README web version of /home/usg/OPS/MTS/readme_xml/readme_84092600
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
ISAAC M-band medium resolution and L band low resolution observations
of ULIRGs.
With M-band MR observations we want to carefully remove telluric lines to detect
the ro-vibrational lines of R- and P- branches of the gaseus CO centered at 4.66
mic. Two central wavelenghts (4.65 and 4.85) are required to cover the entire CO
absorption band in MR spectra.
For sources not yet observed with ISAAC at ~3.5 mic, L-band LR observations will
provide high quality spectra to carefully determine the continuum shape and the
3.3 mic PAH equivalent width, both needed to disentangle the AGN/starburst relative
contribution to the observed emission, and thus estimate the intrinsic optical depth
of the CO absorption band.
To obtain the required S/N, it is important to cover the entire integration time
for a single source. Therefore we request to complete all the OBs for a source before
starting with a different one, following the priority in the OBs
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 15:40:32 2009
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