README web version of /home/usg/OPS/MTS/readme_xml/readme_76050300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Spectroscopy of bright (1 < V <3) stars. ND2/3 filter used for
acquisition; no finding charts provided since these objects are blindingly bright.
However, note that alpha Cru and gamma2 vel are binaries, if the secondary has
crept into the field of view, our science targets are always the brighter of the
pair. All OBs can be done during the end of twilight. Two set-ups per target (blue,
dic) best executed consecutively to avoid excess overheads.
S/N estimates in user comments assume good conditions i.e. seeing=0.8" and airmass=1.2.
S/N degrades quite rapidly in poorer conditions due to the narrow slit (see constraint
set for limiting tolerances).
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Some orders may saturate, that's OK, since we're interested in only the
following wavelengths:
Blue setting: 330nm (approx 1/3 of the way up the CCD from bluest order)
Dic1 390 setting: 390nm (middle of CCD)
Dic1 580 setting: 590nm (2nd bluest order on red CCD)
Special Calibration Information
Final science spectra will have S/N ~400-500, so flat-fields must have
high S/N. I would therefore like to request extra flats to be taken during the
daytime (cleared with Francesca Primas@USD and PSO). Please execute the following
extra flatfields by changing the number produced by calobbuild, consecutive to nights
when science OBs have been executed if possible.
If any science OBs named *_blue were executed, please take *at least* 20 extra D2
flats (40 if the daytime operations schedule permits) for the B346 setting. I estimate
that 20 flats will add 1 hour to the calibration set.
If any science OBs named *_dic were executed, please take 40 (a minimum of 20 could
be tolerated) extra flats for the 390+580 setting. I estimate 40 flats will add
45 minutes to the calibration set.
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 ?
If you need secondary guiding, are there suitable objects within 30 arcsec
from your target ?
Last creation of page: Tue Oct 6 15:40:10 2009
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