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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

Galaxy clustering in harmonic space from the dark energy survey year 1 data: compatibility with real-space results

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Author(s):
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Andrade-Oliveira, F. [1, 2] ; Camacho, H. [1, 2] ; Faga, L. [3, 2] ; Gomes, R. [3, 2] ; Rosenfeld, R. [2, 4] ; Troja, A. [2, 4] ; Alves, O. [5, 1, 2] ; Doux, C. [6] ; Elvin-Poole, J. [7, 8] ; Fang, X. [9] ; Friedrich, O. [10, 11] ; Kokron, N. [12, 13] ; Lima, M. [3, 2] ; Miranda, V [9] ; Pandey, S. [6] ; Porredon, A. [8, 14, 15] ; Sanchez, J. [16] ; Aguena, M. [3, 2] ; Allam, S. [16] ; Annis, J. [16] ; Avila, S. [17] ; Bertin, E. [18, 19] ; Brooks, D. [20] ; Burke, D. L. [21, 12] ; Kind, M. Carrasco [22, 23] ; Carretero, J. [24] ; Cawthon, R. [25] ; Chang, C. [26, 27] ; Choi, A. [8] ; Costanzi, M. [28, 29, 30] ; Crocce, M. [14, 15] ; da Costa, L. N. [31, 2] ; Pereira, M. E. S. [5] ; Desai, S. [32] ; Diehl, H. T. [16] ; Doel, P. [20] ; Drlica-Wagner, A. [26, 27, 16] ; Everett, S. [33] ; Evrard, A. E. [5, 34] ; Ferrero, I [35] ; Frieman, J. [27, 16] ; Garcia-Bellido, J. [17] ; Gaztanaga, E. [14, 15] ; Gerdes, D. W. [5, 34] ; Gruen, D. [21, 12, 13] ; Gruendl, R. A. [22, 23] ; Hinton, S. R. [36] ; Hollowood, D. L. [33] ; Jain, B. [6] ; James, D. J. [37] ; Kuropatkin, N. [16] ; Lahav, O. [20] ; MacCrann, N. [38] ; Maia, M. A. G. [31, 2] ; March, M. [6] ; Melchior, P. [39] ; Menanteau, F. [22, 23] ; Miquel, R. [40, 24] ; Morgan, R. [25] ; Myles, J. [21, 12, 13] ; Ogando, R. L. C. [31, 2] ; Palmese, A. [27, 16] ; Paz-Chinchon, F. [41, 23] ; Malagon, A. A. Plazas [39] ; Rodriguez-Monroy, M. [42] ; Sanchez, E. [42] ; Scarpine, V [16] ; Serrano, S. [14, 15] ; Sevilla-Noarbe, I [42] ; Smith, M. [43] ; Soares-Santos, M. [5] ; Suchyta, E. [44] ; Tarle, G. [5] ; To, C. [21, 12, 13] ; Collaboration, DES
Total Authors: 75
Affiliation:
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[1] Univ Estadual Paulista, Inst Fis Teor, BR-01140070 Sao Paulo - Brazil
[2] Lab Interinst E Astron LIneA, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ - Brazil
[3] Univ Sao Paulo, Inst Fis, Dept Fis Matemat, CP 66318, BR-05314970 Sao Paulo, SP - Brazil
[4] Univ Estadual Paulista, ICTP South Amer Inst Fundamental Res, Inst Fis Teor, BR-01140070 Sao Paulo - Brazil
[5] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 - USA
[6] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 - USA
[7] Ohio State Univ, Dept Phys, Columbus, OH 43210 - USA
[8] Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 - USA
[9] Univ Arizona, Dept Astron, Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 - USA
[10] Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA - England
[11] Univ Cambridge, Churchill Coll, Cambridge CB3 0DS - England
[12] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, POB 2450, Stanford, CA 94305 - USA
[13] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 - USA
[14] CSIC, Inst Space Sci ICE, Campus UAB, Carrer Can Magrans S-N, E-08193 Barcelona - Spain
[15] Inst Estudis Espacials Catalunya IEEC, E-08034 Barcelona - Spain
[16] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 - USA
[17] Univ Autonoma Madrid, Inst Fis Teor UAM CSIC, E-28049 Madrid - Spain
[18] Inst Astrophys Paris, CNRS, UMR 7095, F-75014 Paris - France
[19] Sorbonne Univ, Inst Astrophys Paris, UMR 7095, UPMC Univ Paris 06, F-75014 Paris - France
[20] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT - England
[21] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 - USA
[22] Univ Illinois, Dept Astron, 1002 W Green St, Urbana, IL 61801 - USA
[23] Natl Ctr Supercomp Applicat, Ctr Astrophys Surveys, 1205 West Clark St, Urbana, IL 61801 - USA
[24] Barcelona Inst Sci & Technol, Inst Fis Altes Energies IFAE, Campus UAB, E-08193 Bel Bellaterra, Barcelona - Spain
[25] Univ Wisconsin, Phys Dept, 2320 Chamberlin Hall, 1150 Univ Ave, Madison, WI 53706 - USA
[26] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 - USA
[27] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 - USA
[28] INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste - Italy
[29] Inst Fundamental Phys Universe, Via Beirut 2, I-34014 Trieste - Italy
[30] Univ Trieste, Dept Phys, Astron Unit, Via Tiepolo 11, I-34131 Trieste - Italy
[31] Observ Nacl, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ - Brazil
[32] IIT Hyderabad, Dept Phys, Kandi 502285, Telangana - India
[33] Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 - USA
[34] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 - USA
[35] Univ Oslo, Inst Theoret Astrophys, POB 1029 Blindern, NO-0315 Oslo - Norway
[36] Univ Queensland, Sch Math & Phys, Brisbane, Qld 4072 - Australia
[37] Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 - USA
[38] Univ Cambridge, Dept Appl Math & Theoret Phys, Cambridge CB3 0WA - England
[39] Princeton Univ, Dept Astrophys Sci, Peyton Hall, Princeton, NJ 08544 - USA
[40] Inst Catalana Recerca & Estudis Avancats, E-08010 Barcelona - Spain
[41] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA - England
[42] Ctr Invest Energet Medioambientales & Tecnol CIEM, Madrid 28040 - Spain
[43] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants - England
[44] Oak Ridge Natl Lab, Comp Sci & Math Div, POB 2009, Oak Ridge, TN 37831 - USA
Total Affiliations: 44
Document type: Journal article
Source: Monthly Notices of the Royal Astronomical Society; v. 505, n. 4, p. 5714-5724, AUG 2021.
Web of Science Citations: 0
Abstract

We perform an analysis in harmonic space of the Dark Energy Survey Year 1 Data (DES-Y1) galaxy clustering photometric data using products obtained for the real-space analysis. We test our pipeline with a suite of lognormal simulations, which are used to validate scale cuts in harmonic space as well as to provide a covariance matrix that takes into account the DES-Y1 mask. We then apply this pipeline to DES-Y1 data taking into account survey property maps derived for the real-space analysis. We compare with real-space DES-Y1 results obtained from a similar pipeline. We show that the harmonic space analysis we develop yields results that are compatible with the real-space analysis for the bias parameters. This verification paves the way to performing a harmonic space analysis for the upcoming DES-Y3 data. (AU)

FAPESP's process: 17/05549-1 - Restriction of cosmological parameters using large-scale structure data
Grantee:Antonino Troja
Support type: Scholarships in Brazil - Post-Doctorate
FAPESP's process: 19/04881-8 - Cosmology with large photometric and spectroscopic galaxy surveys
Grantee:Hugo Orlando Camacho Chavez
Support type: Scholarships in Brazil - Post-Doctorate