Imperial College London
Alternate

ProfessorDavidBrooks

Faculty of Medicine, Department of Brain Sciences

Visiting Professor
 
 
 
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Contact

 

david.brooks

 
 
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Assistant

 

Ms Hyacinth Henry +44 (0)20 3313 3172

 
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Location

 

U106Block B Hammersmith HospitalHammersmith Campus

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Summary

 

Publications

Citation

BibTex format

@article{Abbott:2019:2041-8213/ab04fa,
author = {Abbott, TMC and Allam, S and Andersen, P and Angus, C and Asorey, J and Avelino, A and Avila, S and Bassett, BA and Bechtol, K and Bernstein, GM and Bertin, E and Brooks, D and Brout, D and Brown, P and Burke, DL and Calcino, J and Rosell, AC and Carollo, D and Carrasco, Kind M and Carretero, J and Casas, R and Castander, FJ and Cawthon, R and Challis, P and Childress, M and Clocchiatti, A and Cunha, CE and D'Andrea, CB and Da, Costa LN and Davis, C and Davis, TM and De, Vicente J and Depoy, DL and Desai, S and Diehl, HT and Doel, P and Drlica-Wagner, A and Eifler, TF and Evrard, AE and Fernandez, E and Filippenko, AV and Finley, DA and Flaugher, B and Foley, RJ and Fosalba, P and Frieman, J and Galbany, L and García-Bellido, J and Gaztanaga, E and Giannantonio, T and Glazebrook, K and Goldstein, DA and González-Gaitán, S and Gruen, D and Gruendl, RA and Gschwend, J and Gupta, RR and Gutierrez, G and Hartley, WG and Hinton, SR and Hollowood, DL and Honscheid, K and Hoormann, JK and Hoy},
doi = {2041-8213/ab04fa},
journal = {Astrophysical Journal Letters},
title = {First Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: Constraints on Cosmological Parameters},
url = {http://dx.doi.org/10.3847/2041-8213/ab04fa},
volume = {872},
year = {2019}
}
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RIS format (EndNote, RefMan)

TY  - JOUR
AB  - 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 ΛCDM model we find a matter density Ω 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 ω 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 w0 = -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).
AU  - Abbott,TMC
AU  - Allam,S
AU  - Andersen,P
AU  - Angus,C
AU  - Asorey,J
AU  - Avelino,A
AU  - Avila,S
AU  - Bassett,BA
AU  - Bechtol,K
AU  - Bernstein,GM
AU  - Bertin,E
AU  - Brooks,D
AU  - Brout,D
AU  - Brown,P
AU  - Burke,DL
AU  - Calcino,J
AU  - Rosell,AC
AU  - Carollo,D
AU  - Carrasco,Kind M
AU  - Carretero,J
AU  - Casas,R
AU  - Castander,FJ
AU  - Cawthon,R
AU  - Challis,P
AU  - Childress,M
AU  - Clocchiatti,A
AU  - Cunha,CE
AU  - D'Andrea,CB
AU  - Da,Costa LN
AU  - Davis,C
AU  - Davis,TM
AU  - De,Vicente J
AU  - Depoy,DL
AU  - Desai,S
AU  - Diehl,HT
AU  - Doel,P
AU  - Drlica-Wagner,A
AU  - Eifler,TF
AU  - Evrard,AE
AU  - Fernandez,E
AU  - Filippenko,AV
AU  - Finley,DA
AU  - Flaugher,B
AU  - Foley,RJ
AU  - Fosalba,P
AU  - Frieman,J
AU  - Galbany,L
AU  - García-Bellido,J
AU  - Gaztanaga,E
AU  - Giannantonio,T
AU  - Glazebrook,K
AU  - Goldstein,DA
AU  - González-Gaitán,S
AU  - Gruen,D
AU  - Gruendl,RA
AU  - Gschwend,J
AU  - Gupta,RR
AU  - Gutierrez,G
AU  - Hartley,WG
AU  - Hinton,SR
AU  - Hollowood,DL
AU  - Honscheid,K
AU  - Hoormann,JK
AU  - Hoyle,B
AU  - James,DJ
AU  - Jeltema,T
AU  - Johnson,MWG
AU  - Johnson,MD
AU  - Kasai,E
AU  - Kent,S
AU  - Kessler,R
AU  - Kim,AG
AU  - Kirshner,RP
AU  - Kovacs,E
AU  - Krause,E
AU  - Kron,R
AU  - Kuehn,K
AU  - Kuhlmann,S
AU  - Kuropatkin,N
AU  - Lahav,O
AU  - Lasker,J
AU  - Lewis,GF
AU  - Li,TS
AU  - Lidman,C
AU  - Lima,M
AU  - Lin,H
AU  - Macaulay,E
AU  - Maia,MAG
AU  - Mandel,KS
AU  - March,M
AU  - Marriner,J
AU  - Marshall,JL
AU  - Martini,P
AU  - Menanteau,F
AU  - Miller,CJ
AU  - Miquel,R
AU  - Miranda,V
AU  - Mohr,JJ
AU  - Morganson,E
AU  - Muthukrishna,D
DO  - 2041-8213/ab04fa
PY  - 2019///
SN  - 2041-8205
TI  - First Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: Constraints on Cosmological Parameters
T2  - Astrophysical Journal Letters
UR  - http://dx.doi.org/10.3847/2041-8213/ab04fa
VL  - 872
ER  -
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