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Title: Cosmological Constraints from Multiple Probes in the Dark Energy Survey

Abstract

The combination of multiple observational probes has long been advocated as a powerful technique to constrain cosmological parameters, in particular dark energy. The Dark Energy Survey has measured 207 spectroscopically--confirmed Type Ia supernova light curves; the baryon acoustic oscillation feature; weak gravitational lensing; and galaxy clustering. Here we present combined results from these probes, deriving constraints on the equation of state, w, of dark energy and its energy density in the Universe. Independently of other experiments, such as those that measure the cosmic microwave background, the probes from this single photometric survey rule out a Universe with no dark energy, finding w=-0.80+0.09-0.11. The geometry is shown to be consistent with a spatially flat Universe, and we obtain a constraint on the baryon density of Ωb=0.069+0.009-0.012 that is independent of early Universe measurements. These results demonstrate the potential power of large multi-probe photometric surveys and pave the way for order of magnitude advances in our constraints on properties of dark energy and cosmology over the next decade.

Authors:
; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; « less
Publication Date:
Research Org.:
Brookhaven National Laboratory (BNL), Upton, NY (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Carnegie Mellon Univ., Pittsburgh, PA (United States); The Ohio State Univ., Columbus, OH (United States); Univ. of Michigan, Ann Arbor, MI (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Org.:
DES Collaboration
OSTI Identifier:
1487399
Alternate Identifier(s):
OSTI ID: 1510140; OSTI ID: 1550891; OSTI ID: 1602527; OSTI ID: 1643943; OSTI ID: 1755508; OSTI ID: 1781333
Report Number(s):
arXiv:1811.02375; FERMILAB-PUB-18-585-AE
Journal ID: ISSN 0031-9007; PRLTAO; 1702363
Grant/Contract Number:  
AC02-07CH11359; SC0010118; AC02-05CH11231; SC0011726; SC0007859; SC0019193
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review Letters
Additional Journal Information:
Journal Volume: 122; Journal Issue: 17; Journal ID: ISSN 0031-9007
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; Cosmological parameters; Dark energy; Dark matter

Citation Formats

Abbott, T. M. C., Alarcon, A., Allam, S., Andersen, P., Andrade-Oliveira, F., Annis, J., Asorey, J., Avila, S., Bacon, D., Banik, N., Bassett, B. A., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Bertin, E., Blazek, J., Bridle, S. L., Brooks, D., Brout, D., Burke, D. L., Calcino, J., Camacho, H., Campos, A., Carnero Rosell, A., Carollo, D., Carrasco Kind, M., Carretero, J., Castander, F. J., Cawthon, R., Challis, P., Chan, K. C., Chang, C., Childress, M., Crocce, M., Cunha, C. E., D’Andrea, C. B., da Costa, L. N., Davis, C., Davis, T. M., De Vicente, J., DePoy, D. L., DeRose, J., Desai, S., Diehl, H. T., Dietrich, J. P., Dodelson, S., Doel, P., Drlica-Wagner, A., Eifler, T. F., Elvin-Poole, J., Estrada, J., Evrard, A. E., Fernandez, E., Flaugher, B., Foley, R. J., Fosalba, P., Frieman, J., Galbany, L., García-Bellido, J., Gatti, M., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Glazebrook, K., Goldstein, D. A., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoormann, J. K., Hoyle, B., Huterer, D., Jain, B., James, D. J., Jarvis, M., Jeltema, T., Kasai, E., Kent, S., Kessler, R., Kim, A. G., Kokron, N., Krause, E., Kron, R., Kuehn, K., Kuropatkin, N., Lahav, O., Lasker, J., Lemos, P., Lewis, G. F., Li, T. S., Lidman, C., Lima, M., Lin, H., Macaulay, E., MacCrann, N., Maia, M. A. G., March, M., Marriner, J., Marshall, J. L., Martini, P., McMahon, R. G., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morganson, E., Muir, J., Möller, A., Neilsen, E., Nichol, R. C., Nord, B., Ogando, R. L. C., Palmese, A., Pan, Y. -C., Peiris, H. V., Percival, W. J., Plazas, A. A., Porredon, A., Prat, J., Romer, A. K., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, E., Scarpine, V., Schindler, R., Schubnell, M., Scolnic, D., Secco, L. F., Serrano, S., Sevilla-Noarbe, I., Sharp, R., Sheldon, E., Smith, M., Soares-Santos, M., Sobreira, F., Sommer, N. E., Swann, E., Swanson, M. E. C., Tarle, G., Thomas, D., Thomas, R. C., Troxel, M. A., Tucker, B. E., Uddin, S. A., Vielzeuf, P., Walker, A. R., Wang, M., Weaverdyck, N., Wechsler, R. H., Weller, J., Yanny, B., Zhang, B., Zhang, Y., and Zuntz, J. Cosmological Constraints from Multiple Probes in the Dark Energy Survey. United States: N. p., 2019. Web. doi:10.1103/PhysRevLett.122.171301.
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Abbott, T. M. C., Alarcon, A., Allam, S., Andersen, P., Andrade-Oliveira, F., Annis, J., Asorey, J., Avila, S., Bacon, D., Banik, N., Bassett, B. A., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Bertin, E., Blazek, J., Bridle, S. L., Brooks, D., Brout, D., Burke, D. L., Calcino, J., Camacho, H., Campos, A., Carnero Rosell, A., Carollo, D., Carrasco Kind, M., Carretero, J., Castander, F. J., Cawthon, R., Challis, P., Chan, K. C., Chang, C., Childress, M., Crocce, M., Cunha, C. E., D’Andrea, C. B., da Costa, L. N., Davis, C., Davis, T. M., De Vicente, J., DePoy, D. L., DeRose, J., Desai, S., Diehl, H. T., Dietrich, J. P., Dodelson, S., Doel, P., Drlica-Wagner, A., Eifler, T. F., Elvin-Poole, J., Estrada, J., Evrard, A. E., Fernandez, E., Flaugher, B., Foley, R. J., Fosalba, P., Frieman, J., Galbany, L., García-Bellido, J., Gatti, M., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Glazebrook, K., Goldstein, D. A., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoormann, J. K., Hoyle, B., Huterer, D., Jain, B., James, D. J., Jarvis, M., Jeltema, T., Kasai, E., Kent, S., Kessler, R., Kim, A. G., Kokron, N., Krause, E., Kron, R., Kuehn, K., Kuropatkin, N., Lahav, O., Lasker, J., Lemos, P., Lewis, G. F., Li, T. S., Lidman, C., Lima, M., Lin, H., Macaulay, E., MacCrann, N., Maia, M. A. G., March, M., Marriner, J., Marshall, J. L., Martini, P., McMahon, R. G., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morganson, E., Muir, J., Möller, A., Neilsen, E., Nichol, R. C., Nord, B., Ogando, R. L. C., Palmese, A., Pan, Y. -C., Peiris, H. V., Percival, W. J., Plazas, A. A., Porredon, A., Prat, J., Romer, A. K., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, E., Scarpine, V., Schindler, R., Schubnell, M., Scolnic, D., Secco, L. F., Serrano, S., Sevilla-Noarbe, I., Sharp, R., Sheldon, E., Smith, M., Soares-Santos, M., Sobreira, F., Sommer, N. E., Swann, E., Swanson, M. E. C., Tarle, G., Thomas, D., Thomas, R. C., Troxel, M. A., Tucker, B. E., Uddin, S. A., Vielzeuf, P., Walker, A. R., Wang, M., Weaverdyck, N., Wechsler, R. H., Weller, J., Yanny, B., Zhang, B., Zhang, Y., & Zuntz, J. Cosmological Constraints from Multiple Probes in the Dark Energy Survey. United States. https://doi.org/10.1103/PhysRevLett.122.171301
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Abbott, T. M. C., Alarcon, A., Allam, S., Andersen, P., Andrade-Oliveira, F., Annis, J., Asorey, J., Avila, S., Bacon, D., Banik, N., Bassett, B. A., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Bertin, E., Blazek, J., Bridle, S. L., Brooks, D., Brout, D., Burke, D. L., Calcino, J., Camacho, H., Campos, A., Carnero Rosell, A., Carollo, D., Carrasco Kind, M., Carretero, J., Castander, F. J., Cawthon, R., Challis, P., Chan, K. C., Chang, C., Childress, M., Crocce, M., Cunha, C. E., D’Andrea, C. B., da Costa, L. N., Davis, C., Davis, T. M., De Vicente, J., DePoy, D. L., DeRose, J., Desai, S., Diehl, H. T., Dietrich, J. P., Dodelson, S., Doel, P., Drlica-Wagner, A., Eifler, T. F., Elvin-Poole, J., Estrada, J., Evrard, A. E., Fernandez, E., Flaugher, B., Foley, R. J., Fosalba, P., Frieman, J., Galbany, L., García-Bellido, J., Gatti, M., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Glazebrook, K., Goldstein, D. A., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoormann, J. K., Hoyle, B., Huterer, D., Jain, B., James, D. J., Jarvis, M., Jeltema, T., Kasai, E., Kent, S., Kessler, R., Kim, A. G., Kokron, N., Krause, E., Kron, R., Kuehn, K., Kuropatkin, N., Lahav, O., Lasker, J., Lemos, P., Lewis, G. F., Li, T. S., Lidman, C., Lima, M., Lin, H., Macaulay, E., MacCrann, N., Maia, M. A. G., March, M., Marriner, J., Marshall, J. L., Martini, P., McMahon, R. G., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morganson, E., Muir, J., Möller, A., Neilsen, E., Nichol, R. C., Nord, B., Ogando, R. L. C., Palmese, A., Pan, Y. -C., Peiris, H. V., Percival, W. J., Plazas, A. A., Porredon, A., Prat, J., Romer, A. K., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, E., Scarpine, V., Schindler, R., Schubnell, M., Scolnic, D., Secco, L. F., Serrano, S., Sevilla-Noarbe, I., Sharp, R., Sheldon, E., Smith, M., Soares-Santos, M., Sobreira, F., Sommer, N. E., Swann, E., Swanson, M. E. C., Tarle, G., Thomas, D., Thomas, R. C., Troxel, M. A., Tucker, B. E., Uddin, S. A., Vielzeuf, P., Walker, A. R., Wang, M., Weaverdyck, N., Wechsler, R. H., Weller, J., Yanny, B., Zhang, B., Zhang, Y., and Zuntz, J. Wed . "Cosmological Constraints from Multiple Probes in the Dark Energy Survey". United States. https://doi.org/10.1103/PhysRevLett.122.171301. https://www.osti.gov/servlets/purl/1487399.
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@article{osti_1487399,
title = {Cosmological Constraints from Multiple Probes in the Dark Energy Survey},
author = {Abbott, T. M. C. and Alarcon, A. and Allam, S. and Andersen, P. and Andrade-Oliveira, F. and Annis, J. and Asorey, J. and Avila, S. and Bacon, D. and Banik, N. and Bassett, B. A. and Baxter, E. and Bechtol, K. and Becker, M. R. and Bernstein, G. M. and Bertin, E. and Blazek, J. and Bridle, S. L. and Brooks, D. and Brout, D. and Burke, D. L. and Calcino, J. and Camacho, H. and Campos, A. and Carnero Rosell, A. and Carollo, D. and Carrasco Kind, M. and Carretero, J. and Castander, F. J. and Cawthon, R. and Challis, P. and Chan, K. C. and Chang, C. and Childress, M. and Crocce, M. and Cunha, C. E. and D’Andrea, C. B. and da Costa, L. N. and Davis, C. and Davis, T. M. and De Vicente, J. and DePoy, D. L. and DeRose, J. and Desai, S. and Diehl, H. T. and Dietrich, J. P. and Dodelson, S. and Doel, P. and Drlica-Wagner, A. and Eifler, T. F. and Elvin-Poole, J. and Estrada, J. and Evrard, A. E. and Fernandez, E. and Flaugher, B. and Foley, R. J. and Fosalba, P. and Frieman, J. and Galbany, L. and García-Bellido, J. and Gatti, M. and Gaztanaga, E. and Gerdes, D. W. and Giannantonio, T. and Glazebrook, K. and Goldstein, D. A. and Gruen, D. and Gruendl, R. A. and Gschwend, J. and Gutierrez, G. and Hartley, W. G. and Hinton, S. R. and Hollowood, D. L. and Honscheid, K. and Hoormann, J. K. and Hoyle, B. and Huterer, D. and Jain, B. and James, D. J. and Jarvis, M. and Jeltema, T. and Kasai, E. and Kent, S. and Kessler, R. and Kim, A. G. and Kokron, N. and Krause, E. and Kron, R. and Kuehn, K. and Kuropatkin, N. and Lahav, O. and Lasker, J. and Lemos, P. and Lewis, G. F. and Li, T. S. and Lidman, C. and Lima, M. and Lin, H. and Macaulay, E. and MacCrann, N. and Maia, M. A. G. and March, M. and Marriner, J. and Marshall, J. L. and Martini, P. and McMahon, R. G. and Melchior, P. and Menanteau, F. and Miquel, R. and Mohr, J. J. and Morganson, E. and Muir, J. and Möller, A. and Neilsen, E. and Nichol, R. C. and Nord, B. and Ogando, R. L. C. and Palmese, A. and Pan, Y. -C. and Peiris, H. V. and Percival, W. J. and Plazas, A. A. and Porredon, A. and Prat, J. and Romer, A. K. and Roodman, A. and Rosenfeld, R. and Ross, A. J. and Rykoff, E. S. and Samuroff, S. and Sánchez, C. and Sanchez, E. and Scarpine, V. and Schindler, R. and Schubnell, M. and Scolnic, D. and Secco, L. F. and Serrano, S. and Sevilla-Noarbe, I. and Sharp, R. and Sheldon, E. and Smith, M. and Soares-Santos, M. and Sobreira, F. and Sommer, N. E. and Swann, E. and Swanson, M. E. C. and Tarle, G. and Thomas, D. and Thomas, R. C. and Troxel, M. A. and Tucker, B. E. and Uddin, S. A. and Vielzeuf, P. and Walker, A. R. and Wang, M. and Weaverdyck, N. and Wechsler, R. H. and Weller, J. and Yanny, B. and Zhang, B. and Zhang, Y. and Zuntz, J.},
abstractNote = {The combination of multiple observational probes has long been advocated as a powerful technique to constrain cosmological parameters, in particular dark energy. The Dark Energy Survey has measured 207 spectroscopically--confirmed Type Ia supernova light curves; the baryon acoustic oscillation feature; weak gravitational lensing; and galaxy clustering. Here we present combined results from these probes, deriving constraints on the equation of state, w, of dark energy and its energy density in the Universe. Independently of other experiments, such as those that measure the cosmic microwave background, the probes from this single photometric survey rule out a Universe with no dark energy, finding w=-0.80+0.09-0.11. The geometry is shown to be consistent with a spatially flat Universe, and we obtain a constraint on the baryon density of Ωb=0.069+0.009-0.012 that is independent of early Universe measurements. These results demonstrate the potential power of large multi-probe photometric surveys and pave the way for order of magnitude advances in our constraints on properties of dark energy and cosmology over the next decade.},
doi = {10.1103/PhysRevLett.122.171301},
journal = {Physical Review Letters},
number = 17,
volume = 122,
place = {United States},
year = {Wed May 01 00:00:00 EDT 2019},
month = {Wed May 01 00:00:00 EDT 2019}
}
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redMaGiC: selecting luminous red galaxies from the DES Science Verification data
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  • DOI: 10.1093/mnras/stw1281

Correcting Type Ia Supernova Distances for Selection Biases and Contamination in Photometrically Identified Samples
journal, February 2017

Planck 2015 results : XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation
journal, September 2016

Optimized clustering estimators for BAO measurements accounting for significant redshift uncertainty
text, January 2017

  • Ross, Ashley J.; Banik, Nilanjan; Avila, Santiago
  • Apollo - University of Cambridge Repository
  • DOI: 10.17863/cam.10077

Planck 2015 results : VI. LFI mapmaking
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Planck 2015 results : X. Diffuse component separation: Foreground maps
journal, September 2016

Planck 2015 results : XVI. Isotropy and statistics of the CMB
journal, September 2016

Dark Energy Survey Year 1 Results: Photometric Data Set for Cosmology
text, January 2018

  • Drlica-Wagner, A.; Sevilla-Noarbe, I.; Rykoff, Es
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Planck 2015 results : XXVI. The Second
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Dark Energy Survey Year 1 Results: Calibration of redMaGiC redshift distributions in DES and SDSS from cross-correlations
text, January 2018

  • Cawthon, R.; Davis, C.; Gatti, M.
  • Apollo - University of Cambridge Repository
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The Dark Energy Survey Data Management System
text, January 2008

The Carnegie Supernova Project: First Photometry Data Release of Low-Redshift Type Ia Supernovae
text, January 2009

CfA4: Light Curves for 94 Type Ia Supernovae
text, January 2012

CosmoSIS: modular cosmological parameter estimation
text, January 2014

Planck 2015 results. XIII. Cosmological parameters
text, January 2015

Planck 2015 results. XV. Gravitational lensing
text, January 2015

Automated Transient Identification in the Dark Energy Survey
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Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
text, January 2015

H0LiCOW I. $H_0$ Lenses in COSMOGRAIL's Wellspring: Program Overview
text, January 2016

Practical Weak Lensing Shear Measurement with Metacalibration
text, January 2017

Optimized Clustering Estimators for BAO Measurements Accounting for Significant Redshift Uncertainty
text, January 2017

Forward Global Photometric Calibration of the Dark Energy Survey
text, January 2017

Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
text, January 2017

Dark Energy Survey Year 1 Results: Photometric Data Set for Cosmology
text, January 2017

Dark Energy Survey Year 1 Results: Galaxy-Galaxy Lensing
text, January 2017

Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear
text, January 2017

Dark energy two decades after: Observables, probes, consistency tests
text, January 2017

The Dark Energy Survey Image Processing Pipeline
text, January 2018

Bayesian photometric redshift estimation
text, January 1998

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    Type Ia Supernovae are Excellent Standard Candles in the Near-Infrared
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