Built on

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1901
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Davis TM, Hinton SR, Howlett C, Calcino J (2019) Can redshift errors bias measurements of the Hubble Constant? MNRAS2957:2948–2957. https://doi.org/10.1093/mnras/stz2652 . arXiv:1907.12639
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Desmond H, Jain B, Sakstein J (2019) Local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder. Phys. Rev. D100(4):043537. https://doi.org/10.1103/PhysRevD.100.043537 . arXiv:1907.03778
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Bianchini F, Wu WLK, Ade PAR, et al. (2020) Constraints on Cosmological Parameters from the 500 deg 2 SPTPOL Lensing Power Spectrum . The Astrophysical Journal 888(2):119. https://doi.org/10.3847/1538-4357/ab6082 . arXiv:1910.07157
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2021

A buyer's guide to the Hubble Constant

Shah, Paul, Lemos, Pablo, Lahav, Ofer

Understand

Since the expansion of the universe was first established by Edwin Hubble and Georges Lemaitre about a century ago, the Hubble constant H0 which measures its rate has been of great interest to astronomers.

Besides being interesting in its own right, few properties of the universe can be deduced without it.
In the last decade a significant gap has emerged between different methods of measuring it, some anchored in the nearby universe, others at cosmological distances.
The SH0ES team has found $H_0 = 73.2 \pm 1.3$ km sec$^{-1}$ Mpc$^{-1}$ locally, whereas the value found for the early universe by the Planck Collaboration is $H_0 = 67.4 \pm 0.5$ km sec$^{-1}$ Mpc$^{-1}$ from measurements of the cosmic microwave background.

Built on

Kenworthy WD, Scolnic D, Riess A (2019) The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant. The Astrophysical Journal 875(2):145. https://doi.org/10.3847/1538-4357/ab0ebf , URL http://dx.doi.org/10.3847/1538-4357/ab0ebf . arXiv:1901.08681
Original
1901
Earlier work this paper cites.
Soares-Santos M, et al. (2019) First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary-Black-hole Merger GW170814. ApJ876(1):L7. https://doi.org/10.3847/2041-8213/ab14f1 . arXiv:1901.01540 [astro-ph.CO]
Original
1901
Earlier work this paper cites.
Handley W, Lemos P (2019) Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio. Phys. Rev. D100(4):043504. https://doi.org/10.1103/physrevd.100.043504 . arXiv:1902.04029
Original
1902
Earlier work this paper cites.
Kreisch CD, Cyr-Racine FY, Doré O (2020) Neutrino puzzle: Anomalies, interactions, and cosmological tensions. Phys. Rev. D101(12):123505. https://doi.org/10.1103/PhysRevD.101.123505 . arXiv:1902.00534
Original
1902
Earlier work this paper cites.
Schönrich R, McMillan P, Eyer L (2019) Distances and parallax bias in Gaia DR2. MNRAS487(3):3568–3580. https://doi.org/10.1093/mnras/stz1451 . arXiv:1902.02355
Original
1902
Earlier work this paper cites.
Beaton RL, Birrer S, Dell’Antonio I, et al. (2019) Measuring the Hubble Constant Near and Far in the Era of ELT’s. BAAS51(3):456. arXiv:1903.05035
Original
1903
Earlier work this paper cites.
Pietrzyński G, Graczyk D, Gallenne A, et al. (2019) A distance to the Large Magellanic Cloud that is precise to one per cent. Nature 567(7747):200–203. https://doi.org/10.1038/s41586-019-0999-4 . arXiv:1903.08096
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1903
Earlier work this paper cites.
Agrawal P, Cyr-Racine FY, Pinner D, Randall L (2019) Rock ’n’ Roll Solutions to the Hubble Tension. arXiv e-prints p 1. arXiv:1904.01016
Original
1904
Earlier work this paper cites.
Rameez M (2019) Concerns about the reliability of publicly available SNe Ia data. arXiv e-prints arXiv:1905.00221
Original
1905
Earlier work this paper cites.
Chen GCF, Fassnacht CD, Suyu SH, et al. (2019) A SHARP view of H0LiCOW: H0 from three time-delay gravitational lens systems with adaptive optics imaging. MNRAS490(2):1743–1773. https://doi.org/10.1093/mnras/stz2547 . arXiv:1907.02533
Original
1907
Earlier work this paper cites.
Davis TM, Hinton SR, Howlett C, Calcino J (2019) Can redshift errors bias measurements of the Hubble Constant? MNRAS2957:2948–2957. https://doi.org/10.1093/mnras/stz2652 . arXiv:1907.12639
Original
1907
Earlier work this paper cites.
Desmond H, Jain B, Sakstein J (2019) Local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder. Phys. Rev. D100(4):043537. https://doi.org/10.1103/PhysRevD.100.043537 . arXiv:1907.03778
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1907
Earlier work this paper cites.
Freedman WL, Madore BF, Hatt D, et al. (2019) The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch. ApJ882(1):34. https://doi.org/10.3847/1538-4357/ab2f73 . arXiv:1907.05922
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1907
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Vagnozzi S (2020) New physics in light of the H0 tension: An alternative view. Phys. Rev. D102(2):023518. https://doi.org/10.1103/PhysRevD.102.023518 . arXiv:1907.07569
Original
1907
Earlier work this paper cites.
Wong KC, Suyu SH, Chen GCF, et al. (2020) H0LiCOW XIII. A 2.4% measurement of H0 from lensed quasars: 5.3 sigma tension between early and late-Universe probes. MNRAS498(1):1440–1468. arXiv:1907.04869
Original
1907
Earlier work this paper cites.
Huang CD, Riess AG, Yuan W, et al. (2020) Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant. ApJ889(1). arXiv:1908.10883
Original
1908
Earlier work this paper cites.
Knox L, Millea M (2020) Hubble constant hunter’s guide. Phys. Rev. D101(4):043533. https://doi.org/10.1103/PhysRevD.101.043533 . arXiv:1908.03663 [astro-ph.CO]
Original
1908
Earlier work this paper cites.
Reid MJ, Pesce DW, Riess AG (2019) An Improved Distance to NGC 4258 and its Implications for the Hubble Constant. ApJ886(2):L27. https://doi.org/10.3847/2041-8213/ab552d . arXiv:1908.05625
Original
1908
Earlier work this paper cites.
Yuan W, Riess AG, Macri LM, Casertano S, Scolnic DM (2019) Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Redetermination of the Hubble Constant. ApJ886(1):61. https://doi.org/10.3847/1538-4357/ab4bc9 . arXiv:1908.00993
Original
1908
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Howlett C, Davis TM (2020) Standard siren speeds: Improving velocities in gravitational-wave measurements of H0. Monthly Notices of the Royal Astronomical Society 3815(3):3803–3815. https://doi.org/10.1093/mnras/staa049 . arXiv:1909.00587
Original
1909
Earlier work this paper cites.
Mukherjee S, Lavaux G, Bouchet FR, et al. (2021) Velocity correction for Hubble constant measurements from standard sirens. Astronomy and Astrophysics 646:1–11. https://doi.org/10.1051/0004-6361/201936724 . arXiv:1909.08627
Original
1909
Earlier work this paper cites.
Nicolaou C, Lahav O, Lemos P, Hartley W, Braden J (2020) The impact of peculiar velocities on the estimation of the Hubble constant from gravitational wave standard sirens. MNRAS495(1):90–97. https://doi.org/10.1093/mnras/staa1120 . arXiv:1909.09609
Original
1909
Earlier work this paper cites.
Bianchini F, Wu WLK, Ade PAR, et al. (2020) Constraints on Cosmological Parameters from the 500 deg 2 SPTPOL Lensing Power Spectrum . The Astrophysical Journal 888(2):119. https://doi.org/10.3847/1538-4357/ab6082 . arXiv:1910.07157
Original
1910
Earlier work this paper cites.
Efstathiou GP, Gratton S (2019) A detailed description of the CamSpec likelihood pipeline and a reanalysis of the Planck high frequency maps. arXiv arXiv:1910.00483
Original
1910
Earlier work this paper cites.
Yao Y, Miller AA, Kulkarni SR, et al. (2019) ZTF Early Observations of Type Ia Supernovae I: Properties of the 2018 Sample. ApJ886(2):152. https://doi.org/10.3847/1538-4357/ab4cf5 . arXiv:1910.02967
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1910
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Holoien TWS, Brown JS, Vallely PJ, et al. (2018) The ASAS-SN Bright Supernova Catalog – IV. 2017. MNRAS484(2):1899–1911. https://doi.org/10.1093/mnras/stz073 . arXiv:1811.08904
Original
1911
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Einstein A (1917) Kosmologische Betrachtungen zur allgemeinen Relativitätstheorie, translation available at https://einsteinpapers.press.princeton.edu/vol6-trans/433 . Sitzungsber Königl Preuss Akad Wissenschaft pp 142–152
1917
Earlier work this paper cites.
Friedmann A (1922) On the Curvature of Space. Zeitschrift Fuer Physik 10:377–386. https://doi.org/10.1023/A:1026751225741 , URL https://link.springer.com/article/10.1023{%}2FA{%}3A1026751225741
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Earlier work this paper cites.
Malmquist K (1922) On some relations in stellar statistics. Ark Mat Astron Fys 16(23)
1922
Earlier work this paper cites.
Lemaître G (1927) Un Univers Homogene De Mass Constante. Annales de la Société Scientifique de Bruxelles 47A:49–59
1927
Earlier work this paper cites.
Gerasimovic BP (1928) The Absolute Magnitudes of Long Period Variable Stars. PNAS 14(12):963–968. https://doi.org/10.1073/pnas.14.12.963
1928
Earlier work this paper cites.
Hubble E (1929) A relation between distance and radial velocity amoung extra-galactic nebulae. PNAS pp 168–173
1929
Earlier work this paper cites.
Etherington IMH (1933) Republication of: LX. on the definition of distance in general relativity. Gen Relativ Gravit 39(7):1055–1067. https://doi.org/10.1007/s10714-007-0447-x
1933
Earlier work this paper cites.
Fixsen DJ (2009) The temperature of the cosmic microwave background. ApJ707(2):916–920. https://doi.org/10.1088/0004-637X/707/2/916 . arXiv:0911.1955
Original
1955
Earlier work this paper cites.
Sandage A (1958) Current problems in the Extragalactic Distance Scale. ApJ127(3):513–526. https://doi.org/10.1017/CBO9781107415324.004 . arXiv:arXiv:1011.1669v3
Original
1958
Earlier work this paper cites.
Cox JP (1960) Theory of Stellar Pulsation, princeton legacy library edition edn. Princeton Series in Astrophysics ; 31, Princeton University Press
1960
Earlier work this paper cites.
Sachs RK, Wolfe AM (1967) Perturbations of a Cosmological Model and Angular Variations of the Microwave Background. ApJ147:73. https://doi.org/10.1086/148982
1967
Earlier work this paper cites.
Silk J (1968) Cosmic Black-Body Radiation and Galaxy Formation. ApJ151(February):459
1968
Earlier work this paper cites.
Sunyaev RA, Zel’dovich YB (1972) The observation of relic radiation as a test of the nature of X-ray radiation from the clusters of galaxies. Comments on Astrophysics and Space Physics 4:173
1972
Earlier work this paper cites.
Lutz TE, Kelker DH (1973) On the use of Trigonometric Parallaxes for the Calibration of Luminosity Systems: Theory. PASP85(October):573
1973
Earlier work this paper cites.
Brent Tully R, Fisher J (1976) A New Method of Determining Distances to Galaxies. A&A54:661–673
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