ALMA OBSERVATIONS OF SPT-DISCOVERED, STRONGLY LENSED, DUSTY, STAR-FORMING GALAXIES
YD Hezaveh, DP Marrone, CD Fassnacht, JS Spilker, JD Vieira, JE Aguirre, KA Aird, M Aravena, MLN Ashby, M Bayliss, BA Benson, LE Bleem, M Bothwell, M Brodwin, JE Carlstrom, CL Chang, SC Chapman, TM Crawford, AT Crites, C De Breuck Show all
Astrophysical Journal | IOP PUBLISHING LTD | Published : 2013
Awarded by National Science Foundation
Awarded by NASA from the Space Telescope Science Institute
Awarded by Science and Technology Facilities Council
Awarded by Direct For Mathematical & Physical Scien
The SPT is supported by the National Science Foundation through grant ANT-0638937, with partial support through PHY-1125897, the Kavli Foundation, and the Gordon and Betty Moore Foundation. This paper makes use of the following ALMA data: ADS/JAO. ALMA #2011.0.00957. S and #2011.0.00958. S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Partial support for this work was provided by NASA through grant HST-GO-12659 from the Space Telescope Science Institute and an award for Herschel analysis issued by JPL/Caltech for OT2_jvieira_5. Work at McGill is supported by NSERC, the CRC program, and CIfAR. Y.D.H. acknowledges the support of FQRNT through International Training Program and Doctoral Research scholarships. T.R.G. acknowledges support from the Science and Technologies Facilities Council.