Molecular gas masses of gamma-ray burst host galaxies

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[1] [1,Michalowski, Michal J.
[2] Karska, A.
[3] Rizzo, J.R.
[4] Baes, M.
[5] Castro-Tirado, A.J.
[6] Hjorth, J.
[7] Hunt, L.K.
[8] 9,Kamphuis, P.
[9] Koprowski, M.P.
[10] Krumholz, M.R.
[11] Malesani, D.
[12] Nicuesa Guelbenzu, A.
[13] 7,Rasmussen, J.
[14] Rossi, A.
[15] Schady, P.
[16] Sollerman, J.
[17] Van Der Werf, P.
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| 1600年 / EDP Sciences卷 / 617期
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Acknowledgements. We thank Joanna Baradziej and our referee for help with improving this paper; Per Bergman; Carlos De Breuck; Palle Møller and Katha-rina Immer for help with the APEX observations; and Claudia Marka for help with IRAM 30 m observations. M.J.M. acknowledges the support of the National Science Centre; Poland through the POLONEZ grant 2015/19/P/ST9/04010; and the UK Science and Technology Facilities Council; this project has received funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement No. 665778. A.K. acknowledges support from the Polish National Science Center grants 2014/15/B/ST9/02111and 2016/21/D/ST9/01098. J.R.R. acknowledges the support from project ESP2015-65597-C4-1-R (MINECO/FEDER). A.J.C.T. acknowledges support from the Spanish Ministry Project AYA2015-71718-R. J.H. was supported by a VILLUM FONDEN Investigator grant (project number 16599). L.K.H. acknowledges funding from the INAF PRIN-SKA program 1.05.01.88.04. M.R.K. acknowledges support from the Australian government through the Australian Research Council’s Discovery Projects funding scheme (project DP160100695). Based on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere under ESO programmes 096.D-0280(A); 096.F-9302(A); and 097.F-9308(A). This publication is based on data acquired with the Atacama Pathfinder Experiment (APEX). APEX is a collaboration between the Max-Planck-Institut fur Radioastronomie; the European Southern Observatory; and the Onsala Space Observatory. This work is based on observations carried out under project number 172-16 with the IRAM 30 m telescope. IRAM is supported by INSU/CNRS (France); MPG (Germany) and IGN (Spain). This research has made use of the GHostS database (http://www.grbhosts.org); which is partly funded by Spitzer/NASA grant RSA Agreement No. 1287913; the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory; California Institute of Technology; under contract with the National Aeronautics and Space Administration; SAOImage DS9; developed by Smithsonian Astrophysical Observatory (Joye & Mandel 2003); and the NASA’s Astrophysics Data System Bibliographic Services;
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