Overview of New Results from the Stripe 82 Equatorial Field

Details Overview of New Results from the Stripe 82 Equatorial Field Overview of New Results from the Stripe 82 Equatorial Field

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21932406l&link_type=abstract

American Astronomical Society, AAS Meeting #219, #324.06

Astronomy and Astrophysics

Astronomy

Scientific paper

Stripe 82 is emerging as one of the new premier survey fields with an area of over 100 deg^2 and an impressive array of multi-wavelength observations already in hand or in progress (e.g., SDSS ugriz imaging, BOSS spectroscopy of >40,000 galaxies and QSOs, GALEX UV imaging, 1.4 and 3 GHz radio coverage, CFHT i<23.7, J and K imaging from CFHT and VISTA). First, I will give an overview of these data sets, including several new Stripe 82 surveys such as the "CFHT Stripe 82 Survey": a new 170 deg^2 CFHT i-band survey that has been analysed with the state-of-the-art weak lensing quality data processing and shear measurement pipeline from CFHTLenS. Next, I will highlight some new results from Stripe 82 including BOSS galaxy mass functions to z=0.7, weak lensing, new cluster catalogs to z=0.7, and the luminosity dependance of QSO clustering.

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