High- and intermediate-mass YSOs in the LMC (Gruendl+, 2009)

Details High- and intermediate-mass YSOs in the LMC (Gruendl+, 2009) High- and intermediate-mass YSOs in the LMC (Gruendl+, 2009)

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..21840172g&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/184/172. Originally published in: 2009ApJS..184..172G

Computer Science

Photometry: Infrared, Magellanic Clouds, Ysos, Cross Identifications

Scientific paper

The LMC has been observed by the Spitzer Space Telescope using the Infrared Array Camera (IRAC) and the Multiband Imaging Photometer for Spitzer (MIPS). We have obtained complementary optical and near-IR imaging observations using the Blanco 4m telescope at the Cerro Tololo Inter-American Observatory for selected regions throughout the LMC. The MOSAICII camera was used to obtain I-band observations on 2006 February 2-8. The IR Side Port Imager (ISPI) was used to obtain J- and Ks-band observations during three observing runs in 2005 November, 2006 November, and 2007 February.
(9 data files).

Affiliated with

Also associated with

No associations

Rating

High- and intermediate-mass YSOs in the LMC (Gruendl+, 2009) 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 High- and intermediate-mass YSOs in the LMC (Gruendl+, 2009), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High- and intermediate-mass YSOs in the LMC (Gruendl+, 2009) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1427712