= 86 pc STAR F3-F9 NO J2000 J2000 sptyp= F3V; (B-V)= 0.38 mag; dist= 57 pc STAR F3-F9 NO J2000 J2000 sptyp= F3V; (B-V)= 0.39 mag; dist= 73 pc STAR F3-F9 NO J2000 J2000 sptyp= F3V; (B-V)= 0.41 mag; dist= 59 pc STAR F3-F9 NO J2000 J2000 sptyp= F5V; (B-V)= 0.46 mag; dist= 93 pc STAR F3-F9 NO J2000 J2000 sptyp= F6V; (B-V)= 0.41 mag; dist= 57 pc STAR F3-F9 NO J2000 J2000 sptyp= F6V; (B-V)= 0.44 mag; dist= 100 pc STAR F3-F9 NO J2000 J2000 sptyp= F6V; (B-V)= 0.46 mag; dist= 68 pc STAR F3-F9 NO J2000 J2000 sptyp= F6V; (B-V)= 0.48 mag; dist= 86 pc STAR F3-F9 NO J2000 J2000 sptyp= F8V; (B-V)= 0.41 mag; dist= 89 pc STAR F3-F9 NO J2000 J2000 sptyp= F8V; (B-V)= 0.41 mag; dist= 81 pc STAR F3-F9 NO J2000 J2000 sptyp= F8V; (B-V)= 0.53 mag; dist= 54 pc STAR F3-F9 NO J2000 J2000 sptyp= F8V; (B-V)= 0.54 mag; dist= 79 pc STAR F3-F9 NO J2000 J2000 sptyp= F8V; (B-V)= 0.58 mag; dist= 45 pc STAR F3-F9 NO J2000 J2000 sptyp= F9V; (B-V)= 0.52 mag; dist= 46 pc STAR F3-F9 NO J2000 J2000 sptyp= F9V; (B-V)= 0.53 mag; dist= 36 pc STAR G V-IV NO J2000 J2000 sptyp= G0V; (B-V)= 0.56 mag; dist= 47 pc STAR G V-IV NO J2000 J2000 sptyp= G0V; (B-V)= 0.68 mag; dist= 43 pc STAR G V-IV NO J2000 J2000 sptyp= G2V; (B-V)= 0.59 mag; dist= 38 pc STAR G V-IV NO J2000 J2000 sptyp= G2V; (B-V)= 0.61 mag; dist= 44 pc STAR G V-IV NO J2000 J2000 sptyp= G3V; (B-V)= 0.58 mag; dist= 36 pc STAR G V-IV NO J2000 J2000 sptyp= G3V; (B-V)= 0.60 mag; dist= 28 pc STAR G V-IV NO J2000 J2000 sptyp= G3V; (B-V)= 0.64 mag; dist= 33 pc STAR G V-IV NO J2000 J2000 sptyp= G3V; (B-V)= 0.65 mag; dist= 43 pc STAR G V-IV NO J2000 J2000 sptyp= G3V; (B-V)= 0.67 mag; dist= 33 pc STAR G V-IV NO J2000 J2000 sptyp= G5V; (B-V)= 0.60 mag; dist= 35 pc STAR G V-IV NO J2000 J2000 sptyp= G5V; (B-V)= 0.63 mag; dist= 41 pc STAR G V-IV NO J2000 J2000 sptyp= G5V; (B-V)= 0.65 mag; dist= 44 pc STAR G V-IV NO J2000 J2000 sptyp= G5V; (B-V)= 0.66 mag; dist= 29 pc STAR G V-IV NO J2000 J2000 sptyp= G5V; (B-V)= 0.66 mag; dist= 30 pc STAR G V-IV NO J2000 J2000 sptyp= G6V; (B-V)= 0.69 mag; dist= 49 pc STAR G V-IV NO J2000 J2000 sptyp= G7V; (B-V)= 0.63 mag; dist= 22 pc STAR G V-IV NO J2000 J2000 sptyp= G8V; (B-V)= 0.66 mag; dist= 40 pc STAR G V-IV NO J2000 J2000 sptyp= G8V; (B-V)= 0.70 mag; dist= 30 pc STAR G V-IV NO J2000 J2000 sptyp= G8V; (B-V)= 0.77 mag; dist= 28 pc STAR G V-IV NO J2000 J2000 sptyp= G9V; (B-V)= 0.75 mag; dist= 32 pc STAR K V-IV NO J2000 J2000 sptyp= K0V; (B-V)= 0.72 mag; dist= 30 pc STAR K V-IV NO J2000 J2000 sptyp= K0V; (B-V)= 0.74 mag; dist= 32 pc STAR K V-IV NO J2000 J2000 sptyp= K0V; (B-V)= 0.76 mag; dist= 26 pc STAR K V-IV NO J2000 J2000 sptyp= K0V; (B-V)= 0.77 mag; dist= 35 pc STAR K V-IV NO J2000 J2000 sptyp= K1V; (B-V)= 0.76 mag; dist= 24 pc STAR K V-IV NO J2000 J2000 sptyp= K1V; (B-V)= 0.79 mag; dist= 28 pc STAR K V-IV NO J2000 J2000 sptyp= K1V; (B-V)= 0.82 mag; dist= 32 pc STAR K V-IV NO J2000 J2000 sptyp= K1V; (B-V)= 0.84 mag; dist= 37 pc STAR K V-IV NO J2000 J2000 sptyp= K1V; (B-V)= 0.84 mag; dist= 25 pc STAR K V-IV NO J2000 J2000 sptyp= K1V; (B-V)= 0.87 mag; dist= 37 pc STAR K V-IV NO J2000 J2000 sptyp= K2V; (B-V)= 0.88 mag; dist= 21 pc COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G130M 1327 1518475940212 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1535071375000 109.47928357879908 (Tic-Visit :proposal-id 15300 :visit-id "01" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 15:52:19.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518476135641 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1535005407000 242.06947556867345 (Tic-Visit :proposal-id 15300 :visit-id "02" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 15:55:35.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3138 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3471 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518477545511 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. AB 0.4" PA=319 dHp=0.28; ORIENT to separate nearly equal pair spatially 1534476973000 115.87004763019507 (Tic-Visit :proposal-id 15300 :visit-id "03" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 16:19:05.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518477656019 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1544531578000 21.0 (Tic-Visit :proposal-id 15300 :visit-id "04" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 16:20:55.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3252 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3585 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518477909353 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1544901299000 35.0 (Tic-Visit :proposal-id 15300 :visit-id "05" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 16:25:09.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "05" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3252 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3585 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518478146195 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1544402798000 330.7173332050653 (Tic-Visit :proposal-id 15300 :visit-id "06" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 16:29:06.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3138 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3471 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518478305286 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1534757346000 111.1183444628117 (Tic-Visit :proposal-id 15300 :visit-id "07" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 16:31:45.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "07" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3060 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3393 :pcs-gap 0 ) false 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518478610048 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1544647233000 334.0 (Tic-Visit :proposal-id 15300 :visit-id "08" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 16:36:49.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "08" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3212 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3546 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518479747269 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1544469866000 3.846096068820799 (Tic-Visit :proposal-id 15300 :visit-id "09" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 16:55:47.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "09" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3060 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3393 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518491312520 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. AB 0.7" PA=85 dHp=0.35; ORIENT to separate nearly equal pair spatially 1544347699000 20.886037043562112 (Tic-Visit :proposal-id 15300 :visit-id "10" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 20:08:32.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "10" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3138 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3471 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518491536704 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1520313931000 96.83640897102742 (Tic-Visit :proposal-id 15300 :visit-id "11" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 20:12:16.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "11" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3252 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3585 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1523904249235 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. /solaris/user1/dctaylor/proposals2/OP-cache/15300-v51.xml Repeat for failed visit 11. 1535838268000 270.5760869266626 (Tic-Visit :proposal-id 15300 :visit-id "51" :proposal-version -1 :trans-version "20171009" :date "16-Apr-2018 14:44:08.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "51" :obset-id "51" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "51" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3252 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3585 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518491705897 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1534488517000 122.0 (Tic-Visit :proposal-id 15300 :visit-id "12" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 20:15:05.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "12" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518491959474 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1534562854000 146.40730047276912 (Tic-Visit :proposal-id 15300 :visit-id "13" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 20:19:19.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "13" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518492044446 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1534571201000 127.20987852151029 (Tic-Visit :proposal-id 15300 :visit-id "14" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 20:20:44.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 435008 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "14" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3059 :al-overhead-at-end 0 :internal-dur-at-end 350 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3393 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518492241865 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15300 :visit-id "15" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 20:24:01.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "15" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3138 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3471 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518492388793 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1534625620000 140.9961700922014 (Tic-Visit :proposal-id 15300 :visit-id "16" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 20:26:28.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "16" :obset-id "16" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "16" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518492569307 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1534648276000 117.32104958665701 (Tic-Visit :proposal-id 15300 :visit-id "17" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 20:29:29.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "17" :obset-id "17" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "17" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3138 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3471 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518492884209 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1522718738000 110.0 (Tic-Visit :proposal-id 15300 :visit-id "18" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 20:34:44.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "18" :obset-id "18" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "18" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3246 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3579 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518493237562 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1544561414000 35.2179412326318 (Tic-Visit :proposal-id 15300 :visit-id "19" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 20:40:37.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "19" :obset-id "19" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "19" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518493393824 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15300 :visit-id "20" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 20:43:13.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "20" :obset-id "20" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "20" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518494386317 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1544824494000 339.63031300048954 (Tic-Visit :proposal-id 15300 :visit-id "21" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 20:59:46.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "21" :obset-id "21" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "21" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518494417679 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1541044204000 332.0 (Tic-Visit :proposal-id 15300 :visit-id "22" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 21:00:17.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "22" :obset-id "22" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "22" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3212 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3546 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518494443134 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1534655501000 132.47794461705922 (Tic-Visit :proposal-id 15300 :visit-id "23" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 21:00:42.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "23" :obset-id "23" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "23" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3212 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3546 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518494711703 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1545219346000 345.0 (Tic-Visit :proposal-id 15300 :visit-id "24" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 21:05:11.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "24" :obset-id "24" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "24" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3246 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3579 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518495061575 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1534825200000 214.53635032655507 (Tic-Visit :proposal-id 15300 :visit-id "25" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 21:11:01.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "25" :obset-id "25" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "25" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518495446533 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1540839047000 337.49 (Tic-Visit :proposal-id 15300 :visit-id "26" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 21:17:26.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "26" :obset-id "26" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "26" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3138 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3471 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518495832672 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1535081977000 215.8231508465658 (Tic-Visit :proposal-id 15300 :visit-id "27" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 21:23:52.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "27" :obset-id "27" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "27" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518496021057 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1535169802000 204.3 (Tic-Visit :proposal-id 15300 :visit-id "28" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 21:27:00.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "28" :obset-id "28" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "28" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3246 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3579 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518496187573 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1544389926000 348.2842407178242 (Tic-Visit :proposal-id 15300 :visit-id "29" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 21:29:47.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "29" :obset-id "29" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "29" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3252 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3585 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518496895630 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1544378041000 9.179640122044901 (Tic-Visit :proposal-id 15300 :visit-id "30" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 21:41:35.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "30" :obset-id "30" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "30" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3138 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3471 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518497093735 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. AB 2.3" PA=34 dV=5.0; ORIENT to keep faint secondary away from primary spectrum (Tic-Visit :proposal-id 15300 :visit-id "31" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 21:44:53.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "31" :obset-id "31" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "31" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3252 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3585 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518497179276 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1545291171000 337.938225137068 (Tic-Visit :proposal-id 15300 :visit-id "32" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 21:46:19.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "32" :obset-id "32" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "32" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3138 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3471 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518505086400 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1516935403000 288.8 (Tic-Visit :proposal-id 15300 :visit-id "33" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 23:58:05.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 435008 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "33" :obset-id "33" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "33" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3211 :al-overhead-at-end 0 :internal-dur-at-end 350 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3546 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1543333585886 The scheduling data was generated by CASM 26.2. CASM was run in Phase II mode. 1544800928000 5.658869326385911 (Tic-Visit :proposal-id 15300 :visit-id "34" :proposal-version -1 :trans-version "20180927" :date "27-Nov-2018 10:46:25.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "34" :obset-id "34" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "34" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 acquistion changed to MIRROR B (27 NOV 2018) to account for bluer color of target than expected for late-G spectral type; also compatible with the Galex NUV magnitude. ETC simulation done with Cas-Kur G2V model, V=+7.02. Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518498045257 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1525395048000 136.88829491223618 (Tic-Visit :proposal-id 15300 :visit-id "35" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 22:00:45.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "35" :obset-id "35" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "35" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3246 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3579 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518498338775 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1543532615000 62.71357759950891 (Tic-Visit :proposal-id 15300 :visit-id "36" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 22:05:38.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "36" :obset-id "36" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "36" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3252 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3585 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518499395242 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1535316531000 229.32128200074072 (Tic-Visit :proposal-id 15300 :visit-id "37" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 22:23:13.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "37" :obset-id "37" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "37" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3012 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3345 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518500120411 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1534279805000 207.70120042372855 (Tic-Visit :proposal-id 15300 :visit-id "38" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 22:35:20.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "38" :obset-id "38" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "38" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3060 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3393 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518500879152 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1538447574000 76.94661183737298 (Tic-Visit :proposal-id 15300 :visit-id "39" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 22:47:58.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "39" :obset-id "39" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "39" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3252 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3585 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518501119322 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15300 :visit-id "40" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 22:51:59.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "40" :obset-id "40" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "40" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3212 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3546 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518501461363 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1544721516000 354.9317658764203 (Tic-Visit :proposal-id 15300 :visit-id "41" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 22:57:41.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "41" :obset-id "41" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "41" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3252 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3585 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518501735233 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1544367006000 334.4093345886758 (Tic-Visit :proposal-id 15300 :visit-id "42" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 23:02:15.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "42" :obset-id "42" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "42" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518501903809 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1545477309000 342.0016415932514 (Tic-Visit :proposal-id 15300 :visit-id "43" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 23:05:03.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "43" :obset-id "43" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "43" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3212 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3546 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518502137655 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1544809577000 345.0993138466972 (Tic-Visit :proposal-id 15300 :visit-id "44" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 23:08:57.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "44" :obset-id "44" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "44" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3212 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3546 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518502414867 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1529922113000 219.3612640047832 (Tic-Visit :proposal-id 15300 :visit-id "45" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 23:13:34.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "45" :obset-id "45" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "45" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3252 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3585 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518502614736 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. AB 0.5" dHp=3.7 PA=176; ORIENT to separate fainter secondary from primary spectrum 1541009815000 307.0 (Tic-Visit :proposal-id 15300 :visit-id "46" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 23:16:54.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 435008 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "46" :obset-id "46" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "46" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3011 :al-overhead-at-end 0 :internal-dur-at-end 350 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3345 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518502897010 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1534801087000 236.4246891220797 (Tic-Visit :proposal-id 15300 :visit-id "47" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 23:21:36.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "47" :obset-id "47" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "47" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3116 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3449 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518503195262 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15300 :visit-id "48" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 23:26:34.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 435008 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "48" :obset-id "48" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "48" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3011 :al-overhead-at-end 0 :internal-dur-at-end 350 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3345 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1518505090317 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15300 :visit-id "49" :proposal-version -1 :trans-version "20171009" :date "12-Feb-2018 23:58:09.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "49" :obset-id "49" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "49" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3060 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3393 :pcs-gap 0 ) true 1 0 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). 1544737835756 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /private/var/folders/56/c_jk44c970v8fj73rtx427cm0006v6/T/OPVisit5221687581817470779.xml Copy of failed visit 30 (Tic-Visit :proposal-id 15300 :visit-id "53" :proposal-version -1 :trans-version "20181130" :date "13-Dec-2018 16:50:35.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 400256 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15300 :visit-id "53" :obset-id "53" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15300 :visit-id "53" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3136 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3411 :pcs-gap 0 ) true 1 1 Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description). Note: ETC simulation (for G130M-1291, so as to include Ly-alpha) is for an "extreme" FUV spectrum, scaled to V=7.2 mag, and thus will over-predict count rates for most of the targets (see Observation Description).