Name: fpFieldStat-rrrrrr-c-ffff.fit, where rrrrrr is the imaging run number, c is the column location in the Imaging Array of the CCD which acquired the data (1-6), and ffff is the field number.
Produced by: frames
Used by:
Size: 2 * 2880 + Nfields * 120 bytes, rounded up to the nearest multiple of 2880. Total of 126.72 Kb for a single frames pipeline run with 1000 fields.
Archived? Yes
SIMPLE = T BITPIX = 8 NAXIS = 0 EXTEND = T RUN = xxxx / Imaging Run Number CAMCOL = x / Column in imaging camera FIELD = xx / the field reduced FILTERS = 'u g r i z' / Filters processed REFCOLOR= 'r ' / Reference Filter VERSION = 'xxxx ' / Version of software used. DERV_VER= 'xxxx ' ASTR_VER= 'xxxx ' ASTRO_ID= 'xxxx ' / Astrometric pipeline run identifier. BIAS_ID = 'PS ' / Bias pipeline run identifier. FRAME_ID= 'xxxx ' / Frames pipeline run identifier. KO_VER = 'xxxxx ' / Version of known object catalog used. PS_ID = 'xxxxx ' / Postage stamp pipeline run identifier. END
XTENSION= 'BINTABLE' BITPIX = 8 NAXIS = 2 NAXIS1 = 500 NAXIS2 = XXX PCOUNT = 0 GCOUNT = 1 TFIELDS = 28 TFORM1 = '1J ' TTYPE1 = 'status ' / Processed? TFORM2 = '5E ' TTYPE2 = 'rowOffset' / Offset to add to transformed row coordinates. TUNIT2 = 'pixels ' TFORM3 = '5E ' TTYPE3 = 'colOffset' / Offset to add to transformed column coordinates TUNIT3 = 'pixels ' TFORM4 = '1J ' TTYPE4 = 'nObjects' / Number of objects detected. TFORM5 = '1J ' TTYPE5 = 'nChild ' / Number of children in the field. TFORM6 = '1J ' TTYPE6 = 'nStars ' / Number of objects classified as stars. TFORM7 = '1J ' TTYPE7 = 'nGals ' / Number of objects classified as galaxies. TFORM8 = '5J ' TTYPE8 = 'saturation_level' / Saturation level. TFORM9 = '5E ' TTYPE9 = 'neff_psf' / Effective area of the point spread function. TUNIT9 = 'pixels ' TFORM10 = '5E ' TTYPE10 = 'sky_psp ' / Sky from the point spread function. TUNIT10 = 'DNs/pixel' TFORM11 = '5E ' TTYPE11 = 'sky_frames' / Global sky value in the corrected frame. TUNIT11 = 'DNs/pixel' TFORM12 = '5E ' TTYPE12 = 'sky_frames_sub' / Global sky value after object subtraction. TUNIT12 = 'DNs/pixel' TFORM13 = '5E ' TTYPE13 = 'sigPix ' / Clipped sigma of pixel values in corrected fram TUNIT13 = 'DNs ' TFORM14 = '5E ' TTYPE14 = 'deV_ap_correction' TFORM15 = '5E ' TTYPE15 = 'deV_ap_correctionErr' TFORM16 = '5E ' TTYPE16 = 'exp_ap_correction' TFORM17 = '5E ' TTYPE17 = 'exp_ap_correctionErr' TFORM18 = '5E ' TTYPE18 = 'deV_model_ap_correction' TFORM19 = '5E ' TTYPE19 = 'deV_model_ap_correctionErr' TFORM20 = '5E ' TTYPE20 = 'exp_model_ap_correction' TFORM21 = '5E ' TTYPE21 = 'exp_model_ap_correctionErr' TFORM22 = '5J ' TTYPE22 = 'nCR ' / Number of cosmic rays detected on the frame. TFORM23 = '5J ' TTYPE23 = 'nBrightObj' / Number of bright objects detected. TFORM24 = '5J ' TTYPE24 = 'nFaintObj' / Number of faint objects detected. TFORM25 = '5E ' TTYPE25 = 'median_fiberColor' / Median fiber colors of objects. TFORM26 = '5E ' TTYPE26 = 'median_psfColor' / Median PSF colors of objects. TFORM27 = '5E ' TTYPE27 = 'q ' / Mean Stokes Q parameter on the frame? TFORM28 = '5E ' TTYPE28 = 'u ' / Mean Stokes U parameter on the frame? TFORM29 = '5E ' TTYPE29 = 'adopted_cond3_fac2' END
XTENSION= 'BINTABLE' BITPIX = 8 NAXIS = 2 NAXIS1 = 66 NAXIS2 = 5 PCOUNT = 0 GCOUNT = 1 TFIELDS = 3 TYPENAME= 'FIELD_FLAGS' TFORM1 = '31A ' TTYPE1 = 'defName ' TFORM2 = '31A ' TTYPE2 = 'attributeName' TFORM3 = '1J ' TTYPE3 = 'Value ' END