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The Pantheon+ analysis: cosmological constraints

The Pantheon+ analysis: cosmological constraints
The Pantheon+ analysis: cosmological constraints

We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves of 1550 distinct Type Ia supernovae (SNe Ia) ranging in redshift from z = 0.001 to 2.26. This work features an increased sample size from the addition of multiple cross-calibrated photometric systems of SNe covering an increased redshift span, and improved treatments of systematic uncertainties in comparison to the original Pantheon analysis, which together result in a factor of 2 improvement in cosmological constraining power. For a flat ΛCDM model, we find ΩM = 0.334 ± 0.018 from SNe Ia alone. For a flat w0CDM model, we measure w0 = −0.90 ± 0.14 from SNe Ia alone, H0 = 73.5 ± 1.1 km s−1 Mpc−1 when including the Cepheid host distances and covariance (SH0ES), and w0 = -0.978-+0.0310.024 when combining the SN likelihood with Planck constraints from the cosmic microwave background (CMB) and baryon acoustic oscillations (BAO); both w0 values are consistent with a cosmological constant. We also present the most precise measurements to date on the evolution of dark energy in a flat w0waCDM universe, and measure wa = -0.1-+2.00.9 from Pantheon+ SNe Ia alone, H0 = 73.3 ± 1.1 km s−1 Mpc−1 when including SH0ES Cepheid distances, and wa = -0.65-+0.320.28 when combining Pantheon+ SNe Ia with CMB and BAO data. Finally, we find that systematic uncertainties in the use of SNe Ia along the distance ladder comprise less than one-third of the total uncertainty in the measurement of H0. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further and cannot explain the present “Hubble tension” between local measurements and early universe predictions from the cosmological model.

0004-637X
Brout, Dillon
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Scolnic, Dan
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Popovic, Brodie
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Riess, Adam G.
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Carr, Anthony
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Zuntz, Joe
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Kessler, Rick
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Davis, Tamara M.
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Hinton, Samuel
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Jones, David
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Peterson, Erik R.
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Meldorf, Cole
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Vincenzi, Maria
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Wood, Charlotte M.
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Chen, Rebecca
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Chambers, Ken
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Coulter, David A.
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Dai, Mi
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Filippenko, Alexei V.
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Foley, Ryan J.
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Jha, Saurabh W.
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Kelsey, Lisa
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Kirshner, Robert P.
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Möller, Anais
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Muir, Jessie
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Nadathur, Seshadri
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Pan, Yen-Chen
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Rest, Armin
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Siebert, Matthew R.
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Smith, Mat
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Stahl, Benjamin E.
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Wiseman, Phil
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Brout, Dillon
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Scolnic, Dan
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Popovic, Brodie
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Riess, Adam G.
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Carr, Anthony
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Zuntz, Joe
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Kessler, Rick
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Davis, Tamara M.
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Hinton, Samuel
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Jones, David
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D’Arcy Kenworthy, W.
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Peterson, Erik R.
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Said, Khaled
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Taylor, Georgie
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Ali, Noor
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Armstrong, Patrick
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Charvu, Pranav
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Dwomoh, Arianna
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Meldorf, Cole
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Palmese, Antonella
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Qu, Helen
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Rose, Benjamin M.
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Sanchez, Bruno
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Stubbs, Christopher W.
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Vincenzi, Maria
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Wood, Charlotte M.
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Brown, Peter J.
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Chen, Rebecca
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Chambers, Ken
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Coulter, David A.
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Dai, Mi
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Dimitriadis, Georgios
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Filippenko, Alexei V.
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Foley, Ryan J.
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Jha, Saurabh W.
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Kelsey, Lisa
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Kirshner, Robert P.
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Möller, Anais
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Muir, Jessie
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Nadathur, Seshadri
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Pan, Yen-Chen
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Rest, Armin
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Rojas-Bravo, Cesar
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Sako, Masao
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Siebert, Matthew R.
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Smith, Mat
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Stahl, Benjamin E.
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Wiseman, Phil
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Brout, Dillon, Scolnic, Dan, Popovic, Brodie, Riess, Adam G., Carr, Anthony, Zuntz, Joe, Kessler, Rick, Davis, Tamara M., Hinton, Samuel, Jones, David, D’Arcy Kenworthy, W., Peterson, Erik R., Said, Khaled, Taylor, Georgie, Ali, Noor, Armstrong, Patrick, Charvu, Pranav, Dwomoh, Arianna, Meldorf, Cole, Palmese, Antonella, Qu, Helen, Rose, Benjamin M., Sanchez, Bruno, Stubbs, Christopher W., Vincenzi, Maria, Wood, Charlotte M., Brown, Peter J., Chen, Rebecca, Chambers, Ken, Coulter, David A., Dai, Mi, Dimitriadis, Georgios, Filippenko, Alexei V., Foley, Ryan J., Jha, Saurabh W., Kelsey, Lisa, Kirshner, Robert P., Möller, Anais, Muir, Jessie, Nadathur, Seshadri, Pan, Yen-Chen, Rest, Armin, Rojas-Bravo, Cesar, Sako, Masao, Siebert, Matthew R., Smith, Mat, Stahl, Benjamin E. and Wiseman, Phil (2022) The Pantheon+ analysis: cosmological constraints. Astrophysical Journal, 938 (2), [110]. (doi:10.3847/1538-4357/ac8e04).

Record type: Article

Abstract

We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves of 1550 distinct Type Ia supernovae (SNe Ia) ranging in redshift from z = 0.001 to 2.26. This work features an increased sample size from the addition of multiple cross-calibrated photometric systems of SNe covering an increased redshift span, and improved treatments of systematic uncertainties in comparison to the original Pantheon analysis, which together result in a factor of 2 improvement in cosmological constraining power. For a flat ΛCDM model, we find ΩM = 0.334 ± 0.018 from SNe Ia alone. For a flat w0CDM model, we measure w0 = −0.90 ± 0.14 from SNe Ia alone, H0 = 73.5 ± 1.1 km s−1 Mpc−1 when including the Cepheid host distances and covariance (SH0ES), and w0 = -0.978-+0.0310.024 when combining the SN likelihood with Planck constraints from the cosmic microwave background (CMB) and baryon acoustic oscillations (BAO); both w0 values are consistent with a cosmological constant. We also present the most precise measurements to date on the evolution of dark energy in a flat w0waCDM universe, and measure wa = -0.1-+2.00.9 from Pantheon+ SNe Ia alone, H0 = 73.3 ± 1.1 km s−1 Mpc−1 when including SH0ES Cepheid distances, and wa = -0.65-+0.320.28 when combining Pantheon+ SNe Ia with CMB and BAO data. Finally, we find that systematic uncertainties in the use of SNe Ia along the distance ladder comprise less than one-third of the total uncertainty in the measurement of H0. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further and cannot explain the present “Hubble tension” between local measurements and early universe predictions from the cosmological model.

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Accepted/In Press date: 24 August 2022
Published date: 19 October 2022
Additional Information: Funding Information: D.S., D.B., and A.R. thank the John Templeton Foundation for their support of grant No. 62314. D.B. acknowledges support for this work provided by NASA through NASA Hubble Fellowship grant HST-HF2-51430.001 awarded by the Space Telescope Science Institute (STScI), which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. D.S. is supported by DOE grant DE-SC0010007, the David and Lucile Packard Foundation, and NASA under contract No. NNG17PX03C issued through the WFIRST Science Investigation Teams Programme. We acknowledge the generous support of Marc J. Staley, whose fellowship partly funded B.E.S. while contributing to the work presented herein as a graduate student. A.V.F. is grateful for support from the TABASGO Foundation, the Christopher R. Redlich Fund, the U.C. Berkeley Miller Institute for Basic Research in Science (in which he was a Miller Senior Fellow), and many individual donors. S.N. thanks the STFC Ernest Rutherford Fellowship for support via grant ST/T005009/1. L.K. thanks the UKRI Future Leaders Fellowship for support through the grant MR/T01881X/1. This work was completed in part with resources provided by the University of Chicagos Research Computing Center. The Katzman Automatic Imaging Telescope (with which the LOSS samples were obtained) and its ongoing operation were made possible by donations from Sun Microsystems, Inc., the Hewlett-Packard Company, AutoScope Corporation, Lick Observatory, the NSF, the University of California, the Sylvia & Jim Katzman Foundation, and the TABASGO Foundation. Research at Lick Observatory is partially supported by a generous gift from Google.

Identifiers

Local EPrints ID: 483467
URI: http://eprints.soton.ac.uk/id/eprint/483467
ISSN: 0004-637X
PURE UUID: 6610c484-59bc-44a9-b1f0-e0b5e70791d3
ORCID for Mat Smith: ORCID iD orcid.org/0000-0002-3321-1432
ORCID for Phil Wiseman: ORCID iD orcid.org/0000-0002-3073-1512

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Date deposited: 31 Oct 2023 17:49
Last modified: 18 Mar 2024 03:43

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Contributors

Author: Dillon Brout
Author: Dan Scolnic
Author: Brodie Popovic
Author: Adam G. Riess
Author: Anthony Carr
Author: Joe Zuntz
Author: Rick Kessler
Author: Tamara M. Davis
Author: Samuel Hinton
Author: David Jones
Author: W. D’Arcy Kenworthy
Author: Erik R. Peterson
Author: Khaled Said
Author: Georgie Taylor
Author: Noor Ali
Author: Patrick Armstrong
Author: Pranav Charvu
Author: Arianna Dwomoh
Author: Cole Meldorf
Author: Antonella Palmese
Author: Helen Qu
Author: Benjamin M. Rose
Author: Bruno Sanchez
Author: Christopher W. Stubbs
Author: Maria Vincenzi
Author: Charlotte M. Wood
Author: Peter J. Brown
Author: Rebecca Chen
Author: Ken Chambers
Author: David A. Coulter
Author: Mi Dai
Author: Georgios Dimitriadis
Author: Alexei V. Filippenko
Author: Ryan J. Foley
Author: Saurabh W. Jha
Author: Lisa Kelsey
Author: Robert P. Kirshner
Author: Anais Möller
Author: Jessie Muir
Author: Seshadri Nadathur
Author: Yen-Chen Pan
Author: Armin Rest
Author: Cesar Rojas-Bravo
Author: Masao Sako
Author: Matthew R. Siebert
Author: Mat Smith ORCID iD
Author: Benjamin E. Stahl
Author: Phil Wiseman ORCID iD

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