README web version of /home/usg/OPS/MTS/readme_xml/readme_81501700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is the follow-up to the discovery (in mid-May) of a luminous optical
transient in NGC300.
The best current available finding chart we have for the object is in attach.
The object itself needs to be used as natural guiding stars for the AO system,
while it is still bright (V~14.2)!!! (as soon as possible).
The purpose is to image also the surrunding brightest stars to improve the
relative astrometry once compared with HST archive material.
---proposal abstract---
A luminous optical transient discovered in the nearby (~2.2 Mpc)
Sculptor Group spiral NGC 300 in May 2008 appears to be a new member
of the V838 Monocerotis class of stars that expand in a few weeks to
become red supergiants. Spectroscopic observations show that
NGC_300_OT is not a classical nova, supernova, or luminous blue
variable. At an absolute magnitude of -12.5, it is the brightest
star at present in NGC 300, but if it follows the pattern of V838 Mon
and the similar object M31 RV, it will fade away rapidly in about 3
months.
Before it fades, we propose to obtain VLT NACO high resolution images
in order to locate the position of the object to within a few milliarcsec.
This will allow us to identify the progenitor object, based on a superb set of
pre-outburst HST ACS/WFC images of NGC 300 available in the HST archive.
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 have PSF reference star OBs, do the names of those OBs begin with
PSF_ ?
If there are Finding Charts attached to your OBs, is the field-of-view
of at least one of these charts 2' x 2' (with clearly labelled field orientation)
?
Have you clearly marked and labelled your wavefront reference objects
R1, R2, R3, ... (as specified in the NAOS Preparation Software) on your Finding
Charts ?
Have you specified the magnitude of the brightest object in the field-of-view
for each OB ?
Are there objects in any of your fields (including standard stars) which
are brighter than the limits specified in the User Manual and on NACO web Pages
?
If the previous answer is yes, have you given a list of OBs and a justification
for the brightness limit violation in the general description field ?
Last creation of page: Tue Oct 6 15:40:25 2009
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