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4 research outcomes, page 1 of 1
  • publication . Preprint . Research . Article . 2018
    Open Access English
    Authors:
    D Andrea, C. B.; Smith, M.; Sullivan, M.; Nichol, R. C.; Thomas, R. C.; Kim, A. G.; Möller, A.; Sako, M.; Castander, F. J.; Filippenko, A. V.; ...
    Publisher: HAL CCSD
    Project: NSF | Characterizing the Physic... (1517742), NSF | Collaborative Research: T... (1138766), NSF | Prompt Discovery and Inve... (1211916), NSF | Next-Generation Supernova... (1815935), EC | SPCND (615929), NSF | The Progenitors and Explo... (1518052), EC | COSMICDAWN (306478), EC | TESTDE (291329), EC | COGS (240672)

    Comment: 25 pages, 14 figures, 8 tables. Submitted to AJ

  • publication . Article . 2019
    Open Access English
    Authors:
    MacAulay, E; Nichol, RC; Bacon, D; Brout, D; Davis, TM; Zhang, B; Bassett, BA; Scolnic, D; Möller, A; D'Andrea, CB; ...
    Project: NSF | Collaborative Research: T... (1138766), NSF | Prompt Discovery and Inve... (1211916), NSF | Next-Generation Supernova... (1815935), NSF | The Progenitors and Explo... (1518052), EC | SPCND (615929), EC | COSMICDAWN (306478), EC | TESTDE (291329), EC | COGS (240672)

    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 . 2020
    Open Access English
    Authors:
    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), NSF | Prompt Discovery and Inve... (1211916), NSF | The Carnegie Supernova Pr... (0607438), NSF | The Carnegie Supernova Pr... (1008343), NSF | Measuring the Universe wi... (0306969), NSF | Pan-STARRS1: Operations; ... (1238877), EC | COGS (240672), EC | TESTDE (291329), EC | SNDTD (839090), EC | COSMICDAWN (306478)

    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 . 2020
    Open Access English
    Authors:
    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: Oxford University Press
    Project: NSF | The Carnegie Supernova Pr... (0607438), EC | SPCND (615929), NSF | Collaborative Research: T... (1138766), NSF | Prompt Discovery and Inve... (1211916), NSF | Measuring the Universe wi... (0306969), NSF | The Carnegie Supernova Pr... (1008343), NSF | Pan-STARRS1: Operations; ... (1238877), EC | COSMICDAWN (306478), EC | TESTDE (291329), EC | SNDTD (839090),...

    National Science Foundation (NSF) AST-1211916

4 research outcomes, page 1 of 1