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10 results on '"Asorey J"'

1. OzDES reverberation mapping program: Stacking analysis with Hβ, Mg ii and C iv

Author

Malik, U, primary, Sharp, R, additional, Penton, A, additional, Yu, Z, additional, Martini, P, additional, Tucker, B E, additional, Davis, T M, additional, Lewis, G F, additional, Lidman, C, additional, Aguena, M, additional, Alves, O, additional, Annis, J, additional, Asorey, J, additional, Bacon, D, additional, Brooks, D, additional, Rosell, A Carnero, additional, Carretero, J, additional, Cheng, T-Y, additional, da Costa, L N, additional, Pereira, M E S, additional, De Vicente, J, additional, Doel, P, additional, Ferrero, I, additional, Frieman, J, additional, Giannini, G, additional, Gruen, D, additional, Gruendl, R A, additional, Hinton, S R, additional, Hollowood, D L, additional, James, D J, additional, Kuehn, K, additional, Marshall, J L, additional, Mena-Fernández, J, additional, Menanteau, F, additional, Miquel, R, additional, Ogando, R L C, additional, Palmese, A, additional, Pieres, A, additional, Malagón, A A Plazas, additional, Reil, K, additional, Romer, A K, additional, Sanchez, E, additional, Schubnell, M, additional, Smith, M, additional, Suchyta, E, additional, Swanson, M E C, additional, Tarle, G, additional, To, C, additional, Weaverdyck, N, additional, and Wiseman, P, additional

Published
2024
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2. OzDES Reverberation Mapping Program: Hβ lags from the 6-yr survey

Author

Malik, U, primary, Sharp, R, additional, Penton, A, additional, Yu, Z, additional, Martini, P, additional, Lidman, C, additional, Tucker, B E, additional, Davis, T M, additional, Lewis, G F, additional, Aguena, M, additional, Allam, S, additional, Alves, O, additional, Andrade-Oliveira, F, additional, Asorey, J, additional, Bacon, D, additional, Bertin, E, additional, Bocquet, S, additional, Brooks, D, additional, Burke, D L, additional, Carnero Rosell, A, additional, Carollo, D, additional, Carrasco Kind, M, additional, Carretero, J, additional, Costanzi, M, additional, da Costa, L N, additional, Pereira, M E S, additional, De Vicente, J, additional, Desai, S, additional, Diehl, H T, additional, Doel, P, additional, Everett, S, additional, Ferrero, I, additional, Frieman, J, additional, García-Bellido, J, additional, Gerdes, D W, additional, Gruen, D, additional, Gruendl, R A, additional, Gschwend, J, additional, Hinton, S R, additional, Hollowood, D L, additional, Honscheid, K, additional, James, D J, additional, Kuehn, K, additional, Marshall, J L, additional, Mena-Fernández, J, additional, Menanteau, F, additional, Miquel, R, additional, Ogando, R L C, additional, Palmese, A, additional, Paz-Chinchón, F, additional, Pieres, A, additional, Plazas Malagón, A A, additional, Raveri, M, additional, Rodriguez-Monroy, M, additional, Romer, A K, additional, Sanchez, E, additional, Scarpine, V, additional, Sevilla-Noarbe, I, additional, Smith, M, additional, Soares-Santos, M, additional, Suchyta, E, additional, Swanson, M E C, additional, Tarle, G, additional, Taylor, G, additional, Tucker, D L, additional, Weaverdyck, N, additional, and Wilkinson, R D, additional

Published
2023
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3. Using host galaxy spectroscopy to explore systematics in the standardization of Type Ia supernovae

Author

Dixon, M, primary, Lidman, C, additional, Mould, J, additional, Kelsey, L, additional, Brout, D, additional, Möller, A, additional, Wiseman, P, additional, Sullivan, M, additional, Galbany, L, additional, Davis, T M, additional, Vincenzi, M, additional, Scolnic, D, additional, Lewis, G F, additional, Smith, M, additional, Kessler, R, additional, Duffy, A, additional, Taylor, E N, additional, Flynn, C, additional, Abbott, T M C, additional, Aguena, M, additional, Allam, S, additional, Andrade-Oliveira, F, additional, Annis, J, additional, Asorey, J, additional, Bertin, E, additional, Bocquet, S, additional, Brooks, D, additional, Burke, D L, additional, Carnero Rosell, A, additional, Carollo, D, additional, Carrasco Kind, M, additional, Carretero, J, additional, Costanzi, M, additional, da Costa, L N, additional, Pereira, M E S, additional, Doel, P, additional, Everett, S, additional, Ferrero, I, additional, Flaugher, B, additional, Friedel, D, additional, Frieman, J, additional, García-Bellido, J, additional, Gatti, M, additional, Gerdes, D W, additional, Glazebrook, K, additional, Gruen, D, additional, Gschwend, J, additional, Gutierrez, G, additional, Hinton, S R, additional, Hollowood, D L, additional, Honscheid, K, additional, Huterer, D, additional, James, D J, additional, Kuehn, K, additional, Kuropatkin, N, additional, Malik, U, additional, March, M, additional, Menanteau, F, additional, Miquel, R, additional, Morgan, R, additional, Nichol, B, additional, Ogando, R L C, additional, Palmese, A, additional, Paz-Chinchón, F, additional, Pieres, A, additional, Plazas Malagón, A A, additional, Rodriguez-Monroy, M, additional, Romer, A K, additional, Sanchez, E, additional, Scarpine, V, additional, Sevilla-Noarbe, I, additional, Soares-Santos, M, additional, Suchyta, E, additional, Tarle, G, additional, To, C, additional, Tucker, B E, additional, Tucker, D L, additional, and Varga, T N, additional

Published
2022
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4. The dark energy survey 5-yr photometrically identified type Ia supernovae

Author

Möller, A, primary, Smith, M, additional, Sako, M, additional, Sullivan, M, additional, Vincenzi, M, additional, Wiseman, P, additional, Armstrong, P, additional, Asorey, J, additional, Brout, D, additional, Carollo, D, additional, Davis, T M, additional, Frohmaier, C, additional, Galbany, L, additional, Glazebrook, K, additional, Kelsey, L, additional, Kessler, R, additional, Lewis, G F, additional, Lidman, C, additional, Malik, U, additional, Nichol, R C, additional, Scolnic, D, additional, Tucker, B E, additional, Abbott, T M C, additional, Aguena, M, additional, Allam, S, additional, Annis, J, additional, Bertin, E, additional, Bocquet, S, additional, Brooks, D, additional, Burke, D L, additional, Carnero Rosell, A, additional, Carrasco Kind, M, additional, Carretero, J, additional, Castander, F J, additional, Conselice, C, additional, Costanzi, M, additional, Crocce, M, additional, da Costa, L N, additional, De Vicente, J, additional, Desai, S, additional, Diehl, H T, additional, Doel, P, additional, Everett, S, additional, Ferrero, I, additional, Finley, D A, additional, Flaugher, B, additional, Friedel, D, additional, Frieman, J, additional, García-Bellido, J, additional, Gerdes, D W, additional, Gruen, D, additional, Gruendl, R A, additional, Gschwend, J, additional, Gutierrez, G, additional, Herner, K, additional, Hinton, S R, additional, Hollowood, D L, additional, Honscheid, K, additional, James, D J, additional, Kuehn, K, additional, Kuropatkin, N, additional, Lahav, O, additional, March, M, additional, Marshall, J L, additional, Menanteau, F, additional, Miquel, R, additional, Morgan, R, additional, Palmese, A, additional, Paz-Chinchón, F, additional, Pieres, A, additional, Plazas Malagón, A A, additional, Romer, A K, additional, Roodman, A, additional, Sanchez, E, additional, Scarpine, V, additional, Schubnell, M, additional, Serrano, S, additional, Sevilla-Noarbe, I, additional, Suchyta, E, additional, Tarle, G, additional, Thomas, D, additional, To, C, additional, and Varga, T N, additional

Published
2022
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5. Multiwavelength optical and NIR variability analysis of the Blazar PKS 0027-426

Author

Guise, E, primary, Hönig, S F, additional, Almeyda, T, additional, Horne, K, additional, Kishimoto, M, additional, Aguena, M, additional, Allam, S, additional, Andrade-Oliveira, F, additional, Asorey, J, additional, Banerji, M, additional, Bertin, E, additional, Boulderstone, B, additional, Brooks, D, additional, Burke, D L, additional, Carnero Rosell, A, additional, Carollo, D, additional, Carrasco Kind, M, additional, Carretero, J, additional, Costanzi, M, additional, da Costa, L N, additional, Davis, T M, additional, De Vicente, J, additional, Doel, P, additional, Everett, S, additional, Ferrero, I, additional, Flaugher, B, additional, Frieman, J, additional, Gandhi, P, additional, Goad, M, additional, Gruen, D, additional, Gruendl, R A, additional, Gschwend, J, additional, Gutierrez, G, additional, Hinton, S R, additional, Hollowood, D L, additional, Honscheid, K, additional, James, D J, additional, Johnson, M A C, additional, Kuehn, K, additional, Lewis, G F, additional, Lidman, C, additional, Lima, M, additional, Maia, M A G, additional, Malik, U, additional, Menanteau, F, additional, Miquel, R, additional, Morgan, R, additional, Ogando, R L C, additional, Palmese, A, additional, Paz-Chinchón, F, additional, Pereira, M E S, additional, Pieres, A, additional, Plazas Malagón, A A, additional, Sanchez, E, additional, Scarpine, V, additional, Serrano, S, additional, Sevilla-Noarbe, I, additional, Seymour, N, additional, Smith, M, additional, Soares-Santos, M, additional, Suchyta, E, additional, Swanson, M E C, additional, Tarle, G, additional, To, C, additional, and Tucker, B E, additional

Published
2021
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6. OzDES Reverberation Mapping Programme: the first Mg ii lags from 5 yr of monitoring

Author

Yu, Zhefu, primary, Martini, Paul, additional, Penton, A, additional, Davis, T M, additional, Malik, U, additional, Lidman, C, additional, Tucker, B E, additional, Sharp, R, additional, Kochanek, C S, additional, Peterson, B M, additional, Aguena, M, additional, Allam, S, additional, Andrade-Oliveira, F, additional, Annis, J, additional, Asorey, J, additional, Bertin, E, additional, Brooks, D, additional, Burke, D L, additional, Calcino, J, additional, Carnero Rosell, A, additional, Carollo, D, additional, Carrasco Kind, M, additional, Costanzi, M, additional, da Costa, L N, additional, da Silva Pereira, M E S, additional, Diehl, H T, additional, Everett, S, additional, Ferrero, I, additional, Flaugher, B, additional, Frieman, J, additional, García-Bellido, J, additional, Gaztanaga, E, additional, Gerdes, D W, additional, Gruen, D, additional, Gruendl, R A, additional, Gschwend, J, additional, Gutierrez, G, additional, Hinton, S R, additional, Hollowood, D L, additional, James, D J, additional, Kim, A G, additional, Kron, R, additional, Kuehn, K, additional, Kuropatkin, N, additional, Lewis, G F, additional, Maia, M A G, additional, March, M, additional, Marshall, J L, additional, Menanteau, F, additional, Miquel, R, additional, Morgan, R, additional, Möller, A, additional, Palmese, A, additional, Paz-Chinchón, F, additional, Plazas, A A, additional, Sanchez, E, additional, Scarpine, V, additional, Serrano, S, additional, Sevilla-Noarbe, I, additional, Smith, M, additional, Soares-Santos, M, additional, Suchyta, E, additional, Tarle, G, additional, Thomas, D, additional, To, C, additional, and Tucker, D L, additional

Published
2021
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7. Rates and delay times of type Ia supernovae in the Dark Energy Survey

Author

Wiseman, P, primary, Sullivan, M, additional, Smith, M, additional, Frohmaier, C, additional, Vincenzi, M, additional, Graur, O, additional, Popovic, B, additional, Armstrong, P, additional, Brout, D, additional, Davis, T M, additional, Galbany, L, additional, Hinton, S R, additional, Kelsey, L, additional, Kessler, R, additional, Lidman, C, additional, Möller, A, additional, Nichol, R C, additional, Rose, B, additional, Scolnic, D, additional, Toy, M, additional, Zontou, Z, additional, Asorey, J, additional, Carollo, D, additional, Glazebrook, K, additional, Lewis, G F, additional, Tucker, B E, additional, Abbott, T M C, additional, Aguena, M, additional, Allam, S, additional, Andrade-Oliveira, F, additional, Annis, J, additional, Bacon, D, additional, Bertin, E, additional, Brooks, D, additional, Buckley-Geer, E, additional, Burke, D L, additional, Rosell, A Carnero, additional, Kind, M Carrasco, additional, Carretero, J, additional, Costanzi, M, additional, da Costa, L N, additional, Pereira, M E S, additional, Desai, S, additional, Diehl, H T, additional, Doel, P, additional, Everett, S, additional, Ferrero, I, additional, Flaugher, B, additional, Fosalba, P, additional, Frieman, J, additional, García-Bellido, J, additional, Gaztanaga, E, additional, Giannantonio, T, additional, Gruen, D, additional, Gruendl, R A, additional, Gschwend, J, additional, Gutierrez, G, additional, Hollowood, D L, additional, Honscheid, K, additional, Hoyle, B, additional, James, D J, additional, Krause, E, additional, Kuehn, K, additional, Kuropatkin, N, additional, Maia, M A G, additional, Marshall, J L, additional, Martini, P, additional, Menanteau, F, additional, Miquel, R, additional, Morgan, R, additional, Ogando, R L C, additional, Palmese, A, additional, Paz-Chinchón, F, additional, Petravick, D, additional, Pieres, A, additional, Malagón, A A Plazas, additional, Romer, A K, additional, Sanchez, E, additional, Scarpine, V, additional, Schubnell, M, additional, Serrano, S, additional, Sevilla-Noarbe, I, additional, Soares-Santos, M, additional, Suchyta, E, additional, Swanson, M E C, additional, Tarle, G, additional, Thomas, D, additional, To, C, additional, Varga, T N, additional, and Walker, A R, additional

Published
2021
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8. Dark Energy Survey Year 1 results: cross-correlation redshifts – methods and systematics characterization

Author

Gatti, M, primary, Vielzeuf, P, additional, Davis, C, additional, Cawthon, R, additional, Rau, M M, additional, DeRose, J, additional, De Vicente, J, additional, Alarcon, A, additional, Rozo, E, additional, Gaztanaga, E, additional, Hoyle, B, additional, Miquel, R, additional, Bernstein, G M, additional, Bonnett, C, additional, Carnero Rosell, A, additional, Castander, F J, additional, Chang, C, additional, da Costa, L N, additional, Gruen, D, additional, Gschwend, J, additional, Hartley, W G, additional, Lin, H, additional, MacCrann, N, additional, Maia, M A G, additional, Ogando, R L C, additional, Roodman, A, additional, Sevilla-Noarbe, I, additional, Troxel, M A, additional, Wechsler, R H, additional, Asorey, J, additional, Davis, T M, additional, Glazebrook, K, additional, Hinton, S R, additional, Lewis, G, additional, Lidman, C, additional, Macaulay, E, additional, Möller, A, additional, O'Neill, C R, additional, Sommer, N E, additional, Uddin, S A, additional, Yuan, F, additional, Zhang, B, additional, Abbott, T M C, additional, Allam, S, additional, Annis, J, additional, Bechtol, K, additional, Brooks, D, additional, Burke, D L, additional, Carollo, D, additional, Carrasco Kind, M, additional, Carretero, J, additional, Cunha, C E, additional, D'Andrea, C B, additional, DePoy, D L, additional, Desai, S, additional, Eifler, T F, additional, Evrard, A E, additional, Flaugher, B, additional, Fosalba, P, additional, Frieman, J, additional, García-Bellido, J, additional, Gerdes, D W, additional, Goldstein, D A, additional, Gruendl, R A, additional, Gutierrez, G, additional, Honscheid, K, additional, Hoormann, J K, additional, Jain, B, additional, James, D J, additional, Jarvis, M, additional, Jeltema, T, additional, Johnson, M W G, additional, Johnson, M D, additional, Krause, E, additional, Kuehn, K, additional, Kuhlmann, S, additional, Kuropatkin, N, additional, Li, T S, additional, Lima, M, additional, Marshall, J L, additional, Melchior, P, additional, Menanteau, F, additional, Nichol, R C, additional, Nord, B, additional, Plazas, A A, additional, Reil, K, additional, Rykoff, E S, additional, Sako, M, additional, Sanchez, E, additional, Scarpine, V, additional, Schubnell, M, additional, Sheldon, E, additional, Smith, M, additional, Smith, R C, additional, Soares-Santos, M, additional, Sobreira, F, additional, Suchyta, E, additional, Swanson, M E C, additional, Tarle, G, additional, Thomas, D, additional, Tucker, B E, additional, Tucker, D L, additional, Vikram, V, additional, Walker, A R, additional, Weller, J, additional, Wester, W, additional, and Wolf, R C, additional

Published
2018
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10. Using host galaxy spectroscopy to explore systematics in the standardization of Type Ia supernovae

Author

M Dixon, C Lidman, J Mould, L Kelsey, D Brout, A Möller, P Wiseman, M Sullivan, L Galbany, T M Davis, M Vincenzi, D Scolnic, G F Lewis, M Smith, R Kessler, A Duffy, E N Taylor, C Flynn, T M C Abbott, M Aguena, S Allam, F Andrade-Oliveira, J Annis, J Asorey, E Bertin, S Bocquet, D Brooks, D L Burke, A Carnero Rosell, D Carollo, M Carrasco Kind, J Carretero, M Costanzi, L N da Costa, M E S Pereira, P Doel, S Everett, I Ferrero, B Flaugher, D Friedel, J Frieman, J García-Bellido, M Gatti, D W Gerdes, K Glazebrook, D Gruen, J Gschwend, G Gutierrez, S R Hinton, D L Hollowood, K Honscheid, D Huterer, D J James, K Kuehn, N Kuropatkin, U Malik, M March, F Menanteau, R Miquel, R Morgan, B Nichol, R L C Ogando, A Palmese, F Paz-Chinchón, A Pieres, A A Plazas Malagón, M Rodriguez-Monroy, A K Romer, E Sanchez, V Scarpine, I Sevilla-Noarbe, M Soares-Santos, E Suchyta, G Tarle, C To, B E Tucker, D L Tucker, T N Varga, Dixon, M., Lidman, C., Mould, J., Kelsey, L., Brout, D., Möller, A., Wiseman, P., Sullivan, M., Galbany, L., Davis, T. M., Vincenzi, M., Scolnic, D., Lewis, G. F., Smith, M., Kessler, R., Duffy, A., Taylor, E. N., Flynn, C., Abbott, T. M. C., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Asorey, J., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carollo, D., Carrasco Kind, M., Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Doel, P., Everett, S., Ferrero, I., Flaugher, B., Friedel, D., Frieman, J., García-Bellido, J., Gatti, M., Gerdes, D. W., Glazebrook, K., Gruen, D., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Huterer, D., James, D. J., Kuehn, K., Kuropatkin, N., Malik, U., March, M., Menanteau, F., Miquel, R., Morgan, R., Nichol, B., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A. A., Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Scarpine, V., Sevilla-Noarbe, I., Soares-Santos, M., Suchyta, E., Tarle, G., To, C., Tucker, B. E., Tucker, D. L., Varga, T. N., Australian Research Council, Department of Energy (US), National Science Foundation (US), Ministerio de Ciencia, Innovación y Universidades (España), Science and Technology Facilities Council (UK), Agencia Estatal de Investigación (España), Generalitat de Catalunya, European Commission, and European Research Council

Subjects
Galaxies: general, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cosmology: observations, cosmology observations, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Surveys, Astrophysics - Astrophysics of Galaxies, Space and Planetary Science, surveys, galaxies general, Astrophysics of Galaxies (astro-ph.GA), Astrophysics::Solar and Stellar Astrophysics, survey, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

M. Dixon et al., We use stacked spectra of the host galaxies of photometrically identified Type Ia supernovae (SNe Ia) from the Dark Energy Survey (DES) to search for correlations between Hubble diagram residuals and the spectral properties of the host galaxies. Utilizing full spectrum fitting techniques on stacked spectra binned by Hubble residual, we find no evidence for trends between Hubble residuals and properties of the host galaxies that rely on spectral absorption features (, MD would like to acknowledge support through an Australian Government Research Training Program Scholarship. This research was supported by the Australian Research Council The Centre of Excellence for Dark Matter Particle Physics (CDM; project number CE200100008) and the Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav; project number CE170100004). This project/publication was made possible through the support of a grant from the John Templeton Foundation. The authors gratefully acknowledge this grant ID 61807, Two Standard Models Meet. The opinions expressed in this publication are those of the author(s) and do not necessarily reflect the views of the John Templeton Foundation. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft, and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciències de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, NSF’s NOIRLab, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. Based in part on observations at Cerro Tololo Inter-American Observatory at NSF’s NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under Grant Numbers AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under grants ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq grant 465376/2014-2). This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics. Based on data acquired at the Anglo-Australian Telescope, under program A/2013B/012. We acknowledge the traditional custodians of the land on which the AAT stands, the Gamilaraay people, and pay our respects to elders past and present.

Published
2022

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