This page documents some of the main updates to the Legacy Surveys since Data Release 9.
General changes
DR10 only contains updates for the
southpart of the Legacy Surveys from new imaging with DECam. Northern areas can be obtained from DR9 (see, e.g., the status page).The sweep files are now partitioned into 5° x 5° areas rather than 10° x 5° areas.
Changes for optical data
Multiple \(i\hbox{-}\mathrm{band}\) quantities have been added to the Tractor catalogs and the sweep files.
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Gaia quantities included in files and catalogs are now drawn from Gaia EDR3.
Note, though, that the astrometric solution for DR10 was still calculated using positions and proper motions from Gaia DR2.
The
MASKBITSbitmask is now 32-bit rather than 16-bit, as a new bit calledSUB_BLOBwas added. This bit is described on the DR10 bitmasks page under MASKBITS.The
CCD_CUTSbitmask is now 64-bit rather than 32-bit, as two new bits calledPHRMS_S7andDEPTH_CUT_2were added. These bits are described on the DR10 bitmasks page under CCD_CUTS.-
The Tractor catalogs contain a new per-band quantity called
ngood_xwherexis one of \(g\), \(r\), \(i\) or \(z\). These quantities record the number of good (unmasked) images that contribute to a source in a particular band at a particular pixel-location. Prior to DR9, onlynobs_x(the total number of images that contributed to a source in each band) were recorded in the Tractor catalogs, which created an inconsistency with the "nexp" pixel-maps in the image stacks (which only record the number of good images). So,ngood_xis recorded to allow a direct mapping between the number of good images in the Tractor catalogs and image stacks.As an example of the difference, for saturated sources one would expect
ngood_xand the "nexp" pixel maps to be zero, butnobs_xto correspond to the total number of exposures that contributed to the source.The addition of
ngood_xfixes a known issue from DR9.
Changes for WISE data
The WISE imaging has been updated to include observations through the 7th year of the NEOWISE W1/W2 data.
The potential number of unWISE epochs has been expanded for the WISE light curves (e.g. columns such as
lc_flux_w1in the Tractor catalogs can now have up to 17 entries).