README web version of /home/usg/OPS/MTS/readme_xml/readme_77075800
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We intend to spectroscopically verify the reality of a non-luminous mass
concentration (sim 2x10^14 M_sun) at 0.1 < z < 0.3 as detected by weak gravitational
lensing observation. The existence of such an object, usually referred to as dark
clump, is controversial and highly debated. Dark clumps might not be real (statistical
fluke), but the striking possibility that spectroscopic analyses could lead to reliable
constraints on the existence of such objects, and the increasing evidences of the
existence of dark galaxies from HI-surveys (Minchin et al. 2005), should outweigh
such concerns. We propose to observe the quasar 004345.8-294733 (V=19m57; z=1.675),
3'9" off the dark clump candidate SSMC-007, with VLT/UVES, in order to search for
gas associated with SSMC-007. The proposed observations will enable (1) to confirm/infirm
the existence of SSMC-007, and (2) if real, to study important absorption lines
such as MgI and MgII, CaII, MnII, and FeII.
Waiver Requests
Waiver request Jan 20, 2006: We intend to obtain a UVES spectrum from
the QSO 004345.8-294733 (V=19.57mag, z=1.675). [...] As our target object is faint,
it would be most helpful to have longer exposure times in order to circumvent difficulties
in extracting low signals from the blue camera. We therefore request a phase 2 waiver
in order to be able to exceed the execution time limit of 1h. We ask for 5576s exposure
time for each of the seven OBs. This will lead
to a total exposure time of 10:50:32 and a total execution time of 11:59:57.
Waiver was granted Jan 23, 2006: your waiver has been granted, with the restriction
that if the conditions degrade in violation of the constraints after the first hour,
the OB will not be repeated. (Ferdinando Patat, ESO)
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 15:40:14 2009
If you have comments, please contact usd-help@eso.org