README web version of /home/usg/OPS/MTS/readme_xml/readme_84040300

Principal Investigator Email Address

• m.galvez-ortiz@herts.ac.uk

Estimated Total Execution Time (hours, including overheads)

• 30

General Description

• The objective of this observation is to identify and analyse age sensitive
   spectroscopic signatures to asses or dismiss
   youth in a candidate sample. The main features to be analysed are: lithium I (6708),
   H alpha (6562),
   rotational velocity, and  gravity sensitive spectroscopic feature in the optical.
   We need high S/N in all the wavelength of these features for achieve our objectives.

Waiver Requests

• a Waiver Request was submitted due some targets need more than 1:05h in
   total of observing time to achieve, I think 5th Aug. and granted the 12th of Aug.

Critical Observing Condition Constraints

• There is no critical observing conditions

Time-Critical Aspects

• There is no time-critical aspects

Special Execution Requirements

• After every science object a correspondent telluric standart should be
   made.
  HIP 810  should be observed after SIPS 0007-2458, 2MASS 0020-2346 and DENIS 0021-4244.
  HIP 2633 should be observed after SIPS 0027-5401.
  HIP 8352 should be observed after SIPS 0153-5122, SIPS 0214-3237 and LEHPM 6542.
  HIP 14143 should be observed after SIPS 0235-0711 and 2MASS 0334-2130.
  HIP 100170 should be observed after SIPS 2045-6332.
  HIP 101725 should be observed after SIPS 2100-6255.
  HIP 104508 should be observed after SIPS 2114-4339.
  CD-68 2300 should be observed after LEHPM 4908.
  HIP 111954 should be observed after 2MASS 2254-3228.
  HIP 17734  should be observed after LP944-20.
  HIP 112479 should be observed after Gl 876.

Special Calibration Information

• Tellurics should be observed just after every correspondent target. In
   the case two science objects are done in a row, only one telluric should be done.
  HIP 810  should be observed after SIPS 0007-2458, 2MASS 0020-2346 and DENIS 0021-4244.
  HIP 2633 should be observed after SIPS 0027-5401.
  HIP 8352 should be observed after SIPS 0153-5122, SIPS 0214-3237 and LEHPM 6542.
  HIP 14143 should be observed after SIPS 0235-0711 and 2MASS 0334-2130.
  HIP 100170 should be observed after SIPS 2045-6332.
  HIP 101725 should be observed after SIPS 2100-6255.
  HIP 104508 should be observed after SIPS 2114-4339.
  CD-68 2300 should be observed after LEHPM 4908.
  HIP 111954 should be observed after 2MASS 2254-3228.
  HIP 17734  should be observed after LP944-20.
  HIP 112479 should be observed after Gl 876.

ToO Information

• ---(Empty)---

ToO Activators List

• ---(Empty)---

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

• YES

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 specified the S/N ratio at given wavelength in the User Comments
 field of each OB?

• 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