Principal Investigator Email Address
Hans.Ludwig@obspm.fr
Estimated Total Execution Time (hours, including overheads)
7:59:59
General Description
This programme targets a HF molecular line at 2335.7nm. Each observation consists of a calibration (CAL-HF81-*) OB of a telluric standard and a science OB (OBS-HF81-*) to be executed consecutively. The order is stated in the two related OBs and in the "Special Execution Requirements". The observation of the telluric standards is intended for the elimination of telluric features in the spectra of the science targets. All targets (calibration as well as science) are bright objects. High signal-to-noise (>500) ratios are generally expected at 2335.7nm.
Waiver Requests
No Waiver Request was submitted
Critical Observing Condition Constraints
None.
Time-Critical Aspects
None.
Special Execution Requirements
None.
Special Calibration Information
Calibration OBs to be executed consecutively with related science OB (OBS-HF81-*) for removal of telluric features in spectra of science targets. The expected S/N for all calibrators is expected to be S/N (per pixel) >=500 at 2335.7nm. OB names, ID, magnitudes, spectral types of calibration stars, execution oder CAL-HF81-1, HIP 1191 , R_OBJ=5.828; K_OBJ=5.94, B9V immediately before OB OBS-HF81-1 CAL-HF81-2, HIP 24327, R_OBJ=4.37; K_OBJ=4.56, B7V immediately after OB OBS-HF81-2 CAL-HF81-3, HIP 58510, R_OBJ=5.36 ; K_OBJ=5.34, A1V immediately before OB OBS-HF81-3 CAL-HF81-4, HIP 69658, R_OBJ=5.52; K_OBJ=5.55, A0V immediately after OB OBS-HF81-4 CAL-HF81-5, HIP 73087, R_OBJ=5.77; K_OBJ=5.90, A0V immediately before OB OBS-HF81-5 CAL-HF81-6, HIP 72220, R_OBJ=3.66; K_OBJ=3.65, A0V immediately after OB OBS-HF81-6 CAL-HF81-7, HIP 62683, R_OBJ=4.90; K_OBJ=4.89, A0IV immediately before OB OBS-HF81-7 CAL-HF81-8, HIP 62683, R_OBJ=4.90; K_OBJ=4.89, A0IV (identical to CAL-HF81-7) immediately before OB OBS-HF81-8
ToO Information
ToO Activators List
Do the README file and the instrument comments of the telluric stars OBs include the required S/N/pixel of the spectrum of the telluric star, its spectral type and allowed spectral range?
Do any OBs include wavelength or flatfield calibrations?
If you are observing Moving Targets, have you attached suitable ephemeris files to your OBs?
N/A
If the slit viewer guide star is different from the target, are the RA and DEC offsets accurate to within 0.05 arcsec and do they take into account the relative proper motion between the two objects?
N/A
If you have preferences which OBs should be executed first for objects at similar RA, did you make use of the User Priority field in the OBs?
N/A