0Assigned ID: 368
----- Attempting Submission 1 (Fri Apr 11 04:53:28 GMT 2014) -----
HST Phase I Proposal 368 (APT_C22.apt) successfully submitted.
----- Attempting Submission 2 (Fri Apr 11 05:58:05 GMT 2014) -----
HST Phase I Proposal 368 (APT_C22.apt) successfully submitted.
----- Attempting Submission 3 (Fri Apr 11 06:46:30 GMT 2014) -----
HST Phase I Proposal 368 (APT_C22.apt) successfully submitted.
----- Attempting Submission 4 (Fri Apr 11 14:41:03 GMT 2014) -----
HST Phase I Proposal 368 (APT_C22.apt) successfully submitted.
----- Attempting Submission 5 (Fri Apr 11 14:48:09 GMT 2014) -----
HST Phase I Proposal 368 (APT_C22.apt) successfully submitted.
----- Attempting Submission 6 (Fri Apr 11 16:58:39 GMT 2014) -----
HST Phase I Proposal 368 (APT_C22.apt) successfully submitted.
----- Attempting Submission 7 (Fri Apr 11 17:40:14 GMT 2014) -----This target is not used in this proposal.
No Parallel Exposures Specified in Parallel Exposure Group
No Parallel Exposures Specified in Parallel Exposure Group
No Parallel Exposures Specified in Parallel Exposure Group
No Parallel Exposures Specified in Parallel Exposure Group0----- Attempting Submission 1 (Thu Jul 24 15:47:20 GMT 2014) -----
HST Phase II Proposal 13645 (APT_13645_C22_July24.aptbackup) successfully submitted.
----- Attempting Submission 2 (Thu Jul 24 15:54:04 GMT 2014) -----There are no errors for this proposal.
All the warnings are coming from two reasons:
(1) we didn't use the parallel target in this proposal;
(2) we did not have parallel orbits.
Here is the reason:
We found that our individual WFC3 exposure can only be short, ~15-20sec, to avoid the
saturation of the bright quasar. ACS parallel individual exposure has to follow these
same very short exposures according to that of WFC3. ACS parallel exposure, in this
case, is limited by read-out noise and too shallow to meet our original science goal.
We decide to delete the parallel observations for this program.Galactic Environment of A Twenty-Billion Solar-Mass Black Hole at the End of ReionizationWhen did the first supermassive black holes (SMBHs) appear in the universe? How do they co-evolve with and impact their galactic environment? We propose to carry out deep HST ACS and WFC/IR imaging of a newly discovered ultra-luminous quasar at z=6.30. At about 10 times brighter than an average SDSS z~6 quasar, this object is the most luminous quasar yet known at z>5.5 and is powered by a SMBH with an estimated mass of 20 billion M_sun, comparable to the most massive SMBHs found in the local universe. It is among the most massive systems in the observable early universe and likely resides in the densest and most biased environment at the end of cosmic reionization. Our WFC/IR J and H band observations will reveal the rest-frame UV emission in the quasar host galaxy, directly probing the coeval star formation in quasar host when the SMBH is accreting at the highest rate. Deep HST images will be used to rule out or confirm lensing magnification and to search for signatures of major merger activity. We will use the ACS i and z band imaging, combined with WFC/IR imaging, to select young star forming galaxies in the quasar environment and to study whether this ultra-luminous quasar lives in a significant galaxy overdensity, or whether early reionization has suppressed galaxy formation in the quasar environment. The HST observations will provide key insight into the formation and evolution of the earliest 10^10 M_sun BH systems in the universe.Image in F775W for 2 orbits and F850LP for 4 orbits for J0100+2802.
One 5-orbit packages, to observe an J0100+2802 and a nearby star as a PSF model for eventual subtraction. We found that the individual WFC3 exposure can only be short ~20sec to avoid the saturation of the bright quasar. ACS parallel individual exposure has to follow the same very short exposure according to that of WFC3. ACS parallel exposure, in this case, is limited by read-out noise and too shallow to meet our original science goal. We decide to delete the parallel observations for this program.
Visit 1 : SDSSJ0100+2802 : 1-orbit F775W, 2-orbit F850LP
Visit 2 : SDSSJ0100+2802 : 1-orbit F775W, 2-orbit F850LP
Visit 3: SDSSJ0100+2802 : 1-orbit (F125W, F160W), each individual exposure has a different POS-TARG offsets according to 4-point dither pattern and the scale of the 4-point dither pattern. We no longer need parallel at this point
Visit 4: SDSSJ0100+2802 : 1-orbit (F125W, F160W), each individual exposure has the same POS-TARGs offset with that of Visit 03. We no longer need parallel.
Visit 5: PSF STAR (J0059+2809) : 1-orbit (F125W, F160W), each individual exposure has a different POST-TARG offsets according to 4-point dither pattern and the scale of the 4-point dither pattern
Visit 6: SDSSJ0100+2802 : 1-orbit (F125W, F160W), each individual exposure has the same POS-TARGs offset with that of Visit 03. We no longer need parallel. We no longer need parallel
Visit 7: SDSSJ0100+2802 : 1-orbit (F125W, F160W), each individual exposure has the same POS-TARGs offset with that of Visit 03. We no longer need parallel. We no longer need parallelAGN/QUASARSDefaultfalsefalsefalsefalsefalseSUPPORTEDGALAXYHIGH REDSHIFT GALAXYQSOQSOJ2000J2000z_AB=18.4STARM V-IVPSF starPSF-STARJ2000J2000J_Vega=16.75,H_vega=15.67ACS/WFCImagingNoNoF775WACS/WFCImagingNoNoF850LPWFC3/IRImagingNoNoF125WWFC3/IRImagingNoNoF160WACS/WFCImagingNoNoF775WACS/WFCImagingNoNoF850LPWFC3/IRImagingNoNoF125WWFC3/IRImagingNoNoF160WPOS-TARGDITHER0.265LINE0.187falsefalse69.05420.67ACS-WFC-DITHER-BOX1falseTiming link suitability includes constraints ([02 After 01 by at most 60.0 days])The scheduling data was generated by CASM 22.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 13645
:visit-id "01"
:proposal-version -1
:trans-version "20140605"
:date "24-Jul-2014 08:51:23.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "27"
:si-bright-earth-limb-angle 20.0
:data-volume 2273792
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13645
:visit-id "01"
:obset-id "01"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13645
:visit-id "01"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2908
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3241
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 13645
:visit-id "01"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 3019
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3241
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 13645
:visit-id "01"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 3019
:al-overhead-at-end 0
:internal-dur-at-end 347
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3241
:pcs-gap 0
)false30Timing link suitability includes constraints ([02 After 01 by at most 60.0 days])The scheduling data was generated by CASM 22.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 13645
:visit-id "02"
:proposal-version -1
:trans-version "20140605"
:date "24-Jul-2014 08:51:42.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "27"
:si-bright-earth-limb-angle 20.0
:data-volume 2273792
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13645
:visit-id "02"
:obset-id "02"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13645
:visit-id "02"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2908
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3241
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 13645
:visit-id "02"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 3019
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3241
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 13645
:visit-id "02"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 3019
:al-overhead-at-end 0
:internal-dur-at-end 347
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3241
:pcs-gap 0
)false30The scheduling data was generated by CASM 22.2.CASM was run in Phase II mode.First orbit of QSO observations
To ensure maximum thermal stability (and thus PSF stability) for these PSF-sensitive observations, we request one of the following constraints, if possible and if they do not interfere with the schedulability of other programs.
1) If our observations occur directly after an SAA transit, that the telescope be slewed to our initial pointing before the SAA transit, allowing thermal settling to occur during the transit.
2) Our observations occur directly after observations on a nearby target, to minimize the change in pointing angle (and thus thermal settling time) at the beginning of our observations.(Tic-Visit
:proposal-id 13645
:visit-id "03"
:proposal-version -1
:trans-version "20140605"
:date "24-Jul-2014 08:50:48.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 555568
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13645
:visit-id "03"
:obset-id "03"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13645
:visit-id "03"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2841
:al-overhead-at-end 0
:internal-dur-at-end 689
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3241
:pcs-gap 0
)false10Timing link suitability includes constraints ([05 After 04 by 0.1 to 0.1 days])The scheduling data was generated by CASM 22.2.CASM was run in Phase II mode.First orbit of QSO observations
To ensure maximum thermal stability (and thus PSF stability) for these PSF-sensitive observations, we request one of the following constraints, if possible and if they do not interfere with the schedulability of other programs.
1) If our observations occur directly after an SAA transit, that the telescope be slewed to our initial pointing before the SAA transit, allowing thermal settling to occur during the transit.
2) Our observations occur directly after observations on a nearby target, to minimize the change in pointing angle (and thus thermal settling time) at the beginning of our observations.(Tic-Visit
:proposal-id 13645
:visit-id "04"
:proposal-version -1
:trans-version "20140605"
:date "24-Jul-2014 08:33:46.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 555568
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13645
:visit-id "04"
:obset-id "04"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13645
:visit-id "04"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2841
:al-overhead-at-end 0
:internal-dur-at-end 689
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3241
:pcs-gap 0
)false10Timing link suitability includes constraints ([05 After 04 by 0.1 to 0.1 days])The scheduling data was generated by CASM 22.2.CASM was run in Phase II mode.Orbit of PSF star observations(Tic-Visit
:proposal-id 13645
:visit-id "05"
:proposal-version -1
:trans-version "20140605"
:date "24-Jul-2014 08:48:42.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 555568
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13645
:visit-id "05"
:obset-id "05"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13645
:visit-id "05"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2844
:al-overhead-at-end 0
:internal-dur-at-end 689
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3241
:pcs-gap 0
)false10The scheduling data was generated by CASM 22.2.CASM was run in Phase II mode.First orbit of QSO observations
To ensure maximum thermal stability (and thus PSF stability) for these PSF-sensitive observations, we request one of the following constraints, if possible and if they do not interfere with the schedulability of other programs.
1) If our observations occur directly after an SAA transit, that the telescope be slewed to our initial pointing before the SAA transit, allowing thermal settling to occur during the transit.
2) Our observations occur directly after observations on a nearby target, to minimize the change in pointing angle (and thus thermal settling time) at the beginning of our observations.(Tic-Visit
:proposal-id 13645
:visit-id "06"
:proposal-version -1
:trans-version "20140605"
:date "24-Jul-2014 08:33:59.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 555568
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13645
:visit-id "06"
:obset-id "06"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13645
:visit-id "06"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2841
:al-overhead-at-end 0
:internal-dur-at-end 689
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3241
:pcs-gap 0
)false10The scheduling data was generated by CASM 22.2.CASM was run in Phase II mode.First orbit of QSO observations
To ensure maximum thermal stability (and thus PSF stability) for these PSF-sensitive observations, we request one of the following constraints, if possible and if they do not interfere with the schedulability of other programs.
1) If our observations occur directly after an SAA transit, that the telescope be slewed to our initial pointing before the SAA transit, allowing thermal settling to occur during the transit.
2) Our observations occur directly after observations on a nearby target, to minimize the change in pointing angle (and thus thermal settling time) at the beginning of our observations.(Tic-Visit
:proposal-id 13645
:visit-id "07"
:proposal-version -1
:trans-version "20140605"
:date "24-Jul-2014 08:34:04.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 555568
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13645
:visit-id "07"
:obset-id "07"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13645
:visit-id "07"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2841
:al-overhead-at-end 0
:internal-dur-at-end 689
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3241
:pcs-gap 0
)false10