Public_documentation/Appendix A.1
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Detailed Description of mcat Columns
Uppercase column names originate from the source extractor program (SExtractor) which operates on each band separately. These values are copied verbatim from the source extractor result files (*-n/fd-cat.fits) and have either an NUV_ or FUV_ prepended to the column name. For these columns, -99.0 is used for unfilled (or blank) values, but in some cases blank magnitude values appear as +99.0. Please see the SExtractor web pages or Bertin and Arnouts (1996, A&A, 117, 393) for more information about the quantities measured by this progam. Lowercase column names are added by the band merger program. For these columns, -999.0 or -9999.0 are unfilled or blank values. Magnitudes are either on the AB system or are GALEX instrumental magnitudes as stated. Fluxes are counts/second unless stated to be in micro Janskys.
MCAT Columns | ||||
Number | Column Name | Format | Units | Description |
1 | ggoid_hex | 16A | string | Hex string version of Galex Global Object ID |
2 | ggoid_dec | 20A | string | Decimal string version of Galex Global Object ID. |
3 | ggoid | 2J | number | This is the 64-bit integer version of the global object ID. Joining these two integers yields a 64 bit integer uniquely identifying this source including the tile number, band, product number, reduction try (path), etc. These values are also given as individual columns (shown below). The bits from most significant to least significant are:
3 bits: vsn - Version number (of the pipeline) 16 bits: tile- Tile or field or target number 2 bits: type- Observation type (00=single,01=AIS(multi)) 2 bits: ow - optics wheel position (01=direct,10=grism,11=opaque,00=undefined) 4 bits: prod- product number(_visits,_best,etc.) 12 bits: img - visit/sub-visit number {when type=01: 5 bit subvis + 7 bit visit} (This is just the visit number, except for AIS (or multi-leg) observations where the first (highest) 5 bits are used for the sub-visit number. When the data is secondary AIS visit data (vsn=2), then the first (highest) 7 bits are used for the sub-visit number.) 3 bits: try - try number (processing number) 2 bits: band- Band (01=nuv,10=fuv,11=both,00=undefined) 20 bits: xid - Extraction ID |
4 | vsn | 1J | number | "Version" number that indicates whether the data is a secondary coadd or not. Secondary coadds have this value set to 2 while for all other data it is set to 1. This is not to be confused with the pipeline version which can be found in the mcat header. |
5 | tilenum | 1J | number | Tile or target number |
6 | type | 1J | number | Obs.type (0=single,1=multiple subvisits) |
7 | ow | 1J | number | Optics wheel (1=drct,2=grsm,3=opaq) |
8 | prod | 1J | number | Product number (0 indicates a visit while a 1 indicates a coadd) |
9 | img | 1J | number | Visit and sub-visit number, when type=01 then 5 bit subvis + 7 bit visit. This is just the visit number, except for AIS observations when the first (highest) 5 bits are used for the sub-visit number. When the data is secondary AIS visit data (vsn=2), then the first (highest) 7 bits are used for the sub-visit number. |
10 | try | 1J | number | Try number (processing attempt number) |
11 | band | 1J | number | Band number (1=nuv,2=fuv,3=both) |
12 | id | 1J | number | Merged ID. Extraction identification number. This is the same as the NUV ID number from the NUV source catalog (called "NUV_NUMBER" below). In cases where there is no NUV source a new ID is assigned which is large enough not to conflict with any NUV ID number. |
13 | subvisit | 1I | number | Sub-visit number for the All-sky Imaging Survey (AIS). An AIS eclipse may have 12 or more telescope pointings. Each of these pointings is assigned a sub-visit number. Note that a visit number corresponds to one eclipse. |
14 | leg | 1I | number | Similar to the sub-visit number, but this is a planned (but perhaps not observed) pointing (or leg) during an AIS eclipse. |
15 | alpha_j2000 | 1D | degrees | Right Ascension in degrees (0 to 360) in a J2000 reference frame. This position is the NUV source position, or the FUV source position for FUV-only sources. |
16 | delta_j2000 | 1D | degrees | Declination in degrees (-90 to 90) in a J2000 reference frame. This position is the NUV source position, or the FUV source position for FUV-only sources. |
17 | alpha_j2000_merged | 1D | degrees | Bandmerged Right Ascension in degrees (0 to 360) in a J2000 reference frame. This position is a signal-to-noise weighted average of the NUV and FUV source positions. |
18 | delta_j2000_merged | 1D | degrees | Bandmerged Declination in degrees (-90 to 90) in a J2000 reference frame. This position is a signal-to-noise weighted average of the NUV and FUV source positions. |
19 | prob | 1E | probability | A bandmerger quantity computed for a given match. This depends on the separation between sources and an estimate of the positional error. Currently, the radial positional error is set at a constant 1.0 arcsecond for all sources. |
20 | sep | 1E | arcseconds | Separation between two bandmerged (NUV and FUV) source positions in arcseconds. |
21 | sep_img | 1E | arcseconds | Separation on images with no adjustment applied to the FUV positions. |
22 | E_bv | 1E | mag | The Galactic reddening expressed as E(B-V). This is derived from the Galactic extinctions maps from Schlegel et al. (1998, ApJ, 500, 525). Data obtained from http://astron.berkeley.edu/davis/dust/data/data.html |
23 | glon | 1E | degrees | Galactic longitude in degrees. |
24 | glat | 1E | degrees | Galactic latitude in degrees. |
25 | primary | 1J | number | Each tile has a primary region defined based upon the planed tile center. If a source falls within the primary region, it has primary=1 and primary=0 otherwise. |
26 | fov_radius | 1E | degrees | distance from center of FOV in degrees |
27 | nuv_det_x | 1E | pixels | Estimate of NUV detector X position of a given source. Since the telescope is dithered and many eclipse observations are combined, this is only an estimate of the X position. The units are in pixels (1.5 arcseconds per pixel) relative to the nominal field center. |
28 | nuv_det_y | 1E | pixels | Estimate of NUV detector Y position of a given source in pixels (1.5 arcseconds per pixel). |
29 | fuv_det_x | 1E | pixels | Estimate of FUV detector X position of a given source in pixels (1.5 arcseconds per pixel). |
30 | fuv_det_y | 1E | pixels | Estimate of FUV detector Y position of a given source in pixels (1.5 arcseconds per pixel). |
31 | chkobj_type | 1J | number | The GALEX field position is aligned to the sky using the known positions of bright stars. The file with the extension "-cat_mch_rtastar.fits" contains data on the bright stars used to align the GALEX field. The filename of this file is given by the FITS header card "MCHFILE". If the value of "chkobj_type" for a source is 1, then that source (NUV position) has been matched to a known bright star. |
32 | chkobj_id | 1J | number | For a source matched to a known star (chkobj_type=1), this column gives the row number in the match table file (-cat_mch_rtastar.fits) containing the data for this match. |
33 | chkobj_r | 1E | degrees | For a source matched to a known star (chkobj_type=1), this column gives the distance in degrees between the known star and the GALEX NUV source position. |
34 | chkobj_pa | 1E | degrees | For a source matched to a known star (chkobj_type=1), this column gives the position angle in degrees between the known star position and the GALEX NUV source position. |
35 | misc_flags | 1J | value | Not used. |
36 | nuv_flux | 1E | flux (micro-Janskys) | Calibrated NUV flux in micro-Janskys. This is currently always set to the SExtractor "AUTO" flux. The NUV counts/sec is converted to micro Janskys using the header card "N_CUJ" and the formula nuv_flux = NUV_FLUX_AUTO * N_CUJ. The value of "N_CUJ" is equal to 10 ^ ( (NUV_ZPMAG - 23.9) / -2.5 ) . Also note that "nuv_flux" may be zero, in this case refer to the "NUV_FLUX_*" columns for flux values. If "nuv_flux" has a value of -999, then there was no NUV source detection. |
37 | nuv_fluxerr | 1E | flux (micro-Janskys) | The error in nuv_flux in micro-Janskys. |
38 | nuv_mag | 1E | AB mag | Calibrated NUV AB magnitude This is currently always set to the SExtractor "AUTO" magnitude. The NUV catalog magnitude is converted to the true magnitude using the zero-point conversion given by the header card "N_ZPMAG" and the formula nuv_mag = NUV_MAG_AUTO + N_ZPMAG). |
39 | nuv_magerr | 1E | AB mag | Error in nuv_mag. |
40 | fuv_flux | 1E | flux (micro-Janskys) | Calibrated FUV flux in micro-Janskys. This is currently always set to the SExtractor "AUTO" flux. The FUV counts/sec is converted to micro Janskys using the header card "F_CUJ" and the formula fuv_flux = = FUV_FLUX_AUTO * N_FUJ. The value of "N_FUJ" is equal to 10 ^ ( (FUV_ZPMAG - 23.9) / -2.5 ) . Also note that "fuv_flux" may be zero, in this case refer to the "FUV_FLUX_*" columns for flux values. If "fuv_flux" has a value of -999, then there was no FUV source detection. |
41 | fuv_fluxerr | 1E | flux (micro-Janskys) | The error in fuv_flux. |
42 | fuv_mag | 1E | AB mag | Calibrated FUV AB magnitude This is currently always set to the SExtractor "AUTO" magnitude. The FUV catalog magnitude is converted to the true magnitude using the zero-point conversion given by the header card "F_ZPMAG" and the formula fuv_mag = FUV_MAG_AUTO + F_ZPMAG). |
43 | fuv_magerr | 1E | AB mag | The error in fuv_mag. |
44 | nuv_s2n | 1E | ratio | NUV signal-to-noise from 'AUTO' flux value. |
45 | fuv_s2n | 1E | ratio | FUV signal-to-noise from 'AUTO' flux value. |
46 | nuv_fcat_flux | 1E | flux (micro-Janskys) | The calibrated NUV flux derived using the source position given in the FUV catalog. The file with extension "-nd-fcat.fits" contains NUV flux values computed using positions given in the "-fd-cat.fits" file. |
47 | nuv_fcat_fluxerr | 1E | flux (micro-Janskys) | Error for nuv_fcat_flux |
48 | fuv_ncat_flux | 1E | flux (micro-Janskys) | The FUV flux derived using the source position given in the NUV catalog. The file with extension "-fd-ncat.fits" contains FUV flux values computed using positions given in the "-nd-cat.fits" file. |
49 | fuv_ncat_fluxerr | 1E | flux (micro-Janskys) | Error for fuv_ncat_flux |
50 | fuv_ra_adj | 1D | degrees | FUV adjusted RA in degrees to fix the average offset between the FUV and NUV positions. |
51 | fuv_dec_adj | 1D | degrees | FUV adjusted DEC in degrees to fix the average offset between the FUV and NUV positions. |
52 | fuv_ncat_flags | 1I | number | FUV_FLAGS from -fd-ncat.fits |
53 | fuv_ncat_mag | 1E | AB mag | FUV calibrated AB magnitude derived from fuv_ncat_flux. |
54 | fuv_ncat_magerr | 1E | AB mag | Error for nuv_fcat_mag |
55 | fuv_ncat_s2n | 1E | ratio | Signal to noise for fuv_ncat_flux |
56 | nuv_fcat_mag | 1E | AB mag | NUV calibrated AB magnitude derived from nuv_fcat_mag. |
57 | nuv_fcat_magerr | 1E | AB mag | Error for nuv_fcat_mag |
58 | nuv_fcat_s2n | 1E | ratio | Signal to noise for nuv_fcat_flux |
59 | fuv_ncat_fwhm_image | 1E | pixels | FUV FWHM_IMAGE value from -fd-ncat.fits (px) |
60 | fuv_ncat_fwhm_world | 1E | degrees | FUV FWHM_WORLD value from -fd-ncat.fits (deg) |
61 | fuv_ncat_flux_radius_1 | 1E | pixels | FUV FLUX_RADIUS #1 (-fd-ncat)(px)[0.20] |
62 | fuv_ncat_flux_radius_2 | 1E | pixels | FUV FLUX_RADIUS #2 (-fd-ncat)(px)[0.50] |
63 | fuv_ncat_flux_radius_3 | 1E | pixels | FUV FLUX_RADIUS #3 (-fd-ncat)(px)[0.80] |
64 | fuv_ncat_flux_radius_4 | 1E | pixels | FUV FLUX_RADIUS #4 (-fd-ncat)(px)[0.90] |
65 | fuv_ncat_flux_radius_5 | 1E | pixels | FUV FLUX_RADIUS #5 (-fd-ncat)(px)[0.95] |
66 | fuv_ncat_flux_aper_1 | 1E | cnts/sec | FUV FLUX_APER #1 (-fd-ncat)(cnt/sec) Flux aperture ( 2.000 px diameter). All of the columns labeled fuv_ncat_flux_aper_X (where X ranges from 1 to 7) refer to measurements of the FUV flux in a fixed circular aperture with the specified diameter in pixels with center determined by the NUV centroid. The diameters for the 7 fluxes are 2, 3, 5, 8, 12, 17, and 23 pixels. The GALEX image scale is fixed at 1.5 arcsec/pixel. |
67 | fuv_ncat_flux_aper_2 | 1E | cnts/sec | FUV FLUX_APER #2 (-fd-ncat)(cnt/sec)[ 3. px diameter] |
68 | fuv_ncat_flux_aper_3 | 1E | cnts/sec | FUV FLUX_APER #3 (-fd-ncat)(cnt/sec)[ 5. px diameter] |
69 | fuv_ncat_flux_aper_4 | 1E | cnts/sec | FUV FLUX_APER #4 (-fd-ncat)(cnt/sec)[ 8. px diameter] |
70 | fuv_ncat_flux_aper_5 | 1E | cnts/sec | FUV FLUX_APER #5 (-fd-ncat)(cnt/sec)[12. px diameter] |
71 | fuv_ncat_flux_aper_6 | 1E | cnts/sec | FUV FLUX_APER #6 (-fd-ncat)(cnt/sec)[17. px diameter] |
72 | fuv_ncat_flux_aper_7 | 1E | cnts/sec | FUV FLUX_APER #7 (-fd-ncat)(cnt/sec)[23. px diameter] |
73 | fuv_ncat_fluxerr_aper_1 | 1E | cnts/sec | error for fuv_ncat_flux_aper_1 |
74 | fuv_ncat_fluxerr_aper_2 | 1E | cnts/sec | error for fuv_ncat_flux_aper_2 |
75 | fuv_ncat_fluxerr_aper_3 | 1E | cnts/sec | error for fuv_ncat_flux_aper_3 |
76 | fuv_ncat_fluxerr_aper_4 | 1E | cnts/sec | error for fuv_ncat_flux_aper_4 |
77 | fuv_ncat_fluxerr_aper_5 | 1E | cnts/sec | error for fuv_ncat_flux_aper_5 |
78 | fuv_ncat_fluxerr_aper_6 | 1E | cnts/sec | error for fuv_ncat_flux_aper_6 |
79 | fuv_ncat_fluxerr_aper_7 | 1E | cnts/sec | error for fuv_ncat_flux_aper_7 |
80 | fuv_ncat_mag_aper_1 | 1E | raw_mag | FUV MAG_APER #1 (-fd-ncat)(raw mag)[ 2. px diameter] Magnitude aperture ( 2.000 px diameter). All of the columns labeled fuv_ncat_mag_aper_X (where X ranges from 1 to 7) refer to measurements of the FUV magnitude in a fixed circular aperture with the specified diameter in pixels with center determined by the NUV centroid. The diameters for the 7 fluxes are 2, 3, 5, 8, 12, 17, and 23 pixels. The GALEX image scale is fixed at 1.5 arcsec/pixel. |
81 | fuv_ncat_mag_aper_2 | 1E | raw_mag | FUV MAG_APER #2 (-fd-ncat)(raw mag)[ 3. px diameter] |
82 | fuv_ncat_mag_aper_3 | 1E | raw_mag | FUV MAG_APER #3 (-fd-ncat)(raw mag)[ 5. px diameter] |
83 | fuv_ncat_mag_aper_4 | 1E | raw_mag | FUV MAG_APER #4 (-fd-ncat)(raw mag)[ 8. px diameter] |
84 | fuv_ncat_mag_aper_5 | 1E | raw_mag | FUV MAG_APER #5 (-fd-ncat)(raw mag)[12. px diameter] |
85 | fuv_ncat_mag_aper_6 | 1E | raw_mag | FUV MAG_APER #6 (-fd-ncat)(raw mag)[17. px diameter] |
86 | fuv_ncat_mag_aper_7 | 1E | raw_mag | FUV MAG_APER #7 (-fd-ncat)(raw mag)[23. px diameter] |
87 | fuv_ncat_magerr_aper_1 | 1E | raw_mag | error for fuv_ncat_mag_aper_1 |
88 | fuv_ncat_magerr_aper_2 | 1E | raw_mag | error for fuv_ncat_mag_aper_2 |
89 | fuv_ncat_magerr_aper_3 | 1E | raw_mag | error for fuv_ncat_mag_aper_3 |
90 | fuv_ncat_magerr_aper_4 | 1E | raw_mag | error for fuv_ncat_mag_aper_4 |
91 | fuv_ncat_magerr_aper_5 | 1E | raw_mag | error for fuv_ncat_mag_aper_5 |
92 | fuv_ncat_magerr_aper_6 | 1E | raw_mag | error for fuv_ncat_mag_aper_6 |
93 | fuv_ncat_magerr_aper_7 | 1E | raw_mag | error for fuv_ncat_mag_aper_7 |
94 | nuv_nc_r1 | 1I | number | NUV neighbor count out to radius R1. The radii used for this column and all of the following neighbor counts are listed in the FITS header. |
95 | nuv_nc_r2 | 1I | number | NUV neighbor count out to radius R2 |
96 | nuv_nc_r3 | 1I | number | NUV neighbor count out to radius R3 |
97 | fuv_nc_r1 | 1I | number | FUV neighbor count out to radius R1 |
98 | fuv_nc_r2 | 1I | number | FUV neighbor count out to radius R2 |
99 | fuv_nc_r3 | 1I | number | FUV neighbor count out to radius R3 |
100 | nuv_nf_r1 | 1E | flux (micro-Janskys) | NUV neighbor flux out to radius R1 |
101 | nuv_nf_r2 | 1E | flux (micro-Janskys) | NUV neighbor flux out to radius R2 |
102 | nuv_nf_r3 | 1E | flux (micro-Janskys) | NUV neighbor flux out to radius R3 |
103 | fuv_nf_r1 | 1E | flux (micro-Janskys) | FUV neighbor flux out to radius R1 |
104 | fuv_nf_r2 | 1E | flux (micro-Janskys) | FUV neighbor flux out to radius R2 |
105 | fuv_nf_r3 | 1E | flux (micro-Janskys) | FUV neighbor flux out to radius R3 |
106 | cn_radius | 1E | arcseconds | Closest neighbor radius in arcseconds |
107 | cn_pa | 1E | degrees | Closest neighbor position angle in degrees |
108 | cn_mag_nuv | 1E | AB mag | Closest neighbor NUV magnitude |
109 | cn_mag_fuv | 1E | AB mag | Closest neighbor FUV magnitude |
110 | nuv_skybg | 1E | flux (cts/sec/arcsec^2) | Background value in photons per second per square arcsecond at the source position (from "alpha_j2000,delta_j2000" columns). This value is taken from the -nd-skybg.fits file image. |
111 | fuv_skybg | 1E | flux (cts/sec/arcsec^2) | Background value in photons per second per square arcsecond at the source position (from "alpha_j2000,delta_j2000" columns). This value is taken from the -nd-skybg.fits file image. |
112 | nuv_weight | 1E | seconds | Effective exposure time (or flat field response value) in seconds at the source position (center pixel) given by the "alpha_j2000,delta_j2000" columns. This value is taken from the -nd-rrhr.fits file image. |
113 | fuv_weight | 1E | seconds | Effective exposure time (or flat field response value) in seconds at the source position (center pixel) given by the "alpha_j2000,delta_j2000" columns. This value is taken from the -fd-rrhr.fits file image. |
114 | nuv_int | 1E | photons/second/pixel | NUV intensity value in photons per second at the source position (center pixel). This value is taken from the -nd-int.fits file image. |
115 | fuv_int | 1E | photons/second/pixel | FUV intensity value in photons per second at the source position (center pixel). This value is taken from the -fd-int.fits file image. |
116 | nuv_thres | 1E | sigmas | NUV threshold sigmas for source detection at the source position. This value is derived from the -nd-int.fits image, the -nd-skybg.fits image and the -nd-wt.fits images. The formula is thres = ( int - skybg ) / wt. |
117 | fuv_thres | 1E | sigmas | FUV threshold sigmas for source detection at the source position. This value is derived from the -fd-int.fits image, the -fd-skybg.fits image and the -fd-wt.fits images. The formula is thres = ( int - skybg ) / wt. |
118 | nuv_contrast | 1E | ratio | The minimum pixel value divided by the maximum pixel value within the extraction box (from the -rrhr.fits image). The extraction box is defined by the columns NUV_XMIN_IMAGE, NUV_YMIN_IMAGE,NUV_XMAX_IMAGE, and NUV_YMAX_IMAGE. This ratio will be between 0.0 and 1.0, inclusive. The pixel size is given by the header card "NSXPIXS" with a nominal size of 1.5 arcseconds by 1.5 arcseconds. |
119 | fuv_contrast | 1E | ratio | The minimum pixel value divided by the maximum pixel value within the extraction box (from the -rrhr.fits image). The extraction box is defined by the columns FUV_XMIN_IMAGE, FUV_YMIN_IMAGE,FUV_XMAX_IMAGE, and FUV_YMAX_IMAGE. This ratio will be between 0.0 and 1.0, inclusive. The pixel size is given by the header card "FSXPIXS" with a nominal size of 1.5 arcseconds by 1.5 arcseconds. |
120 | nuv_scq_mdn | 1E | value | NUV median Q within 40 arcsec of source |
121 | nuv_scq_p05 | 1E | value | NUV 5th percentile Q: 40 arcssec of source |
122 | nuv_scq_p95 | 1E | value | NUV 95th percentile Q: 40 arcssec of source |
123 | fuv_scq_mdn | 1E | value | FUV median Q within 40 arcsec of source |
124 | fuv_scq_p05 | 1E | value | FUV 5th percentile Q: 40 arcssec of source |
125 | fuv_scq_p95 | 1E | value | FUV 95th percentile Q: 40 arcssec of source |
126 | nuv_maskpix | 1J | number | Number of masked pixels within the NUV extraction box (as described for nuv_contrast). A masked pixel is one whose response value (from the -rrhr.fits image) is NAN or is either less than 0.000001 or greater than 10 times the exposure time. |
127 | fuv_maskpix | 1J | number | Number of masked pixels within the FUV extraction box (as described for fuv_contrast). A masked pixel is one whose response value (from the -rrhr.fits image) is NAN or is either less than 0.000001 or greater than 10 times the exposure time. |
128 | nuv_artifact | 1J | number | Logical OR of artifact flags for pixels within a 3x3 pixel box in the NUV flags image (-nd-flags.fits) centered on the source centroid pixel. The artifact flag is a binary flag with each bit indicating a different artifact. The bits have the meanings indicated below. The decimal equivalent for each flag is given in parantheses.
Artifact 1( 1):(edge) Detector bevel edge reflection (NUV only). Artifact 2( 2):(window) Detector window reflection (NUV only). Artifact 3( 4):(dichroic) Dichroic reflection. Artifact 4( 8):(varpix) Varible pixel based on time slices. Artifact 5( 16):(brtedge) Bright star near field edge (NUV only) Artifact 6( 32):Detector rim(annulus) proximity(>0.6 deg fld ctr) Artifact 7( 64):(dimask) dichroic reflection artifact mask flag Artifact 8(128):(varmask) Masked pixel determined by varpix. Artifact 9(256):(hotmask) Detector hot spots. Artifact 10(512):(yaghost) Possible ghost image from YA slope. |
129 | fuv_artifact | 1J | number | Logical OR of artifact flags for pixels within a 3x3 pixel box in the FUV flags image (-fd-flags.fits) centered on the source centroid pixel. The meanings of the flag values are the same as in the NUV. |
130 | nuv_scx | 1E | number | NUV spacecraft position as computed from the detector positions (n/fuv_det_x/y): nuv_scy = (nuv_det_x * 0.5) + 1125.0 . |
131 | nuv_scy | 1E | number | NUV spacecraft position as computed from the detector positions (n/fuv_det_x/y): nuv_scy = (nuv_det_x * 0.5) + 1125.0 |
132 | fuv_scx | 1E | number | FUV Spacecraft position as computed from the detector positions (n/fuv_det_x/y): fuv_scx = (-1.* fuv_det_y * 0.5) + 1125.0. |
133 | fuv_scy | 1E | number | FUV Spacecraft position as computed from the detector positions (n/fuv_det_x/y): fuv_scy = (-1.* fuv_det_y * 0.5) + 1125.0. |
134 | nuv_Q | 1E | number | NUV Q value taken from the calibrated universal Qmap image file. |
135 | fuv_Q | 1E | number | FUV Q value taken from the calibrated universal Qmap image file. |
136 | nuv_ambg | 1J | number | Ambiguity flag for the NUV source detection which is a potentially bandmerged source. Refers to the match (or lack of match) between the NUV source and the FUV source detection. A filled source has been matched and an unfilled source has no match. The flags are:
0: unfilled, no candidates, no ambiguity. 1: filled, first choice candidates agree, no ambiguity. 2: filled, first choice matches second choice candidate. 3: unfilled, first choice taken, no second choice candidate. 4: filled, second choice matches a first choice candidate. 5: filled, second choice matches a second choice candidate. 6: unfilled, first and second taken, no third choice. -6: unfilled, first and second taken, third choice exists. -1: unfilled, cleared, unchecked. -2: not applicable, does not exist, blank. |
137 | fuv_ambg | 1J | number | Same as nuv_ambg, but for the FUV source detection. |
138 | nuv_nc | 1J | number | Number of potentially bandmerging FUV candidates for the NUV source detection. |
139 | fuv_nc | 1J | number | Number of potentially bandmerging NUV candidates for the FUV source detection. |
140 | nuv_cid1 | 1J | number | Source ID number of the FUV source detection of the first (best) candidate to be merged with the NUV source detection. This ID number will appear in the column FUV_NUMBER for the candidate entry in this table. |
141 | fuv_cid1 | 1J | number | Source ID number of the NUV source detection of the first (best) candidate to be merged with the FUV source detection. This ID number will appear in the column NUV_NUMBER for the candidate entry in this table. |
142 | nuv_cid2 | 1J | number | Source ID number of the FUV source which is the second best candidate to be merged with the NUV source. |
143 | fuv_cid2 | 1J | number | Source ID number of the NUV source which is the second best candidate to be merged with the FUV source. |
144 | nuv_cid3 | 1J | number | Source ID number of the FUV source which is the third best candidate to be merged with the NUV source. Third candidates are rare (less than 0.5% occurrence) for GALEX. |
145 | fuv_cid3 | 1J | number | Source ID number of the NUV source which is the third best candidate to be merged with the FUV source. Third candidates are rare (less than 0.5% occurrence) for GALEX. |
146 | nuv_poserr | 1E | arcseconds | This is the total radial position error (1 sigma) which combines the poisson position error and the field error (see the 'N_FLDERR' header card). The field error is a constant for the entire field and represents errors due to effects not accounted for by counting statistics. |
147 | fuv_poserr | 1E | arcseconds | Same as 'nuv_poserr' for FUV positions. |
148 | ib_poserr | 1E | arcseconds | Interband position error in arcseconds |
149 | nuv_pperr | 1E | arcseconds | The part of the NUV position error due to counting statistics. |
150 | fuv_pperr | 1E | arcseconds | The part of the position error due to counting statistics. |
151 | match_reliability | 1E | number | Reliability based on random unfilled FUV |
152 | sourcepa | 1E | degrees | For filled or bandmerged source pairs, the position angle in degrees of the FUV source position relative to the NUV source position. A value of 0 points east and 90 points north. For example, if the FUV source position is directly west of the NUV source position, the sourcepa value would be 180. If the FUV source is directly south of the NUV source, then the sourcepa angle would 270. |
153 | NUV_NUMBER | 1J | value | Running object number |
154 | NUV_FLUX_ISO | 1E | flux (cts/sec) | Isophotal flux |
155 | NUV_FLUXERR_ISO | 1E | flux (cts/sec) | RMS error for isophotal flux |
156 | NUV_MAG_ISO | 1E | raw_mag | Isophotal magnitude |
157 | NUV_MAGERR_ISO | 1E | raw_mag | RMS error for isophotal magnitude |
158 | NUV_FLUX_APER_1 | 1E | flux (cts/sec) | Flux aperture ( 2.000 px). All of the columns labeled either NUV_FLUX_APER_X or NUV_MAG_APER_X (where X ranges from 1 to 7) refer to measurements of the flux in a fixed circular aperture with the specified diameter in pixels. The diameters for the 7 fluxes are 2, 3, 5, 8, 12, 17, and 23 pixels. The GALEX image scale is fixed at 1.5 arcsec/pixel. |
159 | NUV_FLUX_APER_2 | 1E | flux (cts/sec) | Flux aperture ( 3.000 px diameter) |
160 | NUV_FLUX_APER_3 | 1E | flux (cts/sec) | Flux aperture ( 5.000 px diameter) |
161 | NUV_FLUX_APER_4 | 1E | flux (cts/sec) | Flux aperture ( 8.000 px diameter) |
162 | NUV_FLUX_APER_5 | 1E | flux (cts/sec) | Flux aperture ( 12.000 px diameter) |
163 | NUV_FLUX_APER_6 | 1E | flux (cts/sec) | Flux aperture ( 17.000 px diameter) |
164 | NUV_FLUX_APER_7 | 1E | flux (cts/sec) | Flux aperture ( 23.000 px diameter) |
165 | NUV_FLUXERR_APER_1 | 1E | flux (cts/sec) | Flux error aperture ( 2.000 px diameter) |
166 | NUV_FLUXERR_APER_2 | 1E | flux (cts/sec) | Flux error aperture ( 3.000 px diameter) |
167 | NUV_FLUXERR_APER_3 | 1E | flux (cts/sec) | Flux error aperture ( 5.000 px diameter) |
168 | NUV_FLUXERR_APER_4 | 1E | flux (cts/sec) | Flux error aperture ( 8.000 px diameter) |
169 | NUV_FLUXERR_APER_5 | 1E | flux (cts/sec) | Flux error aperture ( 12.000 px diameter) |
170 | NUV_FLUXERR_APER_6 | 1E | flux (cts/sec) | Flux error aperture ( 17.000 px diameter) |
171 | NUV_FLUXERR_APER_7 | 1E | flux (cts/sec) | Flux error aperture ( 23.000 px diameter) |
172 | NUV_MAG_APER_1 | 1E | raw_mag | Magnitude aperture ( 2.000 px diameter) |
173 | NUV_MAG_APER_2 | 1E | raw_mag | Magnitude aperture ( 3.000 px diameter) |
174 | NUV_MAG_APER_3 | 1E | raw_mag | Magnitude aperture ( 5.000 px diameter) |
175 | NUV_MAG_APER_4 | 1E | raw_mag | Magnitude aperture ( 8.000 px diameter) |
176 | NUV_MAG_APER_5 | 1E | raw_mag | Magnitude aperture ( 12.000 px diameter) |
177 | NUV_MAG_APER_6 | 1E | raw_mag | Magnitude aperture ( 17.000 px diameter) |
178 | NUV_MAG_APER_7 | 1E | raw_mag | Magnitude aperture ( 23.000 px diameter) |
179 | NUV_MAGERR_APER_1 | 1E | raw_mag | Magnitude error aperture ( 2.000 px diameter) |
180 | NUV_MAGERR_APER_2 | 1E | raw_mag | Magnitude error aperture ( 3.000 px diameter) |
181 | NUV_MAGERR_APER_3 | 1E | raw_mag | Magnitude error aperture ( 5.000 px diameter) |
182 | NUV_MAGERR_APER_4 | 1E | raw_mag | Magnitude error aperture ( 8.000 px diameter) |
183 | NUV_MAGERR_APER_5 | 1E | raw_mag | Magnitude error aperture ( 12.000 px diameter) |
184 | NUV_MAGERR_APER_6 | 1E | raw_mag | Magnitude error aperture ( 17.000 px diameter) |
185 | NUV_MAGERR_APER_7 | 1E | raw_mag | Magnitude error aperture ( 23.000 px diameter) |
186 | NUV_FLUX_AUTO | 1E | flux (cts/sec) | Flux within a Kron-like elliptical aperture |
187 | NUV_FLUXERR_AUTO | 1E | flux (cts/sec) | RMS error for AUTO flux |
188 | NUV_MAG_AUTO | 1E | raw_mag | Kron-like elliptical aperture magnitude |
189 | NUV_MAGERR_AUTO | 1E | raw_mag | RMS error for AUTO magnitude |
190 | NUV_FLUX_RADIUS_1 | 1E | pixel | Fraction-of-light radius ( 0.2000) |
191 | NUV_FLUX_RADIUS_2 | 1E | pixel | Fraction-of-light radius ( 0.5000) |
192 | NUV_FLUX_RADIUS_3 | 1E | pixel | Fraction-of-light radius ( 0.8000) |
193 | NUV_FLUX_RADIUS_4 | 1E | pixel | Fraction-of-light radius ( 0.9000) |
194 | NUV_FLUX_RADIUS_5 | 1E | pixel | Fraction-of-light radius ( 0.9500) |
195 | NUV_KRON_RADIUS | 1E | ratio | Kron apertures in units of A or B |
196 | NUV_BACKGROUND | 1E | count | Background at centroid position |
197 | NUV_THRESHOLD | 1E | number | Detection threshold above background |
198 | NUV_MU_THRESHOLD | 1E | number | Detection threshold above background |
199 | NUV_FLUX_MAX | 1E | number | Peak flux above background |
200 | NUV_MU_MAX | 1E | number | Peak surface brightness above background |
201 | NUV_ISOAREA_IMAGE | 1E | pixels | Isophotal area above Analysis threshold |
202 | NUV_ISOAREA_WORLD | 1E | square degrees | Isophotal area above Analysis threshold |
203 | NUV_ISOAREAF_IMAGE | 1E | pixels | Isophotal area (filtered) above Detection thres |
204 | NUV_ISOAREAF_WORLD | 1E | square degrees | Isophotal area (filtered) above Detection thres |
205 | NUV_XMIN_IMAGE | 1J | pixel | Minimum x-coordinate among detected pixels |
206 | NUV_YMIN_IMAGE | 1J | pixel | Minimum y-coordinate among detected pixels |
207 | NUV_XMAX_IMAGE | 1J | pixel | Maximum x-coordinate among detected pixels |
208 | NUV_YMAX_IMAGE | 1J | pixel | Maximum y-coordinate among detected pixels |
209 | NUV_X_IMAGE | 1E | pixel | Object position along x |
210 | NUV_Y_IMAGE | 1E | pixel | Object position along y |
211 | NUV_XPEAK_IMAGE | 1J | count | x-coordinate of the brightest pixel |
212 | NUV_YPEAK_IMAGE | 1J | count | y-coordinate of the brightest pixel |
213 | NUV_ALPHA_J2000 | 1D | degrees | Right ascension of barycenter (J2000) |
214 | NUV_DELTA_J2000 | 1D | degrees | Declination of barycenter (J2000) |
215 | NUV_X2_IMAGE | 1E | pixel | Variance along x |
216 | NUV_Y2_IMAGE | 1E | pixel | Variance along y |
217 | NUV_XY_IMAGE | 1E | pixel | Covariance between x and y |
218 | NUV_X2_WORLD | 1E | degrees | Variance along X-WORLD (alpha) |
219 | NUV_Y2_WORLD | 1E | degrees | Variance along Y-WORLD (delta) |
220 | NUV_XY_WORLD | 1E | degrees | Covariance between X-WORLD and Y-WORLD |
221 | NUV_CXX_IMAGE | 1E | pixels | Cxx object ellipse parameter |
222 | NUV_CYY_IMAGE | 1E | pixels | Cyy object ellipse parameter |
223 | NUV_CXY_IMAGE | 1E | pixels | Cxy object ellipse parameter |
224 | NUV_CXX_WORLD | 1E | degrees | Cxx object ellipse parameter (WORLD units) |
225 | NUV_CYY_WORLD | 1E | degrees | Cyy object ellipse parameter (WORLD units) |
226 | NUV_CXY_WORLD | 1E | degrees | Cxy object ellipse parameter (WORLD units) |
227 | NUV_A_IMAGE | 1E | pixels | Profile RMS along major axis |
228 | NUV_B_IMAGE | 1E | pixels | Profile RMS along minor axis |
229 | NUV_A_WORLD | 1E | degrees | Profile RMS along major axis (world units) |
230 | NUV_B_WORLD | 1E | degrees | Profile RMS along minor axis (world units) |
231 | NUV_THETA_IMAGE | 1E | degrees | Position angle (CCW/x) |
232 | NUV_THETA_WORLD | 1E | degrees | Position angle (CCW/world-x) |
233 | NUV_THETA_J2000 | 1E | degrees | Position angle (east of north) (J2000) |
234 | NUV_ELONGATION | 1E | ratio | A_IMAGE/B_IMAGE |
235 | NUV_ELLIPTICITY | 1E | number | 1 - B_IMAGE/A_IMAGE |
236 | NUV_ERRX2_IMAGE | 1D | pixels | Variance of position along x |
237 | NUV_ERRY2_IMAGE | 1D | pixels | Variance of position along y |
238 | NUV_ERRXY_IMAGE | 1E | pixels | Covariance of position between x and y |
239 | NUV_ERRX2_WORLD | 1D | degrees | Variance of position along X-WORLD (alpha) |
240 | NUV_ERRY2_WORLD | 1D | degrees | Variance of position along Y-WORLD (delta) |
241 | NUV_ERRXY_WORLD | 1E | degrees | Covariance of position X-WORLD/Y-WORLD |
242 | NUV_ERRCXX_IMAGE | 1E | pixels | Cxx error ellipse parameter |
243 | NUV_ERRCYY_IMAGE | 1E | pixels | Cyy error ellipse parameter |
244 | NUV_ERRCXY_IMAGE | 1E | pixels | Cxy error ellipse parameter |
245 | NUV_ERRCXX_WORLD | 1E | degrees | Cxx error ellipse parameter (WORLD units) |
246 | NUV_ERRCYY_WORLD | 1E | degrees | Cyy error ellipse parameter (WORLD units) |
247 | NUV_ERRCXY_WORLD | 1E | degrees | Cxy error ellipse parameter (WORLD units) |
248 | NUV_ERRA_IMAGE | 1E | pixels | RMS position error along major axis |
249 | NUV_ERRB_IMAGE | 1E | pixels | RMS position error along minor axis |
250 | NUV_ERRA_WORLD | 1E | degrees | World RMS position error along major axis |
251 | NUV_ERRB_WORLD | 1E | degrees | World RMS position error along minor axis |
252 | NUV_ERRTHETA_IMAGE | 1E | degrees | Error ellipse position angle (CCW/x) |
253 | NUV_ERRTHETA_WORLD | 1E | degrees | Error ellipse pos. angle (CCW/world-x) |
254 | NUV_ERRTHETA_J2000 | 1E | degrees | J2000 error ellipse pos. angle (east of north) |
255 | NUV_FWHM_IMAGE | 1E | pixel | FWHM assuming a gaussian core |
256 | NUV_FWHM_WORLD | 1E | degrees | FWHM assuming a gaussian core |
257 | NUV_FLAGS | 1I | value | Extraction flags |
258 | NUV_CLASS_STAR | 1E | value | S/G classifier output |
259 | FUV_NUMBER | 1J | value | Running object number |
260 | FUV_FLUX_ISO | 1E | flux (cts/sec) | Isophotal flux |
261 | FUV_FLUXERR_ISO | 1E | flux (cts/sec) | RMS error for isophotal flux |
262 | FUV_MAG_ISO | 1E | raw_mag | Isophotal magnitude |
263 | FUV_MAGERR_ISO | 1E | raw_mag | RMS error for isophotal magnitude |
264 | FUV_FLUX_APER_1 | 1E | flux (cts/sec) | Flux aperture ( 2.000 px diameter). All of the columns labeled either FUV_FLUX_APER_X or FUV_MAG_APER_X (where X ranges from 1 to 7) refer to measurements of the flux in a fixed circular aperture with the specified diameter in pixels. The diameters for the 7 fluxes are 2, 3, 5, 8, 12, 17, and 23 pixels. The GALEX image scale is fixed at 1.5 arcsec/pixel. |
265 | FUV_FLUX_APER_2 | 1E | flux (cts/sec) | Flux aperture ( 3.000 px diameter) |
266 | FUV_FLUX_APER_3 | 1E | flux (cts/sec) | Flux aperture ( 5.000 px diameter) |
267 | FUV_FLUX_APER_4 | 1E | flux (cts/sec) | Flux aperture ( 8.000 px diameter) |
268 | FUV_FLUX_APER_5 | 1E | flux (cts/sec) | Flux aperture ( 12.000 px diameter) |
269 | FUV_FLUX_APER_6 | 1E | flux (cts/sec) | Flux aperture ( 17.000 px diameter) |
270 | FUV_FLUX_APER_7 | 1E | flux (cts/sec) | Flux aperture ( 23.000 px diameter) |
271 | FUV_FLUXERR_APER_1 | 1E | flux (cts/sec) | Flux error aperture ( 2.000 px diameter) |
272 | FUV_FLUXERR_APER_2 | 1E | flux (cts/sec) | Flux error aperture ( 3.000 px diameter) |
273 | FUV_FLUXERR_APER_3 | 1E | flux (cts/sec) | Flux error aperture ( 5.000 px diameter) |
274 | FUV_FLUXERR_APER_4 | 1E | flux (cts/sec) | Flux error aperture ( 8.000 px diameter) |
275 | FUV_FLUXERR_APER_5 | 1E | flux (cts/sec) | Flux error aperture ( 12.000 px diameter) |
276 | FUV_FLUXERR_APER_6 | 1E | flux (cts/sec) | Flux error aperture ( 17.000 px diameter) |
277 | FUV_FLUXERR_APER_7 | 1E | flux (cts/sec) | Flux error aperture ( 23.000 px diameter) |
278 | FUV_MAG_APER_1 | 1E | raw_mag | Magnitude aperture ( 2.000 px diameter) |
279 | FUV_MAG_APER_2 | 1E | raw_mag | Magnitude aperture ( 3.000 px diameter) |
280 | FUV_MAG_APER_3 | 1E | raw_mag | Magnitude aperture ( 5.000 px diameter) |
281 | FUV_MAG_APER_4 | 1E | raw_mag | Magnitude aperture ( 8.000 px diameter) |
282 | FUV_MAG_APER_5 | 1E | raw_mag | Magnitude aperture ( 12.000 px diameter) |
283 | FUV_MAG_APER_6 | 1E | raw_mag | Magnitude aperture ( 17.000 px diameter) |
284 | FUV_MAG_APER_7 | 1E | raw_mag | Magnitude aperture ( 23.000 px diameter) |
285 | FUV_MAGERR_APER_1 | 1E | raw_mag | Magnitude error aperture ( 2.000 px diameter) |
286 | FUV_MAGERR_APER_2 | 1E | raw_mag | Magnitude error aperture ( 3.000 px diameter) |
287 | FUV_MAGERR_APER_3 | 1E | raw_mag | Magnitude error aperture ( 5.000 px diameter) |
288 | FUV_MAGERR_APER_4 | 1E | raw_mag | Magnitude error aperture ( 8.000 px diameter) |
289 | FUV_MAGERR_APER_5 | 1E | raw_mag | Magnitude error aperture ( 12.000 px diameter) |
290 | FUV_MAGERR_APER_6 | 1E | raw_mag | Magnitude error aperture ( 17.000 px diameter) |
291 | FUV_MAGERR_APER_7 | 1E | raw_mag | Magnitude error aperture ( 23.000 px diameter) |
292 | FUV_FLUX_AUTO | 1E | flux (cts/sec) | Flux within a Kron-like elliptical aperture |
293 | FUV_FLUXERR_AUTO | 1E | flux (cts/sec) | RMS error for AUTO flux |
294 | FUV_MAG_AUTO | 1E | raw_mag | Kron-like elliptical aperture magnitude |
295 | FUV_MAGERR_AUTO | 1E | raw_mag | RMS error for AUTO magnitude |
296 | FUV_FLUX_RADIUS_1 | 1E | pixel | Fraction-of-light radius ( 0.2000) |
297 | FUV_FLUX_RADIUS_2 | 1E | pixel | Fraction-of-light radius ( 0.5000) |
298 | FUV_FLUX_RADIUS_3 | 1E | pixel | Fraction-of-light radius ( 0.8000) |
299 | FUV_FLUX_RADIUS_4 | 1E | pixel | Fraction-of-light radius ( 0.9000) |
300 | FUV_FLUX_RADIUS_5 | 1E | pixel | Fraction-of-light radius ( 0.9500) |
301 | FUV_KRON_RADIUS | 1E | ratio | Kron apertures in units of A or B |
302 | FUV_BACKGROUND | 1E | count | Background at centroid position |
303 | FUV_THRESHOLD | 1E | number | Detection threshold above background |
304 | FUV_MU_THRESHOLD | 1E | number | Detection threshold above background |
305 | FUV_FLUX_MAX | 1E | number | Peak flux above background |
306 | FUV_MU_MAX | 1E | number | Peak surface brightness above background |
307 | FUV_ISOAREA_IMAGE | 1E | pixels | Isophotal area above Analysis threshold |
308 | FUV_ISOAREA_WORLD | 1E | square degrees | Isophotal area above Analysis threshold |
309 | FUV_ISOAREAF_IMAGE | 1E | pixels | Isophotal area (filtered) above Detection thres |
310 | FUV_ISOAREAF_WORLD | 1E | square degrees | Isophotal area (filtered) above Detection thres |
311 | FUV_XMIN_IMAGE | 1J | pixel | Minimum x-coordinate among detected pixels |
312 | FUV_YMIN_IMAGE | 1J | pixel | Minimum y-coordinate among detected pixels |
313 | FUV_XMAX_IMAGE | 1J | pixel | Maximum x-coordinate among detected pixels |
314 | FUV_YMAX_IMAGE | 1J | pixel | Maximum y-coordinate among detected pixels |
315 | FUV_X_IMAGE | 1E | pixel | Object position along x |
316 | FUV_Y_IMAGE | 1E | pixel | Object position along y |
317 | FUV_XPEAK_IMAGE | 1J | count | x-coordinate of the brightest pixel |
318 | FUV_YPEAK_IMAGE | 1J | count | y-coordinate of the brightest pixel |
319 | FUV_ALPHA_J2000 | 1D | degrees | Right ascension of barycenter (J2000) |
320 | FUV_DELTA_J2000 | 1D | degrees | Declination of barycenter (J2000) |
321 | FUV_X2_IMAGE | 1E | pixel | Variance along x |
322 | FUV_Y2_IMAGE | 1E | pixel | Variance along y |
323 | FUV_XY_IMAGE | 1E | pixel | Covariance between x and y |
324 | FUV_X2_WORLD | 1E | degrees | Variance along X-WORLD (alpha) |
325 | FUV_Y2_WORLD | 1E | degrees | Variance along Y-WORLD (delta) |
326 | FUV_XY_WORLD | 1E | degrees | Covariance between X-WORLD and Y-WORLD |
327 | FUV_CXX_IMAGE | 1E | pixels | Cxx object ellipse parameter |
328 | FUV_CYY_IMAGE | 1E | pixels | Cyy object ellipse parameter |
329 | FUV_CXY_IMAGE | 1E | pixels | Cxy object ellipse parameter |
330 | FUV_CXX_WORLD | 1E | degrees | Cxx object ellipse parameter (WORLD units) |
331 | FUV_CYY_WORLD | 1E | degrees | Cyy object ellipse parameter (WORLD units) |
332 | FUV_CXY_WORLD | 1E | degrees | Cxy object ellipse parameter (WORLD units) |
333 | FUV_A_IMAGE | 1E | pixels | Profile RMS along major axis |
334 | FUV_B_IMAGE | 1E | pixels | Profile RMS along minor axis |
335 | FUV_A_WORLD | 1E | degrees | Profile RMS along major axis (world units) |
336 | FUV_B_WORLD | 1E | degrees | Profile RMS along minor axis (world units) |
337 | FUV_THETA_IMAGE | 1E | degrees | Position angle (CCW/x) |
338 | FUV_THETA_WORLD | 1E | degrees | Position angle (CCW/world-x) |
339 | FUV_THETA_J2000 | 1E | degrees | Position angle (east of north) (J2000) |
340 | FUV_ELONGATION | 1E | ratio | A_IMAGE/B_IMAGE |
341 | FUV_ELLIPTICITY | 1E | number | 1 - B_IMAGE/A_IMAGE |
342 | FUV_ERRX2_IMAGE | 1D | pixels | Variance of position along x |
343 | FUV_ERRY2_IMAGE | 1D | pixels | Variance of position along y |
344 | FUV_ERRXY_IMAGE | 1E | pixels | Covariance of position between x and y |
345 | FUV_ERRX2_WORLD | 1D | degrees | Variance of position along X-WORLD (alpha) |
346 | FUV_ERRY2_WORLD | 1D | degrees | Variance of position along Y-WORLD (delta) |
347 | FUV_ERRXY_WORLD | 1E | degrees | Covariance of position X-WORLD/Y-WORLD |
348 | FUV_ERRCXX_IMAGE | 1E | pixels | Cxx error ellipse parameter |
349 | FUV_ERRCYY_IMAGE | 1E | pixels | Cyy error ellipse parameter |
350 | FUV_ERRCXY_IMAGE | 1E | pixels | Cxy error ellipse parameter |
351 | FUV_ERRCXX_WORLD | 1E | degrees | Cxx error ellipse parameter (WORLD units) |
352 | FUV_ERRCYY_WORLD | 1E | degrees | Cyy error ellipse parameter (WORLD units) |
353 | FUV_ERRCXY_WORLD | 1E | degrees | Cxy error ellipse parameter (WORLD units) |
354 | FUV_ERRA_IMAGE | 1E | pixels | RMS position error along major axis |
355 | FUV_ERRB_IMAGE | 1E | pixels | RMS position error along minor axis |
356 | FUV_ERRA_WORLD | 1E | degrees | World RMS position error along major axis |
357 | FUV_ERRB_WORLD | 1E | degrees | World RMS position error along minor axis |
358 | FUV_ERRTHETA_IMAGE | 1E | degrees | Error ellipse position angle (CCW/x) |
359 | FUV_ERRTHETA_WORLD | 1E | degrees | Error ellipse pos. angle (CCW/world-x) |
360 | FUV_ERRTHETA_J2000 | 1E | degrees | J2000 error ellipse pos. angle (east of north) |
361 | FUV_FWHM_IMAGE | 1E | pixel | FWHM assuming a gaussian core |
362 | FUV_FWHM_WORLD | 1E | degrees | FWHM assuming a gaussian core |
363 | FUV_FLAGS | 1I | value | Extraction flags |
364 | FUV_CLASS_STAR | 1E | value | S/G classifier output |