Changeset 15511 for trunk/Ohana/src/libautocode
- Timestamp:
- Nov 8, 2007, 10:43:14 AM (19 years ago)
- Location:
- trunk/Ohana/src/libautocode/def
- Files:
-
- 8 edited
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average-panstarrs-dev-0.d (modified) (2 diffs)
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average-panstarrs-dev-1.d (modified) (1 diff)
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average-ps1-dev-1.d (modified) (2 diffs)
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average.d (modified) (2 diffs)
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measure-panstarrs-dev-0.d (modified) (4 diffs)
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measure-panstarrs-dev-1.d (modified) (4 diffs)
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measure-ps1-dev-1.d (modified) (2 diffs)
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measure.d (modified) (4 diffs)
Legend:
- Unmodified
- Added
- Removed
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trunk/Ohana/src/libautocode/def/average-panstarrs-dev-0.d
r15034 r15511 19 19 FIELD dP, PAR_ERR, float, parallax error, arcsec 20 20 21 # XXX drop the old primary magnitude concept22 # FIELD M, MAG, float, primary mag, mag23 # FIELD dM, MAG_ERR, float, error on primary mag, mag24 # FIELD Xm, CHISQ_MAG, short, chisq for primary mag, [100*log(value)]25 # FIELD Xg, CHISQ_GAL, short, chisq for galaxy mags, [100*log(value)]26 27 21 FIELD Xp, SIGMA_POS, short, position scatter, 1/100 arcsec 28 22 FIELD Nm, NMEAS, unsigned short, number of measures … … 41 35 # the index for the secfilt table is just Nsecfilt times the index for the average table. 42 36 43 # XXX after the rest of the DVO re-org work, remove the magnitude based values from this table44 # and move them to the secfilt table.45 46 37 # the DVO object IDs are generated internally and are not equivalent to the PSPS object IDs 47 38 # probably need to add position chisq -
trunk/Ohana/src/libautocode/def/average-panstarrs-dev-1.d
r15510 r15511 35 35 # the index for the secfilt table is just Nsecfilt times the index for the average table. 36 36 37 # XXX after the rest of the DVO re-org work, remove the magnitude based values from this table38 # and move them to the secfilt table.39 40 37 # the DVO object IDs are generated internally and are not equivalent to the PSPS object IDs 41 38 # probably need to add position chisq -
trunk/Ohana/src/libautocode/def/average-ps1-dev-1.d
r15034 r15511 19 19 FIELD dP, PAR_ERR, float, parallax error, arcsec 20 20 21 # XXX drop the old primary magnitude concept22 # FIELD M, MAG, float, primary mag, mag23 # FIELD dM, MAG_ERR, float, error on primary mag, mag24 # FIELD Xm, CHISQ_MAG, short, chisq for primary mag, [100*log(value)]25 # FIELD Xg, CHISQ_GAL, short, chisq for galaxy mags, [100*log(value)]26 27 21 FIELD Xp, SIGMA_POS, short, position scatter, 1/100 arcsec 28 22 FIELD Nm, NMEAS, unsigned short, number of measures … … 41 35 # the index for the secfilt table is just Nsecfilt times the index for the average table. 42 36 43 # XXX after the rest of the DVO re-org work, remove the magnitude based values from this table44 # and move them to the secfilt table.45 46 37 # the DVO object IDs are generated internally and are not equivalent to the PSPS object IDs 47 38 # probably need to add position chisq -
trunk/Ohana/src/libautocode/def/average.d
r14401 r15511 30 30 FIELD objID_lo, OBJ_ID_LO, unsigned int, ID lower bytes 31 31 32 # XXX record the number of detections used for average astrometry33 34 32 # this structure should only be used for internal representations 35 33 # the average-FORMAT structures should be used for external representations … … 37 35 # the index for the secfilt table is just Nsecfilt times the index for the average table. 38 36 39 # XXX after the rest of the DVO re-org work, remove the magnitude based values from this table40 # and move them to the secfilt table.41 42 37 # the DVO object IDs are generated internally and are not equivalent to the PSPS object IDs 43 38 # probably need to add position chisq -
trunk/Ohana/src/libautocode/def/measure-panstarrs-dev-0.d
r15034 r15511 8 8 FIELD dD, D_DEC, float, DEC offset, arcsec 9 9 FIELD M, MAG, float, catalog mag, mag 10 FIELD Mcal, M cal,float, image cal mag, mag11 FIELD Mgal, M gal,float, galaxy mag, mag12 FIELD dM, dM,float, mag error, mag13 FIELD dt, dt,float, exposure time, 2.5*log(exptime)10 FIELD Mcal, M_CAL, float, image cal mag, mag 11 FIELD Mgal, M_GAL, float, galaxy mag, mag 12 FIELD dM, MAG_ERR, float, mag error, mag 13 FIELD dt, M_TIME, float, exposure time, 2.5*log(exptime) 14 14 15 15 # note that with airmass = 1.0 / cos(90 - alt), we have full alt/az representation 16 FIELD airmass, airmass, float, (airmass - 1), airmass16 FIELD airmass, AIRMASS, float, (airmass - 1), airmass 17 17 FIELD az, AZ, float, telescope azimuth 18 18 … … 25 25 FIELD dSky, SKY_FLUX_ERR, float, local estimate of sky flux, counts/sec 26 26 27 FIELD t, t,unsigned int, time in seconds (UNIX)28 FIELD averef, averef,unsigned int, reference to average entry27 FIELD t, TIME, unsigned int, time in seconds (UNIX) 28 FIELD averef, AVE_REF, unsigned int, reference to average entry 29 29 30 30 # Pan-STARRS uses a 64-bit detection ID. keep this in two 32 bit ints for backwards compatibility? … … 35 35 FIELD imageID_lo, IMAGE_ID_LO, unsigned int, reference to image 36 36 37 FIELD FWx, FW x,short, object fwhm major axis, 1/100 of arcsec38 FIELD FWy, FW y,short, object fwhm minor axis, 1/100 of arcsec39 FIELD theta, theta,short, angle wrt ccd X dir, (0xffff/360) deg40 FIELD photcode, photcode, unsigned short, photcode37 FIELD FWx, FWHM_MAJOR, short, object fwhm major axis, 1/100 of arcsec 38 FIELD FWy, FWHM_MINOR, short, object fwhm minor axis, 1/100 of arcsec 39 FIELD theta, PSF_THETA, short, angle wrt ccd X dir, (0xffff/360) deg 40 FIELD photcode, PHOTCODE, unsigned short, photcode 41 41 42 FIELD flags, flags, unsigned short, flags for various uses42 FIELD flags, FLAGS, unsigned short, flags for various uses 43 43 44 44 FIELD dXccd, X_CCD_ERR, short, X coord error on chip, pixels … … 48 48 FIELD qPSF, PSF_QF, short, psf coverage/quality factor 49 49 50 FIELD dophot, dophot, char, dophot type51 FIELD stargal, stargal,char, star-galaxy separator50 FIELD dophot, DOPHOT, char, dophot type 51 FIELD stargal, STAR_GAL, char, star-galaxy separator 52 52 53 53 # we need extra bytes for padding purposes... 54 FIELD dummy, dummy, char[2], padding 55 56 # float : 13 x 4 = 52 57 # int: 6 x 4 = 24 58 # short: 8 x 2 = 16 59 # char : 2 = 2 54 FIELD dummy, DUMMY, char[2], padding -
trunk/Ohana/src/libautocode/def/measure-panstarrs-dev-1.d
r15034 r15511 8 8 FIELD dD, D_DEC, float, DEC offset, arcsec 9 9 FIELD M, MAG, float, catalog mag, mag 10 FIELD Mcal, M cal,float, image cal mag, mag11 FIELD Mgal, M gal,float, galaxy mag, mag12 FIELD dM, dM,float, mag error, mag13 FIELD dt, dt,float, exposure time, 2.5*log(exptime)10 FIELD Mcal, M_CAL, float, image cal mag, mag 11 FIELD Mgal, M_GAL, float, galaxy mag, mag 12 FIELD dM, MAG_ERR, float, mag error, mag 13 FIELD dt, M_TIME, float, exposure time, 2.5*log(exptime) 14 14 15 15 # note that with airmass = 1.0 / cos(90 - alt), we have full alt/az representation 16 FIELD airmass, airmass, float, (airmass - 1), airmass16 FIELD airmass, AIRMASS, float, (airmass - 1), airmass 17 17 FIELD az, AZ, float, telescope azimuth 18 18 … … 25 25 FIELD dSky, SKY_FLUX_ERR, float, local estimate of sky flux, counts/sec 26 26 27 FIELD t, t,unsigned int, time in seconds (UNIX)28 FIELD averef, averef,unsigned int, reference to average entry27 FIELD t, TIME, unsigned int, time in seconds (UNIX) 28 FIELD averef, AVE_REF, unsigned int, reference to average entry 29 29 30 30 # Pan-STARRS uses a 64-bit detection ID. keep this in two 32 bit ints for backwards compatibility? … … 35 35 FIELD imageID_lo, IMAGE_ID_LO, unsigned int, reference to image 36 36 37 FIELD FWx, FW x,short, object fwhm major axis, 1/100 of arcsec38 FIELD FWy, FW y,short, object fwhm minor axis, 1/100 of arcsec39 FIELD theta, theta,short, angle wrt ccd X dir, (0xffff/360) deg40 FIELD photcode, photcode, unsigned short, photcode37 FIELD FWx, FWHM_MAJOR, short, object fwhm major axis, 1/100 of arcsec 38 FIELD FWy, FWHM_MINOR, short, object fwhm minor axis, 1/100 of arcsec 39 FIELD theta, PSF_THETA, short, angle wrt ccd X dir, (0xffff/360) deg 40 FIELD photcode, PHOTCODE, unsigned short, photcode 41 41 42 FIELD flags, flags, unsigned short, flags for various uses42 FIELD flags, FLAGS, unsigned short, flags for various uses 43 43 44 44 FIELD dXccd, X_CCD_ERR, short, X coord error on chip, pixels … … 48 48 FIELD qPSF, PSF_QF, short, psf coverage/quality factor 49 49 50 FIELD dophot, dophot, char, dophot type51 FIELD stargal, stargal,char, star-galaxy separator50 FIELD dophot, DOPHOT, char, dophot type 51 FIELD stargal, STAR_GAL, char, star-galaxy separator 52 52 53 53 # we need extra bytes for padding purposes... 54 FIELD dummy, dummy, char[2], padding 55 56 # float : 13 x 4 = 52 57 # int: 6 x 4 = 24 58 # short: 8 x 2 = 16 59 # char : 2 = 2 54 FIELD dummy, DUMMY, char[2], padding -
trunk/Ohana/src/libautocode/def/measure-ps1-dev-1.d
r15038 r15511 29 29 30 30 # Pan-STARRS uses a 64-bit detection ID. keep this in two 32 bit ints for backwards compatibility? 31 FIELD detID, DET_ID, unsigned int, ID upper bytes31 FIELD detID, DET_ID, unsigned int, detection ID 32 32 FIELD imageID, IMAGE_ID, unsigned int, reference to image 33 33 … … 55 55 56 56 FIELD dummy, DUMMY, char[2], padding 57 58 # float : 17 x 4 = 6859 # int: 6 x 4 = 2460 # short: 8 x 2 = 1661 # char : 2 = 2 -
trunk/Ohana/src/libautocode/def/measure.d
r15038 r15511 8 8 FIELD dD, D_DEC, float, DEC offset, arcsec 9 9 FIELD M, MAG, float, catalog mag, mag 10 FIELD Mcal, M cal,float, image cal mag, mag11 FIELD Mgal, M gal,float, galaxy mag, mag12 FIELD dM, dM,float, mag error, mag13 FIELD dt, dt,float, exposure time, 2.5*log(exptime)10 FIELD Mcal, M_CAL, float, image cal mag, mag 11 FIELD Mgal, M_GAL, float, galaxy mag, mag 12 FIELD dM, MAG_ERR, float, mag error, mag 13 FIELD dt, M_TIME, float, exposure time, 2.5*log(exptime) 14 14 15 15 # note that with airmass = 1.0 / cos(90 - alt), we have full alt/az representation 16 FIELD airmass, airmass, float, (airmass - 1), airmass16 FIELD airmass, AIRMASS, float, (airmass - 1), airmass 17 17 FIELD az, AZ, float, telescope azimuth 18 18 … … 25 25 FIELD dSky, SKY_FLUX_ERR, float, local estimate of sky flux, counts/sec 26 26 27 FIELD t, t,unsigned int, time in seconds (UNIX)28 FIELD averef, averef,unsigned int, reference to average entry27 FIELD t, TIME, unsigned int, time in seconds (UNIX) 28 FIELD averef, AVE_REF, unsigned int, reference to average entry 29 29 30 30 # Pan-STARRS uses a 64-bit detection ID. keep this in two 32 bit ints for backwards compatibility? … … 38 38 FIELD extNsigma, EXT_NSIGMA, float, psf coverage/quality factor 39 39 40 FIELD FWx, FW x,short, object fwhm major axis, 1/100 of arcsec41 FIELD FWy, FW y,short, object fwhm minor axis, 1/100 of arcsec42 FIELD theta, theta,short, angle wrt ccd X dir, (0xffff/360) deg43 FIELD photcode, photcode, unsigned short, photcode40 FIELD FWx, FWHM_MAJOR, short, object fwhm major axis, 1/100 of arcsec 41 FIELD FWy, FWHM_MINOR, short, object fwhm minor axis, 1/100 of arcsec 42 FIELD theta, PSF_THETA, short, angle wrt ccd X dir, (0xffff/360) deg 43 FIELD photcode, PHOTCODE, unsigned short, photcode 44 44 45 45 FIELD dXccd, X_CCD_ERR, short, X coord error on chip, pixels … … 49 49 FIELD photFlags, PHOT_FLAGS, unsigned short, flags supplied by photometry program 50 50 51 FIELD stargal, stargal,char, star-galaxy separator51 FIELD stargal, STAR_GAL, char, star-galaxy separator 52 52 53 53 # absorb these into photFlags? 54 FIELD dophot, dophot, char, dophot type54 FIELD dophot, DOPHOT, char, dophot type 55 55 56 56 FIELD dummy, DUMMY, char[2], padding
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