README web version of /home/usg/OPS/MTS/readme_xml/readme_77017300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We want to obtain an angular diameter for TX Psc, mostly in the
continuum in H and K, including contributions from circumstellar
flux and possible asymmetries.
TX Psc is a carbon star, i.e. V magnitude is variable with
a maximum of 5. K magnitude is not expected to vary very much
and is around K=-0.7.
Visibilities in K are expected in the range 0.4-0.1, depending
on the UT baseline.
Any triplet of UT telescopes will do.
We prefer observations without IRIS, in order to record also
the H-band. For this, we assume that operation without IRIS
will satisfy the specifications of the CfP, i.e. at least 3%
visibility accuracy. Should experience at Paranal in P77
show that this is not the case, we would like to be consulted
again.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
Tet Psc is from the Calvin list, it is 5 deg from TX PSc,
with a K magnitude = 1.86.
Depending on the UT baseline, visibilities are expected
in the range 0.66-0.95 in K
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 for each science star OB the corresponding calibrator
star OB (and vice versa) in the 'Instrument Comments' field ?
If you use calibrator stars which are not in the CalVin database, did
you specify their characteristics in the README file and in the OBs ?
Last creation of page: Tue Oct 6 15:40:12 2009
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