README web version of /home/usg/OPS/MTS/readme_xml/readme_79031200
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a "visual" binary orbit observing program for one M dwarf binary
with an
excellent double-lined spectroscopic orbit, expected to produce masses (and a
distance) with sub-% accuracy.
Important note: the brightest star in the field, specially in the visible, is
Gl570A (V=5.72), and NOT Gl570B (V=8.01). Component A is 25" away, to the SE
of B.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
The orbital period is approximately 10 months,
so for good phase coverage the various observing runs (ABCD) should be spaced
as much as compatible with observability and scheduling contraints. Once a month
or so is fine, and wider spacing is better. Run E is for a different target with
a much shorter period and has independent constraints.
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 indicate for each science star OB the corresponding calibrator
star OB (and vice versa) in the 'Instrument Comments' field ?
Did you check that your chosen calibrator is bright enough for the instrument
mode used ?
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 15:40:18 2009
If you have comments, please contact usd-help@eso.org