README web version of /home/usg/OPS/MTS/readme_xml/readme_60906400
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This program is aimed to obtain NIR spectra of pre-main-sequence stars
surrounded by disks.
We want to detect H2 emission at 2.12 & 2.22 micron and
the forest of ro-vibrational lines of CO at 4.7 micron.
We seek to detect narrow lines with fluxes of the order of 1e-15 ergs/s/cm2
A backup object (HD 190073) is proposed if a target with DEC +20 is required
In each of the observations a template for wave calibrations has been included.
We set the wavelenght, but the lamp selected (4 ThAr) the DIT (30s) and NDIT(1)
are default of the template. We have been informed (A. Smette) that the CRIRES SV
team will select the proper lamp and the DIT and NDIT.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
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 ?
Last creation of page: Tue Oct 6 15:40:06 2009
If you have comments, please contact usd-help@eso.org