Journal article

The nature of the [C II] emission in dusty star-forming galaxies from the SPT survey

B Gullberg, C De Breuck, JD Vieira, A Weiss, JE Aguirre, M Aravena, M Bethermin, CM Bradford, MS Bothwell, JE Carlstrom, SC Chapman, CD Fassnacht, AH Gonzalez, TR Greve, Y Hezaveh, WL Holzapfel, K Husband, J Ma, M Malkan, DP Marrone Show all

ArXiv e-prints | OXFORD UNIV PRESS | Published : 2015

University of Melbourne Researchers

Grants

Awarded by US National Science Foundation


Awarded by National Science Foundation


Awarded by NSF Physics Frontier Center


Awarded by Gordon and Betty Moore Foundation


Awarded by Science and Technology Facilities Council


Funding Acknowledgements

This publication is based on data acquired with the APEX. APEX is a collaboration between the Max-Planck-Institut fur Radioastronomie, the European Southern Observatory, and the Onsala Space Observatory. This paper makes use of the following ALMA data: ADS/JAO. ALMA#2011.0.00957.S, ADS/JAO.ALMA#2011.0.00958.S and ADS/JAO. ALMA#2012.1.00844.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 Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. The ATCA is part of the Australia Telescope National Facility which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. This research has made use of the NED which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research has made use of NASA's Astrophysics Data System Bibliographic ServicesThis material is based on work supported by the US National Science Foundation under grant no. AST-1312950. The SPT is supported by the National Science Foundation through grant PLR-1248097. Partial support is also provided by the NSF Physics Frontier Center grant PHY-1125897 to the Kavli Institute of Cosmological Physics at the University of Chicago, the Kavli Foundation, and the Gordon and Betty Moore Foundation grant GBMF 947.