VizieR Online Data Catalog: Large-scale star formation in Auriga region (Pandey+, 2020)
Abstract
Optical (V and I) data for nine overlapping regions of Auriga were procured with KWFC (FOV ~2.2°x2.2°; scale 0.946arcsec/pix; Sako et al. 2012SPIE.8446E..6LS) on the 1.05-m Schmidt telescope at Kiso Observatory, Japan during the nights of 2012 December 6 and 7 and 2014 December 27. KWFC, an optical wide-field 64 megapixel imager with 4 SITe and 4 MIT Lincoln Laboratory (MIT/LL) 15μm 2Kx4K CCDs is attached to the prime focus of the Kiso Schmidt telescope. The observations were carried out in the unbinned and slow readout mode. In this mode, the readout noise is about 20 and 5-10 electrons for the SITe and MIT/LL CCDs, respectively.
To investigate the star formation in the Auriga Bubble region, we also used near-/mid-IR (NIR/MIR) data from the Two Micron All Sky Survey (2MASS; Cutri et al. 2003tmc..book.....C, Cat. II/246) and the Wide-field Infrared Survey Explorer survey (WISE; Wright et al. 2010AJ....140.1868W) archived data in addition to the optical VI data from the Kiso Schmidt telescope. (4 data files).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- March 2023
- Bibcode:
- 2023yCat..74922446P
- Keywords:
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- YSOs;
- Stars: pre-main sequence;
- Photometry: infrared;
- Optical;
- Stars: masses;
- Stars: ages;
- Models