Difference between revisions of "Analysis Work Space"
(Created page with "just starting to put down some words here, don't look too hard yet:) WISE data in the public release for BRC 27 and additional data to be released in March 2012 will be the...") |
|||
| Line 2: | Line 2: | ||
| − | WISE data in the public release for BRC 27 and additional data | + | WISE data in the public release for BRC 27 and additional data to be released in March 2012 will be the main focus of our research. We will augment this with data from the Spitzer archival data from the Infrared Array Camera (IRAC) and the Multiband Imaging Photometer for Spitzer (MIPS), Two-Micron All-Sky Survey (2MASS) and the Midcourse Space Experiment (MSX). We will re reduce Spitzer data for BRC 38 if necessary. We will also obtain ground based optical data... |
| + | |||
| + | |||
| + | We will use newly released WISE catalog data, performing manual photometric spot checks to assure validity of the data. We will perfrom photometry for Spitzer areas that are outside of existing analyzed Spitzer data. Combining this data with all existing data and what is known in the literature, we will use infrared excess to look for candidate Young Stellar Objects (YSO) and to describe the properties of known YSO. | ||
| + | |||
| + | We will use a version of the Gutermuth and Koenig color selection method to winnow down YSO candidates. | ||
Revision as of 20:33, 1 February 2012
just starting to put down some words here, don't look too hard yet:)
WISE data in the public release for BRC 27 and additional data to be released in March 2012 will be the main focus of our research. We will augment this with data from the Spitzer archival data from the Infrared Array Camera (IRAC) and the Multiband Imaging Photometer for Spitzer (MIPS), Two-Micron All-Sky Survey (2MASS) and the Midcourse Space Experiment (MSX). We will re reduce Spitzer data for BRC 38 if necessary. We will also obtain ground based optical data...
We will use newly released WISE catalog data, performing manual photometric spot checks to assure validity of the data. We will perfrom photometry for Spitzer areas that are outside of existing analyzed Spitzer data. Combining this data with all existing data and what is known in the literature, we will use infrared excess to look for candidate Young Stellar Objects (YSO) and to describe the properties of known YSO.
We will use a version of the Gutermuth and Koenig color selection method to winnow down YSO candidates.
