S. Esco
2 Papers
1 Citations
S. Esco is an academic researcher. The author has an hindex of 1, co-authored 2 publications.
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Papers
Peer Review
Euclid preparation XXIV. Calibration of the halo mass function in Λ ( ν ) CDM cosmologies
Tiago Castro,A. Fumagalli,Raul E. Angulo,Sebastian Bocquet,Stefano Borgani,Carmelita Carbone,Jeppe Dakin,Klaus Dolag,Carlo Giocoli,Pierluigi Monaco,Antonio Ragagnin,A. Saro,Emiliano Sefusatti,M. Costanzi,A. M. C. Le Brun,Pier Stefano Corasaniti,Adam Amara,Luca Amendola,Marco Baldi,Ralf Bender,Christof Tilmann Bodendorf,P. Branchini,Massimo Brescia,Stefano Camera,V. Capobianco,J. Carretero,Marco Castellano,Stefano Cavuoti,Andrea Cimatti,R. Cledassou,G. Congedo,Luca Conversi,Y. Copin,Leonardo Corcione,Frederic Courbin,A Da Silva,H. Degaudenzi,Marian Douspis,F. Dubath,C. A. J. Duncan,X. Dupac,S. Farrens,Sylvain Ferriol,Pablo Fosalba,M. Frailis,E. Franceschi,S. Galeotta,B. Garilli,B. Gillis,Andrea Grazian,Frank Grupp,S. V. Haugan,Felix Hormuth,Allan Hornstrup,P. Hudelot,Knud Jahnke,S. Kermiche,Thomas D. Kitching,Martin Kunz,Hannu Kurki-Suonio,P. B. Lilje,Ivan Lloro,Oriana Mansutti,Ole Marggraf,Federico Marulli,Massimo Meneghetti,Emiliano Merlin,Georges Meylan,Michele Moresco,Lauro Moscardini,E. Munari,Sami Niemi,C. Padilla,Stéphane Paltani,F. Pasian,Kristian Pedersen,Valeria Pettorino,Sandrine Pires,G. Polenta,M. Poncet,L. Popa,Lucia Pozzetti,F. Raison,Rafael Rebolo,A. Renzi,Jason Rhodes,Giuseppe Riccio,E. Romelli,Roberto P. Saglia,Domenico Sapone,Barbara Sartoris,P. Schneider,Gregor Seidel,G. Sirri,Luca Stanco,Paola Crespi,A. N. Taylor,Rafael Toledo-Moreo,F. Torradeflot,Isaac Tutusaus,Edwin A. Valentijn,Luca Valenziano,T. Vassallo,Yu Wang,Jochen Weller,Andrea Zacchei,G. Zamorani,Stefano Andreon,S. Bardelli,Enrico Bozzo,C. Colodro-Conde,D. Di Ferdinando,M. Farina,Javier Graciá-Carpio,V. Lindholm,C. Neissner,V. Scottez,M. Tenti,E. Zucca,Carlo Baccigalupi,A. Balaguera-Antolínez,Mario Ballardini,Francis Bernardeau,Andrea Biviano,Alain Blanchard,Andreea Borla,Carlo Burigana,R. Cabanac,A. Cappi,C. S. Carvalho,S. Casas,Gianluca Castignani,Asantha Cooray,Jean Coupon,Hélène M. Courtois,S. Davini,Gabriella De Lucia,Guillaume Desprez,H. Dole,J. A. Escartín,S. Esco,er,Fabio Finelli,K. Ganga,Juan Garcia-Bellido,Kevin W. George,Ghassem Gozaliasl,Hendrik Hildebrandt,I. M. Hook,Staff ILiC,Vanshika Kansal,E. Keihanen,C. C. Kirkpatrick,Arthur Loureiro,J. F. Macías-Pérez,Manuela Magliocchetti,R. Maoli,S. Marcin,M. Martinelli,N. Martinet,Shibu K. Matthew,Matteo Maturi,R. Benton Metcalf,Gianluca Morgante,Seshadri Nadathur,A. A. Nucita,L. Patrizii,Austin Peel,Victor Popa,Cristiano Porciani,Doug Potter,Alkistis Pourtsidou,Mikko Pöntinen,A. G. Sanchez,Z. Sakr,Mischa Schirmer,Mauricio Moreno Sereno,Alessio Spurio Mancini,Romain Teyssier,Jussi Valiviita,Alfonso Veropalumbo,Matteo Viel +181 more
TL;DR: In this article , the authors present a new calibration of the analytic HMF, at the level of accuracy and precision required for the uncertainty in this quantity to be subdominant with respect to other sources of uncertainty in recovering cosmological parameters from Euclid cluster counts.
Peer Review
Euclid preparation XX. The Complete Calibration of the Color–Redshift Relation survey: LBT observations and data release (cid:63)
Roberto P. Saglia,S. De Nicola,M. H. Fabricius,V. Guglielmo,Jan Snigula,Robert Zöller,Ralf Bender,Jochen Heidt,D. Masters,Daniel Stern,Stéphane Paltani,Adam Amara,Natalia Auricchio,Marco Baldi,Christof Tilmann Bodendorf,D. Bonino,P. Branchini,Massimo Brescia,Jarle Brinchmann,Stefano Camera,V. Capobianco,Carmelita Carbone,J. Carretero,Marco Castellano,Stefano Cavuoti,R. Cledassou,G. Congedo,Christopher J. Conselice,Luca Conversi,Y. Copin,Leonardo Corcione,Frederic Courbin,Matthew M. Cropper,A Da Silva,H. Degaudenzi,Marian Douspis,F. Dubath,C. A. J. Duncan,X. Dupac,S. Dusini,S. Farrens,M. Frailis,E. Franceschi,S. Galeotta,B. Garilli,William Gillard,B. Gillis,Carlo Giocoli,Andrea Grazian,Frank Grupp,S. V. Haugan,Harald Hoekstra,W. Holmes,Felix Hormuth,Allan Hornstrup,Knud Jahnke,M. Kümmel,S. Kermiche,Alina Kiessling,Martin Kunz,Hannu Kurki-Suonio,René J. Laureijs,Sebastiano Ligori,P. B. Lilje,Ivan Lloro,Elena Maiorano,Ole Marggraf,Katarina Markovic,Federico Marulli,Richard Massey,H. J. McCracken,M. Melchior,Georges Meylan,Michele Moresco,Lauro Moscardini,E. Munari,Sami Niemi,C. Padilla,F. Pasian,Kristian Pedersen,Will J. Percival,Valeria Pettorino,Sandrine Pires,M. Poncet,L. Popa,Lucia Pozzetti,F. Raison,A. Renzi,Jason Rhodes,Giuseppe Riccio,E. Romelli,Emanuel Rossetti,Domenico Sapone,Barbara Sartoris,P. Schneider,A. Secroun,Gregor Seidel,Chiara Sirignano,G. Sirri,Luca Stanco,P. Tallada-Crespí,D. Tavagnacco,A. N. Taylor,Ismael Tereno,Rafael Toledo-Moreo,F. Torradeflot,Isaac Tutusaus,Edwin A. Valentijn,Luca Valenziano,T. Vassallo,Yu Wang,Andrea Zacchei,G. Zamorani,Julien Zoubian,Stefano Andreon,S. Bardelli,Javier Graciá-Carpio,Davide Maino,N. Mauri,A. Tramacere,E. Zucca,Alejandro Alvarez Ayllon,Herve Aussel,Carlo Baccigalupi,A. Balaguera-Antolínez,Mario Ballardini,Andrea Biviano,M. Bolzonella,Enrico Bozzo,Carlo Burigana,R. Cabanac,A. Cappi,C. S. Carvalho,S. Casas,Gianluca Castignani,Asantha Cooray,Jean Coupon,Hélène M. Courtois,S. Davini,Guillaume Desprez,H. Dole,J. A. Escartín,S. Esco,er,M. Farina,Sotiria Fotopoulou,K. Ganga,Juan Garcia-Bellido,Kevin W. George,Folco Giacomini,Ghassem Gozaliasl,Hendrik Hildebrandt,I. M. Hook,O. Ilbert,Vanshika Kansal,A. Kashlinsky,E. Keihanen,C. C. Kirkpatrick,Arthur Loureiro,J. F. Macías-Pérez,Manuela Magliocchetti,G. Mainetti,R. Maoli,M. Martinelli,N. Martinet,R. Benton Metcalf,Gianluca Morgante,Seshadri Nadathur,A. A. Nucita,L. Patrizii,V. Popa,Cristiano Porciani,Doug Potter,Alkistis Pourtsidou,Paulo H. F. Reimberg,A. G. Sanchez,Z. Sakr,Mischa Schirmer,Emiliano Sefusatti,Mauro Sereno,J. Stadel,Romain Teyssier,C. Valieri,Jussi Valiviita,Alfonso Veropalumbo,Matteo Viel +185 more
TL;DR: The complete calibration of the Color-Redshift Relation survey (C3R2) is a spectroscopic program designed to empirically calibrate the galaxy color-redshift relation to the Euclid depth (I E = 24 . 5) as mentioned in this paper .