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Wavelength is a required field.0Assigned ID: 2536
----- Attempting Submission 1 (Sun Sep 14 00:47:20 GMT 2014) -----Joint Chandra/HSTThe observations were planned to be executed in two different HST orbits (separated in two visits). This is essential for the science since the two HST orbits must match within a month 2 Chandra observations to be performed with a time separation > 6 months. If by any chance the science is jeopardized I would like to recieve feedback.-1381502269----- Attempting Submission 1 (Thu Oct 30 03:31:48 GMT 2014) -----
HST Phase II Proposal 13948 (phaseII.apt) successfully submitted.
----- Attempting Submission 2 (Thu Oct 30 13:25:06 GMT 2014) -----CONSTRAINING THE WIND-SHIELD SCENARIO OF PG 2112+059The physical scenario describing the origin of quasar winds, still remain largely unsettled due to our failure to account for X-ray weak BALQSOs. In this proposal, we plan to study the relation between the inner part of the wind which is likely to be shielding the X-ray emission and the UV winds characterized by broad absorption lines (BALs). To address this, we propose to probe the shield-wind connection in the highly X-ray variable BALQSO PG 2112+059, which has exhibited periods of X-ray weakness and X-Ray "normality" in the past.The observations will be performed in two different orbits.
In each HST observation orbit we requiere at least an 840 s exposure with the G230L grating and
a 1000 s exposure with the G140L to get a S/N~30 in the continuum, suffcient for high quality
studies of the key O vi, Ly, N v, and C iv absorption lines. Each HST observation orbit must be
contemporaneous to two Chandra observations. Therefore, we require that each HST orbit observation is within a
month of its respective Chandra observation counterpart. Additionally each set of Chandra-HST
observations must be separated by at least eight months.AGN/QUASARSDefaultfalsefalsefalsefalsefalseSUPPORTEDGALAXYQUASARThis object was generated by the targetselector and retrieved from the 2MASS database.PG2112+059J2000COS/FUVSpectroscopicNoNoG140LCOS/NUVSpectroscopicNoNoG230LCOS/FUVSpectroscopicNoNoG140LCOS/NUVSpectroscopicNoNoG230L/private/var/folders/m0/yd5_v10d22vfhwqcg43n4b200000gn/T/OPVisit4252792764834490255.xmlThe scheduling data was generated by CASM 22.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 13948
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:proposal-version -1
:trans-version "20140605"
:date "30-Oct-2014 09:19:52.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
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:data-volume 174416
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(Tic-Orbit
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 2888
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3222
:pcs-gap 0
)true10/private/var/folders/m0/yd5_v10d22vfhwqcg43n4b200000gn/T/OPVisit5968393491423655091.xmlThe scheduling data was generated by CASM 22.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 13948
:visit-id "02"
:proposal-version -1
:trans-version "20140605"
:date "30-Oct-2014 09:20:57.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
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:data-volume 174416
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(Tic-Obset
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 2888
:al-overhead-at-end 0
:internal-dur-at-end 394
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3222
:pcs-gap 0
)true10