Cosmic Surveys – Rich Kron - Fermilab Center for Particle ...
Cosmic Surveys – Rich Kron - Fermilab Center for Particle ... Cosmic Surveys – Rich Kron - Fermilab Center for Particle ...
This high impact is due to several factors: freely accessible database (dr7: arXiv 0812.0649) processing and calibrations: science-ready data uniform and high-quality data large footprint on the sky overlap with other major surveys (2MASS, GALEX) data useful across many fields of astronomy ----------way the telescope is used SDSS Collaboration as a scientific team
SDSS-II (2005 - 2008) extension survey: same instrumentation, same target-selection for Legacy, improvements to processing software for Legacy. Legacy required 1/3 of the total time to “fill the gap.” The other 1/3 and 1/3 were for:
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- Page 23 and 24: Zekser, K. et al. 2006 ApJ 640, 639
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This high impact is due to several factors:<br />
freely accessible database (dr7: arXiv 0812.0649)<br />
processing and calibrations: science-ready data<br />
uni<strong>for</strong>m and high-quality data<br />
large footprint on the sky<br />
overlap with other major surveys (2MASS, GALEX)<br />
data useful across many fields of astronomy<br />
----------way<br />
the telescope is used<br />
SDSS Collaboration as a scientific team
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