README web version of /home/usg/OPS/MTS/readme_xml/readme_81049300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The main scope of this part our project is to obtain 7 accurate RV measurements
for a very blue eclipsing binary in NGC 6822 (with components having spectral type
O5). In order to get desired
S/N ratio a long integration is needed. Therefore each integration was devided into
three subsequent exposures of about 45 minutes each. Observations should be executed
close to the both quadratures.
For these reasins we devided our OBs into two grups (N6822-I-N*, and N6822-II-N*
- to be observed close to the orbital phase of 0.75 and 0.25, respectively).
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Observations should be executed close to the both quadratures.
For this reason we devided our OBs into two grups (N6822-I-N* - to be observed close
to photometric phase of 0.75 and N6822-II-N* to be observed close to the phase of
0.25).
For each set of OBs, a file with the nights on which our binary system has the
appropiate
phases was attached as a ephemeris file. Observations should be performed on these
nights
if the other requirements (dark conditions, seeing) specified in the OBs are fullyfied.
In order to trace out systematics please execute each OB on different night.
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 specified the S/N ratio at given wavelength in the User Comments
field of each OB?
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 ?
If you need secondary guiding, are there suitable objects within 30 arcsec
from your target ?
Last creation of page: Tue Oct 6 15:40:24 2009
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