README web version of /home/usg/OPS/MTS/readme_xml/readme_76036700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
A short PHOTOMETRIC observeration of a SDSS merging cluster at z=0.069.
At this redshift, the [OII] emission line lies in the centre of our chosen narrow
band filter window. By comparing with the SDSS photometry and spectroscopy, we can
use this photometric observation to characterize the ZP of this narrow band (numerous
stars and spectroscopically observed galaxies in the field). Due to allocation,
this is forced to become a PILOT project at this stage.
We can later come back to this target and observe dithered positions in CLR conditions,
to build a mosaic image in [OII] emission of galaxies in the merging cluster and
infall regions, down to 5mags below M* (SDSS limit). NO EXTRA CALIBRATION FRAMES
ARE REQUIRED! We can test the ZP calibration techniques using this data.
Note: within the short allocated time, dithering overheads are too great. However,
we will perform a 3-frame pointed observation on this occasion (STARE mode). Most
targets will not be affected by cosmic rays or bad pixels, allowing an efficient
calibration of ZP using the remainder of targets.
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 ?
Did you set 'New Preset' flag in all acquisition templates to 'True'?
Have all your submitted OBs the same filter for the acquisition template
and for the first science template?
Did you combine calibration templates with science templates for any
OB?
Did you combine imaging and spectroscopic templates for any OB?
Did you submit any Focus template?
Last creation of page: Tue Oct 6 15:40:10 2009
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