Appendix 3. 6x Scan Working Databases and Images


3. 6x Working Databases and Metadata Table Formats

c. 6x Scan Information Table Column Descriptions

The following table contains brief descriptions of the parameters in the 6x Scan Information Table, which provides basic metadata for each survey mode scan taken during 2MASS 6x observations. The table is organized according to the broad function and utility of the parameters: positional information, photometric information, source detection statistics, etc.

The columns in the following table are:

TABLE 1: Description of Fields in the 6x Scan Information Table
Column NameFormatUnitsnullsDescription
Primary Information
scan_key/cntr %5d---no The unique identification number for this scan. This column is called scan_key in the DVD and ftp versions of the Scan Information Table and cntr in the IRSA/GATOR version.
hemis %1s---no Observatory from which data were obtained:
  • "n" = north = Mt. Hopkins
  • "s" = south = Cerro Tololo.
date %10syyyy-mm-ddno The observation reference date for this scan expressed in ISO standard format. This is the UT date at sunrise for the night on which the scan was observed. Because it is possible for the UT date to change during a night of observations, the actual UT date for a source can differ from date by one day. Use the Julian Date (jdate) for a more accurate determination of the observation time of the scan.
scan %3d---no Scan number (unique within date).
tile %6d---no Tile identification number.
Positional Information
ra %10.6fdegno Right ascension of scan center for equinox J2000; this is computed from the interior corners ra_[1,2,3,4] and dec_[1,2,3,4] (see below).
dec/decl %10.6fdegno Declination of scan center for equinox J2000; this is computed from the interior corners ra_[1,2,3,4] and dec_[1,2,3,4] (see below). This column is called decl on the DVD versions of the Scan Information Table and dec in the IRSA/GATOR version.
glon %7.3fdegno Galactic longitude of scan center, as computed from ra and dec above. Galactic coordinates are derived by precessing reconstructed ra and dec to B1950, and performing rotational transformation into the lII, bII coordinate system.
glat %7.3fdegno Galactic latitude of scan center, as computed from ra and dec above. Galactic coordinates are derived by precessing reconstructed ra and dec to B1950, and performing rotational transformation into the lII, bII coordinate system.
ra_1 %10.6fdegno J2000 right ascension of the eastern corner at start of scan. This is the corner fully covered by all three bands.
dec_1 %10.6fdegno J2000 declination of the eastern corner at start of scan. This is the corner fully covered by all three bands.
ra_2 %10.6fdegno J2000 right ascension of the western corner at start of scan. This is the corner fully covered by all three bands.
dec_2 %10.6fdegno J2000 declination of the western corner at start of scan. This is the corner fully covered by all three bands.
ra_3 %10.6fdegno J2000 right ascension of the eastern corner at end of scan. This is the corner fully covered by all three bands.
dec_3 %10.6fdegno J2000 declination of the eastern corner at end of scan. This is the corner fully covered by all three bands.
ra_4 %10.6fdegno J2000 right ascension of the western corner at end of scan. This is the corner fully covered by all three bands.
dec_4 %10.6fdegno J2000 declination of the western corner at end of scan. This is the corner fully covered by all three bands.
General Information
sd %1s --- no Scanning direction:
  • "n" = north-going
  • "s" = south-going.
qual %2d --- no Quality score for scan:
  • "10" is highest grade
  • "0" is lowest.
hgl %1d --- no Special flag indicating whether or not this scan has a single-frame H-band or J-band electronic glitch:
  • "0" indicates no glitch
  • "1" indicates glitch.
cld %1d --- no Special flag indicating whether or not a cloud was found in the scan after comparison of its photometry to that of overlapping scans in the database:
  • "0" indicates no evidence for clouds
  • "1" indicates clouds.
xph %1d --- no Special flag indicating whether or not another photometric problem, not obviously cloud related, was found in the scan after comparing its photometry to that of overlapping scans:
  • "0" indicates no problem
  • "1" indicates compromised photometry.
anom %1d --- no Special flag indicating whether or not an unusual problem was found in the Atlas Images for this scan. Such problem include, but are not limited to, residual meteor trails, satellite trails, insect trails, and unusual reflections or glints from bright stars:
  • "0" indicates no such problem
  • "1" indicates an anomaly.
Time of Observation
ut %9.6fhr no Universal Time (UT) at beginning of scan.
jdate %12.4fdayno Julian Date at beginning of scan.
Telescope and Instrument Fields
airm %4.2f---no Airmass at beginning of scan.
zd %4.1fdegno Scan's distance from the zenith at beginning of scan.
ha %9.6fhrno Hour angle at beginning of scan.
rh %2d%no Relative humidity of telescope enclosure at beginning of scan.
air_temp %4.1fdeg Cno Air temperature at beginning of scan.
tel_temp %4.1fdeg Cno Telescope girdle temperature at beginning of scan. This temperature was used to adjust telescope focus to compensate for variations with temperature.
focus %5d---no Focus setting of telescope at beginning of scan. This is a measure of the position of the focus mechanism, in units of 1.25 microns, relative to a reference position. This reference position changed each time the telescope was collimated.
hry %1s---no Flag indicating the H-band array configuration for the camera:
  • "o" indicates the original configuration
  • "n" indicates the new (modified) configuration.
For the southern camera, the array configuration was never changed, so this flag is always "o". For the northern camera a new H-band array, first used on 13 Sep 1999 (UT), was installed in mid-survey. Before this date the flag is "o" and on or after this date it is "n".
c_strat %1s---no Flag indicating the calibration strategy for this night's data:
  • "o" indicates original strategy in which two calibration fields were observed after every two-hour segment of regular survey scans
  • "n" indicates new strategy in which one calibration field was observed after every hour's segment of regular survey scans.
For data taken from the southern hemisphere, this flag is always "n". For data taken from the northern hemisphere this flag is set to "o" on dates before 11 Oct 1997 (UT), and to "n" for dates of 11 Oct 1997 (UT) or thereafter.
Photometric Information
j_zp_ap %7.4fmagno Photometric zero-point for J-band aperture photometry.
h_zp_ap %7.4fmagno Photometric zero-point for H-band aperture photometry.
k_zp_ap %7.4fmagno Photometric zero-point for Ks-band aperture photometry.
h_zperr_ap %6.4fmagno RMS-error of zero-point for H-band aperture photometry
k_zperr_ap %6.4fmagno RMS-error of zero-point for Ks-band aperture photometry
Source Detection Statistics
j_n_snr10 %6d --- no Number of point sources at J-band with SNR>10 (instrumental mag <=15.8)
h_n_snr10 %6d --- no Number of point sources at H-band with SNR>10 (instrumental mag <=15.1)
k_n_snr10 %6d --- no Number of point sources at Ks-band with SNR>10 (instrumental mag <=14.3)
n_ext %3d --- no Number of regular extended sources detected in scan.
Seeing Statistics
j_shape_avg %5.3f --- no J-band average seeing shape for scan. The seeing full-width at half maximum (in arcseconds) can be obtained from the approximate relation FWHM(arcseconds) = 3.13*(j_shape_avg) - 0.46.
h_shape_avg %5.3f --- no H-band average seeing shape for scan. The seeing full-width at half maximum (in arcseconds) can be obtained from the approximate relation FWHM(arcseconds) = 3.13*(h_shape_avg) - 0.46.
k_shape_avg %5.3f --- no Ks-band average seeing shape for scan. The seeing full-width at half maximum (in arcseconds) can be obtained from the approximate relation FWHM(arcseconds) = 3.13*(k_shape_avg) - 0.46.
j_shape_rms %5.3f --- no RMS-error of J-band average seeing shape.
h_shape_rms %5.3f --- no RMS-error of H-band average seeing shape.
k_shape_rms %5.3f --- no RMS-error of Ks-band average seeing shape.
j_2mrat %5.3f --- no J-band average 2nd image moment ratio.
h_2mrat %5.3f --- no H-band average 2nd image moment ratio.
k_2mrat %5.3f --- no Ks-band average 2nd image moment ratio.
Sensitivity Statistics
j_psp %6.3f --- no J-band photometric sensitivity paramater (PSP).
h_psp %6.3f --- no H-band photometric sensitivity parameter (PSP).
k_psp %6.3f --- no Ks-band photometric sensitivity parameter (PSP).
j_pts_noise %7.3f --- no The base-10 logarithm of the characteristic J-band point source scan noise, in units of log(mJy). This is the mode of the distribution of the noise-equivalent flux densities for all J-band R2-R1 detections in the scan. The noise-equivalent flux density for each detection is given by 1603x103(mJy)*1.0857/m, where m is the photometric uncertainty, in magnitudes, before correction. 1603x103 mJy was a preliminary estimate of the J-band flux-for-zero-magnitude, and it differs slightly from the final estimate of 1592x103 mJy that is described in VI.4.a. To adjust the given value of j_pts_noise for the final calibration, subtract 0.0030.
h_pts_noise %7.3f --- no The base-10 logarithm of the characteristic H-band point source scan noise, in units of log(mJy). This is the mode of the distribution of the noise-equivalent flux densities for all H-band R2-R1 detections in the scan. The noise-equivalent flux density for each detection is given by 1075x103(mJy)*1.0857/σm, where σm is the photometric uncertainty, in magnitudes, before correction. 1075x103 mJy was a preliminary estimate of the H-band flux-for-zero-magnitude, and it differs slightly from the final estimate of 1024x103 mJy that is described in VI.4.a. To adjust the given value of h_pts_noise for the final calibration, subtract 0.0211.
k_pts_noise %7.3f --- no The base-10 logarithm of the characteristic Ks-band point source scan noise, in units of log(mJy). This is the mode of the distribution of the noise-equivalent flux densities for all Ks-band R2-R1 detections in the scan. The noise-equivalent flux density for each detection is given by 698.1x103(mJy)*1.0857/m, where m is the photometric uncertainty, in magnitudes, before correction. 698.1x103 mJy was a preliminary estimate of the Ks-band flux-for-zero-magnitude, and it differs slightly from the final estimate of 666.8x103 mJy that is described in VI.4.a. To adjust the given value of k_pts_noise for the final calibration, subtract 0.0199.
j_msnr10 %5.2f --- no The J-band magnitude at which SNR=10 is achieved for this scan, estimated using the photometric sensitivity parameter j_psp and zero point offset j_zp_ap. This estimate does not take into account the effect of confusion noise in high source density regions.
h_msnr10 %5.2f --- no The H-band magnitude at which SNR=10 is achieved for this scan, estimated using the photometric sensitivity parameter h_psp and zero point offset h_zp_ap. This estimate does not take into account the effect of confusion noise in high source density regions.
k_msnr10 %5.2f --- no The Ks-band magnitude at which SNR=10 is achieved for this scan, estimated using the photometric sensitivity parameter k_psp and zero point offset k_zp_ap. This estimate does not take into account the effect of confusion noise in high source density regions.
Information on Previous Releases
cat %1d --- no Flag indicating whether the scan is included in the subset of 6x observations comprising the 2MASS 6x Catalogs and Atlas.
  • "1" indicates scan is contained in the 6x Catalogs and Atlas.
  • "0" indicates scan is not contained in the 6x Catalogs and Atlas.

[Last Updated: 2006 September 28; Davy Kirkpatrick, Roc Cutri, Tracey Evans]



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