JKs photometry of WLM galaxy carbon stars (Valcheva+, 2007)

Details JKs photometry of WLM galaxy carbon stars (Valcheva+, 2007) JKs photometry of WLM galaxy carbon stars (Valcheva+, 2007)

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34660501v&link_type=abstract

VizieR On-line Data Catalog: J/A+A/466/501. Originally published in: 2007A&A...466..501V

Physics

Galaxies: Nearby, Stars: Carbon, Photometry: Infrared

Scientific paper

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).

Affiliated with

Also associated with

No associations

Rating

JKs photometry of WLM galaxy carbon stars (Valcheva+, 2007) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with JKs photometry of WLM galaxy carbon stars (Valcheva+, 2007), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and JKs photometry of WLM galaxy carbon stars (Valcheva+, 2007) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-955604