README web version of /home/usg/OPS/MTS/readme_xml/readme_60944100
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The purpose of the observation is to observe the double QSO0151+048A+B.
The coordinates are:
RA(2000.0) = 01 53 53.9
Dec(2000.0) = +05 02 57
The magnitudes are about R=17.5 and R=20.8 so an acq. exposure time of a few sec
should be enough.
We would like to observe the field with two different position angles:
1) PA=41.2 EofN, 16 min exposure time
In this observation the slit covers both QSOs in the pair.
Acquire on the brightest QSO in the pair.
2) PA=98.0 EofN, 35 min exposure time
In this observation the slit covers extended Lyman-alpha emission extending
from QSO A.
Acquire on the brightest QSO in the pair.
An OB has been made for each PA.
The science goals are : 1) to measure the systemic redshifts of both quasars, 2)
to detect emission from a intervening DLA (already detected in Lyman-alpha previously),
3) to detect more absorption lines from the DLA absorber to better constrain in
state of chemical evolution.
Waiver Requests
Critical Observing Condition Constraints
Note that Lyman-alpha at this redshift (1.93) is very blue: lambda observed
= 356 nm.
This is particularly relevant for the OB PHL1222_PA98.0EoF, since no previous spectrum
covering Lyman-alpha exists for this PA (postion angle).
Hence, low airmass and dark time would be very beneficial.
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
If you have comments, please contact usd-help@eso.org