README web version of /home/usg/OPS/MTS/readme_xml/readme_81000507
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Run H with triplet D0H0G1
Our principal aim is to image the surface of VX Sgr.
We want to observe VX Sgr at two different epochs:
1st) A0D0H0(1.5h), D0H0G1(1.5h, negative HR), E0G0H0(1.5h), D0H0G1(1.5h, positve
HR) between May 24 and June 7 in the second halfs of the nights
2nd) E0G0H0(1.5h), D0H0G1(1.5h, negative HR), A0K0G1(1.5h), D0H0G1(1.5h, positve
HR) between July 3 and July 11 in the second halfs of the nights
We want to use FINITO on the triplets: A0D0H0 with seeing <= 0.8 (approved by
the waiver team), E0G0H0 with seein <=1.0 (as requested in phase 1). If the
conditions
are very good (seeing <=0.6) we would like to use FINITO also with D0H0G1 triplet.
For this purpose I have prepared two OBs, one with FINITO and one without.
Only three different configurations are available during the two epochs. We would
increase our time constraint from 10 to 14 days. If the configuration schedule changes
and it is faisable, we would like to use also the triplet A0K0G1 in first period
and triplet A0D0H0 in second period (as required in phase 1). Otherwise, we would
use the allocated time left (2 x 1.5h) to observe again with D0H0G1 triplet as indicated
above.
Thank you.
Waiver Requests
Critical Observing Condition Constraints
Only three different configurations are available during the two epochs.
We would increase our time constraint from 10 to 14 days. If the configuration schedule
changes and it is faisable, we would like to use also the triplet A0K0G1 in first
period and triplet A0D0H0 in second period (as required in phase 1). Otherwise,
we would use the allocated time left (2 x 1.5h) to observe again with D0H0G1 triplet
as indicated above.
Time-Critical Aspects
We want to observe VX Sgr at two different epochs:
1st) A0D0H0(1.5h), D0H0G1(1.5h, negative HR), E0G0H0(1.5h), D0H0G1(1.5h, positve
HR) between May 24 and June 7 in the second halfs of the nights
2nd) E0G0H0(1.5h), D0H0G1(1.5h, negative HR), A0K0G1(1.5h), D0H0G1(1.5h, positve
HR) between July 3 and July 11 in the second halfs of the nights
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 ?
Do you use the same DIT for pairs of science target and associated calibrator?
Are the magnitudes of science target and calibrator within +/- 1 mag
?
Did you verify that your coordinates are as accurate as possible (2Mass
coordinates recommended) and that they include proper motions if available ?
Did you specify the LST range of the calibrators such that they cover
the range from 30 min before the start of the LST range of the science target to
30 min after the end of the LST range of the science target ?
Last creation of page: Tue Oct 6 15:40:23 2009
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