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Euclid preparation: XXI. Intermediate-redshift contaminants in the search for z > 6 galaxies within the Euclid Deep Survey

Context. The Euclid mission is expected to discover thousands of z > 6 galaxies in three deep fields, which together will cover a ∼50 deg<sup>2<sup/> area. However, the limited number of Euclid bands (four) and the low availability of ancillary data could make the identification of &l...

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Hauptverfasser: Mierlo, Sophie Emiley van (VerfasserIn) , Caputi, K.I. (VerfasserIn) , Ashby, M. (VerfasserIn) , Atek, H. (VerfasserIn) , Bolzonella, M. (VerfasserIn) , Bowler, R.a.A. (VerfasserIn) , Brammer, G. (VerfasserIn) , Conselice, C.J. (VerfasserIn) , Cuby, J. (VerfasserIn) , Dayal, P. (VerfasserIn) , Díaz-Sánchez, A. (VerfasserIn) , Finkelstein, S.L. (VerfasserIn) , Hoekstra, H. (VerfasserIn) , Humphrey, A. (VerfasserIn) , Ilbert, O. (VerfasserIn) , McCracken, H.J. (VerfasserIn) , Milvang-Jensen, B. (VerfasserIn) , Oesch, P.A. (VerfasserIn) , Pello, R. (VerfasserIn) , Rodighiero, G. (VerfasserIn) , Schirmer, Mischa (VerfasserIn) , Toft, S. (VerfasserIn) , Weaver, J.R. (VerfasserIn) , Wilkins, S.M. (VerfasserIn) , Willott, C.J. (VerfasserIn) , Zamorani, G. (VerfasserIn) , Amara, A. (VerfasserIn) , Auricchio, N. (VerfasserIn) , Baldi, M. (VerfasserIn) , Bender, R. (VerfasserIn) , Bodendorf, C. (VerfasserIn) , Bonino, D. (VerfasserIn) , Branchini, E. (VerfasserIn) , Brescia, M. (VerfasserIn) , Brinchmann, J. (VerfasserIn) , Camera, S. (VerfasserIn) , Capobianco, V. (VerfasserIn) , Carbone, C. (VerfasserIn) , Carretero, J. (VerfasserIn) , Castellano, M. (VerfasserIn) , Cavuoti, S. (VerfasserIn) , Cimatti, A. (VerfasserIn) , Cledassou, R. (VerfasserIn) , Congedo, G. (VerfasserIn) , Conversi, L. (VerfasserIn) , Copin, Y. (VerfasserIn) , Corcione, L. (VerfasserIn) , Courbin, F. (VerfasserIn) , Silva, A. Da (VerfasserIn) , Degaudenzi, H. (VerfasserIn) , Douspis, M. (VerfasserIn) , Dubath, F. (VerfasserIn) , Dupac, X. (VerfasserIn) , Dusini, S. (VerfasserIn) , Farrens, S. (VerfasserIn) , Ferriol, S. (VerfasserIn) , Frailis, M. (VerfasserIn) , Franceschi, E. (VerfasserIn) , Franzetti, P. (VerfasserIn) , Fumana, M. (VerfasserIn) , Galeotta, S. (VerfasserIn) , Garilli, B. (VerfasserIn) , Gillard, W. (VerfasserIn) , Gillis, B. (VerfasserIn) , Giocoli, C. (VerfasserIn) , Grazian, A. (VerfasserIn) , Grupp, F. (VerfasserIn) , Haugan, S.V.H. (VerfasserIn) , Holmes, W. (VerfasserIn) , Hormuth, F. (VerfasserIn) , Hornstrup, A. (VerfasserIn) , Jahnke, Knud (VerfasserIn) , Maturi, Matteo (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2022
In: Astronomy and astrophysics
Year: 2022, Jahrgang: 666, Pages: 1-27
ISSN:1432-0746
DOI:10.1051/0004-6361/202243950
Online-Zugang:Verlag, kostenfrei, Volltext: https://doi.org/10.1051/0004-6361/202243950
Verlag, kostenfrei, Volltext: https://www.aanda.org/articles/aa/abs/2022/10/aa43950-22/aa43950-22.html
Volltext
Verfasserangaben:S.E. van Mierlo, K.I. Caputi, M. Ashby, H. Atek, M. Bolzonella, R.a.A. Bowler, G. Brammer, C.J. Conselice, J. Cuby, P. Dayal, A. Díaz-Sánchez, S.L. Finkelstein, H. Hoekstra, A. Humphrey, O. Ilbert, H. J. McCracken, B. Milvang-Jensen, P. A. Oesch, R. Pello, G. Rodighiero, M. Schirmer, S. Toft, J.R. Weaver, S.M. Wilkins, C.J. Willott, G. Zamorani, A. Amara, N. Auricchio, M. Baldi, R. Bender, C. Bodendorf, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, V. Capobianco, C. Carbone, J. Carretero, M. Castellano, S. Cavuoti, A. Cimatti, R. Cledassou, G. Congedo, L. Conversi, Y. Copin, L. Corcione, F. Courbin, A. Da Silva, H. Degaudenzi, M. Douspis, F. Dubath, X. Dupac, S. Dusini, S. Farrens, S. Ferriol, M. Frailis, E. Franceschi, P. Franzetti, M. Fumana, S. Galeotta, B. Garilli, W. Gillard, B. Gillis, C. Giocoli, A. Grazian, F. Grupp, S.V.H. Haugan, W. Holmes, F. Hormuth, A. Hornstrup, K. Jahnke, M. Kümmel, A. Kiessling, M. Kilbinger, T. Kitching, R. Kohley, M. Kunz, H. Kurki-Suonio, R. Laureijs, S. Ligori, P.B. Lilje, I. Lloro, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovic, F. Marulli, R. Massey, S. Maurogordato, E. Medinaceli, M. Meneghetti, E. Merlin, G. Meylan, M. Moresco, L. Moscardini, E. Munari, S.M. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, V. Pettorino, S. Pires, M. Poncet, L. Popa, L. Pozzetti, F. Raison, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, E. Rossetti, R. Saglia, D. Sapone, B. Sartoris, P. Schneider, A. Secroun, C. Sirignano, G. Sirri, L. Stanco, J.-L. Starck, C. Surace, P. Tallada-Crespí, A.N. Taylor, I. Tereno, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, E.A. Valentijn, L. Valenziano, T. Vassallo, Y. Wang, A. Zacchei, J. Zoubian, S. Andreon, S. Bardelli, A. Boucaud, J. Graciá-Carpio, D. Maino, N. Mauri, S. Mei, F. Sureau, E. Zucca, H. Aussel, C. Baccigalupi, A. Balaguera-Antolínez, A. Biviano, A. Blanchard, S. Borgani, E. Bozzo, C. Burigana, R. Cabanac, F. Calura, A. Cappi, C.S. Carvalho, S. Casas, G. Castignani, C. Colodro-Conde, A.R. Cooray, J. Coupon, H.M. Courtois, M. Crocce, O. Cucciati, S. Davini, H. Dole, J. A. Escartin, S. Escoffier, M. Fabricius, M. Farina, K. Ganga, J. García-Bellido, K. George, F. Giacomini, G. Gozaliasl, S. Gwyn, I. Hook, M. Huertas-Company, V. Kansal, A. Kashlinsky, E. Keihanen, C.C. Kirkpatrick, V. Lindholm, R. Maoli, M. Martinelli, N. Martinet, M. Maturi, R.B. Metcalf, P. Monaco, G. Morgante, A.A. Nucita, L. Patrizii, A. Peel, J. Pollack, V. Popa, C. Porciani, D. Potter, P. Reimberg, A.G. Sánchez, V. Scottez, E. Sefusatti, J. Stadel, R. Teyssier, J. Valiviita, and M. Viel

MARC

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100 1 |a Mierlo, Sophie Emiley van  |e VerfasserIn  |0 (DE-588)1277685983  |0 (DE-627)1830681478  |4 aut 
245 1 0 |a Euclid preparation  |b XXI. Intermediate-redshift contaminants in the search for z > 6 galaxies within the Euclid Deep Survey  |c S.E. van Mierlo, K.I. Caputi, M. Ashby, H. Atek, M. Bolzonella, R.a.A. Bowler, G. Brammer, C.J. Conselice, J. Cuby, P. Dayal, A. Díaz-Sánchez, S.L. Finkelstein, H. Hoekstra, A. Humphrey, O. Ilbert, H. J. McCracken, B. Milvang-Jensen, P. A. Oesch, R. Pello, G. Rodighiero, M. Schirmer, S. Toft, J.R. Weaver, S.M. Wilkins, C.J. Willott, G. Zamorani, A. Amara, N. Auricchio, M. Baldi, R. Bender, C. Bodendorf, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, V. Capobianco, C. Carbone, J. Carretero, M. Castellano, S. Cavuoti, A. Cimatti, R. Cledassou, G. Congedo, L. Conversi, Y. Copin, L. Corcione, F. Courbin, A. Da Silva, H. Degaudenzi, M. Douspis, F. Dubath, X. Dupac, S. Dusini, S. Farrens, S. Ferriol, M. Frailis, E. Franceschi, P. Franzetti, M. Fumana, S. Galeotta, B. Garilli, W. Gillard, B. Gillis, C. Giocoli, A. Grazian, F. Grupp, S.V.H. Haugan, W. Holmes, F. Hormuth, A. Hornstrup, K. Jahnke, M. Kümmel, A. Kiessling, M. Kilbinger, T. Kitching, R. Kohley, M. Kunz, H. Kurki-Suonio, R. Laureijs, S. Ligori, P.B. Lilje, I. Lloro, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovic, F. Marulli, R. Massey, S. Maurogordato, E. Medinaceli, M. Meneghetti, E. Merlin, G. Meylan, M. Moresco, L. Moscardini, E. Munari, S.M. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, V. Pettorino, S. Pires, M. Poncet, L. Popa, L. Pozzetti, F. Raison, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, E. Rossetti, R. Saglia, D. Sapone, B. Sartoris, P. Schneider, A. Secroun, C. Sirignano, G. Sirri, L. Stanco, J.-L. Starck, C. Surace, P. Tallada-Crespí, A.N. Taylor, I. Tereno, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, E.A. Valentijn, L. Valenziano, T. Vassallo, Y. Wang, A. Zacchei, J. Zoubian, S. Andreon, S. Bardelli, A. Boucaud, J. Graciá-Carpio, D. Maino, N. Mauri, S. Mei, F. Sureau, E. Zucca, H. Aussel, C. Baccigalupi, A. Balaguera-Antolínez, A. Biviano, A. Blanchard, S. Borgani, E. Bozzo, C. Burigana, R. Cabanac, F. Calura, A. Cappi, C.S. Carvalho, S. Casas, G. Castignani, C. Colodro-Conde, A.R. Cooray, J. Coupon, H.M. Courtois, M. Crocce, O. Cucciati, S. Davini, H. Dole, J. A. Escartin, S. Escoffier, M. Fabricius, M. Farina, K. Ganga, J. García-Bellido, K. George, F. Giacomini, G. Gozaliasl, S. Gwyn, I. Hook, M. Huertas-Company, V. Kansal, A. Kashlinsky, E. Keihanen, C.C. Kirkpatrick, V. Lindholm, R. Maoli, M. Martinelli, N. Martinet, M. Maturi, R.B. Metcalf, P. Monaco, G. Morgante, A.A. Nucita, L. Patrizii, A. Peel, J. Pollack, V. Popa, C. Porciani, D. Potter, P. Reimberg, A.G. Sánchez, V. Scottez, E. Sefusatti, J. Stadel, R. Teyssier, J. Valiviita, and M. Viel 
264 1 |c 2022 
300 |a 27 
336 |a Text  |b txt  |2 rdacontent 
337 |a Computermedien  |b c  |2 rdamedia 
338 |a Online-Ressource  |b cr  |2 rdacarrier 
500 |a Gesehen am 10.01.2023 
520 |a Context. The Euclid mission is expected to discover thousands of z > 6 galaxies in three deep fields, which together will cover a ∼50 deg<sup>2<sup/> area. However, the limited number of Euclid bands (four) and the low availability of ancillary data could make the identification of <i>z<i/> > 6 galaxies challenging. Aims. In this work we assess the degree of contamination by intermediate-redshift galaxies (z = 1-5.8) expected for z > 6 galaxies within the Euclid Deep Survey. Methods. This study is based on ∼176 000 real galaxies at z = 1-8 in a ∼0.7 deg 2 area selected from the UltraVISTA ultra-deep survey and ∼96 000 mock galaxies with 25.3 ≤ H < 27.0, which altogether cover the range of magnitudes to be probed in the Euclid Deep Survey. We simulate Euclid and ancillary photometry from fiducial 28-band photometry and fit spectral energy distributions to various combinations of these simulated data. Results. We demonstrate that identifying z > 6 galaxies with Euclid data alone will be very effective, with a z > 6 recovery of 91% (88%) for bright (faint) galaxies. For the UltraVISTA-like bright sample, the percentage of z = 1-5.8 contaminants amongst apparent z > 6 galaxies as observed with Euclid alone is 18%, which is reduced to 4% (13%) by including ultra-deep Rubin (Spitzer) photometry. Conversely, for the faint mock sample, the contamination fraction with Euclid alone is considerably higher at 39%, and minimised to 7% when including ultra-deep Rubin data. For UltraVISTA-like bright galaxies, we find that Euclid (IE − YE) > 2.8 and (YE − JE) < 1.4 colour criteria can separate contaminants from true z > 6 galaxies, although these are applicable to only 54% of the contaminants as many have unconstrained (IE − YE) colours. In the best scenario, these cuts reduce the contamination fraction to 1% whilst preserving 81% of the fiducial z > 6 sample. For the faint mock sample, colour cuts are infeasible; we find instead that a 5σ detection threshold requirement in at least one of the Euclid near-infrared bands reduces the contamination fraction to 25%. 
700 1 |a Caputi, K.I.  |e VerfasserIn  |4 aut 
700 1 |a Ashby, M.  |e VerfasserIn  |4 aut 
700 1 |a Atek, H.  |e VerfasserIn  |4 aut 
700 1 |a Bolzonella, M.  |e VerfasserIn  |4 aut 
700 1 |a Bowler, R.a.A.  |e VerfasserIn  |4 aut 
700 1 |a Brammer, G.  |e VerfasserIn  |4 aut 
700 1 |a Conselice, C.J.  |e VerfasserIn  |4 aut 
700 1 |a Cuby, J.  |e VerfasserIn  |4 aut 
700 1 |a Dayal, P.  |e VerfasserIn  |4 aut 
700 1 |a Díaz-Sánchez, A.  |e VerfasserIn  |4 aut 
700 1 |a Finkelstein, S.L.  |e VerfasserIn  |4 aut 
700 1 |a Hoekstra, H.  |e VerfasserIn  |4 aut 
700 1 |a Humphrey, A.  |e VerfasserIn  |4 aut 
700 1 |a Ilbert, O.  |e VerfasserIn  |4 aut 
700 1 |a McCracken, H.J.  |e VerfasserIn  |4 aut 
700 1 |a Milvang-Jensen, B.  |e VerfasserIn  |4 aut 
700 1 |a Oesch, P.A.  |e VerfasserIn  |4 aut 
700 1 |a Pello, R.  |e VerfasserIn  |4 aut 
700 1 |a Rodighiero, G.  |e VerfasserIn  |4 aut 
700 1 |a Schirmer, Mischa  |d 1973-  |e VerfasserIn  |0 (DE-588)128855088  |0 (DE-627)383659418  |0 (DE-576)297365002  |4 aut 
700 1 |a Toft, S.  |e VerfasserIn  |4 aut 
700 1 |a Weaver, J.R.  |e VerfasserIn  |4 aut 
700 1 |a Wilkins, S.M.  |e VerfasserIn  |4 aut 
700 1 |a Willott, C.J.  |e VerfasserIn  |4 aut 
700 1 |a Zamorani, G.  |e VerfasserIn  |4 aut 
700 1 |a Amara, A.  |e VerfasserIn  |4 aut 
700 1 |a Auricchio, N.  |e VerfasserIn  |4 aut 
700 1 |a Baldi, M.  |e VerfasserIn  |4 aut 
700 1 |a Bender, R.  |e VerfasserIn  |4 aut 
700 1 |a Bodendorf, C.  |e VerfasserIn  |4 aut 
700 1 |a Bonino, D.  |e VerfasserIn  |4 aut 
700 1 |a Branchini, E.  |e VerfasserIn  |4 aut 
700 1 |a Brescia, M.  |e VerfasserIn  |4 aut 
700 1 |a Brinchmann, J.  |e VerfasserIn  |4 aut 
700 1 |a Camera, S.  |e VerfasserIn  |4 aut 
700 1 |a Capobianco, V.  |e VerfasserIn  |4 aut 
700 1 |a Carbone, C.  |e VerfasserIn  |4 aut 
700 1 |a Carretero, J.  |e VerfasserIn  |4 aut 
700 1 |a Castellano, M.  |e VerfasserIn  |4 aut 
700 1 |a Cavuoti, S.  |e VerfasserIn  |4 aut 
700 1 |a Cimatti, A.  |e VerfasserIn  |4 aut 
700 1 |a Cledassou, R.  |e VerfasserIn  |4 aut 
700 1 |a Congedo, G.  |e VerfasserIn  |4 aut 
700 1 |a Conversi, L.  |e VerfasserIn  |4 aut 
700 1 |a Copin, Y.  |e VerfasserIn  |4 aut 
700 1 |a Corcione, L.  |e VerfasserIn  |4 aut 
700 1 |a Courbin, F.  |e VerfasserIn  |4 aut 
700 1 |a Silva, A. Da  |e VerfasserIn  |4 aut 
700 1 |a Degaudenzi, H.  |e VerfasserIn  |4 aut 
700 1 |a Douspis, M.  |e VerfasserIn  |4 aut 
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700 1 |a Grupp, F.  |e VerfasserIn  |4 aut 
700 1 |a Haugan, S.V.H.  |e VerfasserIn  |4 aut 
700 1 |a Holmes, W.  |e VerfasserIn  |4 aut 
700 1 |a Hormuth, F.  |e VerfasserIn  |4 aut 
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Intermediate-redshift contaminants in the search for z > 6 galaxies within the Euclid Deep Survey","title":"Euclid preparation","title_sort":"Euclid preparation"}],"type":{"media":"Online-Ressource","bibl":"article-journal"},"note":["Gesehen am 10.01.2023"],"recId":"1830680676","person":[{"given":"Sophie Emiley van","display":"Mierlo, Sophie Emiley van","family":"Mierlo","role":"aut"},{"display":"Caputi, K.I.","given":"K.I.","role":"aut","family":"Caputi"},{"display":"Ashby, M.","given":"M.","family":"Ashby","role":"aut"},{"family":"Atek","role":"aut","given":"H.","display":"Atek, H."},{"display":"Bolzonella, M.","given":"M.","role":"aut","family":"Bolzonella"},{"family":"Bowler","role":"aut","given":"R.a.A.","display":"Bowler, R.a.A."},{"family":"Brammer","role":"aut","display":"Brammer, G.","given":"G."},{"given":"C.J.","display":"Conselice, C.J.","role":"aut","family":"Conselice"},{"role":"aut","family":"Cuby","display":"Cuby, J.","given":"J."},{"family":"Dayal","role":"aut","given":"P.","display":"Dayal, P."},{"display":"Díaz-Sánchez, A.","given":"A.","family":"Díaz-Sánchez","role":"aut"},{"given":"S.L.","display":"Finkelstein, S.L.","family":"Finkelstein","role":"aut"},{"role":"aut","family":"Hoekstra","display":"Hoekstra, H.","given":"H."},{"given":"A.","display":"Humphrey, A.","family":"Humphrey","role":"aut"},{"family":"Ilbert","role":"aut","given":"O.","display":"Ilbert, O."},{"display":"McCracken, H.J.","given":"H.J.","role":"aut","family":"McCracken"},{"family":"Milvang-Jensen","role":"aut","given":"B.","display":"Milvang-Jensen, B."},{"display":"Oesch, P.A.","given":"P.A.","role":"aut","family":"Oesch"},{"role":"aut","family":"Pello","given":"R.","display":"Pello, R."},{"display":"Rodighiero, G.","given":"G.","role":"aut","family":"Rodighiero"},{"role":"aut","family":"Schirmer","display":"Schirmer, Mischa","given":"Mischa"},{"family":"Toft","role":"aut","given":"S.","display":"Toft, S."},{"display":"Weaver, J.R.","given":"J.R.","role":"aut","family":"Weaver"},{"display":"Wilkins, S.M.","given":"S.M.","role":"aut","family":"Wilkins"},{"role":"aut","family":"Willott","given":"C.J.","display":"Willott, C.J."},{"display":"Zamorani, G.","given":"G.","role":"aut","family":"Zamorani"},{"role":"aut","family":"Amara","given":"A.","display":"Amara, A."},{"family":"Auricchio","role":"aut","display":"Auricchio, N.","given":"N."},{"display":"Baldi, M.","given":"M.","family":"Baldi","role":"aut"},{"family":"Bender","role":"aut","display":"Bender, R.","given":"R."},{"role":"aut","family":"Bodendorf","display":"Bodendorf, C.","given":"C."},{"role":"aut","family":"Bonino","display":"Bonino, D.","given":"D."},{"given":"E.","display":"Branchini, E.","family":"Branchini","role":"aut"},{"given":"M.","display":"Brescia, M.","role":"aut","family":"Brescia"},{"role":"aut","family":"Brinchmann","display":"Brinchmann, J.","given":"J."},{"display":"Camera, S.","given":"S.","role":"aut","family":"Camera"},{"display":"Capobianco, V.","given":"V.","family":"Capobianco","role":"aut"},{"family":"Carbone","role":"aut","display":"Carbone, C.","given":"C."},{"family":"Carretero","role":"aut","given":"J.","display":"Carretero, J."},{"family":"Castellano","role":"aut","display":"Castellano, M.","given":"M."},{"given":"S.","display":"Cavuoti, S.","family":"Cavuoti","role":"aut"},{"given":"A.","display":"Cimatti, A.","role":"aut","family":"Cimatti"},{"family":"Cledassou","role":"aut","display":"Cledassou, R.","given":"R."},{"family":"Congedo","role":"aut","display":"Congedo, G.","given":"G."},{"role":"aut","family":"Conversi","given":"L.","display":"Conversi, L."},{"given":"Y.","display":"Copin, Y.","role":"aut","family":"Copin"},{"display":"Corcione, L.","given":"L.","role":"aut","family":"Corcione"},{"role":"aut","family":"Courbin","given":"F.","display":"Courbin, F."},{"family":"Silva","role":"aut","given":"A. 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JSO |a Coupon, H.M. Courtois, M. Crocce, O. Cucciati, S. Davini, H. Dole, J. A. Escartin, S. Escoffier, M. Fabricius, M. Farina, K. Ganga, J. García-Bellido, K. George, F. Giacomini, G. Gozaliasl, S. Gwyn, I. Hook, M. Huertas-Company, V. Kansal, A. Kashlinsky, E. Keihanen, C.C. Kirkpatrick, V. Lindholm, R. Maoli, M. Martinelli, N. Martinet, M. Maturi, R.B. Metcalf, P. Monaco, G. Morgante, A.A. Nucita, L. Patrizii, A. Peel, J. Pollack, V. Popa, C. Porciani, D. Potter, P. Reimberg, A.G. Sánchez, V. Scottez, E. Sefusatti, J. Stadel, R. Teyssier, J. Valiviita, and M. Viel"]},"language":["eng"]} 
SRT |a MIERLOSOPHEUCLIDPREP2022 

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