6533b7dbfe1ef96bd1270a1a
RESEARCH PRODUCT
Euclid preparation XIX. Impact of magnification on photometric galaxy clustering
Lepori F.Tutusaus I.Viglione C.Bonvin C.Camera S.Castander F. J.Durrer R.Fosalba P.Jelic-cizmek G.Kunz M.Adamek J.Casas S.Martinelli M.Sakr Z.Sapone D.Amara A.Auricchio N.Bodendorf C.Bonino D.Branchini E.Brescia M.Brinchmann J.Capobianco V.Carbone C.Carretero J.Castellano M.Cavuoti S.Cimatti A.Cledassou R.Congedo G.Conselice C. J.Conversi L.Copin Y.Corcione L.Courbin F.Da Silva A.Degaudenzi H.Douspis M.Dubath F.Dupac X.Dusini S.Ealet A.Farrens S.Ferriol S.Franceschi E.Fumana M.Garilli B.Gillard W.Gillis B.Giocoli C.Grazian A.Grupp F.Guzzo L.Haugan S. V. H.Holmes W.Hormuth F.Hudelot P.Jahnke K.Kermiche S.Kiessling A.Kilbinger M.Kitching T.Kummel M.Kurki-suonio H.Ligori S.Lilje P. B.Lloro I.Mansutti O.Marggraf O.Markovic K.Marulli F.Massey R.Maurogordato S.Melchior M.Meneghetti M.Merlin E.Meylan G.Moresco M.Moscardini L.Munari E.Nakajima R.Niemi S. M.Padilla C.Paltani S.Pasian F.Pedersen K.Percival W. J.Pettorino V.Pires S.Poncet M.Popa L.Pozzetti L.Raison F.Rhodes J.Roncarelli M.Rossetti E.Saglia R.Schneider P.Secroun A.Seidel G.Serrano S.Sirignano C.Sirri G.Stanco L.Starck J. -L.Tallada-crespi P.Taylor A. N.Tereno I.Toledo-moreo R.Torradeflot F.Valentijn E. A.Valenziano L.Wang Y.Weller J.Zamorani G.Zoubian J.Andreon S.Bardelli S.Fabbian G.Gracia-carpio J.Maino D.Medinaceli E.Mei S.Renzi A.Romelli E.Sureau F.Vassallo T.Zacchei A.Zucca E.Baccigalupi C.Balaguera-antolinez A.Bernardeau F.Biviano A.Blanchard A.Bolzonella M.Borgani S.Bozzo E.Burigana C.Cabanac R.Cappi A.Carvalho C. S.Castignani G.Colodro-conde C.Coupon J.Courtois H. M.Cuby J. -G.Davini S.De La Torre S.Di Ferdinando D.Farina M.Ferreira P. G.Finelli F.Galeotta S.Ganga K.Garcia-bellido J.Gaztanaga E.Gozaliasl G.Hook I. M.Ilic S.Joachimi B.Kansal V.Keihanen E.Kirkpatrick C. C.Lindholm V.Mainetti G.Maoli R.Martinet N.Maturi M.Metcalf R. B.Monaco P.Morgante G.Nightingale J.Nucita A.Patrizii L.Popa V.Potter D.Riccio G.Sanchez A. G.Schirmer M.Schultheis M.Scottez V.Sefusatti E.Tramacere A.Valiviita J.Viel M.Hildebrandt H.subject
Cosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsshearkosmologiapower spectragalaksijoukotredshift-space distortionscosmology: theorycosmological parameterstheorydark energyAstrophysics::Galaxy Astrophysicstheory large-scale structure of Universe [cosmological parameters cosmology]theory [cosmology]massive neutrinosunified pipelineAstronomy and Astrophysics115 Astronomy Space scienceangular cross-correlationshalo-modelSpace and Planetary Science[SDU]Sciences of the Universe [physics]fotometriacosmological parametercosmic magnificationlarge-scale structure of UniversecosmologydipoleAstrophysics - Cosmology and Nongalactic Astrophysicsdescription
Aims. We investigate the importance of lensing magnification for estimates of galaxy clustering and its cross-correlation with shear for the photometric sample of Euclid. Using updated specifications, we study the impact of lensing magnification on the constraints and the shift in the estimation of the best fitting cosmological parameters that we expect if this effect is neglected.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2022-01-01 |