0
Assigned ID: 1337
----- Attempting Submission 1 (Fri Mar 01 01:01:04 GMT 2013) -----
As per the advice of the Contact Scientist, added post-flashes to visit 12.
1998641958
----- Attempting Submission 1 (Thu Jun 20 16:17:24 GMT 2013) -----
----- Attempting Submission 2 (Wed Oct 16 17:26:56 GMT 2013) -----
11 visits: In the ACS ramp filter, we are using small dithers for the purpose of rejecting cosmic rays and
instrument artefacts. The resulting variations in the central wavelength are small enough that they are not going to
affect the science.
1 visit: in the WFC3 quad filter, again we are using dithers to improve image quality. I am not sure
I understand why there is a warning in this case, since the effective wavelength of the filter should
not be affected by the dithers. Possible small variations in the transmission are not a concern.
Taking the measure of quasar winds
Black hole feedback -- the strong interaction between the energy output of supermassive black holes and their surrounding environments -- is routinely invoked to explain the absence of overly luminous galaxies and the black hole / bulge correlations. Yet direct probes of this process in action are scarce and limited to small subsamples of active nuclei. We recently obtained Gemini Integral Field Unit spectroscopy of the distribution of ionized gas around luminous, obscured, radio-quiet quasars on scales 20-30 kpc. These observations provide direct evidence of strong coupling between black hole energy output and gas motions on galaxy-wide scales. We propose to image these 11 objects with the HST to obtain accurate characterization of the physical conditions in the outflowing gas, with a total request of 26 orbits. Using U-band images sensitive to the scattered light from the nucleus, we will obtain a measurement of gas density and determine the geometry of quasar illumination and obscuration. Using yellow-band images we will determine the origin of the gas and characterize host galaxy morphologies at very high quasar luminosities. We will observe one object with a narrow-band filter centered on the [OIII]5007 line to determine the geometry of ionization on small scales and to constrain the clumping of the warm dense component of quasar winds. In combination with our ground-based kinematic maps, these observations will enable us to understand the 3D structure, the energetics and the physical conditions in quasar outflows. These ground-breaking measurements will provide a clear physical picture of the black hole feedback in action.
Each target is observed in a 'blue' and a 'red' broad filter, one orbit each, selected to avoid strong emission lines in the spectra. At z>0.5, ACS 475W is used as the 'blue' filter, and for z<0.5, ACS 435W is used to avoid the [OII]3727 emission line. For the 'red' filter, we use ACS FR914M suitably placed between [OIII] 5007 and Halpha depending on the redshift.
In addition to the broad-band observations, one target (J0858) is also observed for 4 orbits in a narrow-band filter WFC3 FQ727N which happens to be centered nicely on the [OIII]5007 emission line.
AGN/QUASARS
Default
false
false
false
false
false
SUPPORTED
GALAXY
QUASAR
J2000
J2000
GALAXY
QUASAR
J2000
J2000
GALAXY
QUASAR
J2000
J2000
GALAXY
QUASAR
J2000
J2000
GALAXY
QUASAR
J2000
J2000
GALAXY
QUASAR
J2000
J2000
GALAXY
QUASAR
J2000
J2000
GALAXY
QUASAR
J2000
J2000
GALAXY
QUASAR
J2000
J2000
GALAXY
QUASAR
J2000
J2000
GALAXY
QUASAR
J2000
J2000
ACS/WFC
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No
F475W
ACS/WFC
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No
FR914M
ACS/WFC
Imaging
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No
F475W
ACS/WFC
RampFilter
No
No
FR914M
ACS/WFC
Imaging
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No
F475W
ACS/WFC
RampFilter
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FR914M
ACS/WFC
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No
F475W
ACS/WFC
RampFilter
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No
FR914M
ACS/WFC
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No
F475W
ACS/WFC
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FR914M
ACS/WFC
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No
F475W
ACS/WFC
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FR914M
ACS/WFC
Imaging
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No
F475W
ACS/WFC
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No
FR914M
ACS/WFC
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No
F475W
ACS/WFC
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No
FR914M
ACS/WFC
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No
No
F435W
ACS/WFC
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No
FR914M
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
RampFilter
No
No
FR914M
ACS/WFC
Imaging
No
No
F435W
ACS/WFC
RampFilter
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No
FR914M
WFC3/UVIS
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No
No
FQ727N
POS-TARG
DITHER
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LINE
0.187
false
false
69.05
4
20.67
ACS-WFC-DITHER-BOX
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false
POS-TARG
DITHER
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LINE
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false
false
81.785
4
23.884
WFC3-UVIS-DITHER-BOX
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false
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