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Attribute nameAttribute typeDocstringUnit
COIstrList of the CO Investigator names.
creation_datedatetimeThe creation date of the object
DATE_OBSdatetimeUTC date on which the data of this file were obtained. The format used is YYYY-MM-DDThh:mm:ss.sss
DECfloatTelescope pointing in mean places of equinox J2000, expressed in decimal degrees. The comment field include the value expressed in degrees, minutes and seconds. deg
EQUINOXfloatEpoch of the mean equator and equinox of the coordinate system used to express the WCS mapping. Should always be 2000.0 (FK5). Should not be present if RADECSYS=ICRS.
ESO_AOS_HO_LOOP_STintHigh Order loop status
ESO_AOS_JIT_LOOP_STintJitter loop status
ESO_AOS_NGS_ALPHAfloatAlpha coordinate for the natural guide star hms
ESO_AOS_NGS_DELTAfloatDelta coordinate for the natural guide star dms
ESO_AOS_TT_LOOP_STintTip-tilt loop status
ESO_DET_READ_CURIDintUsed readout mode id
ESO_INS_DROT_POSANGfloatInstrument position angle on sky. deg
ESO_INS_MODEstrUsed instrument mode.
ESO_INS_TEMP11_VALfloatLeft IFU temperature C
ESO_OBS_AIRMfloatRequired max. airmass
ESO_OBS_AMBI_FWHMfloatRequired max. seeing
ESO_OBS_IDintObservation block id.
ESO_OBS_NAMEstrObservation block name.
ESO_OBS_PROG_IDstrProgram ID.
ESO_OBS_STARTdatetimeObservation block start time.
ESO_OBS_TARG_NAMEstrTarget package name.
ESO_OCS_SGS_AG_FWHMX_AVGfloatMajor axis of the seeing FWHM from the VLT auto-guider measurement. arcsec
ESO_OCS_SGS_AG_FWHMY_AVGfloatMinor axis of the seeing FWHM from the VLT auto-guider measurement. arcsec
ESO_OCS_SGS_ASM_GL900_MEDfloatmedian of ASM ground layer ratio at 900m
ESO_OCS_SGS_ASM_GL900_RMSfloatRMS of ASM ground layer ratio at 900m
ESO_OCS_SGS_FLUX_AVGfloatSlow guiding system flux measurement average during the exposure. ADU
ESO_OCS_SGS_FLUX_RMSfloatSlow guiding system flux measurement root mean square during the exposure. ADU
ESO_OCS_SGS_FWHM_AVGfloatSlow guiding system FWHM average during the exposure. arcsec
ESO_OCS_SGS_FWHM_RMSfloatSlow guiding system FWHM root mean square during the exposure. arcsec
eso_programEsoProgramThe Eso Program specifics
ESO_TEL_AIRM_ENDfloatAirmass at end
ESO_TEL_AIRM_STARTfloatAirmass at start
ESO_TEL_AMBI_FWHM_ENDfloatAverage FWHM of the observatory seeing at the end of the observation.
ESO_TEL_AMBI_FWHM_STARTfloatAverage FWHM of the observatory seeing at the beginning of the observation.
ESO_TEL_AMBI_TAU0floatAverage coherence time s
ESO_TEL_PARANG_ENDfloatParallactic angle at end deg
ESO_TEL_PARANG_STARTfloatParallactic angle at start deg
ESO_TPL_NEXPintTotal number of exposures within the template.
ESO_TPL_STARTdatetimeObservation template start time. The format is YYYY-MM-DDThh:mm:ss.sss. This keyword also defines which exposures are to be grouped together.
EXPTIMEfloatThe integration time for a single observation. s
file_deletedintSwitch to indicate if file has been deleted from the data server(s)
filenamestrThe name of the associated file
globalnamestrThe name used to store and retrieve file to and from Storage
is_validintManual/external flag to disqualify bad data (SuperFlag)
LSTfloatLocal Sidereal Time at start of the exposure in seconds elapsed since sidereal midnight. The comment includes a civil representation of the value. s
MJD_OBSfloatModified Julian Day of the start of the exposure. The MJD is related to the Julian Day (JD) via the formula: MJD = JD-2400000.5 The comment includes a civil representation of the date and time. 8 decimals are required for a precision of one millisecond, 5 decimals for a precision of one second. d
nifuintThe IFU used to make the observation
OBJECT_NAMEstrIdentification of target observed.
OBSERVERstrInitials, family name of observer.
observing_blockObservingBlockThe Observing Block of the observation
PIstrName of the Primary Investigator.
PI_COIstrName(s) of proposer(s) (as opposed to observer).
RAfloatTelescope pointing in mean places of equinox J2000, expressed in decimal degrees. The comment field include the value expressed in hours, minutes and seconds. deg
RADECSYSstrCoordinate system. Normally FK5 or ICRS.
raw_fitsRawFitsThe unsplitted raw fits data

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