The Star Formation in Nearby Clouds (SFiNCs) project is aimed at providing a detailed study of the young stellar populations and of star cluster formation in the nearby 22 star-forming regions (SFRs) for comparison with our earlier MYStIX survey of richer, more distant clusters. As a foundation for the SFiNCs science studies, here, homogeneous data analyses of the Chandra X-ray and Spitzer mid-infrared archival SFiNCs data are described, and the resulting catalogs of over 15300 X-ray and over 1630000 mid-infrared point sources are presented. On the basis of their X-ray/infrared properties and spatial distributions, nearly 8500 point sources have been identified as probable young stellar members of the SFiNCs regions. Compared to the existing X-ray/mid-infrared publications, the SFiNCs member list increases the census of YSO members by 6%-200% for individual SFRs and by 40% for the merged sample of all 22 SFiNCs SFRs.
Cone search capability for table J/ApJS/229/28/table1 (Star Formation in Nearby Clouds (SFiNCs) star-forming regions)
Cone search capability for table J/ApJS/229/28/table2 (Log of SFiNCs Chandra-ACIS observations)
Cone search capability for table J/ApJS/229/28/xsources (SFiNCs X-ray sources properties (tables 3 and 4))
Cone search capability for table J/ApJS/229/28/table5 (Log of SFiNCs Spitzer-IRAC observations)
Cone search capability for table J/ApJS/229/28/table6 (SFiNCs IRAC sources and photometry)
Cone search capability for table J/ApJS/229/28/spcms (SFiNCs probable cluster members: IR photometry, X-ray and other properties (tables 7 and 8))