'Foreground sources' presentation slideshows

Wideband, Next Gen, Gravitational-Wave Antennae

Wideband, Next Gen, Gravitational-Wave Antennae. APS - Atlanta - April - 2012 Rana Adhikari Caltech. OUTLINE. Gravitational Waves and the Past The LIGO Detectors The Global Network and the Indian Possibility The Future of GW Detectors & Observations. GW Sources in LIGO Band 50-1000 Hz.

595 views • 38 slides

Can dT CMB /dt be Measured?

Can dT CMB /dt be Measured?. R. V. Duncan University of New Mexico, and Caltech Quarks to Cosmos Workshop Airlie Center, May 23, 2006 Work sponsored by NASA, and by and equipment loan from Sandia National Labs

298 views • 20 slides

273 views • 18 slides

What can we learn from Gravitational Magnification with BigBOSS? Alexie Leauthaud LBNL & BCCP

What can we learn from Gravitational Magnification with BigBOSS? Alexie Leauthaud LBNL & BCCP. Kung Fu?. Cross-correlation between Background Population &. Foreground Population. Gravitational Magnification. Image credit: Joerg Colberg, Ryan Scranton, Robert Lupton, SDSS.

264 views • 18 slides