Principal Investigator Email Address
lmr@astro.ru.nl
Estimated Total Execution Time (hours, including overheads)
29.9633
General Description
The program consists in 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, taken over a long time baseline, for each target. Of the 49 targets submitted, 14 have either archive FEROs spectra or will be observed during the 076B period and therefore only need to be observed once. The remaining 35 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.
Waiver Requests
No Waiver Request was submitted
Critical Observing Condition Constraints
N/A
Time-Critical Aspects
35 or the 49 targets require two spectra. The second spectrum must be taken at least 20 days after the first one to be able to detect long term radial velocity variations. The OB associated to the second observation for each object is called like the first OB followed by "-0" and contains a note in the "user comments" indicating this time critical constraint. HS2224+2618-0 must be observed at least 20 days after HS2224+2618 PG2301+259-0 must be observed at least 20 days after PG2301+259 PG0909+276-0 must be observed at least 20 days after PG0909+276 PG0116+242-0 must be observed at least 20 days after PG0116+242 PG2351+198-0 must be observed at least 20 days after PG2351+198 PG2159+051-0 must be observed at least 20 days after PG2159+051 PHL25-0 must be observed at least 20 days after PHL25 PG1654+138-0 must be observed at least 20 days after PG1654+138 HD149382-0 must be observed at least 20 days after HD149382 LSIV-121-0 must be observed at least 20 days after LSIV-121 PG1607+174 must be observed at least 20 days after PG1607+174 PG1336-018-0 must be observed at least 20 days after PG1336-018 PG1047+003-0 must be observed at least 20 days after PG1047+003 UVO0512-08-0 must be observed at least 20 days after UVO0512-08 PHL932-0 must be observed at least 20 days after PHL932 CD-38222-0 must be observed at least 20 days after CD-38222 KUV04110+1434-0 must be observed at least 20 days after KUV04110+1434 EC22081-1916-0 must be observed at least 20 days after EC22081-1916 EC21494-7018-0 must be observed at least 20 days after EC21494-7018 EC21373-3727-0 must be observed at least 20 days after EC21373-3727 EC21079-3548-0 must be observed at least 20 days after EC21079-3548 EC21043-4017-0 must be observed at least 20 days after EC21043-4017 HD146803-0 must be observed at least 20 days after HD146803 HD146628-0 must be observed at least 20 days after HD146628 EC14338-1445-0 must be observed at least 20 days after EC14338-1445 EC13506-3137-0 must be observed at least 20 days after EC13506-3137 KPD0721-0026-0 must be observed at least 20 days after KPD0721-0026 EC05479-5818-0 must be observed at least 20 days after EC05479-5818 EC04170-3433-0 must be observed at least 20 days after EC04170-3433 EC04070-2122-0 must be observed at least 20 days after EC04070-2122 EC03408-1315-0 must be observed at least 20 days after EC03408-1315 EC03263-6403-0 must be observed at least 20 days after EC03263-6403 EC03143-5945-0 must be observed at least 20 days after EC03143-5945 EC01077-1423-0 must be observed at least 20 days after EC01077-1423 EC00042-2737-0 must be observed at least 20 days after EC00042-2737
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
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 ?
N/A
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 ?
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'?
If you use any lamp, did you check that it should never be left on at the end of any OB?
N/A