README web version of /home/usg/OPS/MTS/readme_xml/readme_81052900
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Goal: Get visibilities on U-134 and closure phase on the brightest GC
star GCIRS7\\ If not finding charts are attached there is only one central bright
source (the brightest in the field) which shall be observed\\ one bright star has
been defined as fringe finder (name: *_fringfind), to efficiently search for the
fringe locations in MR-mode if not done before. This OB can be executed, but should
not be accounted to this programme. the science OB shall be encircled by cal_OBs,
whereas the 1st OB has on-axis AO guiding, and the second has off-axis AO-guiding
as the science target has. If time does not permit the second calibration skip it.\\
The visibility calibratos has the following properties: * Name: HD164866
* Coordinates: 18 04 18.303 -26 59 33.55
* V magnitude: 9.5
* K magnitude: 6.5
* Spectral Type: K1III
* Uniform Disk (UD) diameter at K, H, J bands with error estimate: 0.4pm0.3
(spectrl type and lum)
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
The requested Low-Resolution mode implies short coherence lengths ->
fringes are most efficiently found if before the run a bright fringe-finder in MR-mode
is used to locate the fringes, a respective OB has been prepared (*_fringfind).
The sci_OB shall be encircled by two calibrator measurement of the same star (HD164866)
and DIT, but one time with on-axis AO, and one time with off-axis-AO similar to
the SCI-OB. so a CAL-SCI-CAL sequence is requested. If the three observations don't
fit in the 1.5hr-frame given to this run, the second calibration shall be omitted.\\The
calibrator information is not in CalVin and therefore given here * Name: HD164866
* Coordinates: 18:04:18.300; -26:59:33.500
* V magnitude: 9.4
* K magnitude: 6.5
* Spectral Type:K1III
* Uniform Disk (UD) diameter at K, H, J bands with error estimate: 0.4mas+/-0.3mas
in all three bands
* Source of diameter estimate: spectrum and luminosity\\ * no source variability
known
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 15:40:24 2009
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