First Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: Constraints on Cosmological Parameters

被引：198

作者：

Abbott, T. M. C. ^{[1
]}

Allam, S. ^{[2
]}

Andersen, P. ^{[3
,4
]}

Angus, C. ^{[5
]}

Asorey, J. ^{[6
]}

Avelino, A. ^{[7
]}

Avila, S. ^{[8
]}

Bassett, B. A. ^{[9
,10
]}

Bechtol, K. ^{[11
]}

Bernstein, G. M. ^{[12
]}

Bertin, E. ^{[13
,14
]}

Brooks, D. ^{[15
]}

Brout, D. ^{[12
]}

Brown, P. ^{[16
,17
]}

Burke, D. L. ^{[18
,19
]}

Calcino, J. ^{[3
]}

Carnero Rosell, A. ^{[20
,21
]}

Carollo, D. ^{[22
]}

Kind, M. Carrasco ^{[23
,24
]}

Carretero, J. ^{[25
]}

Casas, R. ^{[26
,27
]}

Castander, F. J. ^{[26
,27
]}

Cawthon, R. ^{[28
]}

Challis, P. ^{[7
]}

Childress, M. ^{[5
]}

Clocchiatti, A. ^{[29
,30
]}

Cunha, C. E. ^{[18
]}

D'Andrea, C. B. ^{[12
]}

da Costa, L. N. ^{[21
,31
]}

Davis, C. ^{[18
]}

Davis, T. M. ^{[3
]}

De Vicente, J. ^{[20
]}

DePoy, D. L. ^{[16
,17
]}

Desai, S. ^{[32
]}

Diehl, H. T. ^{[2
]}

Doel, P. ^{[15
]}

Drlica-Wagner, A. ^{[2
,33
]}

Eifler, T. F. ^{[34
,35
]}

Evrard, A. E. ^{[36
,37
]}

Fernandez, E. ^{[25
]}

Filippenko, A., V ^{[38
,39
]}

Finley, D. A. ^{[2
]}

Flaugher, B. ^{[2
]}

Foley, R. J. ^{[40
]}

Fosalba, P. ^{[26
,27
]}

Frieman, J. ^{[2
,33
]}

Galbany, L. ^{[41
]}

Garcia-Bellido, J. ^{[42
]}

Gaztanaga, E. ^{[26
,27
]}

Giannantonio, T. ^{[43
,44
,45
]}

机构：

[1] Natl Opt Astron Observ, Cerro Tololo Interamer Observ, Casilla 603, La Serena, Chile

[2] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA

[3] Univ Queensland, Sch Math & Phys, Brisbane, Qld 4072, Australia

[4] Univ Copenhagen, Dark Cosmol Ctr, Juliane Maries Vej 30, DK-2100 Copenhagen O, Denmark

[5] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England

[6] Korea Astron & Space Sci Inst, Daejeon 305348, South Korea

[7] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[8] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England

[9] African Inst Math Sci, 6 Melrose Rd, ZA-7945 Muizenberg, South Africa

[10] South African Astron Observ, POB 9, ZA-7935 Observatory, South Africa

[11] LSST, 933 North Cherry Ave, Tucson, AZ 85721 USA

[12] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA

[13] CNRS, UMR 7095, Inst Astrophys Paris, F-75014 Paris, France

[14] UPMC Univ Paris 06, Sorbonne Univ, UMR 7095, Inst Astrophys Paris, F-75014 Paris, France

[15] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England

[16] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, College Stn, TX 77843 USA

[17] Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA

[18] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, POB 2450, Stanford, CA 94305 USA

[19] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA

[20] Ctr Invest Energet Medioambientales & Tecnol CIEM, Madrid, Spain

[21] Lab Intinst & Astron LIneA, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[22] INAF, Astrophys Observ Turin, I-10025 Pino Torinese, Italy

[23] Univ Illinois, Dept Astron, 1002 West Green St, Urbana, IL 61801 USA

[24] Natl Ctr Supercomp Applicat, 1205 West Clark St, Urbana, IL 61801 USA

[25] Barcelona Inst Sci & Technol, IFAE, Campus UAB, E-08193 Bellaterra, Barcelona, Spain

[26] IEEC, E-08034 Barcelona, Spain

[27] CSIC, Inst Space Sci ICE, Campus UAB,Caner Can Magrans S-N, E-08193 Barcelona, Spain

[28] Univ Wisconsin, Dept Phys, 2320 Chamberlin Hall,1150 Univ Ave, Madison, WI 53706 USA

[29] Univ Catolica Chile, Millennium Inst Astrophys, Santiago, Chile

[30] Univ Catolica Chile, Dept Phys & Astron, Santiago, Chile

[31] Observ Nacl, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[32] ITT Hyderabad, Dept Phys, Kandi 502285, Telangana, India

[33] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[34] Steward Observ, Dept Astron, 933 North Cherry Ave, Tucson, AZ 85721 USA

[35] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA

[36] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA

[37] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA

[38] Univ Calif Berkeley, Dept Astron, 601 Campbell Hall, Berkeley, CA 94720 USA

[39] Univ Calif Berkeley, Miller Inst Basic Res Sci, Berkeley, CA 94720 USA

[40] Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA

[41] Univ Pittsburgh, Dept Phys & Astron, PITT PACC, Pittsburgh, PA 15260 USA

[42] Univ Autonoma Madrid, Inst Fis Teor UAM CSIC, E-28049 Madrid, Spain

[43] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England

[44] Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England

[45] Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte, Scheinerstr 1, D-81679 Munich, Germany

[46] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia

[47] CALTECH, 1200 East Calif Blvd,MC 249-17, Pasadena, CA 91125 USA

[48] Univ Lisbon, Inst Super Tecn, CENTRA, Av Rovisco Pais 1, P-1049001 Lisbon, Portugal

[49] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA

[50] Swiss Fed Inst Technol, Dept Phys, Wolfgang Pauli Str 16, CH-8093 Zurich, Switzerland

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2019年 / 872卷 / 02期

基金：

美国国家科学基金会; 澳大利亚研究理事会; 欧洲研究理事会; 英国科学技术设施理事会;

关键词：

dark energy; dark matter; LIGHT CURVES; LEGACY SURVEY; REDSHIFT; GALAXIES; SPECTROSCOPY; PHOTOMETRY; PEGASE; AGE;

D O I：

10.3847/2041-8213/ab04fa

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the first cosmological parameter constraints using measurements of type Ia supernovae (SNe Ia) from the Dark Energy Survey Supernova Program (DES-SN). The analysis uses a subsample of 207 spectroscopically confirmed SNe. Ia from the first three years of DES-SN, combined with a low-redshift sample of 122 SNe from the literature. Our "DES-SN3YR" result from these 329 SNe. Ia is based on a series of companion analyses and improvements covering SN. Ia discovery, spectroscopic selection, photometry, calibration, distance bias corrections, and evaluation of systematic uncertainties. For a flat Lambda CDM model we find a matter density Omega(m) = 0.331 +/- 0.038. For a flat wCDM model, and combining our SN. Ia constraints with those from the cosmic microwave background (CMB), we find a dark energy equation of state w = -0.978 +/- 0.059, and Omega(m) = 0.321 +/- 0.018. For a flat w(0)w(a)CDM model, and combining probes from SN. Ia, CMB and baryon acoustic oscillations, we find w(0) = -0.885 +/- 0.114 and w(a) = -0.387 +/- 0.430. These results are in agreement with a cosmological constant and with previous constraints using SNe. Ia (Pantheon, JLA).

引用

页数：9

共 65 条

[31] polychord: nested sampling for cosmology
Handley, W. J.
Hobson, M. P.
Lasenby, A. N.
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2015, 450 (01) : L61 - L65
[32] CfA4: LIGHT CURVES FOR 94 TYPE Ia SUPERNOVAE
Hicken, Malcolm
Challis, Peter
Kirshner, Robert P.
Rest, Armin
Cramer, Claire E.
Wood-Vasey, W. Michael
Bakos, Gaspar
Berlind, Perry
Brown, Warren R.
Caldwell, Nelson
Calkins, Mike
Currie, Thayne
de Kleer, Kathy
Esquerdo, Gil
Everett, Mark
Falco, Emilio
Fernandez, Jose
Friedman, Andrew S.
Groner, Ted
Hartman, Joel
Holman, Matthew J.
Hutchins, Robert
Keys, Sonia
Kipping, David
Latham, Dave
Marion, George H.
Narayan, Gautham
Pahre, Michael
Pal, Andras
Peters, Wayne
Perumpilly, Gopakumar
Ripman, Ben
Sipocz, Brigitta
Szentgyorgyi, Andrew
Tang, Sumin
Torres, Manuel A. P.
Vaz, Amali
Wolk, Scott
Zezas, Andreas
[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2012, 200 (02)
[33] IMPROVED DARK ENERGY CONSTRAINTS FROM ∼ 100 NEW CfA SUPERNOVA TYPE Ia LIGHT CURVES
Hicken, Malcolm
Wood-Vasey, W. Michael
Blondin, Stephane
Challis, Peter
Jha, Saurabh
Kelly, Patrick L.
Rest, Armin
Kirshner, Robert P.
[J]. ASTROPHYSICAL JOURNAL, 2009, 700 (02) : 1097 - 1140
[34] CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA
Hicken, Malcolm
Challis, Peter
Jha, Saurabh
Kirshner, Robert P.
Matheson, Tom
Modjaz, Maryam
Rest, Armin
Wood-Vasey, W. Michael
Bakos, Gaspar
Barton, Elizabeth J.
Berlind, Perry
Bragg, Ann
Briceno, Cesar
Brown, Warren R.
Caldwell, Nelson
Calkins, Mike
Cho, Richard
Ciupik, Larry
Contreras, Maria
Dendy, Kristi-Concannon
Dosaj, Anil
Durham, Nick
Eriksen, Kris
Esquerdo, Gil
Everett, Mark
Falco, Emilio
Fernandez, Jose
Gaba, Alejandro
Garnavich, Peter
Graves, Genevieve
Green, Paul
Groner, Ted
Hergenrother, Carl
Holman, Matthew J.
Hradecky, Vit
Huchra, John
Hutchison, Bob
Jerius, Diab
Jordan, Andres
Kilgard, Roy
Krauss, Miriam
Luhman, Kevin
Macri, Lucas
Marrone, Daniel
McDowell, Jonathan
McIntosh, Daniel
McNamara, Brian
Megeath, Tom
Mochejska, Barbara
Munoz, Diego
[J]. ASTROPHYSICAL JOURNAL, 2009, 700 (01) : 331 - 357
[35] MARZ: Manual and automatic redshifting software
Hinton, S. R.
Davis, Tamara M.
Lidman, C.
Glazebrook, K.
Lewis, G. F.
[J]. ASTRONOMY AND COMPUTING, 2016, 15 : 61 - 71
[36] Hinton S. R, 2018, ARXIV181102381
[37] THE SLOAN DIGITAL SKY SURVEY-II: PHOTOMETRY AND SUPERNOVA IA LIGHT CURVES FROM THE 2005 DATA
Holtzman, Jon A.
Marriner, John
Kessler, Richard
Sako, Masao
Dilday, Ben
Frieman, Joshua A.
Schneider, Donald P.
Bassett, Bruce
Becker, Andrew
Cinabro, David
DeJongh, Fritz
Depoy, Darren L.
Doi, Mamoru
Garnavich, Peter M.
Hogan, Craig J.
Jha, Saurabh
Konishi, Kohki
Lampeitl, Hubert
Marshall, Jennifer L.
McGinnis, David
Miknaitis, Gajus
Nichol, Robert C.
Prieto, Jose Luis
Riess, Adam G.
Richmond, Michael W.
Romani, Roger
Smith, Mathew
Takanashi, Naohiro
Tokita, Kouichi
Van der Heyden, Kurt
Yasuda, Naoki
Zheng, Chen
[J]. ASTRONOMICAL JOURNAL, 2008, 136 (06) : 2306 - 2320
[38] Gemini spectroscopy of supernovae from the supernova legacy survey: Improving high-redshift supernova selection and classification
Howell, DA
Sullivan, M
Perrett, K
Bronder, TJ
Hook, IM
Astier, P
Aubourg, E
Balam, D
Basa, S
Carlberg, RG
Fabbro, S
Fouchez, D
Guy, J
Lafoux, H
Neill, JD
Pain, R
Palanque-Delabrouille, N
Pritchet, CJ
Regnault, N
Rich, J
Taillet, R
Knop, R
McMahon, RG
Perlmutter, S
Walton, NA
[J]. ASTROPHYSICAL JOURNAL, 2005, 634 (02) : 1190 - 1201
[39] UBVRI light curves of 44 type Ia supernovae
Jha, S
Kirshner, RP
Challis, P
Garnavich, PM
Matheson, T
Soderberg, AM
Graves, GJM
Hicken, M
Alves, JF
Arce, HG
Balog, Z
Barmby, P
Barton, EJ
Berlind, P
Bragg, AE
Briceño, C
Brown, WR
Buckley, JH
Caldwell, N
Calkins, ML
Carter, BJ
Concannon, KD
Donnelly, RH
Eriksen, KA
Fabricant, DG
Falco, EE
Fiore, F
Garcia, MR
Gómez, M
Grogin, NA
Groner, T
Groot, PJ
Haisch, KE
Hartmann, L
Hergenrother, CW
Holman, MJ
Huchra, JP
Jayawardhana, R
Jerius, D
Kannappan, SJ
Kim, DW
Kleyna, JT
Kochanek, CS
Koranyi, DM
Krockenberger, M
Lada, CJ
Luhman, KL
Luu, JX
Macri, LM
Mader, JA
[J]. ASTRONOMICAL JOURNAL, 2006, 131 (01) : 527 - 554
[40] HUBBLE RESIDUALS OF NEARBY TYPE Ia SUPERNOVAE ARE CORRELATED WITH HOST GALAXY MASSES
Kelly, Patrick L.
Hicken, Malcolm
Burke, David L.
Mandel, Kaisey S.
Kirshner, Robert P.
[J]. ASTROPHYSICAL JOURNAL, 2010, 715 (02) : 743 - 756

← 1 2 3 4 5 6 7 →