0 Assigned ID: 177 ----- Attempting Submission 1 (Thu Apr 09 07:31:20 GMT 2015) ----- HST Phase I Proposal 177 (ovi_survey_mh1.apt) successfully submitted. Receipt: # 177-1 ----- Attempting Submission 2 (Fri Apr 10 12:01:47 GMT 2015) ----- FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. 2017-05-04: ON HOLD released for visit 39 2016-12-07 : target is point-like in the UV. modified accordingly. 2016-12-07 : ON HOLD status released for Visit 19. Acquisition of ACS+UVIS data for same target now enable permit accurate for the PII. 2016-10-04 : ON HOLD status released for Visit 49. Acquisition of ACS+UVIS data for same target now enable permit accurate for the PII. 2016-07-13 : ON HOLD status released for Visit 29. Acquisition of ACS+UVIS data for same target now enable permit accurate for the PII. 2015-07-23 : two targets replaced in accordance with Change Request 81476. Dithering pattern for SBC visits also improved. 2015-06-30 : estimated exposure times applied for the COS visits 19,29,39,49 907669397 ----- Attempting Submission 1 (Sun Jun 28 18:41:24 GMT 2015) ----- HST Phase II Proposal 14079 (ovi_survey_mh1.apt) successfully submitted. Receipt: # 14079-1 ----- Attempting Submission 2 (Tue Jun 30 12:55:33 GMT 2015) ----- ----- Attempting Submission 3 (Thu Jul 23 09:24:11 GMT 2015) ----- ----- Attempting Submission 4 (Wed Jul 13 12:34:51 GMT 2016) ----- ----- Attempting Submission 5 (Tue Oct 04 09:04:34 GMT 2016) ----- ----- Attempting Submission 6 (Wed Dec 07 15:47:07 GMT 2016) ----- HST Phase II Proposal 14079 (ovi_survey_repl3_mh1.apt) successfully submitted. Receipt: # 14079-6 ----- Attempting Submission 7 (Wed Dec 07 15:48:49 GMT 2016) ----- ----- Attempting Submission 8 (Thu May 04 13:59:46 GMT 2017) ----- 2017-05-04. All warning relate to previosly executed visits and none to the only remaining visit. 2016-12-07. The only modified visit is 19, which shows no errors or warnings. All the others must be accounted for with the comments below. 2016-10-04. The only modified visit is 49, which shows no errors or warnings. All the others must be accounted for with the comments below. 2016-07-13. The only modified visit is 29, which shows no errors or warnings. All the others must be accounted for with the comments below. Warnings relate to: - visibility overrun in the SBC frames, which appears not to be true for any orbits. I beleive this is becuase of the positioning of SHADOW observations within the orbits, but also that that is not true - possible CTE issues with UVIS observations, but the ETC (IDs included here) indicate that the inserted values are correct - The COS visits being placeholders because these visits are ON HOLD. Unveiling the Dark Baryons II: the First Sample of OVI Emission Imaging Hot gas outflows, crossing the extended circumgalactic medium of galaxies, regulate star formation, shape the galaxy luminosity function and mass-metallicity relation, and enrich the intergalactic medium. Over a wide temperature range of 5<log(T/K)<6, the cooling of this hot CGM flow is dominated by OVI (lambda=1032,1038 AA) emission. Thus OVI plays a vital role in driving, cooling, and observationally probing galaxy outflows. The difficulty is that OVI gas is typically only seen in absorption against QSOs: spatial information for a single galaxy has therefore never been available, making it difficult to estimate the mass of missing baryons/metals in this phase and its impact on braking galaxy superwinds and enriching the IGM. We have devised a method of using ACS/SBC to isolate far UV emission lines, demonstrated it many times on Lyman alpha, and in HST Cycle 22 adapted to OVI. For the first time we have mapped OVI emission, revealing the halo of extended emission. We here propose to produce the first set of such images, extending the sample to a total of five galaxies, by targeting four more strong starbursts at <z>=0.25. From calibrated OVI maps we will calculate the allowed ranges of temperature, metallicity, and density, and estimate the OVI mass from resolved information. New constraints on galactic wind models and input for cosmological simulations may be expected. This work is exploratory, but the possible scientific return is extremely high, and the method verified. Results will guide subsequent HST observations and next generation UV satellites, and thus it is truly in the spirit of the UV initiative. We will obtain ACS/SBC imaging, WFC3/UVIS imaging, and COS/FUV spectroscopy of four starburst galaxies that host strong starbursts. The redshift of the objects is between 0.23 and 0.27. For each galaxy we will obtain: - 6 orbits imaging with ACS/SBC, split between the F125LP and F140LP filters. These will be done over 3 visits of 2 orbits each. - 1 orbit imaging with WFC3/UVIS, that obtains F390W, F475W, and F850LP frames - 1 orbit of UV spectroscopy with COS SBC IMAGING ==================== *** As with our other programmes, we request that the SBC amplifiers have been turned off for 24 hours prior to our SBC visits. This allows the SBC to cool and 'reset' the Dark Current to its minimum before our observations begin. *** For the same reasons of Dark Current, the 6 orbits of SBC imaging are split into 3 visits of 2 orbits each 3 x 2-orbit visits in F125LP and F140LP step over 9 positions on a 3x3 grid spaced by 4 arcsec. This is to reduce the effects of lower frequency flatfielding errors. At each position 1 exposure is obtained in each filter that are offset by a manually defined dither that steps over the occulting bar but maintains 1/3 pixel sampling. The F125LP observation must be conducted in earth shadow, and is therefore placed at the end of the orbit. ETC runs have assumed the GALEX FUV and NUV magnitudes, point-sources, : # SDSS name m_FUV [AB] m_NUV F125LP ETC F140LP ETC 1 SDSSJ 1107+4528 19.8646 19.1506 714807 714808 2 SDSSJ 1248+1558 20.6293 20.6776 733008 733010 3 SDSSJ 1112+2732 19.2845 19.5276 714811 714812 4 SDSSJ 1547+5119 19.7606 19.4160 733011 733012 Since our exposure times range between 380 and 500 seconds, we adopt 500 sec throughout - that will give the highest number of counts in a given pixel. UVIS IMAGING ==================== Postflashing is used for WRC3/UVIS observations in order to mitigate CTE effects. The level is determined by the ETC. We enter an infeasibly low source surface brightness (40 AB/arcsec2) and the exposure time, adjusting the number of postflash electrons to not trigger a warning. # EXPTIME ETC ID PF e- F390 F475 F850 F390 F475 F850 F390 F475 F850 1 430 348 348 714824 714832 714835 8 3 8 2 365 348 348 714826 714832 714835 9 3 8 3 368 348 348 714827 714832 714835 9 3 8 4 455 348 348 733021 714832 714835 8 3 8 COS SPECTROSCOPY ==================== COS spectroscopy is done by targeting the brightest regions in the far UV. These are determined by F140LP and F390W imaging from the above sections. A full description of how this is optimized can be found in the comments box for visits 19, 29, 39, and 49. ISM IN EXTERNAL GALAXIES 6 false true false false false false SUPPORTED GALAXY STARBURST YES This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 log L_FUV / Lsun = 10.5 GALAXY STARBURST NO J2000 J2000 log L_FUV / Lsun = 10.5 GALAXY STARBURST YES J2000 J2000 log L_FUV / Lsun = 10.4 GALAXY NUCLEUS STARBURST NO J2000 J2000 log L_FUV / Lsun = 10.4 GALAXY STARBURST YES This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 log L_FUV / Lsun = 10.8 GALAXY STARBURST NO J2000 J2000 log L_FUV / Lsun = 10.8 GALAXY STARBURST YES J2000 J2000 log L_FUV / Lsun = 10.6 GALAXY STARBURST YES J2000 J2000 log L_FUV / Lsun = 10.6 ACS/SBC Imaging No No F125LP ACS/SBC Imaging No No F140LP WFC3/UVIS Imaging No No F390W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F850LP COS/NUV Imaging No No MIRRORA COS/FUV Spectroscopic No No G130M 1300 ACS/SBC Imaging No No F125LP ACS/SBC Imaging No No F140LP WFC3/UVIS Imaging No No F390W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F850LP COS/NUV Imaging No No MIRRORA COS/FUV Spectroscopic No No G130M 1300 ACS/SBC Imaging No No F125LP ACS/SBC Imaging No No F140LP WFC3/UVIS Imaging No No F390W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F850LP COS/NUV Imaging No No MIRRORA COS/FUV Spectroscopic No No G130M 1300 ACS/SBC Imaging No No F125LP ACS/SBC Imaging No No F140LP WFC3/UVIS Imaging No No F390W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F850LP COS/NUV Imaging No No MIRRORA COS/FUV Spectroscopic No No G130M 1300 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. This SBC visit depends critically upon the level of dark current. Please schedule only when the SBC has not been used in the previous 24 hours, so the amplifiers have cooled. 1461145699000 120.6244967691473 (Tic-Visit :proposal-id 14079 :visit-id "11" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:26:57.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "28" :si-bright-earth-limb-angle 20.0 :data-volume 222160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "11" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2984 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset 1591 :dark-utilization 1393 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3352 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14079 :visit-id "11" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3085 :al-overhead-at-end 0 :internal-dur-at-end 279 :dark-offset 1692 :dark-utilization 1393 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3352 :pcs-gap 0 ) false 2 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. This SBC visit depends critically upon the level of dark current. Please schedule only when the SBC has not been used in the previous 24 hours, so the amplifiers have cooled. 1460893865000 120.46676769789252 (Tic-Visit :proposal-id 14079 :visit-id "12" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:26:59.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "28" :si-bright-earth-limb-angle 20.0 :data-volume 222160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "12" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2984 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset 1591 :dark-utilization 1393 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3352 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14079 :visit-id "12" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3085 :al-overhead-at-end 0 :internal-dur-at-end 279 :dark-offset 1692 :dark-utilization 1393 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3352 :pcs-gap 0 ) false 2 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. This SBC visit depends critically upon the level of dark current. Please schedule only when the SBC has not been used in the previous 24 hours, so the amplifiers have cooled. 1461420765000 120.3049428272443 (Tic-Visit :proposal-id 14079 :visit-id "13" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:27:02.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "28" :si-bright-earth-limb-angle 20.0 :data-volume 222160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "13" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2984 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset 1591 :dark-utilization 1393 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3352 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14079 :visit-id "13" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3085 :al-overhead-at-end 0 :internal-dur-at-end 279 :dark-offset 1692 :dark-utilization 1393 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3352 :pcs-gap 0 ) false 2 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. 1480605488000 281.3412392661394 (Tic-Visit :proposal-id 14079 :visit-id "16" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:27:04.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 1732496 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "16" :obset-id "16" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "16" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3018 :al-overhead-at-end 122 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3352 :pcs-gap 0 ) false 1 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. Photometry that guides target acquisition and integration times is done with HST data from visits 11 and 16 from this program. Flux was measured on the brightest UV source in 0.2 arcsec (acquisition) and 1.25 arcsec (spectroscopic observation) apertures, using the F140LP and F390W filters. Then we interpolated (power-law) between the two, to lambda=2300 AA. Fluxes are quoted below. These numbers (and the beta slope) were entered into the acquisition and spectroscopic ETCs. HST Imaging Datasets for Photometry: F140LP 14079 jctd11010 F390W 14079 ictd16010 FUV full = 9.128 adu/sec = 2.4764e-16 cgs/AA FUV ACQ = 3.037 adu/sec = 8.2377e-17 cgs/AA Uband full = 175.235 adu/sec = 9.5808e-17 cgs/AA Uband ACQ = 55.659 adu/sec = 3.0431e-17 cgs/AA Beta full = -1.0070 Beta ACQ = -1.0560 COS/NUV full = 1.8167e-16 cgs/AA COS/NUV ACQ = 5.9527e-17 cgs/AA 1485166494000 248.81602630921384 (Tic-Visit :proposal-id 14079 :visit-id "19" :proposal-version -1 :trans-version "20160601" :date "07-Dec-2016 16:34:30.0" :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 52416 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "19" :obset-id "19" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "19" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3010 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3352 :pcs-gap 0 ) false 1 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. This SBC visit depends critically upon the level of dark current. Please schedule only when the SBC has not been used in the previous 24 hours, so the amplifiers have cooled. 1465983362000 117.72327213882949 (Tic-Visit :proposal-id 14079 :visit-id "21" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:28:03.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "28" :si-bright-earth-limb-angle 20.0 :data-volume 222160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "21" :obset-id "21" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "21" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2864 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset 1531 :dark-utilization 1333 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3221 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14079 :visit-id "21" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2965 :al-overhead-at-end 0 :internal-dur-at-end 279 :dark-offset 1632 :dark-utilization 1333 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3221 :pcs-gap 0 ) false 2 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. This SBC visit depends critically upon the level of dark current. Please schedule only when the SBC has not been used in the previous 24 hours, so the amplifiers have cooled. 1466561579000 115.57747144586972 (Tic-Visit :proposal-id 14079 :visit-id "22" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:28:05.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "28" :si-bright-earth-limb-angle 20.0 :data-volume 222160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "22" :obset-id "22" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "22" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2864 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset 1531 :dark-utilization 1333 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3221 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14079 :visit-id "22" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2965 :al-overhead-at-end 0 :internal-dur-at-end 279 :dark-offset 1632 :dark-utilization 1333 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3221 :pcs-gap 0 ) false 2 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. This SBC visit depends critically upon the level of dark current. Please schedule only when the SBC has not been used in the previous 24 hours, so the amplifiers have cooled. 1466813407000 114.65468690492531 (Tic-Visit :proposal-id 14079 :visit-id "23" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:28:08.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "28" :si-bright-earth-limb-angle 20.0 :data-volume 222160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "23" :obset-id "23" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "23" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2864 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset 1531 :dark-utilization 1333 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3221 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14079 :visit-id "23" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2965 :al-overhead-at-end 0 :internal-dur-at-end 279 :dark-offset 1632 :dark-utilization 1333 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3221 :pcs-gap 0 ) false 2 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. 1460422135000 177.98219796467902 (Tic-Visit :proposal-id 14079 :visit-id "26" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:28:11.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 1732496 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "26" :obset-id "26" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "26" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2888 :al-overhead-at-end 122 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3221 :pcs-gap 0 ) false 1 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. Photometry that guides target acquisition and integration times is done with HST data from visits 21,22,23, and 26 of this program. Flux was measured on the brightest UV source in 0.2 arcsec (acquisition) and 1.25 arcsec (spectroscopic observation) apertures, in the F140LP and F390W filters. Then we interpolated (power-law) between the two, to lambda=2300 AA. Fluxes are quoted below. These numbers (and the beta slope) were entered into the acquisition and spectroscopic ETCs. HST Imaging Datasets for Photometry: F140LP : jctd21010 F390W : ictd26010 FUV full = 8.521 adu/sec = 2.3116e-16 cgs/AA FUV ACQ = 1.850 adu/sec = 5.0201e-17 cgs/AA Uband full = 102.079 adu/sec = 5.5532e-17 cgs/AA Uband ACQ = 25.545 adu/sec = 1.3897e-17 cgs/AA Beta full = -1.5123 Beta ACQ = -1.3620 COS/NUV full = 1.4516e-16 cgs/AA COS/NUV ACQ = 3.3017e-17 cgs/AA 1484916637000 286.0 (Tic-Visit :proposal-id 14079 :visit-id "29" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:29:24.0" :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 52416 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "29" :obset-id "29" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "29" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2886 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3221 :pcs-gap 0 ) false 1 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. This SBC visit depends critically upon the level of dark current. Please schedule only when the SBC has not been used in the previous 24 hours, so the amplifiers have cooled. 1492468478000 126.0 (Tic-Visit :proposal-id 14079 :visit-id "31" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:28:13.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "28" :si-bright-earth-limb-angle 20.0 :data-volume 222160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "31" :obset-id "31" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "31" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2864 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset 1531 :dark-utilization 1333 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14079 :visit-id "31" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2965 :al-overhead-at-end 0 :internal-dur-at-end 279 :dark-offset 1632 :dark-utilization 1333 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) false 2 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. This SBC visit depends critically upon the level of dark current. Please schedule only when the SBC has not been used in the previous 24 hours, so the amplifiers have cooled. 1492868954000 125.60000000000002 (Tic-Visit :proposal-id 14079 :visit-id "32" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:28:20.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "28" :si-bright-earth-limb-angle 20.0 :data-volume 222160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "32" :obset-id "32" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "32" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2864 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset 1531 :dark-utilization 1333 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14079 :visit-id "32" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2965 :al-overhead-at-end 0 :internal-dur-at-end 279 :dark-offset 1632 :dark-utilization 1333 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) false 2 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. This SBC visit depends critically upon the level of dark current. Please schedule only when the SBC has not been used in the previous 24 hours, so the amplifiers have cooled. 1493052023000 132.0 (Tic-Visit :proposal-id 14079 :visit-id "33" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:28:23.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "28" :si-bright-earth-limb-angle 20.0 :data-volume 222160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "33" :obset-id "33" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "33" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2864 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset 1531 :dark-utilization 1333 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14079 :visit-id "33" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2965 :al-overhead-at-end 0 :internal-dur-at-end 279 :dark-offset 1632 :dark-utilization 1333 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) false 2 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. 1459188812000 145.49682118582342 (Tic-Visit :proposal-id 14079 :visit-id "36" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:28:25.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 1732496 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "36" :obset-id "36" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "36" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2894 :al-overhead-at-end 122 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) false 1 0 The scheduling data was generated by CASM 25.0. CASM was run in Phase II mode. /tmp/OPVisit4977119472037096400.xml Photometry that guides target acquisition and integration times is done with HST data from visits 31 and 36 of this program. Flux was measured on the brightest UV source in 0.2 arcsec (acquisition) and 1.25 arcsec (spectroscopic observation) apertures, in the F140LP and F390W filters. Then we interpolated (power-law) between the two, to lambda=2300 AA. Fluxes are quoted below. These numbers (and the beta slope) were entered into the acquisition and spectroscopic ETCs. HST Imaging Datasets for Photometry: F140LP : jctd31010 F390W : ictd36010 FUV full = 18.159 adu/sec = 4.9262e-16 cgs/AA FUV ACQ = 3.710 adu/sec = 1.0064e-16 cgs/AA Uband full = 389.931 adu/sec = 2.1213e-16 cgs/AA Uband ACQ = 71.130 adu/sec = 3.8696e-17 cgs/AA COS/NUV full = 3.7423e-16 cgs/AA COS/NUV ACQ = 7.368e-17 cgs/AA (Tic-Visit :proposal-id 14079 :visit-id "39" :proposal-version -1 :trans-version "20170109" :date "04-May-2017 14:45:06.0" :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 52416 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "39" :obset-id "39" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "39" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2894 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. This SBC visit depends critically upon the level of dark current. Please schedule only when the SBC has not been used in the previous 24 hours, so the amplifiers have cooled. 1469434428000 119.10668066045167 (Tic-Visit :proposal-id 14079 :visit-id "41" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:28:29.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "28" :si-bright-earth-limb-angle 20.0 :data-volume 222160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "41" :obset-id "41" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "41" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3044 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset 1651 :dark-utilization 1393 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14079 :visit-id "41" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3145 :al-overhead-at-end 0 :internal-dur-at-end 279 :dark-offset 1752 :dark-utilization 1393 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) false 2 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. This SBC visit depends critically upon the level of dark current. Please schedule only when the SBC has not been used in the previous 24 hours, so the amplifiers have cooled. 1469520233000 118.22827274625558 (Tic-Visit :proposal-id 14079 :visit-id "42" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:28:32.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "28" :si-bright-earth-limb-angle 20.0 :data-volume 222160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "42" :obset-id "42" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "42" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3044 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset 1651 :dark-utilization 1393 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14079 :visit-id "42" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3145 :al-overhead-at-end 0 :internal-dur-at-end 279 :dark-offset 1752 :dark-utilization 1393 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) false 2 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. This SBC visit depends critically upon the level of dark current. Please schedule only when the SBC has not been used in the previous 24 hours, so the amplifiers have cooled. 1469617523000 117.23136034679442 (Tic-Visit :proposal-id 14079 :visit-id "43" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:28:35.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "28" :si-bright-earth-limb-angle 20.0 :data-volume 222160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "43" :obset-id "43" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "43" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3044 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset 1651 :dark-utilization 1393 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14079 :visit-id "43" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3145 :al-overhead-at-end 0 :internal-dur-at-end 279 :dark-offset 1752 :dark-utilization 1393 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) false 2 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. 1460356783000 220.0542871887381 (Tic-Visit :proposal-id 14079 :visit-id "46" :proposal-version -1 :trans-version "20160601" :date "13-Jul-2016 14:28:37.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 1732496 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "46" :obset-id "46" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "46" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3068 :al-overhead-at-end 122 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) false 1 0 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. Photometry that guides target acquisition and integration times is done with HST data from visits 41 and 46 from this program. Flux was measured on the brightest UV source in 0.2 arcsec (acquisition) and 1.25 arcsec (spectroscopic observation) apertures, using the F140LP and F390W filters. Then we interpolated (power-law) between the two, to lambda=2300 AA. Fluxes are quoted below. These numbers (and the beta slope) were entered into the acquisition and spectroscopic ETCs. HST Imaging Datasets for Photometry ........... F140LP 14079 jctd41010 F390W 14079 ictd46010 Fluxes ........... FUV full = 21.869 adu/sec = 5.9328e-16 cgs/AA FUV ACQ = 3.922 adu/sec = 1.064e-16 cgs/AA Uband full = 370.592 adu/sec = 2.0161e-16 cgs/AA Uband ACQ = 69.632 adu/sec = 3.788e-17 cgs/AA COS/NUV full = 4.1719e-16 cgs/AA COS/NUV ACQ = 7.5968e-17 cgs/AA 1488361614000 258.0 (Tic-Visit :proposal-id 14079 :visit-id "49" :proposal-version -1 :trans-version "20160601" :date "04-Oct-2016 10:49:36.0" :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 87168 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14079 :visit-id "49" :obset-id "49" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14079 :visit-id "49" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3064 :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 3403 :pcs-gap 0 ) false 1 0 Visit is ON HOLD until the UVIS/F390W and one SBC/F140LP image are in hand. This will allow us to properly define the acquisition procedure, and optimise the integration times.