README web version of /home/usg/OPS/MTS/readme_xml/readme_79082301
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Science objectives & strategy:
These observations are part of a Large Program (179.A-0823, PI: T. Contini, Following
the mass assembly of galaxies at the key epoch 1.0 1h length).
Comments on the number and differences between the Finding Charts:
Two Finding Charts (FC) are attached to each OB:
- The first one is based on DSS2 shallow near-infrared images in order to mimic
what will be
seen on the screen by the observer. The scientific target is too faint to be visible
on these FCs.
Nomenclature for these FCs is: 179.A-0823B.VVDSXXXXXXXXX_fc_final_dss.jpg
- The second FC is based on CFHT12K deep I-band images acquired by the VVDS. On
the second FC, the faint scientific target is clearly visible in the SINFONI FoV.
Nomenclature for these FCs is: 179.A-0823B.VVDSXXXXXXXXX_fc_final.jpg
Waiver Requests
WaiverID: 179.A-0823C.01
I am happy to inform you that your waiver request for OB duration
longer than 1 hour for your SINFONI programme 179.A-0823(C) has
been approved. Please be informed that, although we will make
every effort to ensure that your OB will be started in ambient
conditions (seeing, transparency) that are equal or better than
those requested, for OBs with duration longer than one hour, ESO
does not guarantee that those conditions will be met for the entire
duration of your observation. If during the part of the observation
lasting longer than 1 hour ambient conditions degrade beyond those
requested within your OB, your OB will therefore not be aborted or
repeated, as is standard service-mode observing policy for OBs with
duration shorter than one hour.
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
If the scientific targets are observed at different airmasses, we would
like at least one telluric star to be observed to match each of these airmass values:
e.g. ~2, ~1.5 and ~1. But we don't need to have a telluric per OB of scientific
target. Please for the telluric, select star hotter than B4 if available and use
NDIT=1.
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 ?
Did you indicate the magnitude of the brightest object in the field in
each SINFONI OB?
If you are using the AO: Did you indicate for every OB the magnitude
of the guide star, and its distance to the target (if any)?
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 make really sure that none of your OBs ever saturates the detector?
If you are using the AO: did you enter the correct Strehl Ratio (on-axis,
K-band) AND the seeing value in the constraint set?
Last creation of page: Tue Oct 6 15:40:20 2009
If you have comments, please contact usd-help@eso.org