README web version of /home/usg/OPS/MTS/readme_xml/readme_75001600
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Our aim is to obtain low-resolution JHK spectroscopy of the peculiar
eruptive variables V838 Mon, V4332 Sgr and the "Peculiar Variable in Crux" (no
designated name). Each OB employs long-slit, 0.6" slit observing modes.
Slit P.A is not crucial. The progenitor of the Crux Variable is not
visible in the J magnitude finding chart attached. No recent images are
avaiable. The post-eruption object should be visible in the centre of the
circle indicated.
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 ?
Last creation of page: Tue Oct 6 15:40:06 2009
If you have comments, please contact usd-help@eso.org