E
Edwin A. Valentijn
Researcher at Kapteyn Astronomical Institute
Publications - 249
Citations - 10796
Edwin A. Valentijn is an academic researcher from Kapteyn Astronomical Institute. The author has contributed to research in topics: Galaxy & Weak gravitational lensing. The author has an hindex of 48, co-authored 226 publications receiving 8242 citations. Previous affiliations of Edwin A. Valentijn include European Southern Observatory & University of Groningen.
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The Secondary Standards Programme for OmegaCAM
TL;DR: In this paper, the authors present a preliminary catalog for the OmegaCAM wide-field imager, which will be used to bootstrap the construction of the secondary standards catalog for 8 Landolt equatorial fields during the first year of operation.
Journal ArticleDOI
Euclid preparation: XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and H-band images
Euclid Collaboration L. Bisigello,Christopher J. Conselice,Maarten Baes,M. Bolzonella,Massimo Brescia,Stefano Cavuoti,O. Cucciati,Andrew Humphrey,Leslie K. Hunt,C. Maraston11,Lucia Pozzetti,C. Tortora,S. E. V. Mierlo,Nabila Aghanim,Natalia Auricchio,Marco Baldi,Ralf Bender,Christof Tilmann Bodendorf,D. Bonino,P. Branchini,Jarle Brinchmann,Stefano Camera,V. Capobianco,Carmelita Carbone,J. Carretero,Francisco J. Castander,Marco Castellano,Andrea Cimatti,G. Congedo,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,Sylvain Ferriol,M. Frailis,E. Franceschi,P. Franzetti,M. Fumana,B. Garilli,William Gillard,B. Gillis,Carlo Giocoli,Andrea Grazian,Frank Grupp,Luigi Guzzo,S. V. Haugan,W. Holmes,Felix Hormuth,Allan Hornstrup,Knud Jahnke,M. Kummel,S. Kermiche,Alina Kiessling,Martin Kilbinger,R. Kohley,Martin Kunz,Hannu Kurki-Suonio,Sebastiano Ligori,P. B. Lilje,Ivan Lloro,Elena Maiorano,Oriana Mansutti,Ole Marggraf,Katarina Markovic,Federico Marulli,Richard Massey,Sophie Maurogordato,E. Medinaceli,Massimo Meneghetti,Emiliano Merlin,Georges Meylan,Michele Ennio Maria Moresco,Lauro Moscardini,E. Munari,Sami Niemi,C. Padilla,Stéphane Paltani,F. Pasian,Kristian Pedersen,Valeria Pettorino,G. Polenta,M. Poncet,L. Popa,F. Raison,A. Renzi,Jason Rhodes,Giuseppe Riccio,Hans-Walter Rix,E. Romelli,Mauro Roncarelli,C. Rosset,Emanuel Rossetti,Roberto P. Saglia,Domenico Sapone,Barbara Sartoris,P. Schneider,Marco Scodeggio,A. Secroun,Gregor Seidel,Chiara Sirignano,G. Sirri,Luca Stanco,P. Tallada-Cresp'i,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. Boucaud,C. Colodro-Conde,D. Di Ferdinando,J. Graci'a-Carpio,V. Lindholm,Davide Maino,Shao Mei,V. Scottez,F. Sureau,M. Tenti,E. Zucca,Alejandro Borlaff,Mario Ballardini,Andrea Biviano,Enrico Bozzo,Carlo Burigana,R. Cabanac,A. Cappi,C. S. Carvalho,S. Casas,Gianluca Castignani,Asantha Cooray,Jean Coupon,Hélène M. Courtois,Jg Cuby,Simonella Davini,Gabriella De Lucia,Guillaume Desprez,H. Dole,J. A. Escartín,Stephanie Escoffier,M. Farina,Sotiria Fotopoulou,K. Ganga,Juan Garcia-Bellido,Kevin W. George,Folco Giacomini,Ghassem Gozaliasl,Hendrik Hildebrandt,I. M. Hook,Marc Huertas-Company,Vanshika Kansal,E. Keihanen,C. C. Kirkpatrick,Arthur Loureiro,J. Mac'ias-P'erez,Manuela Magliocchetti,G. Mainetti,Stopa Marcin,M. Martinelli,N. Martinet,R. Benton Metcalf,Pierluigi Monaco,Gianluca Morgante,Seshadri Nadathur,A. A. Nucita,L. Patrizii,Austin Peel,Doug Potter,Alkistis Pourtsidou,Michele Pontinen,Paulo H. F. Reimberg,A. S'anchez,Z. Sakr,Mischa Schirmer,Emiliano Sefusatti,Mauro Sereno,J. Stadel,Romain Teyssier,C. Valieri,J. Valiviita111,Matteo Viel +197 more
TL;DR: Deep Learning Neural Networks and Convolutional Neutral Networks perform well in measuring the properties of these galaxies and have an accuracy which is better than traditional methods based on spectral energy distribution, but it is found that the estimates of stellar masses improve with the use of an image, but those of redshift and star-formation rates do not.
Proceedings ArticleDOI
Design and measured performance of the ISO Short Wavelength Spectrometer
D. A. Beintema,T. de Graauw,W. Luinge,Edwin A. Valentijn,J. Wijnbergen,K. Wildeman,L. Barl,Helmut Feuchtgruber,L. Haser,Reinhard O. Katterloher,F. Melzner,J. Stöcker +11 more
TL;DR: The Short Wavelength Spectrometer (SWS) is one of the four instruments for the Infrared Space Observatory (IROSO) as discussed by the authors, which operates at about 3 K employing diffraction gratings, if offers a resolving power between 1000 and 2000 in the wavelength range 245 to 45 micrometers.