VizieR Online Data Catalog: JKs photometry of WLM galaxy carbon stars (Valcheva+, 2007)
Abstract
The observations of WLM were made in Dec. 2004 under non-photometric conditions. To estimate the foreground contamination, an additional field located 14.8' South from the center of the galaxy, far enough to eliminate the galaxy contribution, was observed in July 2006 (hereafter "clear sky" field). The near-IR imaged and spectrograph SofI (Son of ISAAC) at the ESO NTT (New Technology Telescope) on La Silla was used.
(1 data file).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- October 2007
- DOI:
- 10.26093/cds/vizier.34660501
- Bibcode:
- 2007yCat..34660501V
- Keywords:
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- Galaxies: nearby;
- Stars: carbon;
- Photometry: infrared