Observing Constraints and Classification Rules

General Observing Constraints

Every requested observation has multiple observing constraints. The observing constraints are:

  • the allowable brightest lunar phase
  • the allowable smallest moon-to-object angular separation
  • the allowable maximum airmass
  • the allowable maximum image size: 'Image Quality' measure as FWHM at observed wavelength and airmass
  • the Turbulence category (TC) for SPHERE, MUSE, ERIS and VLTI instruments that use full-AO. This combines probability of realisation of seeing and coherence time.
  • the allowable sky transparency
  • the allowable maximum Precipitable Water Vapour (PWV) should be provided for all instruments. The default value is set to 30 mm and should be fine for all non-IR instruments. All instruments include PWV in the ETC calculations that can be used to evaluate the impact of different PWV values on data.
  • the allowable twilight constraint that defines the earliest time in minutes with respect to the end of the evening astronomical twilight when the execution of the OB can be started (see the note below).
  • the allowable absolute time window for the start of the observation (i.e. for time critical events, multi-epoch monitoring)
  • the allowable local sidereal time range for the entire observation (e.g. for ADI observation)

The Observing Constraints are specified by the user at Phase 2 for each Observation Block. Since the execution conditions required by each programme are an important ingredient in the process of building up the Long Term Schedule of an observing semester, and thus determine which programmes can or cannot be scheduled, users are not allowed to specify at Phase 2 constraints that are more strict than those specified in the original proposal. Users can however relax the constraints during the submission of their Phase 2 material. The values in the OB constraint sets that are selected (and approved) during Phase 2 preparation (and review) cannot be changed later during the observing period.

Note about the twilight constraint: this observing constraint has been introduced to allow specifying start of observation with respect to the start of the night: e.g. to delay start of observations for faint targets until the sky gets darker, or allow starting observations for very bright targets already during the twilight. The original motivation for this constraint is related to sky brightness in near-IR that is affected by excitation of OH lines, and is not affected by other constraints (e.g. moon distance/phase). It does not apply to astronomical twilight at the end of the night (i.e. sunrise). 

General Classification Rules

Quality Control of OBs executed in Service Mode will be based on the specified constraints in the OB for airmass, atmospheric transparency, image quality/seeing, moon constraints, twilight constraint, as well as Strehl ratio for Adaptive Optics mode observations (as requested).

Details of the classification rules are available on the PSO QC0 OB grading page.

Additional Observing Constraints for VIRCAM

  • It is recommended to specify the weakest possible Constraint Set values.
  • The minimum image quality for VIRCAM is 0.6 arcsec, due to instrumental PSF of 0.51 arcsec.
  • The recommended airmass is up to ~1.7 (if applicable) due to implemented short term scheduling optimization algorithm.
  • The TWILIGHT constraint can be used to define the earliest time with respect to the end of the astronomical twilight when the execution of the OB can be started. While the relation between the time difference from the evening twilight end and sun elevation varies during the year, for Paranal due to its low latitude this difference is small.Therefore the constraint is given in minutes as a difference in time with respect to the end of astronomical twilight (i.e. the time when the solar elevation is -18 degrees). The default value of twilight constraint is 0. A negative number means that it is allowed to start the observation before the end of the astronomical twilight, a positive number means start the observation at least that many minutes after the end of the astronomical twilight.
    The recommended values for the twilight constraint for deep exposures are given in the VISTA/VIRCAM User's Manual.

Additional Classification Rules for VIRCAM

The following QC rules are implemented for all programmes. They are based on the experience gathered in the first years of VISTA operations, aiming to avoid repeating several times the same OB due to variable seeing during the observation, that affects only a small fraction of images in a tile:

Image quality condition classification rules:

  • C QC grade and status Executed (must be repeated):
    • Average image quality (IQ) over one tile is >10% out of constraint
    • At least one pawprint IQ is >20% out of constraint
  • B QC grade and status Completed:
    • At least one pawprint IQ is between 0% and 20% out of constraints _and_ average IQ is within 10% of the constraints
    • The average image quality is between 0% and 10% out of constraints
  • A QC grade and status Completed:
    • The average IQ _and_ every single pawprint IQ is within constraint

Image ellipticity classification rule:

  • C QC grade and status Executed (must be repeated):
    • there are >10 chips over a full tile with ellipticity >0.2
  • B QC grade and status Completed:
    • there are >4 and <10 chips over a full tile with ellipticity >0.2
    • or ellipticity up to 0.25 if FWHM*(1+ell) is ≤ 0.7
  • A QC grade and status Completed:
    • - there are <=4 chips over a full tile with ellipticity >0.2

Electronic readout failure classification rule (valid from Jan 14th, 2020):

  • If the OB has QC grade A or B based on the above QC classification criteria:
    • If <10% of images in any template of an OB are affected by electronic readout issues, then QC grade gets or stays B,  and a note is added in the night log, which will be visible to all users of this OB in the archive
    • If >10% of images in any template of an OB are affected by electronic readout issues, then QC grade is changed to C
  • If the OB has QC grade C or D based on the above classification criteria, we do not re-classify the OB. Still a note is added in the night log, such that Archive users get warned about the electronic readout issues

OB classification is done on Paranal by the observers and is based on on-the-fly pipeline that reduces all the data as they are observed. It should be noticed that this data reduction uses master calibration files that are updated regularly, but may not be the best ones for a particular observation.


Special Classification Rules for VISTA Public Survey Programmes

Following the VISTA Public Survey Panel recommendation to introduce measures that minimize the number of repeated observations for the Public Survey programmes, the following specific changes in the quality control rules and OB classification were implemented starting from April 1, 2013. Note that for the record (and for archive users as a reference) the classification rules below include also the first generation VISTA public surveys:  

  1. Surveys with multi-filter OBs (VHS)
    If within the same OB, at least one filter has all 6 pawprints completed within constraints (QC grade A or B), and the rest is observed out of constraints, then the OB will get QC0 grade “D” and status (C)ompleted.

  2. Surveys with several concatenated OBs (VVVX and VISIONS)
    If at least two OBs in a concatenation have all 6 pawprints classified A or B, and the rest of the concatenated OBs fail (out of constraints), the whole concatenation will be classified as (C)ompleted. The OBs that failed will get QC grade “D” instead of “C”, and the OBs that were done within constraints will be classified “A” or “B”.

  3. Surveys with only one filter per OB with no concatenations (Ultra-VISTA, VIDEO, VMC, Ultra-VISTANew, VEILS, SHARKS, G-CAV)
    No change with respect to the above QC0 rules that are applicable for all VIRCAM observations.

The responsibility to verify which fraction of the OBs classified "D" are good enough for the science goals of the survey, and which need to be repeated is the responsibility of the survey teams. Following the inspection of the observations, the survey team will determine the fraction of the time corresponding to OBs classified “D” that must be repeated. Within the report for the OPC, delivered every 6 months, the survey PI should request the corresponding "compensation time", that will be then added to the total survey allocation in a future period(s).


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