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- publication . Article . 2019Open AccessAuthors:MacAulay, E.; Nichol, R. C.; Bacon, D.; Brout, D.; Davis, T. M.; Zhang, B.; Bassett, B. A.; Scolnic, D.; Möller, A.; D Andrea, C. B.; ...Publisher: eScholarship, University of CaliforniaProject: EC | COSMICDAWN (306478), NSF | Prompt Discovery and Inve... (1211916), NSF | Collaborative Research: T... (1138766), EC | TESTDE (291329), EC | SPCND (615929), NSF | Next-Generation Supernova... (1815935), EC | COGS (240672), NSF | The Progenitors and Explo... (1518052)
We present an improved measurement of the Hubble constant (H0) using the ‘inverse distance ladder’ method, which adds the information from 207 Type Ia supernovae (SNe Ia) from the Dark Energy Survey (DES) at redshift 0.018 < z < 0.85 to existing distance measurements of...
- publication . Preprint . Article . 2020Open Access EnglishAuthors:Benjamin E. Stahl; W. Zheng; T. de Jaeger; Adam G. Riess; Adam G. Riess; Lluís Galbany; A. V. Filippenko;Project: NSF | Collaborative Research: T... (1138766), EC | TESTDE (291329), EC | SNDTD (839090), NSF | The Carnegie Supernova Pr... (1008343), EC | COSMICDAWN (306478), NSF | Prompt Discovery and Inve... (1211916), EC | COGS (240672), NSF | Pan-STARRS1: Operations; ... (1238877), NSF | Measuring the Universe wi... (0306969), NSF | The Carnegie Supernova Pr... (0607438)
Progressive increases in the precision of the Hubble-constant measurement via Cepheid-calibrated Type Ia supernovae (SNe Ia) have shown a discrepancy of $\sim 4.4\sigma$ with the current value inferred from Planck satellite measurements of the cosmic microwave backgroun...
- publication . Article . Preprint . 2020Open Access EnglishAuthors:B. Flaugher; M. Carrasco Kind; M. Carrasco Kind; Jochen Weller; Felipe Menanteau; Felipe Menanteau; Enrique Gaztañaga; Santiago González-Gaitán; Eric Suchyta; J. De Vicente; ...Publisher: HAL CCSDProject: EC | SNDTD (839090), NSF | The Carnegie Supernova Pr... (0607438), NSF | Prompt Discovery and Inve... (1211916), EC | SPCND (615929), EC | TESTDE (291329), NSF | Measuring the Universe wi... (0306969), NSF | The Carnegie Supernova Pr... (1008343), EC | COGS (240672), NSF | Pan-STARRS1: Operations; ... (1238877), EC | COSMICDAWN (306478),...
Despite vast improvements in the measurement of the cosmological parameters, the nature of dark energy and an accurate value of the Hubble constant (H$_0$) in the Hubble-Lema\^itre law remain unknown. To break the current impasse, it is necessary to develop as many inde...
- publication . Preprint . Article . Research . 2018Open Access EnglishAuthors:M. Smith; C. B. D’Andrea; M. Sullivan; A. Möller; R. C. Nichol; R. C. Thomas; A. G. Kim; M. Sako; F. J. Castander; A. V. Filippenko; ...Publisher: HAL CCSDProject: NSF | Collaborative Research: T... (1138766), EC | COSMICDAWN (306478), EC | TESTDE (291329), NSF | Prompt Discovery and Inve... (1211916), EC | SPCND (615929), NSF | Next-Generation Supernova... (1815935), NSF | The Progenitors and Explo... (1518052), NSF | Characterizing the Physic... (1517742), EC | COGS (240672)
Comment: 25 pages, 14 figures, 8 tables. Submitted to AJ
- publication . Article . Other literature type . Preprint . 2019Open AccessAuthors:Richard Kessler; P. Andersen; P. Andersen; R. J. Foley; Daniela Carollo; J. Calcino; E. Swann; K. Honscheid; Robert A. Gruendl; Robert A. Gruendl; ...Project: EC | TESTDE (291329), NSF | Prompt Discovery and Inve... (1211916), NSF | Characterizing the Physic... (1517742), EC | COGS (240672), NSF | Physics Frontier Center a... (1125897), EC | COSMICDAWN (306478), NSF | Collaborative Research: T... (1138766)
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