Views
3 years ago

Panchroma+c Proper+es of Galaxies in Wide-‐Field Op+cal ...

Panchroma+c Proper+es of Galaxies in Wide-‐Field Op+cal ...

Evolu)on

Evolu)on of the HI (or not?) Redshift430.0 0.2 0.4 0.6 0.8 1.0 2.0 3.0 4.0Star-formation history(Hopkins & Beacom 2006)Stellar density(Wilkins et al. 2008)Gas densityZwaan et al. (2005, HI blind)Lah et al. (2009, 21cm stacking)Rao et al. (2006, MgII Sytems)Prochaska et al. (2009, DLAs)DINGO direct HI detectionsDINGO+AAT z stacking0.20.1520.110.050Deep Ultra-deep (low) Ultra-deep (high)0 2 4 6 8 10 12Lookback time (Gyrs)0

ASKAP (Australian Square Kilometer Array Pathfinder) A$150 million investment to construct unique radio facility to study gas in galaxies

Galaxy Assembly and AGN Growth with the Hubble Wide Field ...
• Integrated C-MOS scanner • Applicable for wide area network ...
Wide-field study of galaxies at z=1-2 Naoyuki Tamura - AstroGrid wiki
Radio Quiet AGN: Black Hole & Host Galaxy Proper es
„Wide-band Investigations of Electromagnetic Field in Space“
Note : In the C/A field, 'C' - WordPress – www.wordpress.com
Cal Poly Geology Club Death Valley Field Trip – 2004
Wide-field performance gradient at a mid-latitude site and at Dome C
Focal Reducer/Wide-Field Corrector for the C. E. Kenneth Mees ...
Star-Forming Galaxies at z ~ 2 in the Hubble Ultra Deep Field ∗
Symphony No. 7 in C Major, Op. 60 “Leningrad” - Detroit Symphony ...
Steinheil 2“ Wide-field Eyepiece (35mm/67°) Made in ... - DD1US
Geomagnetic field variations in India – an analysis by Fuzzy c ... - IGU
C ap ¤¥¦¨ D ivers s¦ip s de f¨()i (es)i ¤¥(dri)as La ecuaci éon de ...
Approved May 19, 2005 Field Marshal – Chris Rines - 495th R/C ...
Field Service Procedure – C-Band Radar Transmit Reject Filter Kit ...