| | 1 | This describes the columns and flags in the smf/cmf files. They are listed in psModules/src/objects/pmSourceIO_CMF_PS1_V1.c, this is a slightly more descriptive version. |
| | 2 | |
| | 3 | == Columns == |
| | 4 | |
| | 5 | * IPP_IDET - detection id (increment from 0 per chip - gaps are from magic) |
| | 6 | * X_PSF -position (in pixels |
| | 7 | * Y_PSF -position in pixels |
| | 8 | * X_PSF_SIGMA -position sigma |
| | 9 | * Y_PSF_SIGMA -position sigma |
| | 10 | * POSANGLE - position angle of the instrument coordinate system at source (ie, the angle between north and the y-axis) in degrees |
| | 11 | * PLTSCALE - plate-scale at the source position (it varies across the exposure!) in arcsec |
| | 12 | * PSF_INST_MAG - PSF Instrumental mag |
| | 13 | * PSF_INST_MAG - error for that |
| | 14 | * AP_MAG - aperture mag |
| | 15 | * AP_MAG_RADIUS - aperture mag radius (pixels) |
| | 16 | * PEAK_FLUX_AS_MAG - as it says, it is the flux (counts/pixel) for the peak pixel expressed as an instrumental magnitude (-2.5*log(flux)) |
| | 17 | * CAL_PSF_MAG - calibrated PSF MAG |
| | 18 | * CAL_PS_MAG_SIG - error |
| | 19 | * RA_PSF - ra |
| | 20 | * DEC_PSF - dec |
| | 21 | * SKY - background in counts (DN, not electrons) |
| | 22 | * SKY_SIGMA -error |
| | 23 | * PSF_CHISQ - chisq of psf |
| | 24 | * CR_NSIGMA - cosmic ray |
| | 25 | * EXT_NSIGMA - extended source |
| | 26 | * PSF_MAJOR - major axis (pixel) |
| | 27 | * PSF_MINOR - minor axis (pixel) |
| | 28 | * PSF_THETA - angle |
| | 29 | * PSF_QF - the psf-weighted fraction of unmasked pixels: |
| | 30 | * {{{\Sum_i (psf_i * !masked) / \Sum_i (psf_i)}}} |
| | 31 | * PSF_NDOF - number of degrees of freedom for the fit -- for the diff detections, the only free parameter is the flux, so N_DOF = N_PIX - 1; in other cases, there may be more parameters (eg, position, size, etc). |
| | 32 | * PSF_NPIX - number of pixels for fit |
| | 33 | * MOMENTS_XX - second moment in x: |
| | 34 | * {{{\Sum ((x_i - x_o)^2 f_i) / \Sum (f_i) }}} where x_o is the centroid {{{ \Sum (x_i f_i) / \Sum f_i }}} |
| | 35 | * MOMENTS_XY - second moment in xy: |
| | 36 | * {{{\Sum ((x_i - x_o)(y_i - y_o)^2 f_i) / \Sum (f_i) }}} |
| | 37 | * MOMENTS_YY - second moment in xy |
| | 38 | * {{{\Sum ((y_i - y_o)^2 f_i) / \Sum (f_i) }}} |
| | 39 | * FLAGS - see below |
| | 40 | * N_FRAMES - this is not currently set, but it is supposed to have the value of the number of input images overlapping the center of the source (for warp-warp diff, it would be 2, for a single image it would be 1, for a stack it may be something else). |
| | 41 | * PADDING - a dummy block of data needed to fit the rows into 8-byte boundaries (this lets me read into structures as a bulk byte read operation). |
| | 42 | |
| | 43 | |
| | 44 | == Flags == |
| | 45 | |
| | 46 | ||DEFAULT || 0 || Initial value: resets all bits || |
| | 47 | ||PSFMODEL||1 || Source fitted with a psf model (linear or non-linear) || |
| | 48 | ||EXTMODEL||2 ||Source fitted with an extended-source model|| |
| | 49 | ||FITTED||4 ||Source fitted with non-linear model (PSF or EXT; good or bad)|| |
| | 50 | ||FITFAIL||8 ||Fit (non-linear) failed (non-converge, off-edge, run to zero)|| |
| | 51 | ||POORFIT||16 ||Fit succeeds, but low-SN, high-Chisq, or large (for PSF -- drop?)|| |
| | 52 | ||PAIR ||32 ||Source fitted with a double psf || |
| | 53 | ||PSFSTAR||64 ||Source used to define PSF model || |
| | 54 | ||SATSTAR||128 ||Source model peak is above saturation || |
| | 55 | ||BLEND ||256 ||Source is a blend with other sourcers || |
| | 56 | ||EXTERNALPOS"|| 512 || Source based on supplied input position || |
| | 57 | ||BADPSF ||1024 || Failed to get good estimate of object's PSF || |
| | 58 | ||DEFECT ||2048 ||Source is thought to be a defect || |
| | 59 | ||SATURATED||4096 ||Source is thought to be saturated pixels (bleed trail) || |
| | 60 | ||CR_LIMIT ||8192 ||Source has crNsigma above limit || |
| | 61 | ||EXT_LIMIT ||16384 ||Source has extNsigma above limit || |
| | 62 | ||MOMENTS_FAILURE ||32768 ||could not measure the moments || |
| | 63 | ||SKY_FAILURE ||65536 ||could not measure the local sky || |
| | 64 | ||SKYVAR_FAILURE ||131072 ||could not measure the local sky variance || |
| | 65 | ||MOMENTS_SN ||262144 ||moments not measured due to low S/N || |
| | 66 | ||BIG_RADIUS ||1048576 ||poor moments for small radius, try large radius|| |
| | 67 | ||AP_MAGS ||2097152 ||source has an aperture magnitude || |
| | 68 | ||BLEND_FIT ||4194304 ||source was fitted as a blend || |
| | 69 | ||EXTENDED_FIT||8388608||full extended fit was used || |
| | 70 | ||EXTENDED_STATS||16777216||extended aperture stats calculated || |
| | 71 | ||LINEAR_FIT|| 33554432||source fitted with the linear fit || |
| | 72 | ||NONLINEAR_FIT||67108864 ||source fitted with the non-linear fit || |
| | 73 | ||RADIAL_FLUX||134217728||radial flux measurements calculated|| |
| | 74 | ||SIZE_SKIPPED||268435456||size could not be determined || |
| | 75 | ||ON_SPIKE||536870912||peak lands on diffraction spike || |
| | 76 | ||ON_GHOST||1073741824||peak lands on ghost or glint || |
| | 77 | ||OFF_CHIP||2147483648||peak lands off edge of chip|| |
| | 78 | ||NOCAL||4294967296||detection ignored for this analysis (photcode, time range) -- internal only || |
| | 79 | ||POOR_PHOTOM||8589934592||detection is photometry outlier || |
| | 80 | ||SKIP_PHOTOM||17179869184||detection was ignored for photometry measurement || |
| | 81 | ||MEAS_AREA||34359738368||detection near image edge || |
| | 82 | ||POOR_ASTROM||68719476736||detection is astrometry outlier || |
| | 83 | ||SKIP_ASTROM||137438953472||detection was ignored for astrometry measurement|| |
| | 84 | ||USED_OBJ||274877906944||detection was used during opdate objects|| |
| | 85 | ||USED_CHIP||549755813888||detection was used during update chips|| |
| | 86 | ||BLEND_MEAS||1099511627776||detection is within radius of multiple objects|| |
| | 87 | ||BLEND_OBJ||2199023255552||multiple detections within radius of object|| |
| | 88 | ||BLEND_MEAS_X||17592186044416||detection is within radius of multiple objects across catalogs|| |
| | 89 | ||ARTIFACT||35184372088832||detection is thought to be non-astronomical|| |
