README web version of /home/usg/OPS/MTS/readme_xml/readme_77052300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Broad Ks-band imaging, using AutoJitter, will be obtained of the host
galaxies of low luminosity radio-quiet quasars at the epoch around the peak of the
quasar activity (redshift range 2 < z < 3). All selected targets have suitable
bright stars in the field of view to ensure an optimal PSF characterization. The
data will extend our NACO pilot study of a few luminous quasars at z > 2, and
will complement our ISAAC imaging study of quasars at 1 < z < 2. The combined
dataset will assess the luminosity evolution of the host galaxies from the peak
of the quasar phenomenon to the present epoch. This is of key importance for testing
the models of joint formation and evolution of galaxies and their active nuclei,
based on the hierarchical structure formation scenario.
Two OBs are planned to be executed for each target, except three OBs for one target
(Q2327).
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Is this a Pre-imaging run ?
Pre-imaging Requirements
Source(s) of Pre-imaging
Pre-imaging sources not listed above
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
Category for each Observing Template ?
Do all your finding charts comply with both the general and instrument-specific
Phase 2 Web Pages ?
If you submitted OBs for standard stars, did you specify the magnitude
and spectral type of all standard stars in the OBs ?
Have you included OBs for any calibrations that you need but which are
not part of the Calibration Plan ?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
If you have preferences which OBs should be executed first, did you make
use of the User Priority field in the OBs ?
If this is a run that requires coordinated observations with other facilities,
did you give proper instructions in the Time-Critical Aspects Section ?
If you submitted OBs for standard stars, did you use the provided StandardStar
templates ?
If you are using a specific offset pattern or position angle, did you
check carefully the definition in the manual ?
If you are doing spectroscopy, did you draw the slit on the Finding Charts
?
Did you enter the magnitude of the brightest star in the field-of-view
in the 'Instrument Comments' field of each OB ?
If you use the MoveToPixel acquisition, have you given clear instructions
on the FC and in the OB comment section as to how the field should be centered ?
Last creation of page: Tue Oct 6 15:40:13 2009
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