A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies
| Autor: | R. L. C. Ogando, Alistair R. Walker, Alyssa Garcia, Marcelle Soares-Santos, V. Scarpine, E. Suchyta, Josh Frieman, August E. Evrard, J. deVicente, C. Nicolaou, Enrique Gaztanaga, M. Carrasco Kind, Michael Schubnell, K. Herner, A. Roodman, Antonella Palmese, W. G. Hartley, D. A. Finley, Alex Drlica-Wagner, O. Lahav, Robert Morgan, Juan Garcia-Bellido, K. Honscheid, Dragan Huterer, J. Carretero, E. Buckley-Geer, David J. James, J. Annis, Pablo Fosalba, I. Sevilla-Noarbe, Maria E. S. Pereira, I. Magaña Hernandez, M. A. G. Maia, W. C. Wester, Samuel Hinton, G. Gutierrez, David J. Brooks, G. Tarle, Elisabeth Krause, Peter Melchior, Ramon Miquel, J. Allyn Smith, Martin Crocce, R. D. Wilkinson, Sunayana Bhargava, Felipe Menanteau, Tamara M. Davis, S. Everett, Ryan J. Foley, K. Bechtol, L. N. da Costa, B. Flaugher, Jennifer L. Marshall, M. N. K. Smith, K. Kuehn, M. Sako, F. Paz-Chinchón, D. L. Hollowood, Daniel E. Holz, S. Serrano, Richard Kessler, J. Zuntz, M. Costanzi, Daniel Gruen, Salcedo Romero de Ávila, Juan Estrada, Michael Troxel, M. March, D. W. Gerdes, E. Bertin, Douglas L. Tucker, J. Gschwend, P. Doel, H. T. Diehl, M. S. S. Gill, Chihway Chang, C. J. Conselice, Huan Lin, S. Desai, Steve Kent, F. J. Castander, T. M. C. Abbott, E. J. Sanchez, D. L. Burke, S. Allam, A. A. Plazas, Robert A. Gruendl, Enrique J. Fernández, Michel Aguena |
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| Přispěvatelé: | European Research Council, European Commission, Ministerio de Economía y Competitividad (España), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), DES, Palmese, A., Devicente, J., Pereira, M. E. S., Annis, J., Hartley, W., Herner, K., Soares-Santos, M., Crocce, M., Huterer, D., Magana Hernandez, I., Davis, T. M., Garcia, A., Garcia-Bellido, J., Gschwend, J., Holz, D. E., Kessler, R., Lahav, O., Morgan, R., Nicolaou, C., Conselice, C., Foley, R. J., Gill, M. S. S., Abbott, T. M. C., Aguena, M., Allam, S., Avila, S., Bechtol, K., Bertin, E., Bhargava, S., Brooks, D., Buckley-Geer, E., Burke, D. L., Carrasco Kind, M., Carretero, J., Castander, F. J., Chang, C., Costanzi, M., da Costa, L. N., Desai, S., Diehl, H. T., Doel, P., Estrada, J., Everett, S., Evrard, A. E., Fernandez, E., Finley, D. A., Flaugher, B., Fosalba, P., Frieman, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kent, S., Krause, E., Kuehn, K., Lin, H., Maia, M. A. G., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Ogando, R. L. C., Paz-Chinchon, F., Plazas, A. A., Roodman, A., Sako, M., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Allyn Smith, J., Smith, M., Suchyta, E., Tarle, G., Troxel, M. A., Tucker, D. L., Walker, A. R., Wester, W., Wilkinson, R. D., Zuntz, J. |
| Jazyk: | angličtina |
| Rok vydání: | 2020 |
| Předmět: |
Cosmological parameter
star: compact cosmological model coalescence 010504 meteorology & atmospheric sciences Physics::Instrumentation and Detectors Astrophysics Surveys 7. Clean energy 01 natural sciences localization Cosmology Cosmological parameters Gravitational waves Hubble constant Redshift surveys Gravitational wave astronomy parameter space LIGO Survey dark energy 010303 astronomy & astrophysics Photometric redshift High Energy Astrophysical Phenomena (astro-ph.HE) Physics density photon Mathematics::History and Overview GALÁXIAS Redshift survey Astrophysics - High Energy Astrophysical Phenomena Gravitational wave Astrophysics - Cosmology and Nongalactic Astrophysics Cosmology and Nongalactic Astrophysics (astro-ph.CO) FOS: Physical sciences Astrophysics::Cosmology and Extragalactic Astrophysics statistical analysis Binary black hole 0103 physical sciences distribution function Astrophysics::Galaxy Astrophysics 0105 earth and related environmental sciences gravitational radiation Astronomy and Astrophysics redshift Galaxy Redshift Black hole VIRGO electromagnetic black hole: binary Space and Planetary Science Dark energy galaxy [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
| Zdroj: | Astrophys.J.Lett. Astrophys.J.Lett., 2020, 900 (2), pp.L33. ⟨10.3847/2041-8213/abaeff⟩ Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) Universidade de São Paulo (USP) instacron:USP Digital.CSIC. Repositorio Institucional del CSIC instname |
| DOI: | 10.3847/2041-8213/abaeff⟩ |
| Popis: | DES Collaboration: et al. arXiv:2006.14961v3 We present a measurement of the Hubble constant H0 using the gravitational wave (GW) event GW190814, which resulted from the coalescence of a 23 M⊙ black hole with a 2.6 M⊙ compact object, as a standard siren. No compelling electromagnetic counterpart has been identified for this event; thus our analysis accounts for thousands of potential host galaxies within a statistical framework. The redshift information is obtained from the photometric redshift (photo-z) catalog from the Dark Energy Survey. The luminosity distance is provided by the LIGO/Virgo gravitational wave sky map. Since this GW event has the second-smallest localization volume after GW170817, GW190814 is likely to provide the best constraint on cosmology from a single standard siren without identifying an electromagnetic counterpart. Our analysis uses photo-z probability distribution functions and corrects for photo-z biases. We also reanalyze the binary black hole GW170814 within this updated framework. We explore how our findings impact the H0 constraints from GW170817, the only GW merger associated with a unique host galaxy. From a combination of GW190814, GW170814, and GW170817, our analysis yields ${H}_{0}={72.0}_{-8.2}^{+12}\,\mathrm{km}\,{{\rm{s}}}^{-1}\,{\mathrm{Mpc}}^{-1}$(68% highest-density interval, HDI) for a prior in H0 uniform between $[20\mathrm{and}140]\,\mathrm{km}\,{{\rm{s}}}^{-1}\,{\mathrm{Mpc}}^{-1}$. The addition of GW190814 and GW170814 to GW170817 improves the 68% HDI from GW170817 alone by ~18%, showing how well-localized mergers without counterparts can provide a significant contribution to standard siren measurements, provided that a complete galaxy catalog is available at the location of the event. Funding for the DES Projects has been provided by the DOE and NSF(USA), MEC/MICINN/MINECO(Spain), STFC(UK), HEFCE(UK). NCSA(UIUC), KICP(U. Chicago), CCAPP(Ohio State), MIFPA(Texas A&M), CNPQ, FAPERJ, FINEP (Brazil), DFG(Germany) and the Collaborating Institutions in the Dark Energy Survey. The DES Data Management System is supported by the NSF under Grant Numbers AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under grants AYA2015-71825, ESP2015-88861, FPA2015-68048, and Centro de Excelencia SEV-2016-0588, SEV-2016-0597 and MDM-2015-0509. Research leading to these results has received funding from the ERC under the EU’s 7th Framework Programme including grants ERC 240672, 291329 and 306478. We acknowledge support from the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020. |
| Databáze: | OpenAIRE |
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