Near-infrared survey of the Magellanic Clouds with IRSF/SIRIUS

Details Near-infrared survey of the Magellanic Clouds with IRSF/SIRIUS Near-infrared survey of the Magellanic Clouds with IRSF/SIRIUS

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005asthe..98..219k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 98, No. 4, p. 219 - 222 (2005)

Astronomy and Astrophysics

Astronomy

Infrared Surveys, Magellanic Clouds

Scientific paper

We are surveying the Large Magellanic Cloud and the Small Magellanic Cloud in the near-infrared wavelengths, J, H, and Ks bands. The 10σ limiting magnitudes of the survey are J~19, H~18, and Ks~17 mag, which correspond to the magnitudes of Herbig Ae/Be stars with masses as low as ~3Msolar in the Clouds. The photometric and positional accuracy of the survey will be 0.03 mag and 0.1 arcsec, respectively. We will publish a point source catalog of the Magellanic Clouds at the end of 2005.

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