Direct Measurement of the H i-halo Mass Relation through Stacking
2020
We thank the anonymous reviewer for the helpful comments
that improve the presentation of this paper. We acknowledge
the work of the entire ALFALFA team for observing, flagging,
and performing signal extraction. We thank Benedikt Diemer
for providing the gas properties from the Illustris and
IllustrisTNG simulations. We also thank Carlton Baugh, Cheng
Li, Zheng Zheng, Claudia Lagos, Garima Chauhan, and Adam
Stevens for helpful discussions.
This work is supported by the National Key R&D Program
of China (grant No. 2018YFA0404503), National Science
Foundation of China (Nos. 11773049, 11833005, 11828302,
11922305), and Spanish Science Ministry “Centro de Excelencia
Severo Ochoa” program under grant SEV-2017-0709. M.G.J.
is supported by a Juan de la Cierva formacion fellowship
(FJCI-2016-29685). M.G.J. also acknowledges support from the
grants AYA2015-65973-C3-1-R and RTI2018-096228-B-C31
(MINECO/FEDER, UE). M.P.H. acknowledges support from
NSF/AST-1714828 and the Brinson Foundation. J.F. acknowledges the support by the Youth innovation Promotion Association
CAS and Shanghai Committee of Science and Technology
grant (No.19ZR1466700). This research was supported by the
Munich Institute for Astro- and Particle Physics (MIAPP), which
is funded by the Deutsche Forschungsgemeinschaft (DFG,
German Research Foundation) under Germany’s Excellence
Strategy C EXC-2094 C 390783311.
Funding for the SDSS and SDSS-II has been provided by the
Alfred P. Sloan Foundation, the Participating Institutions,
the National Science Foundation, the U.S. Department of
Energy, the National Aeronautics and Space Administration,
the Japanese Monbukagakusho, the Max Planck Society, and
the Higher Education Funding Council for England. The SDSS
website is http://www.sdss.org/.
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