README web version of /home/usg/OPS/MTS/readme_xml/readme_75004101
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a simple imaging programme with the aim to derive exact photometry
of VV CrA in different bands (U, B, V, R, and I).
The brightness of VV CrA is almost unknown in the optical. Moreover, the source
is variable. Therefore, we can only estimate the exposure times in the different
filters from the spectral type (hard, since it is a YSO) and a few old V-band measurements.
It will be probably necessary to adjust the DITs to ensure that the exposures are
taken in the linear range of the detector with a reasonable signal-to-noise-ratio.
In the acquisition exposure a DIT that is equal to the DIT of the science template
has been chosen. The acquisiton image thus can be used to adjust the DIT in the
science part of the OBs. This procedure may save time.
We suggest to start with the V-band followed by the R- and I-band filters, where
the object should be fairly bright (circumstellar dust). Then the B-band (priority
2) and the U-band (lowest priority) should follow. If we will run out of time, please
skip the U-band measurements.
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 ?
Last creation of page: Tue Oct 6 15:40:06 2009
If you have comments, please contact usd-help@eso.org