README web version of /home/usg/OPS/MTS/readme_xml/readme_75010400
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
UVES spectroscopy of planeary nebulae. Slit to be centred on emission
nebula which may not always be visible on slit viewer. offset stars are provided
where nebula or central star may be invisible, but may not always be needed where
provided. Position accurate to 1-2 arcsec (there is sometimes a discrepancy between
HST and USNO coordinates). Observations are of extended objects and can be done
under very poor seeing.
First exposure is always a very short integration. The spectra should show obvious
Halpha lines, [NII] and [OIII] 5007A lines. Total OB lengths about 35 minutes plus
overheads, for ~6 exposures, with a range in exposure times to allow for both very
bright and faint lines. Finding charts are from HST images because the fields
are often too crowded for the resolution of the dss2.
A few observations end with a 5-sec integration. This is only used for cases where
Halpha or OIII may be saturated in the first exposure. If they are not saturated,
the 5-sec
exposure may be skipped and/or discounted in the quality control.
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 ?
If you need secondary guiding, are there suitable objects within 30 arcsec
from your target ?
Last creation of page: Tue Oct 6 15:40:06 2009
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