README web version of /home/usg/OPS/MTS/readme_xml/readme_78079001
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
High-res spectroscopy of luminous blue variables (LBVs), to do quantitative
spectroscopy with. Objects are photometrically variable (obviously!) and have variable
H alpha emission. Strategy is to achieve a SNR of >~100 through a series of shorter
exposures. For those objects known to have strong Halpha emission, more individual
exposures are required to achieve the target SNR in the continuum whilst avoiding
saturating the CCD.
Flux standards may not necessarily required, as we could flux calibrate with the
data from the other part of the proposal (078.D-0790(A)). However, if observing
conditions are good we would like a few spectro-photometric standards doing as well,
probably a few of this guy throughout the night (do you do this anyway?):
HR3454 084313.46 +032355.1 2000.0 0. 0. 4.30 B3V
We would appreciate some feed-back on this, as if we don't need to allow for specphot
stds we could spend longer on our targets.
I think the day-time flats and arcs will be sufficient for our needs, although we
are open to comments on this as you guys know more about the instrument stability
than us!
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 set 'New Preset' flag in all acquisition templates to 'True'?
If you use any lamp, did you check that it should never be left on at
the end of any OB?
Last creation of page: Tue Oct 6 15:40:17 2009
If you have comments, please contact usd-help@eso.org