Euclid preparation. XXXI. The effect of the variations in photometric
passbands on photometric-redshift accuracy
Euclid Collaboration,Stéphane Paltani,J. Coupon,W. G. Hartley,A. Alvarez-Ayllon,F. Dubath,J. J. Mohr,M. Schirmer,J. -C. Cuillandre,G. Desprez,O. Ilbert,K. Kuijken,N. Aghanim,B. Altieri,A. Amara,N. Auricchio,M. Baldi,R. Bender,C. Bodendorf,D. Bonino,E. Branchini,M. Brescia,J. Brinchmann,S. Camera,V. Capobianco,C. Carbone,V. F. Cardone,J. Carretero,F. J. Castander,M. Castellano,S. Cavuoti,R. Cledassou,G. Congedo,C. J. Conselice,L. Conversi,Y. Copin,L. Corcione,F. Courbin,M. Cropper,A. Da Silva,H. Degaudenzi,J. Dinis,M. Douspis,X. Dupac,S. Dusini,S. Farrens,S. Ferriol,P. Fosalba,M. Frailis,E. Franceschi,P. Franzetti,S. Galeotta,B. Garilli,W. Gillard,B. Gillis,C. Giocoli,A. Grazian,S. V. Haugan,H. Hoekstra,A. Hornstrup,P. Hudelot,K. Jahnke,M. Kümmel,S. Kermiche,A. Kiessling,M. Kilbinger,T. Kitching,R. Kohley,B. Kubik,M. Kunz,H. Kurki-Suonio,S. Ligori,P. B. Lilje,I. Lloro,E. Maiorano,O. Mansutti,O. Marggraf,K. Markovic,F. Marulli,R. Massey,D. C. Masters,S. Maurogordato,H. J. McCracken,E. Medinaceli,S. Mei,M. Melchior,M. Meneghetti,E. Merlin,G. Meylan,M. Moresco,L. Moscardini,E. Munari,S. -M. Niemi,J. Nightingale,C. Padilla,F. Pasian,K. Pedersen,W. J. Percival,V. Pettorino,G. Polenta,M. Poncet,L. A. Popa,F. Raison,R. Rebolo,A. Renzi,J. Rhodes,G. Riccio,E. Romelli,M. Roncarelli,E. Rossetti,R. Saglia,D. Sapone,B. Sartoris,P. Schneider,A. Secroun,C. Sirignano,G. Sirri,J. Skottfelt,L. Stanco,J. -L. Starck,C. Surace,P. Tallada-Crespí,I. Tereno,R. Toledo-Moreo,F. Torradeflot,I. Tutusaus,E. A. Valentijn,L. Valenziano,T. Vassallo,Y. Wang,G. Zamorani,J. Zoubian,S. Andreon,H. Aussel,S. Bardelli,M. Bolzonella,A. Boucaud,D. Di Ferdinando,M. Farina,J. Graciá-Carpio,V. Lindholm,D. Maino,N. Mauri,C. Neissner,V. Scottez,E. Zucca,C. Baccigalupi,M. Ballardini,A. Biviano,A. Blanchard,S. Borgani,A. S. Borlaff,C. Burigana,R. Cabanac,A. Cappi,C. S. Carvalho,S. Casas,G. Castignani,K. Chambers,A. R. Cooray,H. M. Courtois,O. Cucciati,S. Davini,G. De Lucia,H. Dole,J. A. Escartin,S. Escoffier,F. Finelli,S. Fotopoulou,K. Ganga,K. George,G. Gozaliasl,H. Hildebrandt,I. Hook,A. Jimenez Muñoz,B. Joachimi,V. Kansal,E. Keihanen,C. C. Kirkpatrick,A. Loureiro,J. Macias-Perez,G. Maggio,M. Magliocchetti,R. Maoli,S. Marcin,M. Martinelli,N. Martinet,S. Matthew,L. Maurin,R. B. Metcalf,P. Monaco,G. Morgante,S. Nadathur,A. A. Nucita,L. Patrizii,J. E. Pollack,V. Popa,C. Porciani,D. Potter,A. Pourtsidou,L. Pozzetti,M. Pöntinen,P. Reimberg,A. G. Sánchez,Z. Sakr,E. Sefusatti,M. Sereno,A. Spurio Mancini,J. Stadel,J. Steinwagner,R. Teyssier,C. Valieri,J. Valiviita,S. E. van Mierlo,A. Veropalumbo,M. Viel,J. R. Weaver
Astronomy and Astrophysics（2023）
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摘要
The technique of photometric redshifts has become essential for the
exploitation of multi-band extragalactic surveys. While the requirements on
photo-zs for the study of galaxy evolution mostly pertain to the precision and
to the fraction of outliers, the most stringent requirement in their use in
cosmology is on the accuracy, with a level of bias at the sub-percent level for
the Euclid cosmology mission. A separate, and challenging, calibration process
is needed to control the bias at this level of accuracy. The bias in photo-zs
has several distinct origins that may not always be easily overcome. We
identify here one source of bias linked to the spatial or time variability of
the passbands used to determine the photometric colours of galaxies. We first
quantified the effect as observed on several well-known photometric cameras,
and found in particular that, due to the properties of optical filters, the
redshifts of off-axis sources are usually overestimated. We show using simple
simulations that the detailed and complex changes in the shape can be mostly
ignored and that it is sufficient to know the mean wavelength of the passbands
of each photometric observation to correct almost exactly for this bias; the
key point is that this mean wavelength is independent of the spectral energy
distribution of the source}. We use this property to propose a correction that
can be computationally efficiently implemented in some photo-z algorithms, in
particular template-fitting. We verified that our algorithm, implemented in the
new photo-z code Phosphoros, can effectively reduce the bias in photo-zs on
real data using the CFHTLS T007 survey, with an average measured bias Delta z
over the redshift range 0.4更多
