Spitzer Deep Wide-Field Survey Light Curve Catalog

Description

The Spitzer Deep, Wide-Field Survey (SDWFS) is a four-epoch infrared survey of 10 square degrees in the Boötes field of the NOAO Deep Wide-Field Survey using the IRAC instrument on the Spitzer Space Telescope. SDWFS, a Spitzer Cycle 4 Legacy project, occupies a unique position in the area-depth survey space defined by other Spitzer surveys. The four epochs that make up SDWFS permit - for the first time - the selection of infrared-variable and high proper motion objects over a wide field on timescales of years. Because of its large survey volume, SDWFS is sensitive to galaxies out to z ~ 3 with relatively little impact from cosmic variance for all but the richest systems. The SDWFS data sets will thus be especially useful for characterizing galaxy evolution beyond z ~ 1.5.\n\nThe SDWFS Light Curve Catalog presents the 3.6 and 4.5 micron magnitudes for each SDWFS source in each of the four epochs. For more details see Kozlowski et al. (2010).

Resources

Name Format Description Link
21 sdwfs_lcurve_colDescriptions.html https://irsa.ipac.caltech.edu/data/SPITZER/SDWFS/gator_docs/sdwfs_lcurve_colDescriptions.html
5 https://irsa.ipac.caltech.edu/SCS?table=sdwfs_lcurve&
5 https://irsa.ipac.caltech.edu%2FSCS%3Ftable%3Dsdwfs_lcurve%26
5 https://irsa.ipac.caltech.edu%2Fdata%2FSPITZER%2FSDWFS%2Fgator_docs%2Fsdwfs_lcurve_colDescriptions.html
5 https://heasarc.gsfc.nasa.gov/xamin/vo/cone?showoffsets&table=a2led&
21 a2led.html https://heasarc.gsfc.nasa.gov/W3Browse/all/a2led.html
21 xmmcphotz.html https://heasarc.gsfc.nasa.gov/W3Browse/all/xmmcphotz.html
5 https://heasarc.gsfc.nasa.gov/xamin/vo/cone?showoffsets&table=xmmcphotz&
21 sdwfs_lcurve_colDescriptions.html https://irsa.ipac.caltech.edu/data/SPITZER/SDWFS/gator_docs/sdwfs_lcurve_colDescriptions.html
5 https://irsa.ipac.caltech.edu/SCS?table=sdwfs_lcurve&

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