'Alma evla' diaporamas de présentation

Post-processing

Post-processing. Bryan Butler, for Joe McMullin. Mission: Primary purpose is to provide facilities for post-observational scientific reduction of ALMA and EVLA data Facilities must be: Scientifically complete/correct Robust Acceptably fast Easy to use

398 views • 26 slides

CASA

531 views • 25 slides

Edo Berger Harvard University

The Host Galaxies of High-Redshift GRBs. Edo Berger Harvard University. Outline. 1. GRBs at z<1: Is there a low-metallicity bias?. 2. The ISM of high-redshift galaxies. 3. DLA counterparts & the M-Z relation at z>2. Spitzer stack. Long GRBs Hosts: Metallicity?. metallicity.

400 views • 17 slides