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Comment: Un-crossed the time domain element names.

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Column NameUnitsVO EquivalentSourceComments
sourcename
target_nameOBJECT Keyword
ra (center_position)degs_raCenter of Ra Axis
dec (center_position)degs_decCenter of Dec Axis
field_of_viewdegs_fovAverage of NAXISn*CRDELn of the spatial Axes
spatial_region
s_regionDerived from spatial DataSTC-S String Defined in the TAP (Dowler, et al 2010)
ra_element_count
s_xel1Relevent NAXISn Keyword
dec_element_count
s_xel2Relevent NAXISn Keyword
spatial_resolutionarcsecs_resolutionAverage of CDELTn of the spatial Axes, converted from deg
starttimeMJDt_maxmin

Temporal domain information for an image is dependent upon the observation(s) used in its generation.  Some controlling process (Like Vlass Manager, whatever imaging pipeline we create, and any image manipulation software we use) will need to supply it. 


endtimeMJDt_minmax
exposure_timest_exptime
min_frequency observing_band)Hzem_minMinimum of Spectral Axis


The spectral information is recoverable from the FITS header, and will identify the spectral coverage, and total bandwidth processed for the image. 

(TBD: what further information for unit conversion for the VO? (Hz → m))

max_frequency (observing_band)Hzem_maxMaximum of Spectral Axis
spectral_resolutionunitlessem_res_powerCenter Frequency/CDELTn

polarization_id

(reverting to initial name)


pol_statesPolarization CRVALn value

CASA uses the CRVALn value to convey polarization information, with [1,2,3,4] mapped to [I,Q,U,V].  When we begin dealing with single-polarization images, this will need to be expanded. 

telescope
instrument_nameTELESCOP KeywordThis must accommodate images for multiple instruments (i.e. VLA + Single Dish)
file_id

automatically generatedlink to information about the physical file
image_id
obs_idautomatically generatedUnique Identifier for the Image
image_units

o_ucd

BTYPE & BUNIT KeywordsDescription of the physical quantity measured in the image
max_intensityimage_units


These values are can be determined from the data portion of the image file in conjunction with the BSCALE & BZERO keywords.  The library which is used for FITS interaction for ingestion can perform these calculations, but no information about the speed of results is yet available.

min_intensityimage_units

rms_noiseimage_units

thumbnail

weblog, a PNG with identical name

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