| Texto completo | |
| Autor(es): Mostrar menos - |
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
Número total de Autores: 75
|
| Afiliação do(s) autor(es): Mostrar menos - | [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
Número total de Afiliações: 44
|
| Tipo de documento: | Artigo Científico |
| Fonte: | Monthly Notices of the Royal Astronomical Society; v. 505, n. 4, p. 5714-5724, AUG 2021. |
| Citações Web of Science: | 0 |
| Resumo | |
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) | |
| Processo FAPESP: | 17/05549-1 - Restrição de parâmetros cosmológicos usando dados de estrutura de grande escala |
| Beneficiário: | Antonino Troja |
| Modalidade de apoio: | Bolsas no Brasil - Pós-Doutorado |
| Processo FAPESP: | 19/04881-8 - Cosmologia com grandes levantamentos de galáxias fotométricos e espectroscópicos |
| Beneficiário: | Hugo Orlando Camacho Chavez |
| Modalidade de apoio: | Bolsas no Brasil - Pós-Doutorado |