Service Notice

Subject: CADC/CANFAR authentication downtime — Saturday, Sept 13 (12:00–8:00 pm PT)

Essential network maintenance in Victoria will take place on Saturday, Sept 13, from 12:00–8:00 pm Pacific Time. During this window, any CADC/CANFAR service that requires authentication will be unavailable (e.g., logins to portals, token issuance, authenticated APIs/Python Client/CLI jobs). Please plan accordingly and avoid starting jobs that need credentials during the outage. Other service access may also be affected. Thank you for your patience.

Data Description

Naming Convention

The names start with "GW" (for "Group, WIRwolf") followed by a generation number (which is incremented every six months), followed by numbers indicating the RA and Dec of the group centre. For example: GW002.003.844+33.133 is and older group centred on RA=33.133 and Dec=3.844.

The group names are followed by a character(s) indicating the JHK filter.

Images

These are simple FITS files (not multi-extension FITS files) measuring about 20000 pixels by 20000 pixels or about 1 degree by 1 degree, depending on the input dither pattern, and are about 1.7 Gb in size. They have a sky level of 0 counts. They are scaled to have a photometric zero-point of 30.000 in AB magnitudes. That is to say, for each source:

AB_magnitude = -2.5 * log10(ADU) + 30.000

If you need Vega magnitudes, consult the following table, reproduced from the WIRCam filter set page.

Weight images

These are delivered with in a compressed format. To uncompress them, use CFITSIO's imcopy. For example:

imcopy GW002.003.844+33.133.J.weight.fits.fz GW002.003.844+33.133.J.weight.fits

The values of a weight map pixel is proportional to the inverse of the variance of that pixel in the main image.

Catalogues

The catalogues have a header describing the columns:

#   1 NUMBER          Running object number
#   2 X_IMAGE         Object position along x                         [pixel]
#   3 Y_IMAGE         Object position along y                         [pixel]
#   4 ALPHA_J2000     Right ascension of barycenter (J2000)           [deg]
#   5 DELTA_J2000     Declination of barycenter (J2000)               [deg]
#   6 MAG_AUTO        Kron-like elliptical aperture magnitude         [mag]
#   7 MAGERR_AUTO     RMS error for AUTO magnitude                    [mag]
#   8 MAG_BEST        Best of MAG_AUTO and MAG_ISOCOR                 [mag]
#   9 MAGERR_BEST     RMS error for MAG_BEST                          [mag]
#  10 MAG_APER        Fixed aperture magnitude vector                 [mag]
#  11 MAGERR_APER     RMS error vector for fixed aperture mag.        [mag]
#  12 A_WORLD         Profile RMS along major axis (world units)      [deg]
#  13 ERRA_WORLD      World RMS position error along major axis       [pixel]
#  14 B_WORLD         Profile RMS along minor axis (world units)      [deg]
#  15 ERRB_WORLD      World RMS position error along minor axis       [pixel]
#  16 THETA_J2000     Position angle (east of north) (J2000)          [deg]
#  17 ERRTHETA_J2000  J2000 error ellipse pos. angle (east of north)  [deg]
#  18 ISOAREA_IMAGE   Isophotal area above Analysis threshold         [pixel**2]
#  19 MU_MAX          Peak surface brightness above background        [mag * arcsec**(-2)]
#  20 FLUX_RADIUS     Fraction-of-light radii                         [pixel]
#  21 FLAGS           Extraction flags

All magnitudes are on the AB system. The aperture diameter for MAG_APER is 6.28 times the FWHM of the image. It should be (on average) the same as MAG_AUTO for point sources, as discussed in the photometry section of the stacking procedure.

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