README web version of /home/usg/OPS/MTS/readme_xml/readme_82089001
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This program aims at observing the E-CDFS in Ks band at unprecedented
depth, with 65 minutes total exposure time per pointing.
The large field requires a mosaic of 4 times 4 pointings, overlapped by 20 arcseconds
along each side.
Each pointing is split in 2 OBs of approx 33min duration each called ECDFS_Ks_0x_0y_A
and B, to be executed without any particular time constraint, in clear conditions
and seeing better than 0.6 arcsec (see individual OBs for full constraint set).
In addition we ask for two OBs aimed at providing good photometric calibrations,
to be observed contiguously in photometric conditions:
-"PcalDith" is a dithered sequence of 4x3 shallow pointings at the crossing of the
mosaic tiles (see the large-field FC attached to that OB)
-"CAL Ks" describes the observation of the UKIRT Faint Standard field FS10
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 ?
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 15:40:28 2009
If you have comments, please contact usd-help@eso.org