README web version of /home/usg/OPS/MTS/readme_xml/readme_84014900
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This program aims to observe very early SN Ia candidates jsut 2-3 days
after explosion, with the goal of a) confirming their redshift and nature prior
to TOO observations with HST, and b) to analyse the composition of the SN via the
spectral features.
This is a ToO program. The single submited OB is a dummy OB which represents the
telescope/instrument configuration. The exposure times will be updated when the
target brightnesses are known.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
PI: Mark Sullivan email: sullivan@astro.ox.ac.uk
Other activators:
Sarah Blake, sarah.blake@astro.ox.ac.uk
Andy Howell, ahowell@lcogt.net
Chris Lidman, clidman@eso.org
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
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 specified the S/N ratio at given wavelength in the User Comments
field of each OB?
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 15:40:31 2009
If you have comments, please contact usd-help@eso.org