README web version of /home/usg/OPS/MTS/readme_xml/readme_78002500

Principal Investigator Email Address

• areiners@astro.physik.uni-goettingen.de

Estimated Total Execution Time (hours, including overheads)

• 19:58:50.000

General Description

• High resolution spectroscopy of L-dwarfs.
  
  The OBs are laid out in order to achieve a SNR between 25 and 40 over the spectral
   region in each target. Exposures are split into three to facilitate cosmic ray removal.
   The desired SNR should be reached after summing all three exposures.
  
  All targets are nearby faint objects, they are very red. Since they are nearby,
   many have large proper motions. Not all proper motions are known.
  Two Finding Charts are included for each object, one in the I-Band (sometimes in
   a different band if no I-Band image was available), and one in the J-Band. In the
   J-Band, the objects are much brighter and clearly visible. The J-Band images are
   taken between 1999 and 2000, I-band and other images earlier. Objects are clearly
   marked in the Charts. The motion of the objects can be easily seen in the Charts
   (from I-Band to J-Band) and finding of the relatively bright objects should no problem.
   In 2M0828-1309, no IR finding chart is available, and a "bluer" chart is provided.
   The position of the target is indicated and should be easy to find in the reder
   filter of the UVES camera.
  
  The goal is just to get a nice spectrum.
  
  One telluric reference is added that can be observed any time (only once), preferably
   at relatively high air mass.

Waiver Requests

• 1. Waiver to use the non-standard setting
  DIC-2, Non-std setting: 437+830
  sent       Oct 17, 2006
  approved   Oct 20, 2006
  
  2. Waiver to use OBs that last longer than an hour
  sent       Oct 17, 2006
  approved   Oct 18, 2006

Critical Observing Condition Constraints

• none

Time-Critical Aspects

• none

Special Execution Requirements

• ---(Empty)---

Special Calibration Information

• One telluric standard, CAL HD42167, Vmag=5.0 is provided.
  This OB can be executed any time without any connection to the other OBs.
  It should be observed at relatively high air mass (1.5-2.) or so, but this is not
   critical.

ToO Information

• ---(Empty)---

ToO Activators List

• ---(Empty)---

Is this a Pre-imaging run ?

• false

Pre-imaging Requirements

• ---(Empty)---

Source(s) of Pre-imaging

• ---(Empty)---

Pre-imaging sources not listed above

• ---(Empty)---

Do all your OBs comply with the instrument-specific requirements listed
 on the instrument-specific Phase 2 web page ?

• YES

If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
 Category for each Observing Template ?

• N/A

Do all your finding charts comply with both the general and instrument-specific
 Phase 2 Web Pages ?

• YES

If you submitted OBs for standard stars, did you specify the magnitude
 and spectral type of all standard stars in the OBs ?

• YES

Have you included OBs for any calibrations that you need but which are
 not part of the Calibration Plan ?

• N/A

If you are observing Moving Targets, have you attached suitable ephemeris
 files to your OBs?

• N/A

If you have preferences which OBs should be executed first, did you make
 use of the User Priority field in the OBs ?

• N/A

If this is a run that requires coordinated observations with other facilities,
 did you give proper instructions in the Time-Critical Aspects Section ?

• N/A

If you need secondary guiding, are there suitable objects within 30 arcsec
 from your target ?

• N/A