README web version of /home/usg/OPS/MTS/readme_xml/readme_75503900
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a simple LSS programme that attempts the recovery of the young
SN remnant of SN1998bw.
The SN is not visible anymore and, if any, the signature of the SN remnant should
appear in the form of broad emission lines, possible very faint, and hence not directly
visible in the single CR splitted spectra.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
The only critical aspect of this program is the need for an accurate slit
centering.
The target is NOT expected to be visible in the acquisition and through slit images.
For this reason we have used a blind offset from a reference star (R~17.8). In order
to allow for an easier check of the slit alignment, we rotate the instrument such
that both the reference star and the SN position will fall onto the slit. The angle
has been calculated using FORS1 images taken at an epoch when the SN was still visible
and, therefore, both the position angle and the offsets should be accurate.
We have provided three finding charts:
1) full FORS1 field of view;
2) zoom on the SN region. In this f. chart the SN is still visible. The reference
star
is marked with a circle;
3) zoom on the SN region. Similar to the previous, but the SN has disappeared.
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 have prepared your finding charts with tools other than FIMS,
do they comply with the specifications on the FORS2 Phase 2 web page ?
Last creation of page: Tue Oct 6 15:40:09 2009
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