README web version of /home/usg/OPS/MTS/readme_xml/readme_77055300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Aim: To measure the black hole mass in the Seyfert 1 MCG--6-30-15 by mapping
Ca triplet kinematics around the nucleus using ARGUS high resolution mode. Very
accurate centring is not required, as long as the nucleus is as near the centre
of the ARGUS field as possible.
Fiducial stars, Guide star, sky etc.: all are chosen in a relatively small region
around the nucleus, since they were taken from a FORS image to preserve the same
astrometric system. This also means that some of the stars are faint, but they should
all still be within the guiding and fiducial star brightness limits. Several sky
fibres have been randomly placed over the field. Even if 1 or 2 of these cannot
be observed, that is fine.
Target: Note that target is an AGN, and known to vary in magntiude, i.e. exact magnitude
is unknown, with variation of up to a magnitude in the literature. So even if our
S/N requirement is not met in the outer ARGUS fibres, this is fine.
For any problems, please contact Poshak Gandhi (pgandhi@eso.org; +447905608818)
at any time.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
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 specify in your OBs the hour angle range for which your Target
Setup files are valid ?
Did you specify in your OBs the magnitudes of FACBs and Guide Star for
all your fields ?
Are the FACBs and Guide Star in the brightness ranges specified in the
FLAMES manual ?
Did you enter the expected signal to noise in your OBs ?
Last creation of page: Tue Oct 6 15:40:13 2009
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