• Physique

Laboratoire d'études du rayonnement et de la matière en astrophysique et atmosphères | LERMA

  • Unité mixte de recherche

Le LERMA est une unité mixte de recherche. Son activité est centrée autour des 4 axes suivants:

  • Galaxies et cosmologie ;
  • Dynamique des milieux interstellaires et plasma stellaires ;
  • Molécules dans l'Univers ;
  • Instrumentation et télédétection.

Les méthodologies qui y sont développées vont de l'observation sur les grands instruments internationaux, la modélisation, les expériences de laboratoire et le développement instrumental.

Équipes

  • Pôle 1 : "Galaxies et cosmologie" : l’Univers primordial (inflation, fond cosmologique micro onde, réionisation), matière noire (froide, tiède ou gravité modifiée), la formation des galaxies (galaxies à grand redshift, évolution séculaire et fusion de galaxies), trous noirs et galaxies (AGN, starburst, croissance symbiotique et feedback), formation d’étoiles (efficacité, histoire et populations stellaires).
  • Pôle 2 : "Dynamique des milieux interstellaires et plasmas stellaires" : caractérisation observationnelle du cycle des milieux interstellaires, formation des étoile et des planètes, modélisation du milieu interstellaire du gaz diffus aux étoiles et disques, diagnostic chimique de la dynamique du milieu interstellaire, modélisation des transports mécaniques dans les plasmas circumstellaires, expérience de laboratoire sur les plasmas.
  • Pôle 3 : "Molécules dans l’Univers" : expériences pour l’étude des interactions gaz-surfaces (spin, photons et glaces, réactivité sur les surfaces froides), théorie et simulations (excitation collisionnelle et réactivité de molécules interstellaires), expériences de spectroscopie moléculaire (spectroscopie moléculaire et instrumentation laser pour l’environnement, spectroscopie VUV à haute résolution de molécules interstellaires).
  • Pôle 4 : "Instrumentation Térahertz et télédétection" : développement de l’instrumentation hétérodyne THz pour les observatoires au sol ou embarqués (ballons, satellites) tels que Herschel/HIFI et JUICE/SWI, activité de recherche et développement (mélangeurs HEB et SIS, diodes Schottky), télédétection des surfaces et atmosphères.

Direction

  • Benoit Sémelin

Direction adjointe

  • Martina Wiedner
  • Ludovic Petitdemange

Administration

Autres tutelles

  • Centre National de la Recherche Scientifique | CNRS
  • Sorbonne Université
  • Enseignants-chercheurs : 30
  • Chercheurs : 20
  • Personnels d'appui à la recherche : 33
  • Doctorants : 20
  • Post-doctorants : 6

Publications sur HAL - Archive ouverte

Toutes les publications sur HAL
  • Pré-publication, Document de travail

Euclid Quick Data Release (Q1): VIS processing and data products

H.J Mccracken, K Benson, C Dolding, T Flanet, C Grenet, O Herent, P Hudelot, C Laigle, G Leroy, P Liebing, R Massey, S Mottet, R Nakajima, H.N Nguyen-Kim, J.W Nightingale, J Skottfelt, L.C Smith, F Soldano, E Vilenius, M Wander, M von Wietersheim-Kramsta, M Akhlaghi, H Aussel, S Awan, R Azzollini, A Basset, G.P Candini, P Casenove, M Cropper, H Hoekstra, H Israel, A Khalil, K Kuijken, Y Mellier, L Miller, S.-M Niemi, M.J Page, K Paterson, M Schirmer, N.A Walton, A Zacchei, J.P.L.G Barrios, T Erben, R Hayes, J.A Kegerreis, D.J Lagattuta, A Lançon, N Aghanim, B Altieri, A Amara, S Andreon, P.N Appleton, N Auricchio, C Baccigalupi, M Baldi, A Balestra, S Bardelli, P Battaglia, A.N Belikov, R Bender, F Bernardeau, A Biviano, A Bonchi, E Branchini, M Brescia, J Brinchmann, S Camera, G Cañas-Herrera, V Capobianco, C Carbone, J Carretero, S Casas, F.J Castander, M Castellano, G Castignani, S Cavuoti, K.C Chambers, A Cimatti, C Colodro-Conde, G Congedo, C.J Conselice, L Conversi, Y Copin, F Courbin, H.M Courtois, A da Silva, R da Silva, H Degaudenzi, G de Lucia, A.M Di Giorgio, J Dinis, H Dole, F Dubath, X Dupac, S Dusini, A Ealet, S Escoffier, M Fabricius, M Farina, R Farinelli, S Ferriol, F Finelli, P Fosalba, S Fotopoulou, N Fourmanoit, M Frailis, E Franceschi, S Galeotta, K George, W Gillard, B Gillis, C Giocoli, P Gómez-Alvarez, J Gracia-Carpio, B.R Granett, A Grazian, F Grupp, L Guzzo, M Hailey, S.V.H Haugan, J Hoar, W Holmes, F Hormuth, A Hornstrup, K Jahnke, M Jhabvala, B Joachimi, E Keihänen, S Kermiche, A Kiessling, M Kilbinger, B Kubik, M Kümmel, M Kunz, H Kurki-Suonio, Q Le Boulc'H, A.M.C Le Brun, D Le Mignant, S Ligori, P.B Lilje, V Lindholm, I Lloro, G Mainetti, D Maino, E Maiorano, O Mansutti, S Marcin, O Marggraf, M Martinelli, N Martinet, F Marulli, D.C Masters, S Maurogordato, E Medinaceli, S Mei, M Melchior, M Meneghetti, E Merlin, G Meylan, A Mora, M Moresco, L Moscardini, C Neissner, R.C Nichol, C Padilla, S Paltani, F Pasian, K Pedersen, W.J Percival, V Pettorino, S Pires, G Polenta, M Poncet, L.A Popa, L Pozzetti, G.D Racca, F Raison, R Rebolo, A Renzi, J Rhodes, G Riccio, E Romelli, M Roncarelli, E Rossetti, B Rusholme, R Saglia, Z Sakr, A.G Sánchez, D Sapone, B Sartoris, J.A Schewtschenko, P Schneider, T Schrabback, A Secroun, G Seidel, M Seiffert, S Serrano, P Simon, C Sirignano, G Sirri, A. Spurio Mancini, L Stanco, J Steinwagner, P Tallada-Crespí, D Tavagnacco, A.N Taylor, H.I Teplitz, I Tereno, N Tessore, S Toft, R Toledo-Moreo, F Torradeflot, I Tutusaus, E.A Valentijn, L Valenziano, J Valiviita, T Vassallo, G. Verdoes Kleijn, A Veropalumbo, Y Wang, J Weller, G Zamorani, F.M Zerbi, I.A Zinchenko, E Zucca, V Allevato, M Ballardini, M Bolzonella, E Bozzo, C Burigana, R Cabanac, M Calabrese, A Cappi, D Di Ferdinando, J.A. Escartin Vigo, G Fabbian, L Gabarra, M Huertas-Company, J Martín-Fleitas, S Matthew, N Mauri, R.B Metcalf, A Pezzotta, M Pöntinen, C Porciani, I Risso, V Scottez, M Sereno, M Tenti, M Viel, M Wiesmann, Y Akrami, I.T Andika, S Anselmi, M Archidiacono, F Atrio-Barandela, C Benoist, P Bergamini, D Bertacca, M Bethermin, L Bisigello, A Blanchard, L Blot, S Borgani, A.S Borlaff, M.L Brown, S Bruton, A Calabro, B. Camacho Quevedo, F Caro, C.S Carvalho, T Castro, F Cogato, S Conseil, A.R Cooray, O Cucciati, S Davini, F de Paolis, G Desprez, A Díaz-Sánchez, J.J Diaz, S Di Domizio, J.M Diego, P.-A Duc, A Enia, Y Fang, A.M.N Ferguson, A.G Ferrari, A Finoguenov, A Fontana, A Franco, K Ganga, J García-Bellido, T Gasparetto, V Gautard, E Gaztanaga, F Giacomini, F Gianotti, A.H Gonzalez, G Gozaliasl, A Gregorio, M Guidi, C.M Gutierrez, A Hall, W.G Hartley, C Hernández-Monteagudo, H Hildebrandt, J Hjorth, J.J.E Kajava, Y Kang, V Kansal, D Karagiannis, K Kiiveri, C.C Kirkpatrick, S Kruk, J Le Graet, L Legrand, M Lembo, F Lepori, G.F Lesci, J Lesgourgues, L Leuzzi, T.I Liaudat, S.J Liu, A Loureiro, J Macias-Perez, G Maggio, M Magliocchetti, F Mannucci, R Maoli, C.J.A.P Martins, L Maurin, C.J.R Mcpartland, M Miluzio, P Monaco, A Montoro, C Moretti, G Morgante, C Murray, S Nadathur, K Naidoo, A Navarro-Alsina, S Nesseris, F Passalacqua, L Patrizii, A Pisani, D Potter, S Quai, M Radovich, P Reimberg, P.-F Rocci, G Rodighiero, R.P Rollins, S Sacquegna, M Sahlén, D.B Sanders, E Sarpa, C Scarlata, A Schneider, M Schultheis, D Sciotti, E Sellentin, F Shankar, A Silvestri, K Tanidis, C Tao, G Testera, M Tewes, R Teyssier, S Tosi, A Troja, M Tucci, C Valieri, A Venhola, D Vergani, G Verza, P Vielzeuf, J.R Weaver, D Scott

This paper describes the VIS Processing Function (VIS PF) of the Euclid ground segment pipeline, which processes and calibrates raw data from the VIS camera. We present the algorithms used in each processing element, along with a description of the on-orbit performance of VIS PF, based on…

2025. ⟨hal-05019636⟩

  • Pré-publication, Document de travail

Euclid Quick Data Release (Q1). Photometric redshifts and physical properties of galaxies through the PHZ processing function

M Tucci, S Paltani, W.G Hartley, F Dubath, N Morisset, M Bolzonella, S Fotopoulou, F Tarsitano, C Saulder, L Pozzetti, A Enia, Y Kang, H Degaudenzi, R Saglia, M Salvato, O Ilbert, S.A Stanford, W Roster, F.J Castander, A Humphrey, H Landt, M Selwood, G Stevens, N Aghanim, B Altieri, A Amara, S Andreon, N Auricchio, H Aussel, C Baccigalupi, M Baldi, A Balestra, S Bardelli, P Battaglia, A.N Belikov, F Bernardeau, A Biviano, A Bonchi, E Branchini, M Brescia, J Brinchmann, S Camera, G Cañas-Herrera, V Capobianco, C Carbone, J Carretero, S Casas, M Castellano, G Castignani, S Cavuoti, K.C Chambers, A Cimatti, C Colodro-Conde, G Congedo, C.J Conselice, L Conversi, Y Copin, F Courbin, H.M Courtois, M Cropper, A da Silva, G de Lucia, A.M Di Giorgio, H Dole, C.A.J Duncan, X Dupac, A Ealet, S Escoffier, M Fabricius, M Farina, R Farinelli, S Ferriol, F Finelli, N Fourmanoit, M Frailis, E Franceschi, M Fumana, S Galeotta, K George, W Gillard, B Gillis, C Giocoli, P Gómez-Alvarez, J Gracia-Carpio, B.R Granett, A Grazian, F Grupp, S.V.H Haugan, J Hoar, H Hoekstra, W Holmes, I.M Hook, F Hormuth, A Hornstrup, P Hudelot, K Jahnke, M Jhabvala, B Joachimi, E Keihänen, S Kermiche, A Kiessling, M Kilbinger, B Kubik, M Kümmel, M Kunz, H Kurki-Suonio, Q Le Boulc'H, A.M.C Le Brun, D Le Mignant, P Liebing, S Ligori, P.B Lilje, V Lindholm, I Lloro, G Mainetti, D Maino, E Maiorano, O Mansutti, S Marcin, O Marggraf, M Martinelli, N Martinet, F Marulli, R Massey, D.C Masters, S Maurogordato, H.J Mccracken, E Medinaceli, S Mei, M Melchior, Y Mellier, M Meneghetti, E Merlin, G Meylan, A Mora, M Moresco, L Moscardini, R Nakajima, C Neissner, S.-M Niemi, J.W Nightingale, C Padilla, F Pasian, K Pedersen, W.J Percival, V Pettorino, S Pires, G Polenta, M Poncet, L.A Popa, G.D Racca, F Raison, R Rebolo, A Renzi, J Rhodes, G Riccio, E Romelli, M Roncarelli, B Rusholme, Z Sakr, A.G Sánchez, D Sapone, B Sartoris, J.A Schewtschenko, M Schirmer, P Schneider, A Secroun, E Sefusatti, M Seiffert, S Serrano, P Simon, C Sirignano, G Sirri, A Spurio Mancini, L Stanco, J Steinwagner, P Tallada-Crespí, A.N Taylor, H.I Teplitz, I Tereno, N Tessore, S Toft, R Toledo-Moreo, F Torradeflot, I Tutusaus, E.A Valentijn, L Valenziano, J Valiviita, T Vassallo, G. Verdoes Kleijn, A Veropalumbo, Y Wang, J Weller, A Zacchei, G Zamorani, F.M Zerbi, I.A Zinchenko, E Zucca, V Allevato, M Ballardini, C Burigana, R Cabanac, A Cappi, P Casenove, D Di Ferdinando, J.A. Escartin Vigo, G Fabbian, L Gabarra, M Huertas-Company, J Martín-Fleitas, S Matthew, M Maturi, N Mauri, R.B Metcalf, A.A Nucita, A Pezzotta, M Pöntinen, C Porciani, I Risso, V Scottez, M Sereno, M Tenti, M Viel, M Wiesmann, Y Akrami, I.T Andika, S Anselmi, M Archidiacono, F Atrio-Barandela, C Benoist, K Benson, D Bertacca, M Bethermin, L Bisigello, A Blanchard, L Blot, H Böhringer, S Borgani, M.L Brown, S Bruton, A Calabro, B. Camacho Quevedo, F Caro, C.S Carvalho, T Castro, R Chary, F Cogato, A.R Cooray, O Cucciati, S Davini, F de Paolis, G Desprez, A Díaz-Sánchez, J.J Diaz, S Di Domizio, J.M Diego, P.-A Duc, Y Fang, A.M.N Ferguson, A.G Ferrari, P.G Ferreira, A Finoguenov, A Fontana, A Franco, K Ganga, J García-Bellido, T Gasparetto, V Gautard, E Gaztanaga, F Giacomini, A.H Gonzalez, G Gozaliasl, M Guidi, C.M Gutierrez, A Hall, S Hemmati, C Hernández-Monteagudo, H Hildebrandt, J Hjorth, J.J.E Kajava, V Kansal, D Karagiannis, K Kiiveri, C.C Kirkpatrick, S Kruk, J Le Graet, L Legrand, M Lembo, F Lepori, G Leroy, G.F Lesci, J Lesgourgues, L Leuzzi, T.I Liaudat, A Loureiro, J Macias-Perez, G Maggio, M Magliocchetti, E.A Magnier, F Mannucci, R Maoli, C.J.A.P Martins, L Maurin, M Miluzio, P Monaco, C Moretti, G Morgante, S Nadathur, K Naidoo, A Navarro-Alsina, S Nesseris, M Oguri, F Passalacqua, K Paterson, L Patrizii, A Pisani, D Potter, S Quai, M Radovich, P.-F Rocci, G Rodighiero, S Sacquegna, M Sahlén, D.B Sanders, E Sarpa, C Scarlata, J Schaye, A Schneider, D Sciotti, E Sellentin, L.C Smith, K Tanidis, G Testera, R Teyssier, S Tosi, A Troja, C Valieri, A Venhola, D Vergani, G Verza, P Vielzeuf, N.A Walton, J.R Weaver, J.G Sorce, E Soubrie, D Scott

The ESA Euclid mission will measure the photometric redshifts of billions of galaxies in order to provide an accurate 3D view of the Universe at optical and near-infrared wavelengths. Photometric redshifts are determined by the PHZ processing function on the basis of the multi-wavelength photometry…

2025. ⟨hal-05019498⟩

  • Pré-publication, Document de travail

Euclid Quick Data Release (Q1), A first look at the fraction of bars in massive galaxies at $z<1$

M Huertas-Company, M Walmsley, M Siudek, P Iglesias-Navarro, J.H Knapen, S Serjeant, H.J Dickinson, L Fortson, I Garland, T Géron, W Keel, S Kruk, C.J Lintott, K Mantha, K Masters, D O'Ryan, J.J Popp, H Roberts, C Scarlata, J.S Makechemu, B Simmons, R.J Smethurst, A Spindler, M Baes, E.M Corsini, H. Domínguez Sánchez, E Duran-Camacho, H Fu, J Junais, J Mendez-Abreu, A Nersesian, F Shankar, M.N Le, J Vega-Ferrero, L Wang, N Aghanim, B Altieri, A Amara, S Andreon, N Auricchio, C Baccigalupi, M Baldi, A Balestra, S Bardelli, A Basset, P Battaglia, F Bernardeau, A Biviano, A Bonchi, E Branchini, M Brescia, J Brinchmann, S Camera, V Capobianco, C Carbone, J Carretero, S Casas, M Castellano, G Castignani, S Cavuoti, K.C Chambers, A Cimatti, C Colodro-Conde, G Congedo, C.J Conselice, L Conversi, Y Copin, F Courbin, H.M Courtois, M Cropper, A da Silva, H Degaudenzi, G de Lucia, A.M Di Giorgio, C Dolding, H Dole, F Dubath, C.A.J Duncan, X Dupac, S Dusini, A Ealet, S Escoffier, M Fabricius, M Farina, R Farinelli, F Faustini, S Ferriol, F Finelli, S Fotopoulou, M Frailis, S Galeotta, K George, W Gillard, B Gillis, C Giocoli, J Gracia-Carpio, A Grazian, F Grupp, S Gwyn, S.V.H Haugan, H Hoekstra, W Holmes, I.M Hook, F Hormuth, A Hornstrup, P Hudelot, K Jahnke, M Jhabvala, E Keihänen, S Kermiche, B Kubik, K Kuijken, M Kümmel, M Kunz, H Kurki-Suonio, Q Le Boulc'H, A.M.C Le Brun, D Le Mignant, S Ligori, P.B Lilje, V Lindholm, I Lloro, D Maino, E Maiorano, O Mansutti, S Marcin, O Marggraf, M Martinelli, N Martinet, F Marulli, R Massey, H.J Mccracken, E Medinaceli, M Melchior, Y Mellier, M Meneghetti, E Merlin, G Meylan, A Mora, M Moresco, L Moscardini, C Neissner, R.C Nichol, S.-M Niemi, J.W Nightingale, C Padilla, S Paltani, F Pasian, K Pedersen, W.J Percival, V Pettorino, S Pires, G Polenta, M Poncet, L.A Popa, L Pozzetti, F Raison, A Renzi, J Rhodes, G Riccio, E Romelli, M Roncarelli, R Saglia, Z Sakr, D Sapone, B Sartoris, M Schirmer, P Schneider, M Scodeggio, A Secroun, G Seidel, M Seiffert, S Serrano, P Simon, C Sirignano, G Sirri, L Stanco, J Steinwagner, P Tallada-Crespí, A.N Taylor, I Tereno, S Toft, R Toledo-Moreo, F Torradeflot, I Tutusaus, L Valenziano, J Valiviita, T Vassallo, G. Verdoes Kleijn, Y Wang, J Weller, A Zacchei, G Zamorani, F.M Zerbi, I.A Zinchenko, E Zucca, V Allevato, M Ballardini, M Bolzonella, E Bozzo, C Burigana, A Cappi, D Di Ferdinando, J.A. Escartin Vigo, L Gabarra, J Martín-Fleitas, S Matthew, N Mauri, R.B Metcalf, A Pezzotta, M Pöntinen, C Porciani, I Risso, V Scottez, M Sereno, M Tenti, M Viel, M Wiesmann, Y Akrami, I.T Andika, S Anselmi, M Archidiacono, F Atrio-Barandela, C Benoist, K Benson, D Bertacca, M Bethermin, L Bisigello, A Blanchard, L Blot, H Böhringer, S Borgani, M.L Brown, S Bruton, A Calabro, B. Camacho Quevedo, F Caro, C.S Carvalho, T Castro, Y Charles, F Cogato, T Contini, A.R Cooray, O Cucciati, S Davini, F de Paolis, G Desprez, A Díaz-Sánchez, J.J Diaz, S Di Domizio, J.M Diego, P.-A Duc, A Enia, Y Fang, A.G Ferrari, A Finoguenov, A Fontana, F Fontanot, A Franco, K Ganga, J García-Bellido, T Gasparetto, V Gautard, E Gaztanaga, F Giacomini, G Gozaliasl, M Guidi, C.M Gutierrez, A Hall, W.G Hartley, S Hemmati, C Hernández-Monteagudo, H Hildebrandt, J Hjorth, J.J.E Kajava, Y Kang, V Kansal, D Karagiannis, K Kiiveri, C.C Kirkpatrick, J Le Graet, L Legrand, M Lembo, F Lepori, G Leroy, G.F Lesci, J Lesgourgues, L Leuzzi, T.I Liaudat, A Loureiro, J Macias-Perez, G Maggio, M Magliocchetti, E.A Magnier, F Mannucci, R Maoli, C.J.A.P Martins, L Maurin, M Miluzio, P Monaco, C Moretti, G Morgante, C Murray, K Naidoo, A Navarro-Alsina, S Nesseris, F Passalacqua, K Paterson, L Patrizii, A Pisani, D Potter, S Quai, M Radovich, G Rodighiero, S Sacquegna, M Sahlén, D.B Sanders, E Sarpa, J Schaye, A Schneider, M Schultheis, D Sciotti, E Sellentin, L.C Smith, K Tanidis, G Testera, R Teyssier, S Tosi, A Troja, M Tucci, C Valieri, A Venhola, D Vergani, G Verza, P Vielzeuf, N.A Walton, E Soubrie, D Scott

Stellar bars are key structures in disc galaxies, driving angular momentum redistribution and influencing processes such as bulge growth and star formation. Quantifying the bar fraction as a function of redshift and stellar mass is therefore important for constraining the physical processes that…

  • Pré-publication, Document de travail

Euclid Quick Data Release (Q1). NIR processing and data products

G Polenta, M Frailis, A Alavi, P.N Appleton, P Awad, A Bonchi, R Bouwens, L Bramante, D Busonero, G Calderone, F Cogato, S Conseil, M Correnti, R da Silva, I Das, F Faustini, Y Fu, T Gasparetto, W Gillard, A Grazian, S Hemmati, J Jacobson, K Jahnke, B Kubik, X Liu, C Macabiau, E Medinaceli, P.W Morris, K Paterson, M Radovich, M Schirmer, A Shulevski, H.I Teplitz, B Venemans, N Aghanim, B Altieri, A Amara, S Andreon, N Auricchio, H Aussel, C Baccigalupi, M Baldi, A Balestra, S Bardelli, A Basset, P Battaglia, A.N Belikov, R Bender, A Biviano, E Branchini, M Brescia, J Brinchmann, A Caillat, S Camera, G Cañas-Herrera, V Capobianco, C Carbone, J Carretero, S Casas, F.J Castander, M Castellano, G Castignani, S Cavuoti, K.C Chambers, A Cimatti, C Colodro-Conde, G Congedo, C.J Conselice, L Conversi, Y Copin, L Corcione, A Costille, F Courbin, H.M Courtois, A da Silva, H Degaudenzi, G de Lucia, A.M Di Giorgio, H Dole, F Dubath, C.A.J Duncan, X Dupac, S Dusini, A Ealet, S Escoffier, M Fabricius, M Farina, R Farinelli, S Ferriol, F Finelli, S Fotopoulou, N Fourmanoit, E Franceschi, M Fumana, S Galeotta, K George, B Gillis, C Giocoli, P Gómez-Alvarez, J Gracia-Carpio, B.R Granett, F Grupp, S.V.H Haugan, J Hoar, H Hoekstra, W Holmes, I.M Hook, F Hormuth, A Hornstrup, P Hudelot, M Jhabvala, E Keihänen, S Kermiche, A Kiessling, K Kuijken, M Kümmel, M Kunz, H Kurki-Suonio, Q Le Boulc'H, A.M.C Le Brun, D Le Mignant, P Liebing, S Ligori, P.B Lilje, V Lindholm, I Lloro, G Mainetti, D Maino, E Maiorano, O Mansutti, S Marcin, O Marggraf, M Martinelli, N Martinet, F Marulli, R Massey, S Maurogordato, H.J Mccracken, S Mei, M Melchior, Y Mellier, M Meneghetti, E Merlin, G Meylan, A Mora, M Moresco, L Moscardini, R Nakajima, C Neissner, R.C Nichol, S.-M Niemi, J.W Nightingale, C Padilla, S Paltani, F Pasian, K Pedersen, W.J Percival, V Pettorino, S Pires, M Poncet, L.A Popa, L Pozzetti, G.D Racca, F Raison, R Rebolo, A Renzi, J Rhodes, G Riccio, E Romelli, M Roncarelli, E Rossetti, B Rusholme, R Saglia, Z Sakr, A.G Sánchez, D Sapone, B Sartoris, J.A Schewtschenko, P Schneider, M Scodeggio, A Secroun, E Sefusatti, G Seidel, M Seiffert, S Serrano, P Simon, C Sirignano, G Sirri, A. Spurio Mancini, L Stanco, J Steinwagner, P Tallada-Crespí, D Tavagnacco, A.N Taylor, I Tereno, N Tessore, S Toft, R Toledo-Moreo, F Torradeflot, I Tutusaus, E.A Valentijn, L Valenziano, J Valiviita, T Vassallo, G. Verdoes Kleijn, A Veropalumbo, Y Wang, J Weller, A Zacchei, G Zamorani, F.M Zerbi, I.A Zinchenko, E Zucca, V Allevato, M Ballardini, M Bolzonella, E Bozzo, C Burigana, R Cabanac, M Calabrese, A Cappi, P Casenove, D Di Ferdinando, J.A. Escartin Vigo, G Fabbian, L Gabarra, M Huertas-Company, J Martín-Fleitas, S Matthew, N Mauri, A.A Nucita, A Pezzotta, M Pöntinen, C Porciani, I Risso, V Scottez, M Sereno, M Tenti, M Viel, M Wiesmann, Y Akrami, I.T Andika, S Anselmi, M Archidiacono, F Atrio-Barandela, C Benoist, P Bergamini, D Bertacca, M Bethermin, L Bisigello, A Blanchard, L Blot, S Borgani, A.S Borlaff, M.L Brown, S Bruton, A Calabro, B. Camacho Quevedo, F Caro, C.S Carvalho, T Castro, Y Charles, R Chary, A.R Cooray, O Cucciati, S Davini, F de Paolis, G Desprez, A Díaz-Sánchez, J.J Diaz, S Di Domizio, J.M Diego, P.-A Duc, A Enia, Y Fang, A.M.N Ferguson, A.G Ferrari, P.G Ferreira, A Finoguenov, A Fontana, A Franco, K Ganga, J García-Bellido, V Gautard, E Gaztanaga, F Giacomini, F Gianotti, A.H Gonzalez, G Gozaliasl, A Gregorio, A Gruppuso, M Guidi, C.M Gutierrez, A Hall, W.G Hartley, C Hernández-Monteagudo, H Hildebrandt, J Hjorth, J.J.E Kajava, Y Kang, V Kansal, D Karagiannis, K Kiiveri, C.C Kirkpatrick, S Kruk, V Le Brun, J Le Graet, L Legrand, M Lembo, F Lepori, G Leroy, G.F Lesci, J Lesgourgues, L Leuzzi, T.I Liaudat, S.J Liu, A Loureiro, J Macias-Perez, G Maggio, M Magliocchetti, F Mannucci, R Maoli, C.J.A.P Martins, L Maurin, C.J.R Mcpartland, M Miluzio, P Monaco, A Montoro, C Moretti, G Morgante, S Nadathur, K Naidoo, P Natoli, A Navarro-Alsina, S Nesseris, L Nicastro, F Passalacqua, L Patrizii, A Pisani, D Potter, S Quai, P.-F Rocci, G Rodighiero, S Sacquegna, M Sahlén, D.B Sanders, E Sarpa, C Scarlata, A Schneider, D Sciotti, E Sellentin, F Shankar, L.C Smith, K Tanidis, C Tao, G Testera, R Teyssier, S Tosi, A Troja, M Tucci, C Valieri, A Venhola, D Vergani, G Verza, P Vielzeuf, N.A Walton, J.R Weaver, M Bella, D Scott

This paper describes the near-infrared processing function (NIR PF) that processes near-infrared images from the Near-Infrared Spectrometer and Photometer (NISP) instrument onboard the Euclid satellite. NIR PF consists of three main components: (i) a common pre-processing stage for both photometric…

2025. ⟨hal-05018834⟩

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LERMA, Observatoire de Paris, 77 Avenue Denfert Rochereau
75014 PARIS
Adresse physique
LERMA, Observatoire de Paris
77 Avenue Denfert Rochereau
75014 Paris
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