DETERMINING THE HUBBLE CONSTANT FROM HUBBLE PARAMETER MEASUREMENTS
We use 28 measurements of the Hubble parameter, H(z), at intermediate redshifts to determine the present-day Hubble constant H0 in four cosmological models. We measure , and Mpc−1 (1 errors) in the ΛCDM (spatially flat and non-flat), CDM, and φCDM models, respectively. These measured H0 values are m...
Gespeichert in:
| Veröffentlicht in: | The Astrophysical journal Jg. 835; H. 1; S. 86 - 89 |
|---|---|
| Hauptverfasser: | , , |
| Format: | Journal Article |
| Sprache: | Englisch |
| Veröffentlicht: |
Philadelphia
The American Astronomical Society
20.01.2017
IOP Publishing Institute of Physics (IOP) |
| Schlagworte: | |
| ISSN: | 0004-637X, 1538-4357, 1538-4357 |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| Abstract | We use 28 measurements of the Hubble parameter, H(z), at intermediate redshifts to determine the present-day Hubble constant H0 in four cosmological models. We measure , and Mpc−1 (1 errors) in the ΛCDM (spatially flat and non-flat), CDM, and φCDM models, respectively. These measured H0 values are more consistent with the lower values determined from recent data on the cosmic microwave background and baryon acoustic oscillations, as well as with the value found from a median statistical analysis of Huchra's compilation of H0 measurements, but include the higher local measurements of H0 within the 2 confidence limits. |
|---|---|
| AbstractList | We use 28 measurements of the Hubble parameter, H(z), at intermediate redshifts to determine the present-day Hubble constant H0 in four cosmological models. We measure , and Mpc−1 (1 errors) in the ΛCDM (spatially flat and non-flat), CDM, and φCDM models, respectively. These measured H0 values are more consistent with the lower values determined from recent data on the cosmic microwave background and baryon acoustic oscillations, as well as with the value found from a median statistical analysis of Huchra's compilation of H0 measurements, but include the higher local measurements of H0 within the 2 confidence limits. We use 28 measurements of the Hubble parameter, H(z), at intermediate redshifts \(0.07\leqslant z\leqslant 2.3\) to determine the present-day Hubble constant H0 in four cosmological models. We measure \({H}_{0}={68.3}_{-2.6}^{+2.7},{68.4}_{-3.3}^{+2.9},{65.0}_{-6.6}^{+6.5}\), and \({67.9}_{-2.4}^{+2.4}\,\mathrm{km}\ {{\rm{s}}}^{-1}\) Mpc−1 (1σ errors) in the ΛCDM (spatially flat and non-flat), ωCDM, and ϕCDM models, respectively. These measured H0 values are more consistent with the lower values determined from recent data on the cosmic microwave background and baryon acoustic oscillations, as well as with the value found from a median statistical analysis of Huchra’s compilation of H0 measurements, but include the higher local measurements of H0 within the 2σ confidence limits. We use 28 measurements of the Hubble parameter, H ( z ), at intermediate redshifts to determine the present-day Hubble constant H 0 in four cosmological models. We measure , and Mpc −1 (1 σ errors) in the ΛCDM (spatially flat and non-flat), ω CDM, and ϕ CDM models, respectively. These measured H 0 values are more consistent with the lower values determined from recent data on the cosmic microwave background and baryon acoustic oscillations, as well as with the value found from a median statistical analysis of Huchra’s compilation of H 0 measurements, but include the higher local measurements of H 0 within the 2 σ confidence limits. We use 28 Hubble parameter, H($z$), measurements at intermediate redshifts 0.07 $\leqslant z \leqslant$ 2.3 to determine the present-day Hubble constant H0 in four cosmological models. We measure H0 = 68:3$^{+2.7}_{-2.6}$, 68.4$^{+2.9}_{-3.3}$, 65.0$^{+6.5}_{-6:6}$ and 67.9$^{+2.4}_{-2.4}$ km s-1 Mpc-1 ( σ errors) in the ΛCDM (spatially flat and non-flat), ωCDM and ΦCDM models, respectively. These measured H0 values are more consistent with the lower values determined from recent cosmic microwave background and baryon acoustic oscillation data, as well as with that found from a median statistics analysis of Huchra’s compilation of H0 measurements, but include the higher local measurements of H0 within the 2σ confidence limits. |
| Author | Chen, Yun Kumar, Suresh Ratra, Bharat |
| Author_xml | – sequence: 1 givenname: Yun orcidid: 0000-0001-8919-7409 surname: Chen fullname: Chen, Yun email: chenyun@bao.ac.cn organization: Chinese Academy of Sciences Key Laboratory for Computational Astrophysics, National Astronomical Observatories, Beijing, 100012, China – sequence: 2 givenname: Suresh orcidid: 0000-0002-1638-2264 surname: Kumar fullname: Kumar, Suresh email: suresh.kumar@pilani.bits-pilani.ac.in organization: Department of Mathematics, BITS Pilani, Pilani Campus, Rajasthan-333031, India – sequence: 3 givenname: Bharat surname: Ratra fullname: Ratra, Bharat email: ratra@phys.ksu.edu organization: Kansas State University Department of Physics, 116 Cardwell Hall, Manhattan, KS 66506, USA |
| BackLink | https://www.osti.gov/servlets/purl/1532969$$D View this record in Osti.gov |
| BookMark | eNp9kE1Pg0AURSemJrbVP-CKqFvKfDLDklb6kRRqKE3cTWDKRJoKCHThvxeC1sSYribzcs7Ne3cEBnmRpwDcIzghgnILMSJMShi3BGEWsoR9BYbn4QAMIYTUtAl_vQGjuj50X-w4QzB99iIv9FfBKlgY0dIzlrvpdO0Zs02wjdwgMubhxv8Zvrih63e84Xvudhd6vhdE21twreNjnd59v2Owm3vRbGmuN4vVzF2bigrYmJgqzTRTyiGKcyEgS3TCYwxjRZnmKUWJIHHiKJggpBRHiFFbE-qofcodrckYPPS5Rd1kslZZk6o3VeR5qhrZ3ood22mhxx4qq-LjlNaNPBSnKm_3kpjYTGBsY9pSoqdUVdR1lWrZpsVNVuRNFWdHiaDsau1ShewalG2tEklhtyr-o5ZV9h5Xn5elSS9lRfm70EXh6R8hLg9nRJZ7Tb4ACKGPtg |
| CitedBy_id | crossref_primary_10_1016_j_dark_2020_100711 crossref_primary_10_1088_1475_7516_2021_05_009 crossref_primary_10_1093_mnras_staa101 crossref_primary_10_3847_1538_4357_aadcf3 crossref_primary_10_3847_1538_4357_aa8f48 crossref_primary_10_1093_mnras_staa1855 crossref_primary_10_1134_S0202289324700282 crossref_primary_10_3390_sym11080986 crossref_primary_10_1007_s10509_019_3663_4 crossref_primary_10_1016_j_dark_2025_102012 crossref_primary_10_1016_j_nuclphysb_2023_116233 crossref_primary_10_1016_j_dark_2022_101043 crossref_primary_10_1093_ptep_ptad110 crossref_primary_10_1088_1674_4527_20_9_151 crossref_primary_10_1088_1475_7516_2019_02_053 crossref_primary_10_1140_epjc_s10052_024_13307_2 crossref_primary_10_3847_1538_4357_ab88d2 crossref_primary_10_1093_mnras_stac1141 crossref_primary_10_3847_1538_4357_ac7de5 crossref_primary_10_1140_epjp_s13360_020_00308_9 crossref_primary_10_3847_1538_4357_ab3641 crossref_primary_10_1093_mnras_stac1978 crossref_primary_10_1093_mnras_sty3191 crossref_primary_10_1088_1475_7516_2020_09_053 crossref_primary_10_1007_s10509_019_3627_8 crossref_primary_10_1007_s12648_017_1126_8 crossref_primary_10_1093_mnras_stac517 crossref_primary_10_1093_mnras_stac914 crossref_primary_10_3390_universe6080114 crossref_primary_10_1088_1475_7516_2018_04_051 crossref_primary_10_3847_1538_4357_aad633 crossref_primary_10_1016_j_newar_2022_101659 crossref_primary_10_1093_mnras_stab942 crossref_primary_10_1016_j_physletb_2023_137886 crossref_primary_10_3847_1538_4357_ab12d6 crossref_primary_10_1016_j_cjph_2023_10_050 crossref_primary_10_1088_1402_4896_ad14d3 crossref_primary_10_3390_universe9010030 crossref_primary_10_1140_epjc_s10052_019_7230_5 crossref_primary_10_1093_mnras_staa2190 crossref_primary_10_1093_mnras_stab3559 crossref_primary_10_1093_mnras_sty1939 crossref_primary_10_1140_epjc_s10052_020_8289_8 crossref_primary_10_3847_1538_4357_aa92cc crossref_primary_10_3847_1538_4357_aae82d crossref_primary_10_1007_s10509_019_3567_3 crossref_primary_10_3847_1538_4357_ac66d3 crossref_primary_10_1142_S0219887824400139 crossref_primary_10_1093_mnras_staa366 crossref_primary_10_1140_epjc_s10052_020_8120_6 crossref_primary_10_3847_1538_4357_aaec6f crossref_primary_10_1088_0253_6102_71_7_826 crossref_primary_10_1016_j_ascom_2023_100768 crossref_primary_10_3390_sym15020549 crossref_primary_10_1140_epjc_s10052_023_11794_3 crossref_primary_10_1007_s12648_019_01381_2 crossref_primary_10_1051_0004_6361_201833032 crossref_primary_10_1007_s11433_017_9079_1 crossref_primary_10_1140_epjp_s13360_023_04666_y crossref_primary_10_1007_s10714_020_2664_5 crossref_primary_10_1093_mnras_sty1922 crossref_primary_10_1140_epjc_s10052_021_09099_4 crossref_primary_10_3847_1538_4357_aa88cc crossref_primary_10_3847_1538_4357_aab0a2 crossref_primary_10_1016_j_cjph_2022_06_028 crossref_primary_10_1093_mnras_stz1966 crossref_primary_10_1093_mnras_stab3304 crossref_primary_10_1093_mnras_stz3308 crossref_primary_10_3847_2041_8213_ad2e97 crossref_primary_10_1088_0253_6102_70_4_445 crossref_primary_10_1007_s12648_023_02669_0 crossref_primary_10_1088_1538_3873_aac767 crossref_primary_10_1093_mnras_stx627 crossref_primary_10_1007_s12648_024_03271_8 crossref_primary_10_1016_j_cjph_2022_09_007 crossref_primary_10_1016_j_newast_2020_101567 crossref_primary_10_1093_mnras_stab486 crossref_primary_10_1007_s13538_018_0581_9 crossref_primary_10_1088_1572_9494_ac6ac1 crossref_primary_10_1140_epjc_s10052_023_11744_z crossref_primary_10_1088_1475_7516_2018_09_017 crossref_primary_10_3390_universe10030122 crossref_primary_10_1016_j_dark_2024_101799 crossref_primary_10_1088_1475_7516_2020_07_009 crossref_primary_10_1093_mnras_staa2779 crossref_primary_10_3847_1538_4357_ab39e6 crossref_primary_10_1007_s10701_018_0202_z crossref_primary_10_1093_mnras_staa3748 crossref_primary_10_1088_1475_7516_2017_03_028 crossref_primary_10_1007_s41114_018_0017_4 crossref_primary_10_1088_1475_7516_2018_05_033 crossref_primary_10_1016_j_physletb_2019_04_032 crossref_primary_10_1142_S0217732325500877 crossref_primary_10_1093_mnras_sty1835 |
| Cites_doi | 10.1093/mnras/stt1290 10.1088/0004-637X/815/2/87 10.1088/2041-8205/766/1/L7 10.1086/508662 10.1086/322409 10.1016/j.physletb.2016.08.043 10.1093/mnras/stw964 10.3847/0004-637X/829/2/61 10.1086/662131 10.1016/j.physletb.2011.08.035 10.1016/j.physletb.2013.04.044 10.1088/1674-4527/14/10/002 10.1088/0004-637X/764/2/138 10.1088/1475-7516/2016/05/014 10.3847/0004-637X/818/2/132 10.1051/0004-6361/201525830 10.1103/PhysRevD.71.123001 10.1093/mnras/stu278 10.1140/epjc/s10052-016-4016-x 10.1086/185100 10.1088/0067-0049/208/2/19 10.1086/591785 10.1016/j.physletb.2013.08.078 10.1051/0004-6361/201628217 10.1142/S0217732315501230 10.1086/319055 10.1088/1475-7516/2012/08/006 10.1016/j.physletb.2014.03.059 10.1088/1475-7516/2013/10/060 10.1016/j.dark.2014.09.003 10.1103/PhysRevD.92.123516 10.1086/320638 10.1103/PhysRevD.37.3406 10.3847/0004-637X/826/1/56 10.1093/mnras/stv154 10.1051/0004-6361/201220724 10.1086/162425 10.1103/PhysRevD.66.103511 10.1103/PhysRevD.86.043520 10.1088/0004-637X/758/1/24 10.1086/377112 10.1088/1475-7516/2015/02/010 10.3847/0004-637X/825/1/17 10.1088/1475-7516/2016/10/019 10.1088/2041-8205/803/2/L22 10.1103/PhysRevD.90.044016 10.1088/0004-637X/730/2/119 10.1086/379219 10.1088/1475-7516/2010/02/008 10.1111/j.1365-2966.2012.21473.x |
| ContentType | Journal Article |
| Copyright | 2017. The American Astronomical Society. All rights reserved. Copyright IOP Publishing Jan 20, 2017 |
| Copyright_xml | – notice: 2017. The American Astronomical Society. All rights reserved. – notice: Copyright IOP Publishing Jan 20, 2017 |
| CorporateAuthor | Kansas State Univ., Manhattan, KS (United States) |
| CorporateAuthor_xml | – name: Kansas State Univ., Manhattan, KS (United States) |
| DBID | AAYXX CITATION 7TG 8FD H8D KL. L7M OIOZB OTOTI |
| DOI | 10.3847/1538-4357/835/1/86 |
| DatabaseName | CrossRef Meteorological & Geoastrophysical Abstracts Technology Research Database Aerospace Database Meteorological & Geoastrophysical Abstracts - Academic Advanced Technologies Database with Aerospace OSTI.GOV - Hybrid OSTI.GOV |
| DatabaseTitle | CrossRef Aerospace Database Meteorological & Geoastrophysical Abstracts Technology Research Database Advanced Technologies Database with Aerospace Meteorological & Geoastrophysical Abstracts - Academic |
| DatabaseTitleList | Aerospace Database CrossRef |
| DeliveryMethod | fulltext_linktorsrc |
| Discipline | Astronomy & Astrophysics Physics |
| DocumentTitleAlternate | DETERMINING THE HUBBLE CONSTANT FROM HUBBLE PARAMETER MEASUREMENTS |
| EISSN | 1538-4357 |
| ExternalDocumentID | 1532969 10_3847_1538_4357_835_1_86 apjaa5313 |
| GroupedDBID | -DZ -~X 123 1JI 23N 2FS 2WC 4.4 6J9 85S AAFWJ AAGCD AAJIO AALHV ABHWH ACBEA ACGFS ACHIP ACNCT ADACN AEFHF AENEX AFPKN AKPSB ALMA_UNASSIGNED_HOLDINGS ASPBG ATQHT AVWKF AZFZN CJUJL CRLBU CS3 EBS EJD F5P FRP GROUPED_DOAJ IJHAN IOP KOT M~E N5L O3W O43 OK1 PJBAE RIN RNS ROL SJN SY9 T37 TN5 TR2 WH7 XSW AAYXX AEINN CITATION 7TG 8FD H8D KL. L7M OIOZB OTOTI |
| ID | FETCH-LOGICAL-c480t-24cf5f5cc93c778805bfb7a20ac45f7e41b83ab9c0b11cc711546f349cde79ff3 |
| IEDL.DBID | O3W |
| ISICitedReferencesCount | 117 |
| ISICitedReferencesURI | http://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=Summon&SrcAuth=ProQuest&DestLinkType=CitingArticles&DestApp=WOS_CPL&KeyUT=000393455400086&url=https%3A%2F%2Fcvtisr.summon.serialssolutions.com%2F%23%21%2Fsearch%3Fho%3Df%26include.ft.matches%3Dt%26l%3Dnull%26q%3D |
| ISSN | 0004-637X 1538-4357 |
| IngestDate | Tue Nov 05 04:37:23 EST 2024 Wed Aug 13 06:43:39 EDT 2025 Sat Nov 29 06:20:22 EST 2025 Tue Nov 18 21:04:37 EST 2025 Thu Jan 07 13:49:50 EST 2021 Wed Aug 21 03:33:03 EDT 2024 |
| IsDoiOpenAccess | true |
| IsOpenAccess | true |
| IsPeerReviewed | true |
| IsScholarly | true |
| Issue | 1 |
| Language | English |
| LinkModel | DirectLink |
| MergedId | FETCHMERGED-LOGICAL-c480t-24cf5f5cc93c778805bfb7a20ac45f7e41b83ab9c0b11cc711546f349cde79ff3 |
| Notes | Galaxies and Cosmology AAS01522 ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 FG03-99ER41093 USDOE Office of Science (SC) |
| ORCID | 0000-0002-1638-2264 0000-0001-8919-7409 0000000189197409 0000000216382264 |
| OpenAccessLink | https://www.osti.gov/servlets/purl/1532969 |
| PQID | 2365822624 |
| PQPubID | 4562441 |
| PageCount | 4 |
| ParticipantIDs | crossref_citationtrail_10_3847_1538_4357_835_1_86 crossref_primary_10_3847_1538_4357_835_1_86 osti_scitechconnect_1532969 proquest_journals_2365822624 iop_journals_10_3847_1538_4357_835_1_86 |
| PublicationCentury | 2000 |
| PublicationDate | 20170120 2017-01-20 |
| PublicationDateYYYYMMDD | 2017-01-20 |
| PublicationDate_xml | – month: 01 year: 2017 text: 20170120 day: 20 |
| PublicationDecade | 2010 |
| PublicationPlace | Philadelphia |
| PublicationPlace_xml | – name: Philadelphia – name: United States |
| PublicationTitle | The Astrophysical journal |
| PublicationTitleAbbrev | APJ |
| PublicationTitleAlternate | Astrophys. J |
| PublicationYear | 2017 |
| Publisher | The American Astronomical Society IOP Publishing Institute of Physics (IOP) |
| Publisher_xml | – name: The American Astronomical Society – name: IOP Publishing – name: Institute of Physics (IOP) |
| References | Chen (apjaa5313bib13) 2011a; 123 Hinshaw (apjaa5313bib36) 2013; 208 Zheng (apjaa5313bib60) 2016; 825 Farooq (apjaa5313bib25) 2013 Podariu (apjaa5313bib46) 2001; 559 Farooq (apjaa5313bib29) 2015; 357 Bernal (apjaa5313bib6) 2016; 10 Di Valentino (apjaa5313bib23) 2016; 761 Samushia (apjaa5313bib51) 2009 Croft (apjaa5313bib21) 2015; 1 Calabrese (apjaa5313bib9) 2012; 86 Chen (apjaa5313bib15) 2015; 1502 Chen (apjaa5313bib16) 2016; 829 Efstathiou (apjaa5313bib24) 2014; 440 Ratra (apjaa5313bib47) 1988; 37 Mukherjee (apjaa5313bib43) 2016; 460 Aubourg (apjaa5313bib5) 2015; 92 Farooq (apjaa5313bib31) 2013b; 766 Andreon (apjaa5313bib4) 2012 Verde (apjaa5313bib58) 2014; 5–6 Stern (apjaa5313bib57) 2010; 1002 Samushia (apjaa5313bib53) 2006; 650 Freedman (apjaa5313bib33) 2012; 758 Chen (apjaa5313bib11) 2003; 115 Busca (apjaa5313bib8) 2013; 552 Ding (apjaa5313bib22) 2015; 803 Meng (apjaa5313bib40) 2015 Farooq (apjaa5313bib28) 2013b; 764 Addison (apjaa5313bib1) 2016; 818 Gott (apjaa5313bib34) 2001; 549 Crandall (apjaa5313bib20) 2015; 815 Freedman (apjaa5313bib32) 2001; 553 Crandall (apjaa5313bib18) 2015; 30 Luković (apjaa5313bib39) 2016; 595 Farooq (apjaa5313bib27) 2016 L’Huillier (apjaa5313bib38) 2016 Moresco (apjaa5313bib41) 2012; 1208 Riess (apjaa5313bib48) 2011; 730 Chen (apjaa5313bib12) 2003; 115 Farooq (apjaa5313bib30) 2013a; 723 Ade (apjaa5313bib2) 2015; 594 Chuang (apjaa5313bib17) 2013; 435 Peebles (apjaa5313bib45) 1988; 325 Blake (apjaa5313bib7) 2012; 425 Chen (apjaa5313bib14) 2011b; 703 Peebles (apjaa5313bib44) 1984; 284 Capozziello (apjaa5313bib10) 2014; 90 Riess (apjaa5313bib49) 2016; 826 Solà (apjaa5313bib56) 2016 Guo (apjaa5313bib35) 2016; 76 Lewis (apjaa5313bib37) 2002; 66 Mamajek (apjaa5313bib61) 2008; 687 Zhang (apjaa5313bib59) 2014; 14 Simon (apjaa5313bib55) 2005; 71 Farooq (apjaa5313bib26) 2013a; 726 Moresco (apjaa5313bib42) 2016; 1605 Sievers (apjaa5313bib54) 2013; 1310 Ross (apjaa5313bib50) 2015; 449 Alam (apjaa5313bib3) 2016 Crandall (apjaa5313bib19) 2014; 732 Samushia (apjaa5313bib52) 2007 |
| References_xml | – year: 2007 ident: apjaa5313bib52 – volume: 435 start-page: 255 year: 2013 ident: apjaa5313bib17 publication-title: MNRAS doi: 10.1093/mnras/stt1290 – volume: 815 start-page: 87 year: 2015 ident: apjaa5313bib20 publication-title: ApJ doi: 10.1088/0004-637X/815/2/87 – volume: 766 start-page: L7 year: 2013b ident: apjaa5313bib31 publication-title: ApJL doi: 10.1088/2041-8205/766/1/L7 – volume: 650 start-page: L5 year: 2006 ident: apjaa5313bib53 publication-title: ApJL doi: 10.1086/508662 – volume: 559 start-page: 9 year: 2001 ident: apjaa5313bib46 publication-title: ApJ doi: 10.1086/322409 – volume: 1 start-page: 1 year: 2015 ident: apjaa5313bib21 publication-title: Quarterly Phys. Rev. – volume: 761 start-page: 242 year: 2016 ident: apjaa5313bib23 doi: 10.1016/j.physletb.2016.08.043 – year: 2016 ident: apjaa5313bib38 – volume: 460 start-page: 273 year: 2016 ident: apjaa5313bib43 doi: 10.1093/mnras/stw964 – year: 2016 ident: apjaa5313bib56 – volume: 829 start-page: 61 year: 2016 ident: apjaa5313bib16 doi: 10.3847/0004-637X/829/2/61 – volume: 123 start-page: 1127 year: 2011a ident: apjaa5313bib13 publication-title: PASP doi: 10.1086/662131 – volume: 703 start-page: 406 year: 2011b ident: apjaa5313bib14 publication-title: PhLB doi: 10.1016/j.physletb.2011.08.035 – volume: 723 start-page: 1 year: 2013a ident: apjaa5313bib30 publication-title: PhLB doi: 10.1016/j.physletb.2013.04.044 – volume: 14 start-page: 1221 year: 2014 ident: apjaa5313bib59 publication-title: RAA doi: 10.1088/1674-4527/14/10/002 – volume: 764 start-page: 138 year: 2013b ident: apjaa5313bib28 publication-title: ApJ doi: 10.1088/0004-637X/764/2/138 – year: 2009 ident: apjaa5313bib51 – volume: 1605 start-page: 014 year: 2016 ident: apjaa5313bib42 publication-title: JCAP doi: 10.1088/1475-7516/2016/05/014 – volume: 818 start-page: 132 year: 2016 ident: apjaa5313bib1 publication-title: ApJ doi: 10.3847/0004-637X/818/2/132 – volume: 594 start-page: A13 year: 2015 ident: apjaa5313bib2 doi: 10.1051/0004-6361/201525830 – volume: 71 start-page: 123001 year: 2005 ident: apjaa5313bib55 publication-title: PhRvD doi: 10.1103/PhysRevD.71.123001 – volume: 440 start-page: 1138 year: 2014 ident: apjaa5313bib24 publication-title: MNRAS doi: 10.1093/mnras/stu278 – volume: 76 start-page: 163 year: 2016 ident: apjaa5313bib35 publication-title: EPJC doi: 10.1140/epjc/s10052-016-4016-x – volume: 325 start-page: L17 year: 1988 ident: apjaa5313bib45 publication-title: ApJL doi: 10.1086/185100 – year: 2012 ident: apjaa5313bib4 – volume: 357 start-page: 11 year: 2015 ident: apjaa5313bib29 publication-title: ApSS – volume: 208 start-page: 19 year: 2013 ident: apjaa5313bib36 publication-title: ApJS doi: 10.1088/0067-0049/208/2/19 – volume: 687 start-page: 1264 year: 2008 ident: apjaa5313bib61 doi: 10.1086/591785 – volume: 726 start-page: 72 year: 2013a ident: apjaa5313bib26 publication-title: PhLB doi: 10.1016/j.physletb.2013.08.078 – volume: 595 start-page: A109 year: 2016 ident: apjaa5313bib39 doi: 10.1051/0004-6361/201628217 – volume: 30 start-page: 25 year: 2015 ident: apjaa5313bib18 publication-title: MPLA doi: 10.1142/S0217732315501230 – year: 2015 ident: apjaa5313bib40 – volume: 549 start-page: 1 year: 2001 ident: apjaa5313bib34 publication-title: ApJ doi: 10.1086/319055 – volume: 1208 start-page: 006 year: 2012 ident: apjaa5313bib41 publication-title: JCAP doi: 10.1088/1475-7516/2012/08/006 – volume: 732 start-page: 330 year: 2014 ident: apjaa5313bib19 publication-title: PhLB doi: 10.1016/j.physletb.2014.03.059 – volume: 1310 start-page: 060 year: 2013 ident: apjaa5313bib54 publication-title: JCAP doi: 10.1088/1475-7516/2013/10/060 – volume: 5–6 start-page: 307 year: 2014 ident: apjaa5313bib58 publication-title: PDU doi: 10.1016/j.dark.2014.09.003 – volume: 92 start-page: 123516 year: 2015 ident: apjaa5313bib5 publication-title: PhRvD doi: 10.1103/PhysRevD.92.123516 – volume: 553 start-page: 47 year: 2001 ident: apjaa5313bib32 publication-title: ApJ doi: 10.1086/320638 – volume: 37 start-page: 3406 year: 1988 ident: apjaa5313bib47 publication-title: PhRvD doi: 10.1103/PhysRevD.37.3406 – volume: 826 start-page: 56 year: 2016 ident: apjaa5313bib49 doi: 10.3847/0004-637X/826/1/56 – volume: 449 start-page: 835 year: 2015 ident: apjaa5313bib50 publication-title: MNRAS doi: 10.1093/mnras/stv154 – volume: 552 start-page: A96 year: 2013 ident: apjaa5313bib8 publication-title: A&A doi: 10.1051/0004-6361/201220724 – volume: 284 start-page: 439 year: 1984 ident: apjaa5313bib44 publication-title: ApJ doi: 10.1086/162425 – volume: 66 start-page: 103511 year: 2002 ident: apjaa5313bib37 publication-title: PhRvD doi: 10.1103/PhysRevD.66.103511 – volume: 86 start-page: 043520 year: 2012 ident: apjaa5313bib9 publication-title: PhRvD doi: 10.1103/PhysRevD.86.043520 – volume: 758 start-page: 24 year: 2012 ident: apjaa5313bib33 publication-title: ApJ doi: 10.1088/0004-637X/758/1/24 – volume: 115 start-page: 1143 year: 2003 ident: apjaa5313bib12 publication-title: PASP doi: 10.1086/377112 – year: 2016 ident: apjaa5313bib27 – year: 2016 ident: apjaa5313bib3 – volume: 1502 start-page: 010 year: 2015 ident: apjaa5313bib15 publication-title: JCAP doi: 10.1088/1475-7516/2015/02/010 – volume: 825 start-page: 17 year: 2016 ident: apjaa5313bib60 doi: 10.3847/0004-637X/825/1/17 – year: 2013 ident: apjaa5313bib25 – volume: 10 start-page: 019 year: 2016 ident: apjaa5313bib6 doi: 10.1088/1475-7516/2016/10/019 – volume: 803 start-page: L22 year: 2015 ident: apjaa5313bib22 publication-title: ApJL doi: 10.1088/2041-8205/803/2/L22 – volume: 90 start-page: 044016 year: 2014 ident: apjaa5313bib10 publication-title: PhRvD doi: 10.1103/PhysRevD.90.044016 – volume: 730 start-page: 119 year: 2011 ident: apjaa5313bib48 publication-title: ApJ doi: 10.1088/0004-637X/730/2/119 – volume: 115 start-page: 1269 year: 2003 ident: apjaa5313bib11 publication-title: PASP doi: 10.1086/379219 – volume: 1002 start-page: 008 year: 2010 ident: apjaa5313bib57 publication-title: JCAP doi: 10.1088/1475-7516/2010/02/008 – volume: 425 start-page: 405 year: 2012 ident: apjaa5313bib7 publication-title: MNRAS doi: 10.1111/j.1365-2966.2012.21473.x |
| SSID | ssj0004299 |
| Score | 2.6060448 |
| Snippet | We use 28 measurements of the Hubble parameter, H(z), at intermediate redshifts to determine the present-day Hubble constant H0 in four cosmological models. We... We use 28 measurements of the Hubble parameter, H ( z ), at intermediate redshifts to determine the present-day Hubble constant H 0 in four cosmological... We use 28 measurements of the Hubble parameter, H(z), at intermediate redshifts \(0.07\leqslant z\leqslant 2.3\) to determine the present-day Hubble constant... We use 28 Hubble parameter, H($z$), measurements at intermediate redshifts 0.07 $\leqslant z \leqslant$ 2.3 to determine the present-day Hubble constant H0 in... |
| SourceID | osti proquest crossref iop |
| SourceType | Open Access Repository Aggregation Database Enrichment Source Index Database Publisher |
| StartPage | 86 |
| SubjectTerms | Astronomical models astronomy & astrophysics ASTRONOMY AND ASTROPHYSICS Astrophysics Big Bang theory Confidence limits Cosmic microwave background Cosmological models cosmological parameters Cosmology dark energy Hubble constant Parameters Statistical analysis |
| Title | DETERMINING THE HUBBLE CONSTANT FROM HUBBLE PARAMETER MEASUREMENTS |
| URI | https://iopscience.iop.org/article/10.3847/1538-4357/835/1/86 https://www.proquest.com/docview/2365822624 https://www.osti.gov/servlets/purl/1532969 |
| Volume | 835 |
| WOSCitedRecordID | wos000393455400086&url=https%3A%2F%2Fcvtisr.summon.serialssolutions.com%2F%23%21%2Fsearch%3Fho%3Df%26include.ft.matches%3Dt%26l%3Dnull%26q%3D |
| hasFullText | 1 |
| inHoldings | 1 |
| isFullTextHit | |
| isPrint | |
| journalDatabaseRights | – providerCode: PRVIOP databaseName: Institute of Physics Journals Open Access customDbUrl: eissn: 1538-4357 dateEnd: 99991231 omitProxy: false ssIdentifier: ssj0004299 issn: 0004-637X databaseCode: O3W dateStart: 19950701 isFulltext: true titleUrlDefault: http://iopscience.iop.org/ providerName: IOP Publishing – providerCode: PRVHPJ databaseName: ROAD: Directory of Open Access Scholarly Resources customDbUrl: eissn: 1538-4357 dateEnd: 99991231 omitProxy: false ssIdentifier: ssj0004299 issn: 0004-637X databaseCode: M~E dateStart: 18950101 isFulltext: true titleUrlDefault: https://road.issn.org providerName: ISSN International Centre |
| link | http://cvtisr.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwpV3db9MwED_RARIvGwymdV_KA4IHFJrYjj8e0y2lk5a06jrom5U4sQRibbV2SLzwt3NO0k0TYkLi7ZRcLtb5Pn5n2WeAt6XDpJJzn1Be-oyI3JeSVn7JS2KptWWzm_DzhcgyOZupcbs3pz4Ls1i2of8jkk2j4EaFzr8pxtJe7aOY5UUP0UMv7EnegadUYiJHcx7RL_fHIolq0S_zORWz5szMX2Q8yEsd_DfG6AV62R8xuk48g53_HPJL2G4Rpxc3zK_gSTXfhf145dbAF9c_vXdeTTdLHKtdeD5uqNfQP0sQ7Kbn2Xn2yZsOE2941e9fJN7pKLucxtnUG0xG6ebhOJ7EqeP30gRj9aS-JeDyDVwNkunp0G_vXPANk8HaJ8zYyEbGKGoElsdBVNhC5CTIDYusqFhYSJoXygRFGBojXDcfbilTpqyEspbuwdZ8Ma_2wSuMlJGDkIIxJogsRFVGgmJFo8JSctqFcKNxbdqG5O5ejO8aCxOnNu3Upp3aNKpNh1ryLny4-2bZtON4lPs9zohuvXL1KOfxA858-e3unV6WtguHzhg0TrTrrWvcJiSzdoKI4qoLRxsbuReBxh8h-uKEHfzzMA7hBXGwIQgxeh3B1vrmtjqGZ-bH-uvq5gQ66a_kpLbx345Y7Xk |
| linkProvider | IOP Publishing |
| linkToPdf | http://cvtisr.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwrV3Nb9MwFH9i40Nc-BiglW3gA4IDCklsx3aO6ZbSijatuo71ZiVOLG2CtloLEv89z0m6aUJMHLhZzvOL9b78e5b9DPCudJhUCeFRJkqPU5l7SrHKK0VJLbO2bE4Tfh3KLFPzeTxpTxPWd2GWqzb0f8JmUyi4EaHzb4ax1K99FFd56SN68ENfCX9V2h247yqVOMMes_Obq5E0bhEw9wST8-bezF_43FqbdvD_GKeX6Gl_xOl68ek9_Q_TfgZPWuRJkmbAc7hXLfZgP1m7vfDl91_kPanbzVbHeg8eTprWC-iepAh6R4NskH0ms35K-mfd7jAlx-PsdJZkM9KbjkfbzkkyTUaOnoxSjNnT-rWA05dw1ktnx32vfXvBM1wFG49yYyMbGRMzIzFNDqLCFjKnQW54ZGXFw0KxvIhNUIShMdJV9RGW8diUlYytZa9gd7FcVPtACqNU5KCk5JxLqgpZlZFkmNnEYakE60C4lbo2bWFy9z7GN40JihOddqLTTnQaRadDrUQHPl6PWTVlOe6k_oBa0a13ru-kPLpFma8ur79pVFcHDpxBaFS2q7Fr3GEks3GMaCziDhxu7eSGBTpBhChMUP76n6fxFh5NTnp6OMi-HMBj6pBEEGJAO4TdzdWP6ggemJ-bi_XVm9rYfwNZ9PGw |
| openUrl | ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=DETERMINING+THE+HUBBLE+CONSTANT+FROM+HUBBLE+PARAMETER+MEASUREMENTS&rft.jtitle=The+Astrophysical+journal&rft.au=Chen%2C+Yun&rft.au=Kumar%2C+Suresh&rft.au=Ratra%2C+Bharat&rft.date=2017-01-20&rft.pub=The+American+Astronomical+Society&rft.issn=0004-637X&rft.eissn=1538-4357&rft.volume=835&rft.issue=1&rft_id=info:doi/10.3847%2F1538-4357%2F835%2F1%2F86&rft.externalDocID=apjaa5313 |
| thumbnail_l | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=0004-637X&client=summon |
| thumbnail_m | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=0004-637X&client=summon |
| thumbnail_s | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=0004-637X&client=summon |