SPITZER-SWIRE Catalog : SWIRE Final Data Release Aperture-Corrected Fluxes as per SWIRE Data Release Documents by Surace+ (2005) and Surace+ (in prep) The column indices below refer to *-full-spitzer.fits.gz legacy catalogs, but *-full-spitzer-all.fits.gz catalogs now provide a more comprehensive set of quantities and should be used whenever possible for any new work. More in general *-full-spitzer.fits.gz catalogs are now mildly deprecated. IRAC aperture radii [arcsec] (Map Pixel Size = 0.6 arcsec) ap1 = 1.4 ap2 = 1.9 ap3 = 2.9 ap4 = 4.1 ap5 = 5.8 MIPS 24 aperture radii [arcsec] (Map Pixel Size = 1.2 arcsec) ap1 = 3.00 ap2 = 5.25 ap3 = 7.50 ap4 = 10.5 ap5 = 15.0 MIPS 70 & 160 aperture radii [arcsec] (Map Pixel Size = 4 & 8 arcsec) Aperture-Radius-1 = 3.0 Aperture-Radius-2 = 5.0 Aperture-Radius-3 = 7.1 Aperture-Radius-4 = 10.0 Aperture-Radius-5 = 12.0 Aperture-Radius-6 = 15.0 Aperture-Radius-7 = 20.0 Aperture-Radius-8 = 30.0 1) Index Spitzer 2) RA Spitzer 3) Dec Spitzer 4) tile : tile ID number containing the source 5) 3.6 micron ap2 flux muJy 6) 4.5 micron ap2 flux muJy 7) 5.8 micron ap2 flux muJy 8) 8.0 micron ap2 flux muJy 9) 3.6 micron ap2 flux error muJy 10) 4.5 micron ap2 flux error muJy 11) 5.8 micron ap2 flux error muJy 12) 8.0 micron ap2 flux error muJy 13) 3.6 micron Kron flux muJy 14) 4.5 micron Kron flux muJy 15) 5.8 micron Kron flux muJy 16) 8.0 micron Kron flux muJy 17) 3.6 micron Kron flux error muJy 18) 4.5 micron Kron flux error muJy 19) 5.8 micron Kron flux error muJy 20) 8.0 micron Kron flux error muJy 21) Stellarity prob 3.6 : stellarity index at each IRAC band. The single digit stellarity indices generated by the SExtractor software package, one per IRAC band. 22) Stellarity prob 4.5 23) Stellarity prob 5.8 24) Stellarity prob 8.0 25) SNR of ap2 3.6 flux 26) SNR of ap2 4.5 flux 27) SNR of ap2 5.8 flux 28) SNR of ap2 8.0 flux 29) Index MIPS 24 micron 30) RA MIPS 24 micron 31) Dec MIPS 24 micron 32) Index MIPS 70 micron 33) RA MIPS 70 micron 34) Dec MIPS 70 micron 35) Index MIPS 160 micron 36) RA MIPS 160 micron 37) Dec MIPS 160 micron 38) MIPS 24 micron ap1 flux muJy 39) MIPS 24 micron ap2 flux muJy 40) MIPS 24 micron ap3 flux muJy 41) MIPS 24 micron ap4 flux muJy 42) MIPS 24 micron ap5 flux muJy 43) *** NOW MIPS 24 micron ap2 flux muJy - used to be : MIPS 24 micron PRF-fitting flux muJy 44) *** NOW MIPS 24 micron ap2 flux error muJy - used to be : MIPS 24 micron PRF-fitting flux error muJy 45) *** NOW MIPS 24 micron ap2 SNR - used to be : MIPS 24 micron PRF-fitting SNR : SNR of Kron flux 46) *** NOW EMPTY - used to be : MIPS 24 micron ap2 SNR : SNR of MIPS 24 micron ap2 flux 47) *** NOW EMPTY - used to be : MIPS 24 micron PRF-fitting status (>0: successful; <0: unsuccessful) 48) *** NOW EMPTY - used to be : MIPS 24 micron chi2 per DOF of PRF-fitting 49) MIPS 24 micron vs IRAC Distance arcsec 50) MIPS 24 micron Reliability 51) MIPS 70 micron PRF-fitting flux mJy 52) MIPS 70 micron PRF-fitting flux error mJy 53) MIPS 70 micron SNR 54) MIPS 70 micron vs MIPS 24 micron Distance arcsec 55) MIPS 70 micron Reliability 56) MIPS 160 micron PRF-fitting flux mJy 57) MIPS 160 micron PRF-fitting flux error mJy 58) MIPS 160 micron SNR 59) MIPS 160 micron vs MIPS 24 micron Distance arcsec 60) MIPS 160 micron Reliability 61) extended source flag IRAC 3.6: source extension flag at each IRAC band and MIPS 24. A value of -1 indicates a definitely point-like object, a value of 2 indicates an object that is clearly extended, a value of 1 indicates an idea that might be extended, and a value of 0 is indeterminate. In general, objects with this flag set equal to one will have poor aperture photometry, and the Kron flux will be preferable. 62) extended source flag IRAC 4.5 micron 63) extended source flag IRAC 5.8 micron 64) extended source flag IRAC 8.0 micron 65) NOW EMPTY - used to be : extended source flag MIPS 24 micron 66) Catalog flag: Spitzer Catalog Reliability Flag cat = 0 = duplicates, tile intersection and edge of fields (UNRELIABLE) cat = 1 = full coverage and moderately reliable cat = 2 = full coverage and fully reliable 67) NOW EMPTY - used to be : 2mass source flag a flag used to identify sources which lie close to a bright 2MASS star (flag value set to 1). If a source is found to lie within a given radius of a bright star then there is a possibility that in one or more bands its flux may be affected by artifacts from the star, or it may have missed detection altogether due to the exclusion zone of the SExtractor software. Caution should therefore be used in interpreting the spectral energy distribution of such a source.