Science Keywords: Select from 2 to 5 items. Science Keywords is a required field. Small GO Proposals are not allowed in Cycle 26 unless they are Joint Programs. Wavelength is a required field. Wavelength is a required field. Wavelength is a required field. Wavelength is a required field. Please specify your scheduling constraints or 'No Constraints' on all Observation forms. 0 Assigned ID: 617 ----- Attempting Submission 1 (Tue Nov 27 14:52:33 GMT 2018) ----- Joint HST/XMM 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. 0 ----- Attempting Submission 1 (Mon Jan 07 21:18:31 GMT 2019) ----- For the short exposures in this proposal, 4 FPPOS positions in G160M is overkill. We have used two central wavelength settings and two FPPOS positions apiece, thus having four independent detector positions for each wavelength. AGN can be obscured by gas streams close to the black hole that shield remote regions from ionising radiation. We witnessed such an event in NGC 5548 and NGC 3783 where 90% of the soft X-rays are blocked by a dense gas stream close to the BLR. Our joint observations with XMM-Newton, NuSTAR and HST/COS showed UV broad absorption lines associated with the X-ray absorption and allowed us to characterise this unique obscuration event completely. We propose to investigate a similar event in another Seyfert 1 using the same instruments. Swift monitoring (98 ks) will be used to find the event, which will be characterised by joint ToO observations with XMM-Newton (150 ks), HST/COS (4 orbits) and NuSTAR (50 ks). We will observe a Seyfert 1 galaxy that has entered an obscured phase similar to NGC 5548, NGC 985, or Mrk 335 in order to use simultaneous XMM-Newton, NuSTAR, and HST/COS observations to measure the physical characteristics of the outflow causing the obscuration. Our observations will be triggered via a monitoring program conducted on 7 bright Seyfert 1 galaxies with Swift. The first XMM-Newton observation will be as soon as possible after the trigger and 100 ks in duration in order to have well-determined obscurer parameters. An additional observation of 50 ks following the first observation but before the end of the XMM visibility window will enable us to study the variability of the obscurer. As nearly simultaneous with each XMM visit as possible, we will observe for 25 ks with NuSTAR and for 2 orbits with HST/COS. Our COS observations will use gratings G130M and G160M in order to observe the main absorption line transitions in C III* 1176, Ly alpha, N V, Si IV, and C IV. Our previous observational campaigns on Mrk 279, Mrk 509, NGC 5548, and NGC 985 all achieved good results with a signal-to-noise ratio of 20 per resolution element in the continuum for these objects. To achieve a 4-fold diversity of grating settings for each grating, we use all 4 FP-POS positions with CENWAVE=1222 for G130M. For G160M, we use CENWAVES 1533 and 1629 to cover the full FUV wavelength range and to span the gap between segments A and B. We use 2 FP-POS positions for each CENWAVE. To outline the ETC calculations for our potential targets, we tabulate results for all 8 here. (Fluxes are obtained from Dunn et al. 2006, PASP, 118, 572, and from the MAST archive.) Source z E(B-V) Min_Flam Max_Flam Mean_Flam NGC 3227 0.003859 0.020 0.05e-14 0.4e-14 0.12e-14 NGC 4593 0.00900 0.022 0.5e-14 2.4e-14 1.5e-14 Mrk 841 0.036422 0.026 2.0e-14 4.3e-14 3.2e-14 Mrk 509 0.034397 0.051 4.1e-14 1.4e-13 9.0e-14 Ark 564 0.024684 0.053 0.6e-14 1.0e-14 0.8e-14 MR2251-178 0.063980 0.035 1.8e-14 4.7e-14 3.3e-14 NGC 7469 0.016317 0.061 2.7e-14 7.1e-14 4.9e-14 We note that our triggered TOO observation will observe only *one* of these objects. These observations pose no bright object concerns. All historical flux levels for each of the AGN in our sample lie below the bright object limits for COS. Since all of these objects have been observed successfully before using either COS or STIS, there are also no surrounding field objects that are too bright. All of our targets are faint enough that we can use an imaging target acquisition with Mirror B, except for Mrk 509, for which we use a spectroscopic target acquisition. Rather than do a separate ETC check on bright object constraints for each AGN, we simply show here calculations for the brightest object for which we do an imaging target acquisition, NGC 7469, and the brightest overall, Mrk 509. (We note that the only AGN that could ever violate the COS brightness limits are NGC 4151 and 3C 273.) Our ETC calculations use the ETC FOS quasar spectrum redshifted appropriately with foreground Milky Way extinction from NED. Here we show calculations relevant for the minimum and maximum fluxes expected (Dunn et al. 2006) in order to get our limiting cases: - ACQUISITION (for Mrk 509)- Configuration Flux EXP time Max cts/s/pix Total rate Buffer Time COS ETC ID G130M/1291 0.5e-14 11.0 s 0.10 504 4679 COS.sa.1306938 G130M/1291 1.4e-13 0.4 s 0.13 5570 423 COS.sa.1306936 - ACQUISITION (for MR2251-178)- Configuration Flux EXP time Max cts/s/pix Total rate COS ETC ID PSA/Mirror B 1.8e-14 6.6 s 8 1011 COS.ta.1306935 PSA/Mirror B 4.7e-14 2.5 s 22 1156 COS.ta.1306930 - ACQUISITION (for NGC 3227)- Configuration Flux EXP time Max cts/s/pix Total rate COS ETC ID PSA/Mirror B 0.05e-14 131 s 0.4 925 COS.ta.1306969 PSA/Mirror B 0.4e-14 16.0 s 4 958 COS.ta.1306973 - EXPOSURES (for Mrk 509)- Configuration Flux EXP time Max cts/s/pix Total rate Buffer Time COS ETC ID G130M/1222 5.0e-14 1000 0.01 236 10011 COS.sp.1306947 G130M/1222 1.4e-13 1000 0.03 4663 505 COS.sp.1306941 G160M/1533 5.0e-14 1000 0.001 168 14027 COS.sp.1306951 G160M/1533 1.4e-13 1000 0.032 3232 729 COS.sp.1306954 Although it is recommended to use a BUFFER-TIME that is 2/3 of that given by the ETC, our general strategy is to choose a value that is less than that, and also an integer divisor of the exposure time minus 110 s. This minimizes the overhead between exposures while doing buffer dumps, e.g., BUFFER-TIME = (Exposure Time - 110) / n Massive Black Holes And Their Host Galaxies 6 false false false false false false false SUPPORTED GALAXY ACCRETION DISK BLR NLR SEYFERT WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 F(1368)=0.3e-14 GALAXY ACCRETION DISK BLR NLR SEYFERT WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 F(1368)=1.5e-14 GALAXY ACCRETION DISK BLR NLR SEYFERT WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 F(1368)=3.2e-14 GALAXY ACCRETION DISK BLR NLR SEYFERT WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 F(1368)=9.0e-14 GALAXY ACCRETION DISK BLR NLR SEYFERT WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. UGC-12163 J2000 F(1368)=0.8e-14 GALAXY ACCRETION DISK BLR NLR SEYFERT WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 F(1368)=3.3e-14 GALAXY ACCRETION DISK BLR NLR SEYFERT WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 F(1368)=4.9e-14 COS/FUV Spectroscopic No No G130M COS/FUV Spectroscopic No No G160M COS/FUV Spectroscopic No No G130M COS/FUV Spectroscopic No No G160M 1546631003965 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v01.xml This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. (Tic-Visit :proposal-id 15673 :visit-id "01" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:23.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 504704 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2594 :al-overhead-at-end 0 :internal-dur-at-end 48 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2929 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "01" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2929 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 0.05e-14. 1546631236443 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v02.xml This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. (Tic-Visit :proposal-id 15673 :visit-id "02" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:47:16.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 504704 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2594 :al-overhead-at-end 0 :internal-dur-at-end 48 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2929 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "02" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2929 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 0.05e-14. 1546631007400 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v03.xml This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. (Tic-Visit :proposal-id 15673 :visit-id "03" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:27.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 852544 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2587 :al-overhead-at-end 0 :internal-dur-at-end 57 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2922 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "03" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2922 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 0.5e-14. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 1546631009012 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v04.xml This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. (Tic-Visit :proposal-id 15673 :visit-id "04" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:28.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 852544 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2587 :al-overhead-at-end 0 :internal-dur-at-end 57 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2922 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "04" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2922 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 0.5e-14. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 1546631010685 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v05.xml This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. (Tic-Visit :proposal-id 15673 :visit-id "05" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:30.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 852544 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "05" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2591 :al-overhead-at-end 0 :internal-dur-at-end 57 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "05" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2927 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 2.0e-14. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 1546631012647 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v06.xml This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. (Tic-Visit :proposal-id 15673 :visit-id "06" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:32.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 852544 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2591 :al-overhead-at-end 0 :internal-dur-at-end 57 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "06" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2927 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 2.0e-14. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 1546631015287 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v07.xml This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. (Tic-Visit :proposal-id 15673 :visit-id "07" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:34.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 869936 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "07" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2593 :al-overhead-at-end 0 :internal-dur-at-end 67 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "07" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2927 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 0.5e-14. Exposure time is chosen for the faintest historical flux, 0.5e-14. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 1546631017221 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v08.xml This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. (Tic-Visit :proposal-id 15673 :visit-id "08" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:36.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 869936 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "08" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2593 :al-overhead-at-end 0 :internal-dur-at-end 67 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "08" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2927 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 0.5e-14. Exposure time is chosen for the faintest historical flux, 0.5e-14. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 1546631018835 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v09.xml This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. (Tic-Visit :proposal-id 15673 :visit-id "09" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:38.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 852544 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "09" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2593 :al-overhead-at-end 0 :internal-dur-at-end 57 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "09" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2928 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 0.6e-14. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 1546631020863 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v10.xml This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. (Tic-Visit :proposal-id 15673 :visit-id "10" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:40.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 852544 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "10" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2593 :al-overhead-at-end 0 :internal-dur-at-end 57 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "10" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2928 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 0.6e-14. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 1546631022560 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v11.xml This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. (Tic-Visit :proposal-id 15673 :visit-id "11" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:42.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 869936 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "11" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2594 :al-overhead-at-end 0 :internal-dur-at-end 67 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2929 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "11" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2929 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 1.8e-14. Exposure time is chosen for the faintest historical flux, 1.8e-14. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 1546631024450 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v12.xml This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. (Tic-Visit :proposal-id 15673 :visit-id "12" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:44.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 869936 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "12" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2594 :al-overhead-at-end 0 :internal-dur-at-end 67 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2929 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "12" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2929 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 1.8e-14. Exposure time is chosen for the faintest historical flux, 1.8e-14. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 1546631026137 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v13.xml This visit is to be coordinated as close in time as practical with the first triggered XMM-Newton visit (100 ks in length) without disrupting the HST timeline. (Tic-Visit :proposal-id 15673 :visit-id "13" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:45.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 869936 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "13" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2589 :al-overhead-at-end 0 :internal-dur-at-end 67 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2922 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "13" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2922 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 1.2e-14. Exposure time is chosen for the faintest historical flux, 1.2e-14. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. 1546631028064 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /Users/gak/proposals/XMM_2018/too/phase2/OP-cache/too_15673v1_010419-v14.xml This visit is to be coordinated as close in time as practical with the second XMM-Newton visit (50 ks in length), which would occur near the end of the XMM visibility window for this target. (Tic-Visit :proposal-id 15673 :visit-id "14" :proposal-version -1 :trans-version "20181130" :date "04-Jan-2019 14:43:47.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 869936 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15673 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15673 :visit-id "14" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2589 :al-overhead-at-end 0 :internal-dur-at-end 67 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2922 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15673 :visit-id "14" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2620 :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 2922 :pcs-gap 0 ) true 2 0 This visit is on hold until the TOO is triggered. Exposure time is chosen for the faintest historical flux, 1.2e-14. Exposure time is chosen for the faintest historical flux, 1.2e-14. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures. We use BUFFER-TIMES much shorter than the 2/3*ETC value for brightest historical flux since this is even safer. They are optimized to be 110 s less than the exposure time to minimize the overhead between exposures.