The Young Stellar Object VARiability (YSOVAR) Spitzer Space Telescope observing
program obtained the first extensive mid-infrared (IRAC 3.6 and 4.5 micron) time
series photometry of the Orion Nebula Cluster plus smaller fields in 11 other
star-forming cores (AFGL 490, NGC 1333, Mon R2, GGD 12-15, NGC 2264, L1688,
Serpens Main, Serpens South, IRAS 20050+2720, IC 1396A, and Ceph C).
There are ~29,000 unique objects with light curves in either or both IRAC
channels in the YSOVAR data set. YSOVAR is a sister project to the Coordinated
Synoptic Investigation of NGC 2264 (CSI
2264; Cody et al. 2014).
Initial YSOVAR results were described in Morales-Calderon et
al. (2011).
Rebull et al.
(2014) describes the details of target selection, data reduction, and other
conventions established for this project.
If you use YSOVAR data, please cite both the journal article Rebull et al.
(2014) and the dataset Digital Object Identifier (DOI): 10.26131/IRSA518.
Jump to documentation.
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YSOVAR Overview
YSOVAR Primary Data Access
YSOVAR Catalogs