README web version of /home/usg/OPS/MTS/readme_xml/readme_60943200
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This program is aimed at measuring the emission lines of a so-called
Lyman-alpha blob at high redshift. Lyman-alpha blobs are large
clouds of hydrogen emitting light mainly in the Lyman-alpha line.
The blob observed in this program is located at a redshift of 2.4
and with these observations we aim to observe the Lyman-alpha line
of the blob, as well as potential oxygen and Balmer lines in the
near-infrared.
We wish to observe the blob in the LSS mode. The slit should have
width 1.2 arcsec in VIS/NIR and 1.3 arcsec in UV. It should be tilted
at an angle of 25 degrees clockwise compared to North-South, see also the
finding chart. The blob consists of a main component seen in the Finding
chart and a faint, extended part towards the south-east, not seen in the
Finding chart. For that reason the slit should be offset slightly from the
main target and should center on R.A. 21 42 42.774, Dec. -44 30 12.03.
For the different arms, please note the following details:
UV: Exp time 600 s., detector read-out 1x2, slow
VIS: Exp time 600 s., detector read-out 1x2, slow
NIR: Exp time 600 s.
This target is not observable in the September SV run due to the moon constraints.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
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 15:40:06 2009
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