First cosmological results using Type Ia supernovae from the Dark Energy Survey: Measurement of the Hubble constant

E. MacAulay; R. C. Nichol; D. Bacon; D. Brout; T. M. Davis; B. Zhang; B. A. Bassett; D. Scolnic; A. Möller; C. B. D'Andrea; S. R. Hinton; R. Kessler; A. G. Kim; J. Lasker; C. Lidman; M. Sako; M. Smith; M. Sullivan; T. M.C. Abbott; S. Allam; J. Annis; J. Asorey; S. Avila; K. Bechtol; D. Brooks; P. Brown; D. L. Burke; J. Calcino; A. Carnero Rosell; D. Carollo; M. Carrasco Kind; J. Carretero; F. J. Castander; T. Collett; M. Crocce; C. E. Cunha; L. N. Da Costa; C. Davis; J. De Vicente; H. T. Diehl; P. Doel; A. Drlica-Wagner; T. F. Eifler; J. Estrada; A. E. Evrard; A. V. Filippenko; D. A. Finley; B. Flaugher; R. J. Foley; P. Fosalba; J. Frieman; L. Galbany; J. García-Bellido; E. Gaztanaga; K. Glazebrook; S. González-Gaitán; D. Gruen; R. A. Gruendl; J. Gschwend; G. Gutierrez; W. G. Hartley; D. L. Hollowood; K. Honscheid; J. K. Hoormann; B. Hoyle; D. Huterer; B. Jain; D. J. James; T. Jeltema; E. Kasai; E. Krause; K. Kuehn; N. Kuropatkin; O. Lahav; G. F. Lewis; T. S. Li; M. Lima; H. Lin; M. A.G. Maia; J. L. Marshall; P. Martini; R. Miquel; P. Nugent; A. Palmese; Y. C. Pan; A. A. Plazas; A. K. Romer; A. Roodman; E. Sanchez; V. Scarpine; R. Schindler; M. Schubnell; S. Serrano; I. Sevilla-Noarbe; R. Sharp; M. Soares-Santos; F. Sobreira; N. E. Sommer; E. Suchyta; E. Swann; M. E.C. Swanson; G. Tarle; D. Thomas; R. C. Thomas; B. E. Tucker; S. A. Uddin; V. Vikram; A. R. Walker; P. Wiseman

doi:10.1093/mnras/stz978

First cosmological results using Type Ia supernovae from the Dark Energy Survey: Measurement of the Hubble constant

E. MacAulay, R. C. Nichol, D. Bacon, D. Brout, T. M. Davis, B. Zhang, B. A. Bassett, D. Scolnic, A. Möller, C. B. D'Andrea, S. R. Hinton, R. Kessler, A. G. Kim, J. Lasker, C. Lidman, M. Sako, M. Smith, M. Sullivan, T. M.C. Abbott, S. AllamJ. Annis, J. Asorey, S. Avila, K. Bechtol, D. Brooks, P. Brown, D. L. Burke, J. Calcino, A. Carnero Rosell, D. Carollo, M. Carrasco Kind, J. Carretero, F. J. Castander, T. Collett, M. Crocce, C. E. Cunha, L. N. Da Costa, C. Davis, J. De Vicente, H. T. Diehl, P. Doel, A. Drlica-Wagner, T. F. Eifler, J. Estrada, A. E. Evrard, A. V. Filippenko, D. A. Finley, B. Flaugher, R. J. Foley, P. Fosalba, J. Frieman, L. Galbany, J. García-Bellido, E. Gaztanaga, K. Glazebrook, S. González-Gaitán, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutierrez, W. G. Hartley, D. L. Hollowood, K. Honscheid, J. K. Hoormann, B. Hoyle, D. Huterer, B. Jain, D. J. James, T. Jeltema, E. Kasai, E. Krause, K. Kuehn, N. Kuropatkin, O. Lahav, G. F. Lewis, T. S. Li, M. Lima, H. Lin, M. A.G. Maia, J. L. Marshall, P. Martini, R. Miquel, P. Nugent, A. Palmese, Y. C. Pan, A. A. Plazas, A. K. Romer, A. Roodman, E. Sanchez, V. Scarpine, R. Schindler, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, R. Sharp, M. Soares-Santos, F. Sobreira, N. E. Sommer, E. Suchyta, E. Swann, M. E.C. Swanson, G. Tarle, D. Thomas, R. C. Thomas, B. E. Tucker, S. A. Uddin, V. Vikram, A. R. Walker, P. Wiseman

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摘要

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 122 low-redshift (z<0.07) SNe Ia (Low-z) and measurements ofBaryon Acoustic Oscillations (BAOs). Whereas traditional measurements of H0 with SNe Ia use a distance ladder of parallax and Cepheid variable stars, the inverse distance ladder relies on absolute distance measurements from the BAOs to calibrate the intrinsic magnitude of the SNe Ia.We find H0 = 67.8 1.3 km s^-1 Mpc^-1 (statistical and systematic uncertainties, 68 per cent confidence). Our measurement makes minimal assumptions about the underlying cosmological model, and our analysis was blinded to reduce confirmation bias. We examine possible systematic uncertainties and all are below the statistical uncertainties. Our H0 value is consistent with estimates derived from the Cosmic Microwave Background assuming a ΛCDM universe.

原文	???core.languages.en_GB???
頁（從 - 到）	2184-2196
頁數	13
期刊	Monthly Notices of the Royal Astronomical Society
卷	486
發行號	2
DOIs	https://doi.org/10.1093/mnras/stz978
出版狀態	已出版 - 1 6月 2019

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10.1093/mnras/stz978

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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., Hinton, S. R., Kessler, R., Kim, A. G., Lasker, J., Lidman, C., Sako, M., Smith, M., Sullivan, M., Abbott, T. M. C., ... Wiseman, P. (2019). First cosmological results using Type Ia supernovae from the Dark Energy Survey: Measurement of the Hubble constant. Monthly Notices of the Royal Astronomical Society, 486(2), 2184-2196. https://doi.org/10.1093/mnras/stz978

@article{3ed0832c449f45a184c4c15ad6a5bf9a,

title = "First cosmological results using Type Ia supernovae from the Dark Energy Survey: Measurement of the Hubble constant",

abstract = "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 -1 Mpc-1 (statistical and systematic uncertainties, 68 per cent confidence). Our measurement makes minimal assumptions about the underlying cosmological model, and our analysis was blinded to reduce confirmation bias. We examine possible systematic uncertainties and all are below the statistical uncertainties. Our H0 value is consistent with estimates derived from the Cosmic Microwave Background assuming a ΛCDM universe.",

keywords = "cosmological parameters, cosmology: observations, distance scale.",

author = "E. MacAulay and Nichol, {R. C.} and D. Bacon and D. Brout and Davis, {T. M.} and B. Zhang and Bassett, {B. A.} and D. Scolnic and A. M{\"o}ller and D'Andrea, {C. B.} and Hinton, {S. R.} and R. Kessler and Kim, {A. G.} and J. Lasker and C. Lidman and M. Sako and M. Smith and M. Sullivan and Abbott, {T. M.C.} and S. Allam and J. Annis and J. Asorey and S. Avila and K. Bechtol and D. Brooks and P. Brown and Burke, {D. L.} and J. Calcino and {Carnero Rosell}, A. and D. Carollo and {Carrasco Kind}, M. and J. Carretero and Castander, {F. J.} and T. Collett and M. Crocce and Cunha, {C. E.} and {Da Costa}, {L. N.} and C. Davis and {De Vicente}, J. and Diehl, {H. T.} and P. Doel and A. Drlica-Wagner and Eifler, {T. F.} and J. Estrada and Evrard, {A. E.} and Filippenko, {A. V.} and Finley, {D. A.} and B. Flaugher and Foley, {R. J.} and P. Fosalba and J. Frieman and L. Galbany and J. Garc{\'i}a-Bellido and E. Gaztanaga and K. Glazebrook and S. Gonz{\'a}lez-Gait{\'a}n and D. Gruen and Gruendl, {R. A.} and J. Gschwend and G. Gutierrez and Hartley, {W. G.} and Hollowood, {D. L.} and K. Honscheid and Hoormann, {J. K.} and B. Hoyle and D. Huterer and B. Jain and James, {D. J.} and T. Jeltema and E. Kasai and E. Krause and K. Kuehn and N. Kuropatkin and O. Lahav and Lewis, {G. F.} and Li, {T. S.} and M. Lima and H. Lin and Maia, {M. A.G.} and Marshall, {J. L.} and P. Martini and R. Miquel and P. Nugent and A. Palmese and Pan, {Y. C.} and Plazas, {A. A.} and Romer, {A. K.} and A. Roodman and E. Sanchez and V. Scarpine and R. Schindler and M. Schubnell and S. Serrano and I. Sevilla-Noarbe and R. Sharp and M. Soares-Santos and F. Sobreira and Sommer, {N. E.} and E. Suchyta and E. Swann and Swanson, {M. E.C.} and G. Tarle and D. Thomas and Thomas, {R. C.} and Tucker, {B. E.} and Uddin, {S. A.} and V. Vikram and Walker, {A. R.} and P. Wiseman",

note = "Publisher Copyright: {\textcopyright} 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.",

year = "2019",

month = jun,

day = "1",

doi = "10.1093/mnras/stz978",

language = "???core.languages.en_GB???",

volume = "486",

pages = "2184--2196",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

number = "2",

}

MacAulay, E, Nichol, RC, Bacon, D, Brout, D, Davis, TM, Zhang, B, Bassett, BA, Scolnic, D, Möller, A, D'Andrea, CB, Hinton, SR, Kessler, R, Kim, AG, Lasker, J, Lidman, C, Sako, M, Smith, M, Sullivan, M, Abbott, TMC, Allam, S, Annis, J, Asorey, J, Avila, S, Bechtol, K, Brooks, D, Brown, P, Burke, DL, Calcino, J, Carnero Rosell, A, Carollo, D, Carrasco Kind, M, Carretero, J, Castander, FJ, Collett, T, Crocce, M, Cunha, CE, Da Costa, LN, Davis, C, De Vicente, J, Diehl, HT, Doel, P, Drlica-Wagner, A, Eifler, TF, Estrada, J, Evrard, AE, Filippenko, AV, Finley, DA, Flaugher, B, Foley, RJ, Fosalba, P, Frieman, J, Galbany, L, García-Bellido, J, Gaztanaga, E, Glazebrook, K, González-Gaitán, S, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Hartley, WG, Hollowood, DL, Honscheid, K, Hoormann, JK, Hoyle, B, Huterer, D, Jain, B, James, DJ, Jeltema, T, Kasai, E, Krause, E, Kuehn, K, Kuropatkin, N, Lahav, O, Lewis, GF, Li, TS, Lima, M, Lin, H, Maia, MAG, Marshall, JL, Martini, P, Miquel, R, Nugent, P, Palmese, A, Pan, YC, Plazas, AA, Romer, AK, Roodman, A, Sanchez, E, Scarpine, V, Schindler, R, Schubnell, M, Serrano, S, Sevilla-Noarbe, I, Sharp, R, Soares-Santos, M, Sobreira, F, Sommer, NE, Suchyta, E, Swann, E, Swanson, MEC, Tarle, G, Thomas, D, Thomas, RC, Tucker, BE, Uddin, SA, Vikram, V, Walker, AR & Wiseman, P 2019, 'First cosmological results using Type Ia supernovae from the Dark Energy Survey: Measurement of the Hubble constant', Monthly Notices of the Royal Astronomical Society, 卷 486, 編號 2, 頁 2184-2196. https://doi.org/10.1093/mnras/stz978

TY - JOUR

T1 - First cosmological results using Type Ia supernovae from the Dark Energy Survey

T2 - Measurement of the Hubble constant

AU - MacAulay, E.

AU - Nichol, R. C.

AU - Bacon, D.

AU - Brout, D.

AU - Davis, T. M.

AU - Zhang, B.

AU - Bassett, B. A.

AU - Scolnic, D.

AU - Möller, A.

AU - D'Andrea, C. B.

AU - Hinton, S. R.

AU - Kessler, R.

AU - Kim, A. G.

AU - Lasker, J.

AU - Lidman, C.

AU - Sako, M.

AU - Smith, M.

AU - Sullivan, M.

AU - Abbott, T. M.C.

AU - Allam, S.

AU - Annis, J.

AU - Asorey, J.

AU - Avila, S.

AU - Bechtol, K.

AU - Brooks, D.

AU - Brown, P.

AU - Burke, D. L.

AU - Calcino, J.

AU - Carnero Rosell, A.

AU - Carollo, D.

AU - Carrasco Kind, M.

AU - Carretero, J.

AU - Castander, F. J.

AU - Collett, T.

AU - Crocce, M.

AU - Cunha, C. E.

AU - Da Costa, L. N.

AU - Davis, C.

AU - De Vicente, J.

AU - Diehl, H. T.

AU - Doel, P.

AU - Drlica-Wagner, A.

AU - Eifler, T. F.

AU - Estrada, J.

AU - Evrard, A. E.

AU - Filippenko, A. V.

AU - Finley, D. A.

AU - Flaugher, B.

AU - Foley, R. J.

AU - Fosalba, P.

AU - Frieman, J.

AU - Galbany, L.

AU - García-Bellido, J.

AU - Gaztanaga, E.

AU - Glazebrook, K.

AU - González-Gaitán, S.

AU - Gruen, D.

AU - Gruendl, R. A.

AU - Gschwend, J.

AU - Gutierrez, G.

AU - Hartley, W. G.

AU - Hollowood, D. L.

AU - Honscheid, K.

AU - Hoormann, J. K.

AU - Hoyle, B.

AU - Huterer, D.

AU - Jain, B.

AU - James, D. J.

AU - Jeltema, T.

AU - Kasai, E.

AU - Krause, E.

AU - Kuehn, K.

AU - Kuropatkin, N.

AU - Lahav, O.

AU - Lewis, G. F.

AU - Li, T. S.

AU - Lima, M.

AU - Lin, H.

AU - Maia, M. A.G.

AU - Marshall, J. L.

AU - Martini, P.

AU - Miquel, R.

AU - Nugent, P.

AU - Palmese, A.

AU - Pan, Y. C.

AU - Plazas, A. A.

AU - Romer, A. K.

AU - Roodman, A.

AU - Sanchez, E.

AU - Scarpine, V.

AU - Schindler, R.

AU - Schubnell, M.

AU - Serrano, S.

AU - Sevilla-Noarbe, I.

AU - Sharp, R.

AU - Soares-Santos, M.

AU - Sobreira, F.

AU - Sommer, N. E.

AU - Suchyta, E.

AU - Swann, E.

AU - Swanson, M. E.C.

AU - Tarle, G.

AU - Thomas, D.

AU - Thomas, R. C.

AU - Tucker, B. E.

AU - Uddin, S. A.

AU - Vikram, V.

AU - Walker, A. R.

AU - Wiseman, P.

PY - 2019/6/1

Y1 - 2019/6/1

N2 - 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 -1 Mpc-1 (statistical and systematic uncertainties, 68 per cent confidence). Our measurement makes minimal assumptions about the underlying cosmological model, and our analysis was blinded to reduce confirmation bias. We examine possible systematic uncertainties and all are below the statistical uncertainties. Our H0 value is consistent with estimates derived from the Cosmic Microwave Background assuming a ΛCDM universe.

AB - 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 -1 Mpc-1 (statistical and systematic uncertainties, 68 per cent confidence). Our measurement makes minimal assumptions about the underlying cosmological model, and our analysis was blinded to reduce confirmation bias. We examine possible systematic uncertainties and all are below the statistical uncertainties. Our H0 value is consistent with estimates derived from the Cosmic Microwave Background assuming a ΛCDM universe.

KW - cosmological parameters

KW - cosmology: observations

KW - distance scale.

UR - http://www.scopus.com/inward/record.url?scp=85064830189&partnerID=8YFLogxK

U2 - 10.1093/mnras/stz978

DO - 10.1093/mnras/stz978

M3 - 期刊論文

AN - SCOPUS:85064830189

SN - 0035-8711

VL - 486

SP - 2184

EP - 2196

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 2

ER -

First cosmological results using Type Ia supernovae from the Dark Energy Survey: Measurement of the Hubble constant

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