README web version of /home/usg/OPS/MTS/readme_xml/readme_78009800

Principal Investigator Email Address

• lmr@astro.ru.nl

Estimated Total Execution Time (hours, including overheads)

• 29.0

General Description

• The program consists of taking spectra of a sample of stars.
  
  The spectra will be used to measure the radial velocity of the star by fitting its
   absorption lines. As we want to measure radial velocity variations associated to
   long period binaries, we need a few spectra for each target, taken over a long time
   baseline. Of the 53 objects sumitted, 35 have either FEROS archive spectra or will
   be observed during the 077 period and therefore only need to be observed once. The
   remaining 18 targets need to be observed twice and two OBs have been submitted for
   each of those targets. To detect long periods in one given target, its two spectra
   must be taken at least 20 days apart.
  
  I have reused finding charts from other observing periods thus the Observing Run
   ID on the top of the finding charts does not correspond to the present programme
   ID in most cases.

Waiver Requests

• No Waiver Request was submitted

Critical Observing Condition Constraints

• N/A

Time-Critical Aspects

• EC12234-2607-0 must be observed at least 20 days after EC12234-2607
  PB8783-0 must be observed at least 20 days after PB8783-0
  EC02542-3019-0 must be observed at least 20 days after EC02542-3019
  EC03470-5039-0 must be observed at least 20 days after EC03470-5039
  PG0909+164-0 must be observed at least 20 days after PG0909+164
  PG1303+097-0 must be observed at least 20 days after PG1303+097
  PG1616+144-0 must be observed at least 20 days after PG1616+144
  PG1653+131-0 must be observed at least 20 days after PG1653+131
  EC19563-7205-0 must be observed at least 20 days after EC19563-7205
  KPD2022+2033-0 must be observed at least 20 days after KPD2022+2033
  EC20387-1716-0 must be observed at least 20 days after EC20387-1716
  PG2111+023-0 must be observed at least 20 days after PG2111+023
  PG2118+126-0 must be observed at least 20 days after PG2118+126
  PG2148+095-0 must be observed at least 20 days after PG2148+095
  PG2205+023-0 must be observed at least 20 days after PG2205+023
  EC22591-7129-0 must be observed at leas20 days after EC22591-7129
  PG2314+076-0 must be observed at least 20 days after PG2314+076
  PG2349+002-0 must be observed at least 20 days after PG2349+002

Special Execution Requirements

• No other special execution requirements exist

Special Calibration Information

• Only standard calibrations are required

ToO Information

• N/A

ToO Activators List

• N/A

Is this a Pre-imaging run ?

• false

Pre-imaging Requirements

• N/A

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 ?

• N/A

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

Did you set 'New Preset' flag in all acquisition templates to 'True'?

• YES

If you use any lamp, did you check that it should never be left on at
 the end of any OB?

• N/A