README web version of /home/usg/OPS/MTS/readme_xml/readme_77003501
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Our program aims at measuring the abundances of Fe, and a few other important
elements, of metal-poor stars that appear to have [Fe/H] < -3.5 from moderate-resolution
(R=2000) spectroscopy. These estimates of [Fe/H] are indirect, since they are based
on calibrations of the strength of Ca K. The history of the discovery of the two
known stars with [Fe/H] < -5.0 has shown that the [Fe/H] of these stars can be
overestimated by more than a factor of 10, due to e.g. blending of the Ca K line
with interstellar absorption, or CH lines.
Therefore we now want to obtain "snapshot" spectra (i.e., typically R=20,000 and
S/N=50 per pixel) of stars with [Fe/H] < -3.5 for which high-resolution spectroscopy
does not yet exists, in order to identify any stars with [Fe/H] < -5.0 among
them.
We have created three OBs for observations of HE1218-1828, which was estimated from
moderate-resolution spectroscopy to have [Fe/H] = -3.8. We want to use the B390+R580
standard setting, which covers a number of crucial absorption lines of Li, Na, Mg,
Fe, Sr, Ba, and Eu. For this relatively faint star (B = 16.8), we aim at S/N = 35
per rebinned pixel in the coadded spectrum at 400nm. The slit widths shall be 0.8''
and 0.7'' arcsec in the blue and red arm, respectively.
The constraint set corresponds to the observing conditions at the time when our
Visitor Mode program was interrupted by 3 hours for Rapid Response Mode observations
of a GRB, i.e., seeing 0.8'', and moon illumination 80%.
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 need secondary guiding, are there suitable objects within 30 arcsec
from your target ?
Last creation of page: Tue Oct 6 15:40:12 2009
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