README web version of /home/usg/OPS/MTS/readme_xml/readme_81071707
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a plain imaging program.
We will observe the same field (GOODS-S, sourthern pointing, here named GOODS1)
in the J and Ks filter for a grandtotal of 14 hours (including overheads).
For all, I have selected a standard dithered procedure.
Each OB is about 1hr long, for a total of 15 OBs.
Only the first one of each filter is required to be photometric, for calibration
purposes.
OBs have PA orientation rotated of 90 to allow for a proper cross-calibration
of the mosaic images and removal of defects.
As a minor midification with respect to the approved program, I have switched a
30 minnute exposure in the Ks band to a 30 minutes exposure in the Y band, in photometric
conditions, placed in the middle between the two pointing that we covered in the
LP (GOODS1 and GOODS2) since we need to cross-calibrate the images acquired in the
Hawk-I Science Verification.
The targted is named GOODScen in this case.
Waiver Requests
As a minor midification with respect to the approved program, I have switched
a 30 minnute exposure in the Ks band to a 30 minutes exposure in the Y band, in
photometric conditions, placed in the middle between the two pointing that we covered
in the LP (GOODS1 and GOODS2) since we need to cross-calibrate the images acquired
in the Hawk-I Science Verification.
The targted is named GOODScen in this case.
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 ?
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 15:40:25 2009
If you have comments, please contact usd-help@eso.org