README web version of /home/usg/OPS/MTS/readme_xml/readme_77017200
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
A deep narrow-band imaging of a blank field to try to detect
faint Lyman continua (ionizing radiation) from High-z galaxies.
We only use the OII+44 filter and point to just one field.
We request one OB to be taken under photometric condition
for reliable calibration, and for other OBs we accept
clear condition.
As it is described in the FORS User Manual, standard stars
should be taken after the execution of science narrow-band
imagings. In addition to these standard star data in FORS
calibration plan, we add one OB for a standard star LTT4816.
That OB (CAL_STD) should be executed just after the execution of
PHOT_Lymancont.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
As it is described in the FORS User Manual, standard stars
should be taken after the execution of science narrow-band
imagings. Because standard star observations in ESO calibration
plan might not be executed just before or after our OBs,
we add a "CAL_STD" OB which should be executed just
after "PHOT_Lymancont" OB to confirm the reliablity of
flux calibration.
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 FORS1 Phase 2 web page ?
Last creation of page: Tue Oct 6 15:40:12 2009
If you have comments, please contact usd-help@eso.org