Shining light on obscured AGN outflows 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 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 BAL 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 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 8 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 multiple central wavelengths for G130M and G160M to make sure we span the gap between segments A and B, and we use different FPPOS positions for each of those. To outline the ETC calculations for our potential targets, we tabulate results for all 8 here: Source z E(B-V) Min_Flam Max_Flam Mean_Flam Mrk 335 0.025785 0.030 3.8e-14 8.7e-14 6.3e-14 NGC 3783 0.00973 0.101 1.2e-14 1.1e-13 5.0e-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 can get bright enough that we use a spectroscopic target acquisition to ensure there are no bright object violations with an imaging target acquisition. Rather than do a separate ETC check on bright object constraints for each AGN, we simply show here calculations for the faintest object, NGC 4593, and the brightest, 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 the historical minimum flux for the faintest (NGC 4593, flam_min=0.5e-14) and the maximum flux at 1368 A (observed for Mrk 509, flam_max=1.4e-13, Dunn et al. 2006) in order to get our limiting cases: - ACQUISITION - Configuration Flux EXP time Max cts/s/pix Total rate Buffer Time COS ETC ID G130M/1291 0.5e-14 8.6 s 0.10 690 3419 COS.sa.768422 G130M/1291 1.4e-13 0.3 s 0.19 7322 322 COS.sa.768423 - EXPOSURES - Configuration Flux EXP time Max cts/s/pix Total rate Buffer Time COS ETC ID G130M/1291 5.0e-14 1000 0.13 2816 837 COS.sp.768426 G130M/1291 1.4e-13 1000 0.15 7238 325 COS.sp.768427 G160M/1600 5.0e-14 1000 0.016 1231 1915 COS.sp.768429 G160M/1600 1.4e-13 1000 0.044 3208 735 COS.sp.768428 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 AGN/QUASARS 12 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)=6.3e-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)=5.0e-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 Timing link suitability includes constraints ([02 After 01]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "01" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 14:41:42.0" :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 835136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14481 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2657 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "01" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2770 :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 2993 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([02 After 01]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "02" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 14:41:50.0" :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 835136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14481 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2657 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "02" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2770 :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 2993 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([04 After 03]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "03" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 14:42:00.0" :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 835136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14481 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2657 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "03" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2770 :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 2992 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([04 After 03]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "04" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 14:42:10.0" :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 835136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14481 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2657 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "04" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2770 :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 2992 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([06 After 05]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "05" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 14:42:13.0" :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 835136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14481 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "05" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2659 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "05" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2770 :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 2992 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([06 After 05]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "06" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 14:42:23.0" :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 835136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14481 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2659 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "06" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2770 :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 2992 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([08 After 07]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "07" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 15:02:31.0" :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 14481 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "07" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2652 :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 2988 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "07" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2764 :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 2988 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([08 After 07]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "08" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 15:04:04.0" :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 14481 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "08" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2652 :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 2988 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "08" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2764 :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 2988 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([10 After 09]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "09" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 15:05:56.0" :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 14481 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "09" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2652 :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 2988 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "09" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2764 :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 2988 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([10 After 09]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "10" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 15:07:56.0" :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 14481 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "10" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2652 :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 2988 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "10" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2764 :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 2988 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([12 After 11]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "11" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 15:10:55.0" :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 14481 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "11" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2659 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "11" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2770 :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 2993 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([12 After 11]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "12" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 15:12:10.0" :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 14481 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "12" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2659 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "12" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2770 :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 2993 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([14 After 13]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "13" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 14:43:10.0" :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 835136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14481 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "13" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2657 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "13" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2770 :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 2992 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([14 After 13]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "14" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 14:43:19.0" :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 835136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14481 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "14" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2657 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "14" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2770 :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 2992 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([16 After 15]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "15" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 14:47:54.0" :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 835136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14481 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "15" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2657 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "15" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2770 :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 2992 :pcs-gap 0 ) false 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. 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. Timing link suitability includes constraints ([16 After 15]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 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 14481 :visit-id "16" :proposal-version -1 :trans-version "20150609" :date "29-Jan-2016 14:47:57.0" :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 835136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14481 :visit-id "16" :obset-id "16" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14481 :visit-id "16" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2657 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14481 :visit-id "16" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2770 :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 2992 :pcs-gap 0 ) false 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. 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.