STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354

Shajib, A. J.; Birrer, S.; Treu, T.; Agnello, A.; Buckley-Geer, E. J.; Chan, J. H. H.; Christensen, L.; Lemon, C.; Lin, H.; Millon, M.; Poh, J.; Rusu, C. E.; Sluse, D.; Spiniello, C.; Chen, G. C-F; Collett, T.; Courbin, F.; Fassnacht, C. D.; Frieman, J.; Galan, A.; Gilman, D.; More, A.; Anguita, T.; Auger, M. W.; Bonvin, V.; McMahon, R.; Meylan, G.; Wong, K. C.; Abbott, T. M. C.; Annis, J.; Avila, S.; Bechtol, K.; Brooks, D.; Brout, D.; Burke, D. L.; Carnero Rosell, A.; Carrasco Kind, M.; Carretero, J.; Castander, F. J.; Costanzi, M.; da Costa, L. N.; De Vicente, J.; Desai, S.; Dietrich, J. P.; Doel, P.; Drlica-Wagner, A.; Evrard, A. E.; Finley, D. A.; Flaugher, B.; Fosalba, P.; García-Bellido, J.; Gerdes, D. W.; Gruen, D.; Gruendl, R. A.; Gschwend, J.; Gutierrez, G.; Hollowood, D. L.; Honscheid, K.; Huterer, D.; James, D. J.; Jeltema, T.; Krause, E.; Kuropatkin, N.; Li, T. S.; Lima, M.; MacCrann, N.; Maia, M. A. G.; Marshall, J. L.; Melchior, P.; Miquel, R.; Ogando, R. L. C.; Palmese, A.; Paz-Chinchón, F.; Plazas, A. A.; Romer, A. K.; Roodman, A.; Sako, M.; Sanchez, E.; Santiago, B.; Scarpine, V.; Schubnell, M.; Scolnic, D.; Serrano, S.; Sevilla-Noarbe, I.; Smith, M.; Soares-Santos, M.; Suchyta, E.; Tarle, G.; Thomas, D.; Walker, A. R.; Zhang, Y.

doi:10.1093/mnras/staa828

Title: STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354

Abstract

We present a blind time-delay cosmographic analysis for the lens system DES J0408-5354. This system is extraordinary for the presence of two sets of multiple images at different redshifts, which provide the opportunity to obtain more information at the cost of increased modelling complexity with respect to previously analysed systems. We perform detailed modelling of the mass distribution for this lens system using three band Hubble Space Telescope imaging. We combine the measured time delays, line-of-sight central velocity dispersion of the deflector, and statistically constrained external convergence with our lens models to estimate two cosmological distances. We measure the ‘effective’ time-delay distance corresponding to the redshifts of the deflector and the lensed quasar $$D_{\Delta t}^{\rm eff}=$$$$3382_{-115}^{+146}$$ Mpc and the angular diameter distance to the deflector Dd = $$1711_{-280}^{+376}$$ Mpc, with covariance between the two distances. From these constraints on the cosmological distances, we infer the Hubble constant H0= $$74.2_{-3.0}^{+2.7}$$ km s-1 Mpc-1 assuming a flat ΛCDM cosmology and a uniform prior for Ωm as $$\Omega _{\rm m} \sim \mathcal {U}(0.05, 0.5)$$. This measurement gives the most precise constraint on H0 to date from a single lens. Our measurement is consistent with that obtained from the previous sample of six lenses analysed by the H0 Lenses in COSMOGRAIL’s Wellspring (H0LiCOW) collaboration. It is also consistent with measurements of H0 based on the local distance ladder, reinforcing the tension with the inference from early Universe probes, for example, with 2.2σ discrepancy from the cosmic microwave background measurement.

Authors:

^[1]; Birrer, S. ^[2]; Treu, T. ^[1]; Agnello, A. ^[3]; Buckley-Geer, E. J. ^[4];

^[5]; Christensen, L. ^[3];

^[5]; Lin, H. ^[4]; Millon, M. ^[5]; Poh, J. ^[6];

^[7]; Sluse, D. ^[8];

^[9];

^[10];

^[11]; Courbin, F. ^[5]; Fassnacht, C. D. ^[10]; Frieman, J. ^[12]; Galan, A. ^[5] more »

Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1547, USA
Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1547, USA; Kavli Institute for Particle Astrophysics and Cosmology and Department of Physics, Stanford University, Stanford, CA 94305, USA
DARK, Niels Bohr Institute, University of Copenhagen, Lyngbyvej 2, DK-2100 Copenhagen, Denmark
Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, IL 60510, USA
Institute of Physics, Laboratoire d’Astrophysique, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, Switzerland
Department of Astronomy & Astrophysics, University of Chicago, Chicago, IL 60637, USA; Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
STAR Institute, Quartier Agora - Allée du six Août, 19c B-4000 Liège, Belgium
INAF - Osservatorio Astronomico di Capodimonte, Salita Moiariello, 16, I-80131 Napoli, Italy; European Southern Observatory, Karl-Schwarschild-Str. 2, D-85748 Garching, Germany
Physics Department, UC Davis, 1 Shields Ave., Davis, CA 95616, USA
Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK
Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, IL 60510, USA; Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
The Inter-University Center for Astronomy and Astrophysics, Post bag 4, Ganeshkhind, Pune 411007, India
Departamento de Ciencias Fisicas, Universidad Andres Bello, Fernandez Concha 700, Las Condes, Santiago, Chile
Institute of Astronomy, Madingley Rd, Cambridge CB3 0HA, UK; Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
Kavli IPMU (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan
Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile
Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, Spain
LSST, 933 North Cherry Avenue, Tucson, AZ 85721, USA; Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue Madison, WI 53706-1390, USA
Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK
Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104, USA
Kavli Institute for Particle Astrophysics and Cosmology, P. O. Box 2450, Stanford University, Stanford, CA 94305, USA; SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain; Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, IL 61801, USA; National Center for Supercomputing Applications, 1205 West Clark St., Urbana, IL 61801, USA
Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona) Spain
Institut d’Estudis Espacials de Catalunya (IEEC), E-08034 Barcelona, Spain; Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain
INAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Italy; Institute for Fundamental Physics of the Universe, Via Beirut 2, I-34014 Trieste, Italy
Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil; Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India
Excellence Cluster Origins, Boltzmannstr. 2, D-85748 Garching, Germany; Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 Munich, Germany
Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA; Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
Kavli Institute for Particle Astrophysics and Cosmology, P. O. Box 2450, Stanford University, Stanford, CA 94305, USA; SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA; Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, USA
Santa Cruz Institute for Particle Physics, Santa Cruz, CA 95064, USA
Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA; Department of Physics, The Ohio State University, Columbus, OH 43210, USA
Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
Center for Astrophysics, Harvard and Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA
Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721-0065, USA
Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, IL 60510, USA; Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA; Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544, USA; Observatories of the Carnegie Institution for Science, 813 Santa Barbara St., Pasadena, CA 91101, USA
Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil; Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP 05314-970, Brazil
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544, USA
Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona) Spain; Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain
Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton BN1 9QH, UK
Laboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil; Instituto de Física, UFRGS, Caixa Postal 15051, Porto Alegre, RS - 91501-970, Brazil
Department of Physics, Duke University Durham, NC 27708, USA
Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain; Institut d’Estudis Espacials de Catalunya (IEEC), E-08034 Barcelona, Spain
School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK
Physics Department, Brandeis University, 415 South Street, Waltham, MA 02453, USA
Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA

Publication Date:: 2020-03-28

Research Org.:: Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Michigan, Ann Arbor, MI (United States)

Sponsoring Org.:: USDOE Office of Science (SC), High Energy Physics (HEP); National Aeronautics and Space Administration (NASA); National Science Foundation (NSF); USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR)

Contributing Org.:: DES Collaboration

OSTI Identifier:: 1574968

Alternate Identifier(s):: OSTI ID: 1638052; OSTI ID: 1646600; OSTI ID: 1659591; OSTI ID: 1697972; OSTI ID: 1784944

Report Number(s):: arXiv:1910.06306; FERMILAB-PUB-19-523-AE-SCD; DES-2019-0475
Journal ID: ISSN 0035-8711; oai:inspirehep.net:1759600; TRN: US2001370

Grant/Contract Number:: AC02-07CH11359; SC0007859; SC0019193; AC05-00OR22725; AC02-76SF00515; HST-GO-15320; AST-1714953; AST-1906976; AST-1715611; ACI-1548562; ACI-1445606; PHY-1607611; AST-1138766; AST-1536171; 787866; 664931; AYA2015-71825; ESP2015-66861; FPA2015-68048; SEV-2016-0588; SEV-2016-0597; MDM-2015-0509; 240672; 291329; 306478

Resource Type:: Accepted Manuscript

Journal Name:: Monthly Notices of the Royal Astronomical Society

Additional Journal Information:: Journal Volume: 494; Journal Issue: 4; Journal ID: ISSN 0035-8711

Publisher:: Royal Astronomical Society

Country of Publication:: United States

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; gravitational lensing: strong; cosmological parameters; distance scale; cosmology: observations

Citation Formats


                    Shajib, A. J., Birrer, S., Treu, T., Agnello, A., Buckley-Geer, E. J., Chan, J. H. H., Christensen, L., Lemon, C., Lin, H., Millon, M., Poh, J., Rusu, C. E., Sluse, D., Spiniello, C., Chen, G. C-F, Collett, T., Courbin, F., Fassnacht, C. D., Frieman, J., Galan, A., Gilman, D., More, A., Anguita, T., Auger, M. W., Bonvin, V., McMahon, R., Meylan, G., Wong, K. C., Abbott, T. M. C., Annis, J., Avila, S., Bechtol, K., Brooks, D., Brout, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Drlica-Wagner, A., Evrard, A. E., Finley, D. A., Flaugher, B., Fosalba, P., García-Bellido, J., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., Huterer, D., James, D. J., Jeltema, T., Krause, E., Kuropatkin, N., Li, T. S., Lima, M., MacCrann, N., Maia, M. A. G., Marshall, J. L., Melchior, P., Miquel, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Romer, A. K., Roodman, A., Sako, M., Sanchez, E., Santiago, B., Scarpine, V., Schubnell, M., Scolnic, D., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., Walker, A. R., and Zhang, Y. STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354.  United States: N. p., 2020. 
Web.  doi:10.1093/mnras/staa828.

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                    Shajib, A. J., Birrer, S., Treu, T., Agnello, A., Buckley-Geer, E. J., Chan, J. H. H., Christensen, L., Lemon, C., Lin, H., Millon, M., Poh, J., Rusu, C. E., Sluse, D., Spiniello, C., Chen, G. C-F, Collett, T., Courbin, F., Fassnacht, C. D., Frieman, J., Galan, A., Gilman, D., More, A., Anguita, T., Auger, M. W., Bonvin, V., McMahon, R., Meylan, G., Wong, K. C., Abbott, T. M. C., Annis, J., Avila, S., Bechtol, K., Brooks, D., Brout, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Drlica-Wagner, A., Evrard, A. E., Finley, D. A., Flaugher, B., Fosalba, P., García-Bellido, J., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., Huterer, D., James, D. J., Jeltema, T., Krause, E., Kuropatkin, N., Li, T. S., Lima, M., MacCrann, N., Maia, M. A. G., Marshall, J. L., Melchior, P., Miquel, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Romer, A. K., Roodman, A., Sako, M., Sanchez, E., Santiago, B., Scarpine, V., Schubnell, M., Scolnic, D., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., Walker, A. R., & Zhang, Y. STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354.  United States.  https://doi.org/10.1093/mnras/staa828

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                    Shajib, A. J., Birrer, S., Treu, T., Agnello, A., Buckley-Geer, E. J., Chan, J. H. H., Christensen, L., Lemon, C., Lin, H., Millon, M., Poh, J., Rusu, C. E., Sluse, D., Spiniello, C., Chen, G. C-F, Collett, T., Courbin, F., Fassnacht, C. D., Frieman, J., Galan, A., Gilman, D., More, A., Anguita, T., Auger, M. W., Bonvin, V., McMahon, R., Meylan, G., Wong, K. C., Abbott, T. M. C., Annis, J., Avila, S., Bechtol, K., Brooks, D., Brout, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Drlica-Wagner, A., Evrard, A. E., Finley, D. A., Flaugher, B., Fosalba, P., García-Bellido, J., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., Huterer, D., James, D. J., Jeltema, T., Krause, E., Kuropatkin, N., Li, T. S., Lima, M., MacCrann, N., Maia, M. A. G., Marshall, J. L., Melchior, P., Miquel, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Romer, A. K., Roodman, A., Sako, M., Sanchez, E., Santiago, B., Scarpine, V., Schubnell, M., Scolnic, D., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., Walker, A. R., and Zhang, Y. Sat .  
"STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354".  United States.  https://doi.org/10.1093/mnras/staa828.  https://www.osti.gov/servlets/purl/1574968.

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@article{osti_1574968,

  title        = {STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354},

  author       = {Shajib, A. J. and Birrer, S. and Treu, T. and Agnello, A. and Buckley-Geer, E. J. and Chan, J. H. H. and Christensen, L. and Lemon, C. and Lin, H. and Millon, M. and Poh, J. and Rusu, C. E. and Sluse, D. and Spiniello, C. and Chen, G. C-F and Collett, T. and Courbin, F. and Fassnacht, C. D. and Frieman, J. and Galan, A. and Gilman, D. and More, A. and Anguita, T. and Auger, M. W. and Bonvin, V. and McMahon, R. and Meylan, G. and Wong, K. C. and Abbott, T. M. C. and Annis, J. and Avila, S. and Bechtol, K. and Brooks, D. and Brout, D. and Burke, D. L. and Carnero Rosell, A. and Carrasco Kind, M. and Carretero, J. and Castander, F. J. and Costanzi, M. and da Costa, L. N. and De Vicente, J. and Desai, S. and Dietrich, J. P. and Doel, P. and Drlica-Wagner, A. and Evrard, A. E. and Finley, D. A. and Flaugher, B. and Fosalba, P. and García-Bellido, J. and Gerdes, D. W. and Gruen, D. and Gruendl, R. A. and Gschwend, J. and Gutierrez, G. and Hollowood, D. L. and Honscheid, K. and Huterer, D. and James, D. J. and Jeltema, T. and Krause, E. and Kuropatkin, N. and Li, T. S. and Lima, M. and MacCrann, N. and Maia, M. A. G. and Marshall, J. L. and Melchior, P. and Miquel, R. and Ogando, R. L. C. and Palmese, A. and Paz-Chinchón, F. and Plazas, A. A. and Romer, A. K. and Roodman, A. and Sako, M. and Sanchez, E. and Santiago, B. and Scarpine, V. and Schubnell, M. and Scolnic, D. and Serrano, S. and Sevilla-Noarbe, I. and Smith, M. and Soares-Santos, M. and Suchyta, E. and Tarle, G. and Thomas, D. and Walker, A. R. and Zhang, Y.},

  abstractNote = {We present a blind time-delay cosmographic analysis for the lens system DES J0408-5354. This system is extraordinary for the presence of two sets of multiple images at different redshifts, which provide the opportunity to obtain more information at the cost of increased modelling complexity with respect to previously analysed systems. We perform detailed modelling of the mass distribution for this lens system using three band Hubble Space Telescope imaging. We combine the measured time delays, line-of-sight central velocity dispersion of the deflector, and statistically constrained external convergence with our lens models to estimate two cosmological distances. We measure the ‘effective’ time-delay distance corresponding to the redshifts of the deflector and the lensed quasar $D_{\Delta t}^{\rm eff}=$$3382_{-115}^{+146}$ Mpc and the angular diameter distance to the deflector Dd = $1711_{-280}^{+376}$ Mpc, with covariance between the two distances. From these constraints on the cosmological distances, we infer the Hubble constant H0= $74.2_{-3.0}^{+2.7}$ km s-1 Mpc-1 assuming a flat ΛCDM cosmology and a uniform prior for Ωm as $\Omega _{\rm m} \sim \mathcal {U}(0.05, 0.5)$. This measurement gives the most precise constraint on H0 to date from a single lens. Our measurement is consistent with that obtained from the previous sample of six lenses analysed by the H0 Lenses in COSMOGRAIL’s Wellspring (H0LiCOW) collaboration. It is also consistent with measurements of H0 based on the local distance ladder, reinforcing the tension with the inference from early Universe probes, for example, with 2.2σ discrepancy from the cosmic microwave background measurement.},

  doi          = {10.1093/mnras/staa828},

  journal      = {Monthly Notices of the Royal Astronomical Society},

  number       = 4,

  volume       = 494,

  place        = {United States},

  year         = {2020},

  month        = {3}

}

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H0LiCOW – IV. Lens mass model of HE 0435-1223 and blind measurement of its time-delay distance for cosmology

Journal Article Wong, Kenneth C. ; Suyu, Sherry H. ; Auger, Matthew W. ; ... - Monthly Notices of the Royal Astronomical Society

Strong gravitational lenses with measured time delays between the multiple images allow a direct measurement of the time-delay distance to the lens, and thus a measure of cosmological parameters, particularly the Hubble constant, H0. We present a blind lens model analysis of the quadruply imaged quasar lens HE 0435-1223 using deep Hubble Space Telescope imaging, updated time-delay measurements from the COSmological MOnitoring of GRAvItational Lenses (COSMOGRAIL), a measurement of the velocity dispersion of the lens galaxy based on Keck data, and a characterization of the mass distribution along the line of sight. HE 0435-1223 is the third lens analysed as a part of the H0 Lenses in COSMOGRAIL's Wellspring (H0LiCOW) project. We account for various sources of systematic uncertainty, including the detailed treatment of nearby perturbers, the parametrization of the galaxy light and mass profile, and the regions used for lens modelling. We constrain the effective time-delay distance to be D_Δt=2612more »« less
Cited by 121
https://doi.org/10.1093/mnras/stw3077

Full Text Available
H0LiCOW XII. Lens mass model of WFI2033 − 4723 and blind measurement of its time-delay distance and H0

Journal Article Rusu, Cristian E. ; Wong, Kenneth C. ; Bonvin, Vivien ; ... - Monthly Notices of the Royal Astronomical Society

ABSTRACT We present the lens mass model of the quadruply-imaged gravitationally lensed quasar WFI2033 − 4723, and perform a blind cosmographical analysis based on this system. Our analysis combines (1) time-delay measurements from 14 yr of data obtained by the COSmological MOnitoring of GRAvItational Lenses (COSMOGRAIL) collaboration, (2) high-resolution Hubble Space Telescope imaging, (3) a measurement of the velocity dispersion of the lens galaxy based on ESO-MUSE data, and (4) multi-band, wide-field imaging and spectroscopy characterizing the lens environment. We account for all known sources of systematics, including the influence of nearby perturbers and complex line-of-sight structure, as well as the parametrization of the light and mass profiles of the lensing galaxy. After unblinding, we determine the effective time-delay distance to bemore »« less
https://doi.org/10.1093/mnras/stz3451
TDCOSMO: XII. Improved Hubble constant measurement from lensing time delays using spatially resolved stellar kinematics of the lens galaxy

Journal Article Shajib, Anowar J. ; Mozumdar, Pritom ; Chen, Geoff C.-F. ; ... - Astronomy and Astrophysics

Strong-lensing time delays enable the measurement of the Hubble constant (H₀) independently of other traditional methods. The main limitation to the precision of time-delay cosmography is mass-sheet degeneracy (MSD). Some of the previous TDCOSMO analyses broke the MSD by making standard assumptions about the mass density profile of the lens galaxy, reaching 2% precision from seven lenses. However, this approach could potentially bias the H₀ measurement or underestimate the errors. For this work, we broke the MSD for the first time using spatially resolved kinematics of the lens galaxy in RXJ1131–1231 obtained from the Keck Cosmic Web Imager spectroscopy, in combination with previously published time delay and lens models derived from Hubble Space Telescope imaging. This approach allowed us to robustly estimate H₀, effectively implementing a maximally flexible mass model. Following a blind analysis, we estimated the angular diameter distance to the lens galaxy D_d = 865more »« less
https://doi.org/10.1051/0004-6361/202345878

Full Text Available
TWO ACCURATE TIME-DELAY DISTANCES FROM STRONG LENSING: IMPLICATIONS FOR COSMOLOGY

Journal Article Suyu, S. H. ; Treu, T. ; Auger, M. W. ; ... - Astrophysical Journal

Strong gravitational lenses with measured time delays between the multiple images and models of the lens mass distribution allow a one-step determination of the time-delay distance, and thus a measure of cosmological parameters. We present a blind analysis of the gravitational lens RXJ1131-1231 incorporating (1) the newly measured time delays from COSMOGRAIL, the COSmological MOnitoring of GRAvItational Lenses, (2) archival Hubble Space Telescope imaging of the lens system, (3) a new velocity-dispersion measurement of the lens galaxy of 323 {+-} 20 km s{sup -1} based on Keck spectroscopy, and (4) a characterization of the line-of-sight structures via observations of themore »« less
https://doi.org/10.1088/0004-637X/766/2/70
TDCOSMO: IV. Hierarchical time-delay cosmography – joint inference of the Hubble constant and galaxy density profiles

Journal Article Birrer, S. ; Shajib, A. J. ; Galan, A. ; ... - Astronomy and Astrophysics

We report the H0LiCOW collaboration inferred via strong gravitational lensing time delays a Hubble constant value ofmore »« less
https://doi.org/10.1051/0004-6361/202038861

Full Text Available

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Title: STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354

Abstract

Citation Formats

The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package journal, August 2018

The STRong lensing Insights into the Dark Energy Survey (STRIDES) 2016 follow-up campaign – I. Overview and classification of candidates selected by two techniques journal, August 2018

Nested Sampling conference, January 2004

VDES J2325−5229 a z = 2.7 gravitationally lensed quasar discovered using morphology-independent supervised machine learning journal, November 2016

Models of the strongly lensed quasar DES J0408−5354 journal, September 2017

Astrometric requirements for strong lensing time-delay cosmography journal, August 2019

Looking at the Fundamental Plane through a Gravitational Lens journal, August 2006

Two Accurate Time-Delay Distances from Strong Lensing: Implications for Cosmology journal, March 2013

David Draper and E. I. George, and a rejoinder by the authors journal, November 1999

Abel integral equation inversion and deconvolution by multi-Gaussian approximation journal, January 1991

Discovery of the Lensed Quasar System DES J0408-5354 journal, March 2017

The STRong lensing Insights into the Dark Energy Survey (STRIDES) 2016 follow-up campaign. II. New quasar lenses from double component fitting. journal, August 2018

lenstronomy: Multi-purpose gravitational lens modelling software package journal, December 2018

H0LiCOW – III. Quantifying the effect of mass along the line of sight to the gravitational lens HE 0435−1223 through weighted galaxy counts★ journal, February 2017

The mass-sheet degeneracy and time-delay cosmography: analysis of the strong lens RXJ1131-1231 journal, August 2016

COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses: XVI. Time delays for the quadruply imaged quasar DES J0408−5354 with high-cadence photometric monitoring⋆ journal, January 2018

SHARP – III. First use of adaptive-optics imaging to constrain cosmology with gravitational lens time delays journal, August 2016

ZAP – enhanced PCA sky subtraction for integral field spectroscopy journal, March 2016

Spherical stellar systems with spheroidal velocity distributions journal, June 1985

On the Possibility of Determining Hubble's Parameter and the Masses of Galaxies from the Gravitational Lens Effect journal, September 1964

Cosmological constraints from the double source plane lens SDSSJ0946+1006 journal, July 2014

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample journal, March 2017

KiDS-SQuaD: The KiDS Strongly lensed Quasar Detection project journal, July 2018

A SHARP view of H0LiCOW: H0 from three time-delay gravitational lens systems with adaptive optics imaging journal, September 2019

Measuring angular diameter distances of strong gravitational lenses journal, November 2015

Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant journal, September 1998

H0LiCOW – V. New COSMOGRAIL time delays of HE 0435−1223: H 0 to 3.8 per cent precision from strong lensing in a flat ΛCDM model journal, November 2016

Cosmological Applications of Gravitational Lensing journal, January 1992

Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics journal, February 2020

The relationship between infrared, optical, and ultraviolet extinction journal, October 1989

Tensions between the early and late Universe journal, September 2019

An Accurate Physical Model for Halo Concentrations journal, January 2019

Is every strong lens model unhappy in its own way? Uniform modelling of a sample of 13 quadruply+ imaged quasars journal, December 2018

COLOSSUS: A Python Toolkit for Cosmology, Large-scale Structure, and Dark Matter Halos journal, December 2018

Time-delay cosmography: increased leverage with angular diameter distances journal, April 2016

DES meets Gaia: discovery of strongly lensed quasars from a multiplet search journal, June 2018

Microlensing makes lensed quasar time delays significantly time variable journal, September 2017

UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10 journal, May 2019

Bridges: a uniquely flexible HPC resource for new communities and data analytics conference, January 2015

Data mining for gravitationally lensed quasars journal, February 2015

Fast Calculation of a Family of Elliptical Gravitational Lens Models journal, August 1998

Quantifying Environmental and Line-of-sight Effects in Models of Strong Gravitational Lens Systems journal, February 2017

nestcheck: error analysis, diagnostic tests and plots for nested sampling calculations journal, September 2018

The Sloan Lens ACS Survey. VI. Discovery and Analysis of a Double Einstein Ring1 journal, April 2008

Cosmological parameters from CMB and other data: A Monte Carlo approach journal, November 2002

Discovery of two gravitationally lensed quasars in the Dark Energy Survey journal, October 2015

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

H0LiCOW – IV. Lens mass model of HE 0435−1223 and blind measurement of its time-delay distance for cosmology journal, November 2016

THE SCALING OF STELLAR MASS AND CENTRAL STELLAR VELOCITY DISPERSION FOR QUIESCENT GALAXIES AT z < 0.7 journal, December 2016

Distribution functions for spherical galaxies journal, May 1985

Observation and Confirmation of six Strong-Lensing Systems in the dark Energy Survey Science Verification data journal, August 2016

The Quadruple Gravitational Lens PG 1115+080: Time Delays and Models journal, February 1997

Simulations of the formation, evolution and clustering of galaxies and quasars journal, June 2005

“Refsdal” Meets Popper: Comparing Predictions of the Re-Appearance of the Multiply Imaged Supernova Behind Macsj1149.5+2223 journal, January 2016

Measuring the Value of the Hubble Constant “à la Refsdal” journal, June 2018

Matplotlib: A 2D Graphics Environment journal, January 2007

The SWELLS survey - II. Breaking the disc-halo degeneracy in the spiral galaxy gravitational lens SDSS J2141−0001★: The SWELLS survey - II journal, September 2011

Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships journal, April 2006

Measurements of Ω and Λ from 42 High‐Redshift Supernovae journal, June 1999

The Sloan Lens ACS Survey. I. A Large Spectroscopically Selected Sample of Massive Early‐Type Lens Galaxies journal, February 2006

Gravitational lens Modeling with Basis sets journal, November 2015

SExtractor: Software for source extraction journal, June 1996

Shapelets -- I. A method for image analysis journal, January 2003

A Universal Density Profile from Hierarchical Clustering journal, December 1997

Ray-tracing through the Millennium Simulation: Born corrections and lens-lens coupling in cosmic shear and galaxy-galaxy lensing journal, March 2009

Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing journal, August 2018

iPTF16geu: A multiply imaged, gravitationally lensed type Ia supernova journal, April 2017

SHARP - I. A high-resolution multiband view of the infrared Einstein ring of JVAS B1938+666: SHARP - I. JVAS B1938+666 journal, July 2012

The Sloan Lens ACS Survey. IV. The Mass Density Profile of Early‐Type Galaxies out to 100 Effective Radii journal, September 2007

Cosmology from Gravitational lens time Delays and Planck data journal, June 2014

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

polychord: next-generation nested sampling journal, September 2015

emcee : The MCMC Hammer journal, March 2013

Toward a Halo Mass Function for Precision Cosmology: The Limits of Universality journal, December 2008

Constraining the dark energy equation of state with double-source plane strong lenses: Constraining wDE with compound lenses journal, July 2012

COSMOGRAIL: XVII. Time delays for the quadruply imaged quasar PG 1115+080⋆ journal, August 2018

XSEDE: Accelerating Scientific Discovery journal, September 2014

The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package
journal, August 2018

The STRong lensing Insights into the Dark Energy Survey (STRIDES) 2016 follow-up campaign – I. Overview and classification of candidates selected by two techniques
journal, August 2018

Nested Sampling
conference, January 2004

VDES J2325−5229 a z = 2.7 gravitationally lensed quasar discovered using morphology-independent supervised machine learning
journal, November 2016

Models of the strongly lensed quasar DES J0408−5354
journal, September 2017

Astrometric requirements for strong lensing time-delay cosmography
journal, August 2019

Looking at the Fundamental Plane through a Gravitational Lens
journal, August 2006

Two Accurate Time-Delay Distances from Strong Lensing: Implications for Cosmology
journal, March 2013

David Draper and E. I. George, and a rejoinder by the authors
journal, November 1999

Abel integral equation inversion and deconvolution by multi-Gaussian approximation
journal, January 1991

Discovery of the Lensed Quasar System DES J0408-5354
journal, March 2017

The STRong lensing Insights into the Dark Energy Survey (STRIDES) 2016 follow-up campaign. II. New quasar lenses from double component fitting.
journal, August 2018

lenstronomy: Multi-purpose gravitational lens modelling software package
journal, December 2018

H0LiCOW – III. Quantifying the effect of mass along the line of sight to the gravitational lens HE 0435−1223 through weighted galaxy counts★
journal, February 2017

The mass-sheet degeneracy and time-delay cosmography: analysis of the strong lens RXJ1131-1231
journal, August 2016

COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses: XVI. Time delays for the quadruply imaged quasar DES J0408−5354 with high-cadence photometric monitoring⋆
journal, January 2018

SHARP – III. First use of adaptive-optics imaging to constrain cosmology with gravitational lens time delays
journal, August 2016

ZAP – enhanced PCA sky subtraction for integral field spectroscopy
journal, March 2016

Spherical stellar systems with spheroidal velocity distributions
journal, June 1985

On the Possibility of Determining Hubble's Parameter and the Masses of Galaxies from the Gravitational Lens Effect
journal, September 1964

Cosmological constraints from the double source plane lens SDSSJ0946+1006
journal, July 2014

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
journal, March 2017

KiDS-SQuaD: The KiDS Strongly lensed Quasar Detection project
journal, July 2018

A SHARP view of H0LiCOW: H0 from three time-delay gravitational lens systems with adaptive optics imaging
journal, September 2019

Measuring angular diameter distances of strong gravitational lenses
journal, November 2015

Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
journal, September 1998

H0LiCOW – V. New COSMOGRAIL time delays of HE 0435−1223: H ₀ to 3.8 per cent precision from strong lensing in a flat ΛCDM model
journal, November 2016

Cosmological Applications of Gravitational Lensing
journal, January 1992

Time-delay cosmographic forecasts with strong lensing and JWST stellar kinematics
journal, February 2020

The relationship between infrared, optical, and ultraviolet extinction
journal, October 1989

Tensions between the early and late Universe
journal, September 2019

An Accurate Physical Model for Halo Concentrations
journal, January 2019

Is every strong lens model unhappy in its own way? Uniform modelling of a sample of 13 quadruply+ imaged quasars
journal, December 2018

COLOSSUS: A Python Toolkit for Cosmology, Large-scale Structure, and Dark Matter Halos
journal, December 2018

Time-delay cosmography: increased leverage with angular diameter distances
journal, April 2016

DES meets Gaia: discovery of strongly lensed quasars from a multiplet search
journal, June 2018

Microlensing makes lensed quasar time delays significantly time variable
journal, September 2017

UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10
journal, May 2019

Bridges: a uniquely flexible HPC resource for new communities and data analytics
conference, January 2015

Data mining for gravitationally lensed quasars
journal, February 2015

Fast Calculation of a Family of Elliptical Gravitational Lens Models
journal, August 1998

Quantifying Environmental and Line-of-sight Effects in Models of Strong Gravitational Lens Systems
journal, February 2017

nestcheck: error analysis, diagnostic tests and plots for nested sampling calculations
journal, September 2018

The Sloan Lens ACS Survey. VI. Discovery and Analysis of a Double Einstein Ring1
journal, April 2008

Cosmological parameters from CMB and other data: A Monte Carlo approach
journal, November 2002

Discovery of two gravitationally lensed quasars in the Dark Energy Survey
journal, October 2015

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

H0LiCOW – IV. Lens mass model of HE 0435−1223 and blind measurement of its time-delay distance for cosmology
journal, November 2016

THE SCALING OF STELLAR MASS AND CENTRAL STELLAR VELOCITY DISPERSION FOR QUIESCENT GALAXIES AT z < 0.7
journal, December 2016

Distribution functions for spherical galaxies
journal, May 1985

Observation and Confirmation of six Strong-Lensing Systems in the dark Energy Survey Science Verification data
journal, August 2016

The Quadruple Gravitational Lens PG 1115+080: Time Delays and Models
journal, February 1997

Simulations of the formation, evolution and clustering of galaxies and quasars
journal, June 2005

“Refsdal” Meets Popper: Comparing Predictions of the Re-Appearance of the Multiply Imaged Supernova Behind Macsj1149.5+2223
journal, January 2016

Measuring the Value of the Hubble Constant “à la Refsdal”
journal, June 2018

Matplotlib: A 2D Graphics Environment
journal, January 2007

The SWELLS survey - II. Breaking the disc-halo degeneracy in the spiral galaxy gravitational lens SDSS J2141−0001★: The SWELLS survey - II
journal, September 2011

Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships
journal, April 2006

Measurements of Ω and Λ from 42 High‐Redshift Supernovae
journal, June 1999

The Sloan Lens ACS Survey. I. A Large Spectroscopically Selected Sample of Massive Early‐Type Lens Galaxies
journal, February 2006

Gravitational lens Modeling with Basis sets
journal, November 2015

SExtractor: Software for source extraction
journal, June 1996

Shapelets -- I. A method for image analysis
journal, January 2003

A Universal Density Profile from Hierarchical Clustering
journal, December 1997

Ray-tracing through the Millennium Simulation: Born corrections and lens-lens coupling in cosmic shear and galaxy-galaxy lensing
journal, March 2009

Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing
journal, August 2018

iPTF16geu: A multiply imaged, gravitationally lensed type Ia supernova
journal, April 2017

SHARP - I. A high-resolution multiband view of the infrared Einstein ring of JVAS B1938+666: SHARP - I. JVAS B1938+666
journal, July 2012

The Sloan Lens ACS Survey. IV. The Mass Density Profile of Early‐Type Galaxies out to 100 Effective Radii
journal, September 2007

Cosmology from Gravitational lens time Delays and Planck data
journal, June 2014

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

polychord: next-generation nested sampling
journal, September 2015

`emcee` : The MCMC Hammer
journal, March 2013

Toward a Halo Mass Function for Precision Cosmology: The Limits of Universality
journal, December 2008

Constraining the dark energy equation of state with double-source plane strong lenses: Constraining wDE with compound lenses
journal, July 2012

COSMOGRAIL: XVII. Time delays for the quadruply imaged quasar PG 1115+080⋆
journal, August 2018

XSEDE: Accelerating Scientific Discovery
journal, September 2014

Analytical models for galactic nuclei
journal, January 1996

The relation between velocity dispersion and mass in simulated clusters of galaxies: dependence on the tracer and the baryonic physics
journal, February 2013

The halos of satellite galaxies: the companion of the massive elliptical lens SL2S J08544−0121
journal, November 2010