Journal article

Red and Reddened: Ultraviolet through Near-infrared Observations of Type Ia Supernova 2017erp

Peter J Brown, Griffin Hosseinzadeh, Saurabh W Jha, David Sand, Ethan Vieira, Xiaofeng Wang, Mi Dai, Kyle G Dettman, Jeremy Mould, Syed Uddin, Lifan Wang, Iair Arcavi, Joao Bento, Chris R Burns, Tiara Diamond, Daichi Hiramatsu, D Andrew Howell, EY Hsiao, GH Marion, Curtis McCully Show all

The Astrophysical Journal | IOP PUBLISHING LTD | Published : 2019

University of Melbourne Researchers

Grants

Awarded by NASA from the Space Telescope Science Institute


Awarded by NASA


Awarded by NASA's Astrophysics Data Analysis Program


Awarded by NSF


Awarded by Gemini Observatory


Awarded by US Department of Energy


Awarded by Australian Research Council


Awarded by Chinese Academy of Sciences President's International Fellowship Initiative grant


Awarded by National Science Foundation


Funding Acknowledgements

Support for program #14665 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. The Swift Optical/Ultraviolet Supernova Archive (SOUSA) is supported by NASA's Astrophysics Data Analysis Program through grant NNX13AF35G. We thank N. Suntzeff and K. Krisciunas for helpful comments and support during the process of analysis and writing. We acknowledge the work of Jamison Burke, Shuhrat A. Ehgamberdiev, Han Lin, Jun Mo, Liming Rui, and Lingzhi Wang in obtaining some of this data. This work made use of public data in the Swift data archive and the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. This work makes use of observations from the Las Cumbres Observatory network and the Global Supernova Project. D.A.H., C.M., and G.H. are supported by NSF grant AST 1313484. Research by D.J.S. is supported by NSF grants AST-1821967, 1821987, 1813708, and 1813466. Based on observations obtained at the Gemini Observatory under programs GS-2017A-Q-33 (PI: Sand). Gemini is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the NSF (United States), the National Research Council (Canada), CONICYT (Chile), Ministerio de Ciencia, Tecnologia e Innovacion Productiva (Argentina), and Ministerio da Ciencia, Tecnologia e Inovacao (Brazil). The data were processed using the Gemini IRAF package. We thank the queue service observers and technical support staff at Gemini Observatory for their assistance. Some of the observations reported in this paper were obtained with the Southern African Large Telescope (SALT). This supernova research at Rutgers University is supported by NASA grant NNG17PX03C and US Department of Energy award DE-SC0011636. A.J.R. has been supported by the Australian Research Council through grant numbers CE110001020 and FT170100243. Syed A Uddin was supported by the Chinese Academy of Sciences President's International Fellowship Initiative grant No. 2016PM014. E.Y. H. acknowledges the support provided by the National Science Foundation under grant No. AST-1613472.