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Euclid: Testing photometric selection of emission-line galaxy targets

Research output: Contribution to Journal/Magazine › Journal article › peer-review

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Euclid: Testing photometric selection of emission-line galaxy targets. / Euclid Collaboration.
In: Astronomy and Astrophysics, 27.05.2024.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Euclid Collaboration 2024, 'Euclid: Testing photometric selection of emission-line galaxy targets', Astronomy and Astrophysics. <http://adsabs.harvard.edu/abs/2024arXiv240308726C>

APA

Euclid Collaboration (in press). Euclid: Testing photometric selection of emission-line galaxy targets. Astronomy and Astrophysics. http://adsabs.harvard.edu/abs/2024arXiv240308726C

Vancouver

Euclid Collaboration. Euclid: Testing photometric selection of emission-line galaxy targets. Astronomy and Astrophysics. 2024 May 27.

Author

Euclid Collaboration. / Euclid: Testing photometric selection of emission-line galaxy targets. In: Astronomy and Astrophysics. 2024.

Bibtex

@article{daffbf7aa0d64dfc934244dc539928fb,
title = "Euclid: Testing photometric selection of emission-line galaxy targets",
abstract = "Multi-object spectroscopic galaxy surveys typically make use of photometric and colour criteria to select targets. Conversely, the Euclid NISP slitless spectrograph will record spectra for every source over its field of view. Slitless spectroscopy has the advantage of avoiding defining a priori a galaxy sample, but at the price of making the selection function harder to quantify. The Euclid Wide Survey aims at building robust statistical samples of emission-line galaxies with fluxes in the Halpha-NII complex brighter than 2e-16 erg/s/cm^2 and within 0.9",
keywords = "Astrophysics - Cosmology and Nongalactic Astrophysics",
author = "{Euclid Collaboration} and Cagliari, {M. S.} and Granett, {B. R.} and L. Guzzo and M. Bethermin and M. Bolzonella and {de la Torre}, S. and P. Monaco and M. Moresco and Percival, {W. J.} and C. Scarlata and Y. Wang and M. Ezziati and O. Ilbert and {Le Brun}, V. and A. Amara and S. Andreon and N. Auricchio and M. Baldi and S. Bardelli and R. Bender and C. Bodendorf and E. Branchini and M. Brescia and J. Brinchmann and S. Camera and V. Capobianco and C. Carbone and J. Carretero and S. Casas and M. Castellano and S. Cavuoti and A. Cimatti and G. Congedo and Conselice, {C. J.} and L. Conversi and Y. Copin and L. Corcione and F. Courbin and Courtois, {H. M.} and {Da Silva}, A. and H. Degaudenzi and {Di Giorgio}, {A. M.} and J. Dinis and F. Dubath and Duncan, {C. A. J.} and X. Dupac and S. Dusini and A. Ealet and M. Farina and I. Hook",
year = "2024",
month = may,
day = "27",
language = "English",
journal = "Astronomy and Astrophysics",
issn = "1432-0746",
publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - Euclid: Testing photometric selection of emission-line galaxy targets

AU - Euclid Collaboration

AU - Cagliari, M. S.

AU - Granett, B. R.

AU - Guzzo, L.

AU - Bethermin, M.

AU - Bolzonella, M.

AU - de la Torre, S.

AU - Monaco, P.

AU - Moresco, M.

AU - Percival, W. J.

AU - Scarlata, C.

AU - Wang, Y.

AU - Ezziati, M.

AU - Ilbert, O.

AU - Le Brun, V.

AU - Amara, A.

AU - Andreon, S.

AU - Auricchio, N.

AU - Baldi, M.

AU - Bardelli, S.

AU - Bender, R.

AU - Bodendorf, C.

AU - Branchini, E.

AU - Brescia, M.

AU - Brinchmann, J.

AU - Camera, S.

AU - Capobianco, V.

AU - Carbone, C.

AU - Carretero, J.

AU - Casas, S.

AU - Castellano, M.

AU - Cavuoti, S.

AU - Cimatti, A.

AU - Congedo, G.

AU - Conselice, C. J.

AU - Conversi, L.

AU - Copin, Y.

AU - Corcione, L.

AU - Courbin, F.

AU - Courtois, H. M.

AU - Da Silva, A.

AU - Degaudenzi, H.

AU - Di Giorgio, A. M.

AU - Dinis, J.

AU - Dubath, F.

AU - Duncan, C. A. J.

AU - Dupac, X.

AU - Dusini, S.

AU - Ealet, A.

AU - Farina, M.

AU - Hook, I.

PY - 2024/5/27

Y1 - 2024/5/27

N2 - Multi-object spectroscopic galaxy surveys typically make use of photometric and colour criteria to select targets. Conversely, the Euclid NISP slitless spectrograph will record spectra for every source over its field of view. Slitless spectroscopy has the advantage of avoiding defining a priori a galaxy sample, but at the price of making the selection function harder to quantify. The Euclid Wide Survey aims at building robust statistical samples of emission-line galaxies with fluxes in the Halpha-NII complex brighter than 2e-16 erg/s/cm^2 and within 0.9

AB - Multi-object spectroscopic galaxy surveys typically make use of photometric and colour criteria to select targets. Conversely, the Euclid NISP slitless spectrograph will record spectra for every source over its field of view. Slitless spectroscopy has the advantage of avoiding defining a priori a galaxy sample, but at the price of making the selection function harder to quantify. The Euclid Wide Survey aims at building robust statistical samples of emission-line galaxies with fluxes in the Halpha-NII complex brighter than 2e-16 erg/s/cm^2 and within 0.9

KW - Astrophysics - Cosmology and Nongalactic Astrophysics

M3 - Journal article

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 1432-0746

ER -