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Title: Cosmological implications of baryon acoustic oscillation measurements

Abstract

We derive constraints on cosmological parameters and tests of dark energy models from the combination of baryon acoustic oscillation (BAO) measurements with cosmic microwave background (CMB) data and a recent reanalysis of Type Ia supernova (SN) data. In particular, we take advantage of high-precision BAO measurements from galaxy clustering and the Lyman-α forest (LyaF) in the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS). Treating the BAO scale as an uncalibrated standard ruler, BAO data alone yield a high confidence detection of dark energy; in combination with the CMB angular acoustic scale they further imply a nearly flat universe. Adding the CMB-calibrated physical scale of the sound horizon, the combination of BAO and SN data into an "inverse distance ladder" yields a measurement of H0=67.3±1.1 km s-1 Mpc-1, with 1.7% precision. This measurement assumes standard prerecombination physics but is insensitive to assumptions about dark energy or space curvature, so agreement with CMB-based estimates that assume a flat ΛCDM cosmology is an important corroboration of this minimal cosmological model. For constant dark energy (Λ), our BAO+SN+CMB combination yields matter density Ωm=0.301±0.008 and curvature Ωk=-0.003±0.003. When we allow more general forms of evolving dark energy, the BAO+SN+CMB parameter constraints are always consistent with flatmore » ΛCDM values at ≈1σ. While the overall χ2 of model fits is satisfactory, the LyaF BAO measurements are in moderate (2-2.5σ) tension with model predictions. Models with early dark energy that tracks the dominant energy component at high redshift remain consistent with our expansion history constraints, and they yield a higher H0 and lower matter clustering amplitude, improving agreement with some low redshift observations. Expansion history alone yields an upper limit on the summed mass of neutrino species, mν < 0.56 eV (95% confidence), improving to mν < 0.25 eV if we include the lensing signal in the Planck CMB power spectrum. In a flat ΛCDM model that allows extra relativistic species, our data combination yields Neff=3.43±0.26; while the LyaF BAO data prefer higher Neff when excluding galaxy BAO, the galaxy BAO alone favor Neff≈3. When structure growth is extrapolated forward from the CMB to low redshift, standard dark energy models constrained by our data predict a level of matter clustering that is high compared to most, but not all, observational estimates.« less

Authors:
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Publication Date:
Research Org.:
Brookhaven National Laboratory (BNL), Upton, NY (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)
Contributing Org.:
BOSS Collaboration
OSTI Identifier:
1335432
Alternate Identifier(s):
OSTI ID: 1229593; OSTI ID: 1335397; OSTI ID: 1378692
Report Number(s):
BNL-112091-2016-JA; BNL-111835-2016-JA
Journal ID: ISSN 1550-7998; PRVDAQ; KA2301020
Grant/Contract Number:  
SC00112704; AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review. D, Particles, Fields, Gravitation and Cosmology
Additional Journal Information:
Journal Volume: 92; Journal Issue: 12; Journal ID: ISSN 1550-7998
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS

Citation Formats

Aubourg, Éric, Bailey, Stephen, Bautista, Julian E., Beutler, Florian, Bhardwaj, Vaishali, Bizyaev, Dmitry, Blanton, Michael, Blomqvist, Michael, Bolton, Adam S., Bovy, Jo, Brewington, Howard, Brinkmann, J., Brownstein, Joel R., Burden, Angela, Busca, Nicolás G., Carithers, William, Chuang, Chia-Hsun, Comparat, Johan, Croft, Rupert A. C., Cuesta, Antonio J., Dawson, Kyle S., Delubac, Timothée, Eisenstein, Daniel J., Font-Ribera, Andreu, Ge, Jian, Le Goff, J. -M., Gontcho, Satya Gontcho A., Gott, J. Richard, Gunn, James E., Guo, Hong, Guy, Julien, Hamilton, Jean-Christophe, Ho, Shirley, Honscheid, Klaus, Howlett, Cullan, Kirkby, David, Kitaura, Francisco S., Kneib, Jean-Paul, Lee, Khee-Gan, Long, Dan, Lupton, Robert H., Magaña, Mariana Vargas, Malanushenko, Viktor, Malanushenko, Elena, Manera, Marc, Maraston, Claudia, Margala, Daniel, McBride, Cameron K., Miralda-Escudé, Jordi, Myers, Adam D., Nichol, Robert C., Noterdaeme, Pasquier, Nuza, Sebastián E., Olmstead, Matthew D., Oravetz, Daniel, Pâris, Isabelle, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Pan, Kaike, Pellejero-Ibanez, Marcos, Percival, Will J., Petitjean, Patrick, Pieri, Matthew M., Prada, Francisco, Reid, Beth, Rich, James, Roe, Natalie A., Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rubiño-Martín, Jose Alberto, Sánchez, Ariel G., Samushia, Lado, Santos, Ricardo Tanausú Génova, Scóccola, Claudia G., Schlegel, David J., Schneider, Donald P., Seo, Hee-Jong, Sheldon, Erin, Simmons, Audrey, Skibba, Ramin A., Slosar, Anže, Strauss, Michael A., Thomas, Daniel, Tinker, Jeremy L., Tojeiro, Rita, Vazquez, Jose Alberto, Viel, Matteo, Wake, David A., Weaver, Benjamin A., Weinberg, David H., Wood-Vasey, W. M., Yèche, Christophe, Zehavi, Idit, and Zhao, Gong-Bo. Cosmological implications of baryon acoustic oscillation measurements. United States: N. p., 2015. Web. doi:10.1103/PhysRevD.92.123516.
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Aubourg, Éric, Bailey, Stephen, Bautista, Julian E., Beutler, Florian, Bhardwaj, Vaishali, Bizyaev, Dmitry, Blanton, Michael, Blomqvist, Michael, Bolton, Adam S., Bovy, Jo, Brewington, Howard, Brinkmann, J., Brownstein, Joel R., Burden, Angela, Busca, Nicolás G., Carithers, William, Chuang, Chia-Hsun, Comparat, Johan, Croft, Rupert A. C., Cuesta, Antonio J., Dawson, Kyle S., Delubac, Timothée, Eisenstein, Daniel J., Font-Ribera, Andreu, Ge, Jian, Le Goff, J. -M., Gontcho, Satya Gontcho A., Gott, J. Richard, Gunn, James E., Guo, Hong, Guy, Julien, Hamilton, Jean-Christophe, Ho, Shirley, Honscheid, Klaus, Howlett, Cullan, Kirkby, David, Kitaura, Francisco S., Kneib, Jean-Paul, Lee, Khee-Gan, Long, Dan, Lupton, Robert H., Magaña, Mariana Vargas, Malanushenko, Viktor, Malanushenko, Elena, Manera, Marc, Maraston, Claudia, Margala, Daniel, McBride, Cameron K., Miralda-Escudé, Jordi, Myers, Adam D., Nichol, Robert C., Noterdaeme, Pasquier, Nuza, Sebastián E., Olmstead, Matthew D., Oravetz, Daniel, Pâris, Isabelle, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Pan, Kaike, Pellejero-Ibanez, Marcos, Percival, Will J., Petitjean, Patrick, Pieri, Matthew M., Prada, Francisco, Reid, Beth, Rich, James, Roe, Natalie A., Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rubiño-Martín, Jose Alberto, Sánchez, Ariel G., Samushia, Lado, Santos, Ricardo Tanausú Génova, Scóccola, Claudia G., Schlegel, David J., Schneider, Donald P., Seo, Hee-Jong, Sheldon, Erin, Simmons, Audrey, Skibba, Ramin A., Slosar, Anže, Strauss, Michael A., Thomas, Daniel, Tinker, Jeremy L., Tojeiro, Rita, Vazquez, Jose Alberto, Viel, Matteo, Wake, David A., Weaver, Benjamin A., Weinberg, David H., Wood-Vasey, W. M., Yèche, Christophe, Zehavi, Idit, & Zhao, Gong-Bo. Cosmological implications of baryon acoustic oscillation measurements. United States. https://doi.org/10.1103/PhysRevD.92.123516
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Aubourg, Éric, Bailey, Stephen, Bautista, Julian E., Beutler, Florian, Bhardwaj, Vaishali, Bizyaev, Dmitry, Blanton, Michael, Blomqvist, Michael, Bolton, Adam S., Bovy, Jo, Brewington, Howard, Brinkmann, J., Brownstein, Joel R., Burden, Angela, Busca, Nicolás G., Carithers, William, Chuang, Chia-Hsun, Comparat, Johan, Croft, Rupert A. C., Cuesta, Antonio J., Dawson, Kyle S., Delubac, Timothée, Eisenstein, Daniel J., Font-Ribera, Andreu, Ge, Jian, Le Goff, J. -M., Gontcho, Satya Gontcho A., Gott, J. Richard, Gunn, James E., Guo, Hong, Guy, Julien, Hamilton, Jean-Christophe, Ho, Shirley, Honscheid, Klaus, Howlett, Cullan, Kirkby, David, Kitaura, Francisco S., Kneib, Jean-Paul, Lee, Khee-Gan, Long, Dan, Lupton, Robert H., Magaña, Mariana Vargas, Malanushenko, Viktor, Malanushenko, Elena, Manera, Marc, Maraston, Claudia, Margala, Daniel, McBride, Cameron K., Miralda-Escudé, Jordi, Myers, Adam D., Nichol, Robert C., Noterdaeme, Pasquier, Nuza, Sebastián E., Olmstead, Matthew D., Oravetz, Daniel, Pâris, Isabelle, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Pan, Kaike, Pellejero-Ibanez, Marcos, Percival, Will J., Petitjean, Patrick, Pieri, Matthew M., Prada, Francisco, Reid, Beth, Rich, James, Roe, Natalie A., Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rubiño-Martín, Jose Alberto, Sánchez, Ariel G., Samushia, Lado, Santos, Ricardo Tanausú Génova, Scóccola, Claudia G., Schlegel, David J., Schneider, Donald P., Seo, Hee-Jong, Sheldon, Erin, Simmons, Audrey, Skibba, Ramin A., Slosar, Anže, Strauss, Michael A., Thomas, Daniel, Tinker, Jeremy L., Tojeiro, Rita, Vazquez, Jose Alberto, Viel, Matteo, Wake, David A., Weaver, Benjamin A., Weinberg, David H., Wood-Vasey, W. M., Yèche, Christophe, Zehavi, Idit, and Zhao, Gong-Bo. Mon . "Cosmological implications of baryon acoustic oscillation measurements". United States. https://doi.org/10.1103/PhysRevD.92.123516. https://www.osti.gov/servlets/purl/1335432.
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@article{osti_1335432,
title = {Cosmological implications of baryon acoustic oscillation measurements},
author = {Aubourg, Éric and Bailey, Stephen and Bautista, Julian E. and Beutler, Florian and Bhardwaj, Vaishali and Bizyaev, Dmitry and Blanton, Michael and Blomqvist, Michael and Bolton, Adam S. and Bovy, Jo and Brewington, Howard and Brinkmann, J. and Brownstein, Joel R. and Burden, Angela and Busca, Nicolás G. and Carithers, William and Chuang, Chia-Hsun and Comparat, Johan and Croft, Rupert A. C. and Cuesta, Antonio J. and Dawson, Kyle S. and Delubac, Timothée and Eisenstein, Daniel J. and Font-Ribera, Andreu and Ge, Jian and Le Goff, J. -M. and Gontcho, Satya Gontcho A. and Gott, J. Richard and Gunn, James E. and Guo, Hong and Guy, Julien and Hamilton, Jean-Christophe and Ho, Shirley and Honscheid, Klaus and Howlett, Cullan and Kirkby, David and Kitaura, Francisco S. and Kneib, Jean-Paul and Lee, Khee-Gan and Long, Dan and Lupton, Robert H. and Magaña, Mariana Vargas and Malanushenko, Viktor and Malanushenko, Elena and Manera, Marc and Maraston, Claudia and Margala, Daniel and McBride, Cameron K. and Miralda-Escudé, Jordi and Myers, Adam D. and Nichol, Robert C. and Noterdaeme, Pasquier and Nuza, Sebastián E. and Olmstead, Matthew D. and Oravetz, Daniel and Pâris, Isabelle and Padmanabhan, Nikhil and Palanque-Delabrouille, Nathalie and Pan, Kaike and Pellejero-Ibanez, Marcos and Percival, Will J. and Petitjean, Patrick and Pieri, Matthew M. and Prada, Francisco and Reid, Beth and Rich, James and Roe, Natalie A. and Ross, Ashley J. and Ross, Nicholas P. and Rossi, Graziano and Rubiño-Martín, Jose Alberto and Sánchez, Ariel G. and Samushia, Lado and Santos, Ricardo Tanausú Génova and Scóccola, Claudia G. and Schlegel, David J. and Schneider, Donald P. and Seo, Hee-Jong and Sheldon, Erin and Simmons, Audrey and Skibba, Ramin A. and Slosar, Anže and Strauss, Michael A. and Thomas, Daniel and Tinker, Jeremy L. and Tojeiro, Rita and Vazquez, Jose Alberto and Viel, Matteo and Wake, David A. and Weaver, Benjamin A. and Weinberg, David H. and Wood-Vasey, W. M. and Yèche, Christophe and Zehavi, Idit and Zhao, Gong-Bo},
abstractNote = {We derive constraints on cosmological parameters and tests of dark energy models from the combination of baryon acoustic oscillation (BAO) measurements with cosmic microwave background (CMB) data and a recent reanalysis of Type Ia supernova (SN) data. In particular, we take advantage of high-precision BAO measurements from galaxy clustering and the Lyman-α forest (LyaF) in the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS). Treating the BAO scale as an uncalibrated standard ruler, BAO data alone yield a high confidence detection of dark energy; in combination with the CMB angular acoustic scale they further imply a nearly flat universe. Adding the CMB-calibrated physical scale of the sound horizon, the combination of BAO and SN data into an "inverse distance ladder" yields a measurement of H0=67.3±1.1 km s-1 Mpc-1, with 1.7% precision. This measurement assumes standard prerecombination physics but is insensitive to assumptions about dark energy or space curvature, so agreement with CMB-based estimates that assume a flat ΛCDM cosmology is an important corroboration of this minimal cosmological model. For constant dark energy (Λ), our BAO+SN+CMB combination yields matter density Ωm=0.301±0.008 and curvature Ωk=-0.003±0.003. When we allow more general forms of evolving dark energy, the BAO+SN+CMB parameter constraints are always consistent with flat ΛCDM values at ≈1σ. While the overall χ2 of model fits is satisfactory, the LyaF BAO measurements are in moderate (2-2.5σ) tension with model predictions. Models with early dark energy that tracks the dominant energy component at high redshift remain consistent with our expansion history constraints, and they yield a higher H0 and lower matter clustering amplitude, improving agreement with some low redshift observations. Expansion history alone yields an upper limit on the summed mass of neutrino species, mν < 0.56 eV (95% confidence), improving to mν < 0.25 eV if we include the lensing signal in the Planck CMB power spectrum. In a flat ΛCDM model that allows extra relativistic species, our data combination yields Neff=3.43±0.26; while the LyaF BAO data prefer higher Neff when excluding galaxy BAO, the galaxy BAO alone favor Neff≈3. When structure growth is extrapolated forward from the CMB to low redshift, standard dark energy models constrained by our data predict a level of matter clustering that is high compared to most, but not all, observational estimates.},
doi = {10.1103/PhysRevD.92.123516},
journal = {Physical Review. D, Particles, Fields, Gravitation and Cosmology},
number = 12,
volume = 92,
place = {United States},
year = {Mon Dec 14 00:00:00 EST 2015},
month = {Mon Dec 14 00:00:00 EST 2015}
}
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Detection of the Baryon Acoustic Peak in the Large‐Scale Correlation Function of SDSS Luminous Red Galaxies
journal, November 2005

  • Eisenstein, Daniel J.; Zehavi, Idit; Hogg, David W.
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Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
journal, August 2014

The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations: WiggleZ Survey: BAOs in redshift slices
journal, October 2011

The Weak Lensing Signal and the Clustering of BOSS Galaxies II: Astrophysical and Cosmological Constraints
text, January 2015

  • More, Surhud; Miyatake, Hironao; Mandelbaum, Rachel
  • Carnegie Mellon University
  • DOI: 10.1184/r1/6509375

CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA
text, January 2009

  • Mark, Everett,; Kyle, Smalley,; Diab, Jerius,
  • The University of North Carolina at Chapel Hill University Libraries
  • DOI: 10.17615/adda-h866

Cosmology with decaying particles
report, September 1984

Measurement of baryon acoustic oscillations in the Lyman-α forest fluctuations in BOSS data release 9
text, January 2013

Cosmological parameter constraints from galaxy-galaxy lensing and galaxy clustering with the SDSS DR7
text, January 2013

Model Independent Early Expansion History and Dark Energy
text, January 2012

Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
text, January 2013

Neutrino clustering around spherical dark matter halos
text, January 2013

The Sloan Digital Sky Survey quasar catalog: tenth data release
text, January 2013

Weighing the Giants IV: Cosmology and Neutrino Mass
text, January 2014

Cosmic Discordance: Are Planck CMB and CFHTLenS weak lensing measurements out of tune?
preprint, January 2014

Towards a Precise Measurement of Matter Clustering: Lyman-alpha Forest Data at Redshifts 2-4
text, January 2000

Efficient Cosmological Parameter Estimation from Microwave Background Anisotropies
text, January 2002

Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
text, January 2002

The Lyman-α forest in three dimensions: measurements of large scale flux correlations from BOSS 1st-year data
text, January 2011

  • Slosar, A.; Font-Ribera, A.; Pieri, M. M.
  • Institute of Physics Publishing
  • DOI: 10.5167/uzh-60152
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    journal, February 2020

    The Simons Observatory: Science goals and forecasts
    text, January 2019

    • Ade, P.; Aguirre, J.; Ahmed, Z.
    • Apollo - University of Cambridge Repository
    • DOI: 10.17863/cam.38168

    Dynamical Effects of the Scale Invariance of the Empty Space: The Fall of Dark Matter?
    journal, November 2017

    Probing Cosmic Acceleration Using Model-independent Parameterizations and Three Kinds of Supernova Statistics Techniques
    journal, March 2019

    Sounds Discordant: Classical Distance Ladder and ΛCDM-based Determinations of the Cosmological Sound Horizon
    journal, March 2019

    Are H 0 and σ 8 Tensions Generic to Present Cosmological Data?
    journal, May 2019

    • Bhattacharyya, Archita; Alam, Ujjaini; Pandey, Kanhaiya Lal
    • The Astrophysical Journal, Vol. 876, Issue 2
    • DOI: 10.3847/1538-4357/ab12d6

    A Future Percent-level Measurement of the Hubble Expansion at Redshift 0.8 with Advanced LIGO
    journal, October 2019

    Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
    journal, August 2019

    Cosmological constraints from the Hubble diagram of quasars at high redshifts
    journal, January 2019

    Cosmology with gamma-ray bursts: II. Cosmography challenges and cosmological scenarios for the accelerated Universe
    journal, February 2017

    Constraining the cosmic deceleration-acceleration transition with type Ia supernova, BAO/CMB and H(z) data
    journal, February 2016

    • Santos, M. Vargas dos; Reis, R. R. R.; Waga, I.
    • Journal of Cosmology and Astroparticle Physics, Vol. 2016, Issue 02
    • DOI: 10.1088/1475-7516/2016/02/066

    Possible signals of vacuum dynamics in the Universe
    journal, May 2018

    • Solà Peracaula, Joan; de Cruz Pérez, Javier; Gómez-Valent, Adrià
    • Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 4
    • DOI: 10.1093/mnras/sty1253

    Constraining the microlensing effect on time delays with a new time-delay prediction model in H0 measurements
    journal, September 2018

    • Chen, Geoff C-F; Chan, James H. H.; Bonvin, Vivien
    • Monthly Notices of the Royal Astronomical Society, Vol. 481, Issue 1
    • DOI: 10.1093/mnras/sty2350

    Simultaneous calibration of spectro-photometric distances and the Gaia DR2 parallax zero-point offset with deep learning
    journal, August 2019

    • Leung, Henry W.; Bovy, Jo
    • Monthly Notices of the Royal Astronomical Society, Vol. 489, Issue 2
    • DOI: 10.1093/mnras/stz2245

    Atomic interferometry test of dark energy
    journal, November 2016

    Cosmological Distance Indicators
    journal, July 2018

    • Suyu, Sherry H.; Chang, Tzu-Ching; Courbin, Frédéric
    • Space Science Reviews, Vol. 214, Issue 5
    • DOI: 10.1007/s11214-018-0524-3

    Dynamical dark energy in light of the latest observations
    journal, August 2017

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

    Constraining early and interacting dark energy with gravitational wave standard sirens: the potential of the eLISA mission
    journal, October 2016

    Density perturbations for running vacuum: a successful approach to structure formation and to the σ8-tension
    journal, April 2018

    • Gómez-Valent, Adrià; Solà Peracaula, Joan
    • Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 1
    • DOI: 10.1093/mnras/sty1028

    First study of reionization in the Planck 2015 normalized closed ΛCDM inflation model
    journal, July 2018

    • Mitra, Sourav; Choudhury, Tirthankar Roy; Ratra, Bharat
    • Monthly Notices of the Royal Astronomical Society, Vol. 479, Issue 4
    • DOI: 10.1093/mnras/sty1835

    Cosmology with powerful radio-loud AGNs
    journal, March 2019

    • Turner, Ross J.; Shabala, Stanislav S.
    • Monthly Notices of the Royal Astronomical Society, Vol. 486, Issue 1
    • DOI: 10.1093/mnras/stz922

    First cosmological results using Type Ia supernovae from the Dark Energy Survey: measurement of the Hubble constant
    journal, April 2019

    • Macaulay, E.; Nichol, R. C.; Bacon, D.
    • Monthly Notices of the Royal Astronomical Society, Vol. 486, Issue 2
    • DOI: 10.1093/mnras/stz978

    Cosmological tests of an axiverse-inspired quintessence field
    journal, June 2016

    Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
    text, January 2017

    • Blanton, Mr; Bershady, Ma; Abolfathi, B.
    • Apollo - University of Cambridge Repository
    • DOI: 10.17863/cam.25008

    Model independent H(z) reconstruction using the cosmic inverse distance ladder
    text, January 2019

    • Lemos, P.; Lee, E.; Efstathiou, George
    • Apollo - University of Cambridge Repository
    • DOI: 10.17863/cam.38453

    A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light $\gamma$-ray attenuation
    text, January 2019

    • Domínguez, Alberto; Wojtak, Radoslaw; Finke, Justin
    • Deutsches Elektronen-Synchrotron, DESY, Hamburg
    • DOI: 10.3204/pubdb-2020-00208

    The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
    other, January 2019

    • Freedman, Wendy L.; Madore, Barry F.; Hatt, Dylan
    • London : Institute of Physics Publ.
    • DOI: 10.34657/5339

    Planck 2015 Constraints on the Non-flat ΛCDM Inflation Model
    journal, August 2018

    • Ooba, Junpei; Ratra, Bharat; Sugiyama, Naoshi
    • The Astrophysical Journal, Vol. 864, Issue 1
    • DOI: 10.3847/1538-4357/aad633

    Photometric Redshift Calibration Requirements for WFIRST Weak-lensing Cosmology: Predictions from CANDELS
    journal, June 2019

    • Hemmati, Shoubaneh; Capak, Peter; Masters, Daniel
    • The Astrophysical Journal, Vol. 877, Issue 2
    • DOI: 10.3847/1538-4357/ab1be5

    Planck 2015 results : XXVI. The Second
    journal, September 2016

    H i and cosmological constraints from intensity mapping, optical and CMB surveys
    journal, June 2017

    • Pourtsidou, Alkistis; Bacon, David; Crittenden, Robert
    • Monthly Notices of the Royal Astronomical Society, Vol. 470, Issue 4
    • DOI: 10.1093/mnras/stx1479

    Sample variance in the local measurements of the Hubble constant
    journal, August 2017

    • Wu, Hao-Yi; Huterer, Dragan
    • Monthly Notices of the Royal Astronomical Society, Vol. 471, Issue 4
    • DOI: 10.1093/mnras/stx1967

    H0LiCOW – I. H0 Lenses in COSMOGRAIL's Wellspring: program overview
    journal, February 2017

    • Suyu, S. H.; Bonvin, V.; Courbin, F.
    • Monthly Notices of the Royal Astronomical Society, Vol. 468, Issue 3
    • DOI: 10.1093/mnras/stx483

    Impact of simulated 1/f noise for HI intensity mapping experiments
    journal, May 2018

    • Harper, S. E.; Dickinson, C.; Battye, R. A.
    • Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 2
    • DOI: 10.1093/mnras/sty1238

    The varying cosmological constant: a new approximation to the Friedmann equations and universe model
    journal, January 2018

    • Öztaş, Ahmet M.; Dil, Emre; Smith, Michael L.
    • Monthly Notices of the Royal Astronomical Society, Vol. 476, Issue 1
    • DOI: 10.1093/mnras/sty221

    Insensitivity of the distance ladder Hubble constant determination to Cepheid calibration modelling choices
    journal, March 2018

    • Follin, B.; Knox, L.
    • Monthly Notices of the Royal Astronomical Society, Vol. 477, Issue 4
    • DOI: 10.1093/mnras/sty720

    General cosmography model with spatial curvature
    journal, December 2019

    • Li, En-Kun; Du, Minghui; Xu, Lixin
    • Monthly Notices of the Royal Astronomical Society, Vol. 491, Issue 4
    • DOI: 10.1093/mnras/stz3308

    Probing dark energy in the scope of a Bianchi type I spacetime
    journal, March 2018

    Cosmic distance inference from purely geometric BAO methods: Linear point standard ruler and correlation function model fitting
    journal, June 2019

    • Anselmi, Stefano; Corasaniti, Pier-Stefano; Sanchez, Ariel G.
    • Physical Review D, Vol. 99, Issue 12
    • DOI: 10.1103/physrevd.99.123515

    Flavor versus mass eigenstates in neutrino asymmetries: implications for cosmology
    journal, September 2017

    Constraining the dark energy equation of state with H ii galaxies
    text, January 2016

    • Chávez, R.; Plionis, M.; Basilakos, S.
    • Apollo - University of Cambridge Repository
    • DOI: 10.17863/cam.4507

    An Alternative to the Λcdm Model: the case of Scale Invariance
    journal, January 2017

    An Evaluation of Cosmological Models from the Expansion and Growth of Structure Measurements
    journal, December 2017

    • Zhai, Zhongxu; Blanton, Michael; Slosar, Anže
    • The Astrophysical Journal, Vol. 850, Issue 2
    • DOI: 10.3847/1538-4357/aa9888

    Measuring neutrino masses with large-scale structure: Euclid forecast with controlled theoretical error
    journal, November 2019

    Constraints on the interacting vacuum–geodesic CDM scenario
    journal, July 2019

    • Martinelli, Matteo; Hogg, Natalie B.; Peirone, Simone
    • Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 3
    • DOI: 10.1093/mnras/stz1915

    Friedmann–Robertson–Walker (FRW) cosmological model in the present perspective
    journal, June 2019

    A 2.4% Determination of the Local Value of the Hubble Constant
    text, January 2016

    Constraining the Cosmology of the Phantom Brane using Distance Measures
    text, January 2016

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

    Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
    text, January 2017

    Is exponential gravity a viable description for the whole cosmological history?
    text, January 2017

    Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data
    text, January 2017

    A Hubble constant measurement from superluminal motion of the jet in GW170817
    preprint, January 2018

    Hot Axions and the $H_0$ tension
    text, January 2018

    Low redshift observational constraints on tachyon models of dark energy
    text, January 2018

    The local and distant Universe: stellar ages and $H_0$
    text, January 2019

    Cosmology with powerful radio-loud AGNs
    text, January 2019

    Can redshift errors bias measurements of the Hubble Constant?
    text, January 2019

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