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Euclid: Fast two-point correlation function covariance through linear construction

Authors :
Keihanen, E.
Lindholm, V.
Monaco, P.
Blot, L.
Carbone, C.
Kiiveri, K.
Sánchez, A. G.
Viitanen, A.
Valiviita, J.
Amara, A.
Auricchio, N.
Baldi, M.
Bonino, D.
Branchini, E.
Brescia, M.
Brinchmann, J.
Camera, S.
Capobianco, V.
Carretero, J.
Castellano, M.
Cavuoti, S.
Cimatti, A.
Cledassou, R.
Congedo, G.
Conversi, L.
Copin, Y.
Corcione, L.
Cropper, M.
Da Silva, A.
Degaudenzi, H.
Douspis, M.
Dubath, F.
Duncan, C. A. J.
Dupac, X.
Dusini, S.
Ealet, A.
Farrens, S.
Ferriol, S.
Frailis, M.
Franceschi, E.
Fumana, M.
Gillis, B.
Giocoli, C.
Grazian, A.
Grupp, F.
Guzzo, L.
Haugan, S. V. H.
Hoekstra, H.
Holmes, W.
Hormuth, F.
Jahnke, K.
Kümmel, M.
Kermiche, S.
Kiessling, A.
Kitching, T.
Kunz, M.
Kurki-Suonio, H.
Ligori, S.
Lilje, P. B.
Lloro, I.
Maiorano, E.
Mansutti, O.
Marggraf, O.
Marulli, F.
Massey, R.
Melchior, M.
Meneghetti, M.
Meylan, G.
Moresco, M.
Morin, B.
Moscardini, L.
Munari, E.
Niemi, S. M.
Padilla, C.
Paltani, S.
Pasian, F.
Pedersen, K.
Pettorino, V.
Pires, S.
Polenta, G.
Poncet, M.
Popa, L.
Raison, F.
Renzi, A.
Rhodes, J.
Romelli, E.
Saglia, R.
Sartoris, B.
Schneider, P.
Schrabback, T.
Secroun, A.
Seidel, G.
Sirignano, C.
Sirri, G.
Stanco, L.
Surace, C.
Tallada-Crespí, P.
Tavagnacco, D.
Taylor, A. N.
Tereno, I.
Toledo-Moreo, R.
Torradeflot, F.
Valentijn, E. A.
Valenziano, L.
Vassallo, T.
Wang, Y.
Weller, J.
Zamorani, G.
Zoubian, J.
Andreon, S.
Maino, D.
de la Torre, S.
Centre National d'Études Spatiales [Toulouse] (CNES)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)
Institut de Physique des 2 Infinis de Lyon (IP2I Lyon)
Université Claude Bernard Lyon 1 (UCBL)
Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Institut d'astrophysique spatiale (IAS)
Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES)
Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Centre de Physique des Particules de Marseille (CPPM)
Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire d'Astrophysique de Marseille (LAM)
Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Euclid
E. Keih??nen
V. Lindholm
P. Monaco
L. Blot
C. Carbone
K. Kiiveri
A. G. S??nchez
A. Viitanen
J. Valiviita
A. Amara
N. Auricchio
M. Baldi
D. Bonino
E. Branchini
M. Brescia
J. Brinchmann
S. Camera
V. Capobianco
J. Carretero
M. Castellano
S. Cavuoti
A. Cimatti
R. Cledassou
G. Congedo
L. Conversi
Y. Copin
L. Corcione
M. Cropper
A. Da Silva
H. Degaudenzi
M. Douspi
F. Dubath
C. A. J. Duncan
X. Dupac
S. Dusini
A. Ealet
S. Farren
S. Ferriol
M. Fraili
E. Franceschi
M. Fumana
B. Gilli
C. Giocoli
A. Grazian
F. Grupp
L. Guzzo
S. V. H. Haugan
H. Hoekstra
W. Holme
F. Hormuth
K. Jahnke
M. K??mmel
S. Kermiche
A. Kiessling
T. Kitching
M. Kunz
H. Kurki-Suonio
S. Ligori
P. B. Lilje
I. Lloro
E. Maiorano
O. Mansutti
O. Marggraf
F. Marulli
R. Massey
M. Melchior
M. Meneghetti
G. Meylan
M. Moresco
B. Morin
L. Moscardini
E. Munari
S. M. Niemi
C. Padilla
S. Paltani
F. Pasian
K. Pedersen
V. Pettorino
S. Pire
G. Polenta
M. Poncet
L. Popa
F. Raison
A. Renzi
J. Rhode
E. Romelli
R. Saglia
B. Sartori
P. Schneider
T. Schrabback
A. Secroun
G. Seidel
C. Sirignano
G. Sirri
L. Stanco
C. Surace
P. Tallada-Cresp??
D. Tavagnacco
A. N. Taylor
I. Tereno
R. Toledo-Moreo
F. Torradeflot
E. A. Valentijn
L. Valenziano
T. Vassallo
Y. Wang
J. Weller
G. Zamorani
J. Zoubian
S. Andreon
D. Maino
S. de la Torre
Keihanen, E.
Lindholm, V.
Monaco, P.
Blot, L.
Carbone, C.
Kiiveri, K.
Sánchez, A. G.
Viitanen, A.
Valiviita, J.
Amara, A.
Auricchio, N.
Baldi, M.
Bonino, D.
Branchini, E.
Brescia, M.
Brinchmann, J.
Camera, S.
Capobianco, V.
Carretero, J.
Castellano, M.
Cavuoti, S.
Cimatti, A.
Cledassou, R.
Congedo, G.
Conversi, L.
Copin, Y.
Corcione, L.
Cropper, M.
Da Silva, A.
Degaudenzi, H.
Douspis, M.
Dubath, F.
Duncan, C. A. J.
Dupac, X.
Dusini, S.
Ealet, A.
Farrens, S.
Ferriol, S.
Frailis, M.
Franceschi, E.
Fumana, M.
Gillis, B.
Giocoli, C.
Grazian, A.
Grupp, F.
Guzzo, L.
Haugan, S. V. H.
Hoekstra, H.
Holmes, W.
Hormuth, F.
Jahnke, K.
Kümmel, M.
Kermiche, S.
Kiessling, A.
Kitching, T.
Kunz, M.
Kurki-Suonio, H.
Ligori, S.
Lilje, P. B.
Lloro, I.
Maiorano, E.
Mansutti, O.
Marggraf, O.
Marulli, F.
Massey, R.
Melchior, M.
Meneghetti, M.
Meylan, G.
Moresco, M.
Morin, B.
Moscardini, L.
Munari, E.
Niemi, S. M.
Padilla, C.
Paltani, S.
Pasian, F.
Pedersen, K.
Pettorino, V.
Pires, S.
Polenta, G.
Poncet, M.
Popa, L.
Raison, F.
Renzi, A.
Rhodes, J.
Romelli, E.
Saglia, R.
Sartoris, B.
Schneider, P.
Schrabback, T.
Secroun, A.
Seidel, G.
Sirignano, C.
Sirri, G.
Stanco, L.
Surace, C.
Tallada-Crespí, P.
Tavagnacco, D.
Taylor, A. N.
Tereno, I.
Toledo-Moreo, R.
Torradeflot, F.
Valentijn, E. A.
Valenziano, L.
Vassallo, T.
Wang, Y.
Weller, J.
Zamorani, G.
Zoubian, J.
Andreon, S.
Maino, D.
de la Torre, S.
Astronomy
Department of Physics
Helsinki Institute of Physics
Particle Physics and Astrophysics
Source :
Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, 2022, 666, pp.A129. ⟨10.1051/0004-6361/202244065⟩, Astronomy and astrophysics, 666:A129. EDP Sciences, Astronomy & Astrophysics, 666, A129
Publication Year :
2022
Publisher :
HAL CCSD, 2022.

Abstract

We present a method for fast evaluation of the covariance matrix for a two-point galaxy correlation function (2PCF) measured with the Landy-Szalay estimator. The standard way of evaluating the covariance matrix consists in running the estimator on a large number of mock catalogs, and evaluating their sample covariance. With large random catalog sizes (data-to-random objects ratio M>>1) the computational cost of the standard method is dominated by that of counting the data-random and random-random pairs, while the uncertainty of the estimate is dominated by that of data-data pairs. We present a method called Linear Construction (LC), where the covariance is estimated for small random catalogs of size M = 1 and M = 2, and the covariance for arbitrary M is constructed as a linear combination of these. We validate the method with PINOCCHIO simulations in range r = 20-200 Mpc/h, and show that the covariance estimate is unbiased. With M = 50 and with 2 Mpc/h bins, the theoretical speed-up of the method is a factor of 14. We discuss the impact on the precision matrix and parameter estimation, and derive a formula for the covariance of covariance.<br />17 pages, 11 figures

Details

Language :
English
ISSN :
00046361
Database :
OpenAIRE
Journal :
Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, 2022, 666, pp.A129. ⟨10.1051/0004-6361/202244065⟩, Astronomy and astrophysics, 666:A129. EDP Sciences, Astronomy & Astrophysics, 666, A129
Accession number :
edsair.doi.dedup.....726089e54577f2daa91e1cdf804e556b
Full Text :
https://doi.org/10.1051/0004-6361/202244065⟩