Zobrazeno 1 - 10
of 38
pro vyhledávání: '"S. Lauger"'
Autor:
Jorge Iglesias-Páramo, Barry F. Madore, R. Michael Rich, C. Kevin Xu, Roger F. Malina, Tom A. Barlow, S. Lauger, Susan G. Neff, Young-Wook Lee, Patrick Morrissey, Luciana Bianchi, Bruno Milliard, Barry Y. Welsh, Alexander S. Szalay, Karl Forster, Denis Burgarella, Ted K. Wyder, Oswald H. W. Siegmund, Timothy M. Heckman, Peter G. Friedman, Patrick N. Jelinsky, Todd Small, David Schiminovich, D. Christopher Martin, Yong-Ik Byun
Publikováno v:
The Astrophysical Journal. 619:L95-L98
We present the first Galaxy Evolution Explorer (GALEX) UV images of the well-known interacting group of galaxies, Stephan's Quintet (SQ). We detect widespread UV emission throughout the group. However, there is no consistent coincidence between UV st
Autor:
J. E. Hibbard, Luciana Bianchi, David A. Thilker, R. Michael Rich, David Schiminovich, C. Kevin Xu, Susan G. Neff, Mark Seibert, S. Lauger, D. Burgarella, Tom A. Barlow, Yong-Ik Byun, Jose Donas, Karl Forster, Peter G. Friedman, Timothy M. Heckman, Patrick N. Jelinsky, Young-Wook Lee, Barry F. Madore, Roger F. Malina, D. Christopher Martin, Bruno Milliard, Patrick Morrissey, Oswald H. W. Siegmund, Todd Small, Alex S. Szalay, Barry Y. Welsh, Ted K. Wyder
Publikováno v:
The Astrophysical Journal. 619:L87-L90
We present GALEX FUV (1530 A) and NUV (2310 A) observations of the archetypal merging system NGC 4038/39, ``The Antennae". Both tails are relatively bright in the UV, especially in the vicinity of the Tidal Dwarf Galaxy candidates at the end of the s
Publikováno v:
Astrophysics and Space Science. 284:969-972
We present a quantitative method of classification of the multi-wavelength morphology of galaxies, elaborated from the nearby galaxies and usable to high redshift objects. We use the morphological parameters of concentration of light at the galaxy ce
Autor:
Paolo Ciliegi, Angela Bongiorno, Paola Merluzzi, C. Adami, Marco Scodeggio, G. Mathez, Denis Burgarella, G. Busarello, Luigi Guzzo, Stéphane Charlot, D. Rizzo, S. Paltani, Roberto Scaramella, A. Zanichelli, H. J. McCracken, D. Maccagni, Lucia Pozzetti, M. Bolzonella, R. Merighi, O. Le Fevre, V. Le Brun, O. Ilbert, T. Contini, M. Bondi, D. Bottini, A. Cappi, Christian Marinoni, E. Zucca, S. Lauger, S. Arnout, R. Pello, G. Zamorani, L. Tresse, J. P. Picat, A. Pollo, Bruno Marano, P. Franzetti, I. Gavignaud, Mario Radovich, Sylvie Foucaud, A. Iovino, V. Ripepi, S. Bardelli, Yannick Mellier, G. Vettolani, V. Buat, B. Garilli, B. Meneux, M. Arnaboldi, Alain Mazure
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2006, 453, pp.809-815. ⟨10.1051/0004-6361:20053632⟩
Astronomy and Astrophysics-A&A, 2006, 453, pp.809-815. ⟨10.1051/0004-6361:20053632⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2006, 453, pp.809-815. ⟨10.1051/0004-6361:20053632⟩
Astronomy and Astrophysics-A&A, 2006, 453, pp.809-815. ⟨10.1051/0004-6361:20053632⟩
Aims.We have computed the evolution of the rest-frame B-band luminosity function (LF) for bulge and disk-dominated galaxies since z=1.2. Methods: .We use a sample of 605 spectroscopic redshifts with IAB≤ 24 in the Chandra Deep Field South from th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3837918d2e7889124f52738f094a7be7
https://hal.archives-ouvertes.fr/hal-00287311
https://hal.archives-ouvertes.fr/hal-00287311
Autor:
Young-Wook Lee, Olivier Ilbert, Alexander S. Szalay, K. D. Tyler, Pablo G. Pérez-González, Stéphane Arnouts, Tom A. Barlow, S. Lauger, George H. Rieke, Luciana Bianchi, Tsutomu T. Takeuchi, Sukyoung K. Yi, V. Buat, Barry F. Madore, Denis Burgarella, Roger F. Malina
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2006, 450, pp.69
Astronomy and Astrophysics-A&A, 2006, 450, pp.69
Astronomy and Astrophysics-A&A, EDP Sciences, 2006, 450, pp.69
Astronomy and Astrophysics-A&A, 2006, 450, pp.69
We present the first large, unbiased sample of Lyman Break Galaxies (LBGs) at z ~ 1. Far ultraviolet-dropout (1530 A) galaxies in the Chandra Deep Field South have been selected using GALEX data. This first large sample in the z ~ 1 universe provides
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e259f65c5432e3bcb19b112c205478e1
http://arxiv.org/abs/astro-ph/0601123
http://arxiv.org/abs/astro-ph/0601123
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 434, pp.77. ⟨10.1051/0004-6361:200400138⟩
Astronomy and Astrophysics-A&A, 2005, 434, pp.77. ⟨10.1051/0004-6361:200400138⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 434, pp.77. ⟨10.1051/0004-6361:200400138⟩
Astronomy and Astrophysics-A&A, 2005, 434, pp.77. ⟨10.1051/0004-6361:200400138⟩
We present a quantitative method to classify galaxies, based on multi-wavelength data and constructed from the properties of nearby galaxies. Our objective is to define an classification method that can be used for low and high redshift objects. We e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2d5e1aff1bb80a49289da37d18944bfc
https://hal.archives-ouvertes.fr/hal-00017332
https://hal.archives-ouvertes.fr/hal-00017332
Autor:
C. Adami, A. Mazure, O. Ilbert, A. Cappi, D. Bottini, B. Garilli, V. Le Brun, O. Le Fèvre, D. Maccagni, J. P. Picat, R. Scaramella, M. Scodeggio, L. Tresse, G. Vettolani, A. Zanichelli, M. Arnaboldi, S. Arnouts, S. Bardelli, M. Bolzonella, S. Charlot, P. Ciliegi, T. Contini, G. Covone, S. Foucaud, P. Franzetti, I. Gavignaud, L. Guzzo, A. Iovino, S. Lauger, H. J. McCracken, B. Marano, C. Marinoni, B. Meneux, R. Merighi, S. Paltani, R. Pellò, A. Pollo, L. Pozzetti, M. Radovich, G. Zamorani, E. Zucca, M. Bondi, A. Bongiorno, G. Busarello, L. Gregorini, G. Mathez, Y. Mellier, P. Merluzzi, V. Ripepi, D. Rizzo
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2005, 443, pp.805-818. ⟨10.1051/0004-6361:20053202⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 443, pp.805
Astronomy and Astrophysics-A&A, 2005, 443, pp.805
Astronomy and Astrophysics-A&A, 2005, 443, pp.805-818. ⟨10.1051/0004-6361:20053202⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 443, pp.805
Astronomy and Astrophysics-A&A, 2005, 443, pp.805
We have used the Vimos VLT Deep Survey in combination with other spectroscopic, photometric and X-ray surveys from literature to detect several galaxy structures in the Chandra Deep Field South (CDFS). Both a friend-of-friend based algorithm applied
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f0987e4f9eba740a1189dc1045e81de
Publikováno v:
Multiwavelength Cosmology ISBN: 9781402019715
The Evolution of Galaxies ISBN: 9789048162482
The Evolution of Galaxies ISBN: 9789048162482
We present a quantitative method to classify galaxies, based on multi-wavelength data and elaborated from the properties of nearby galaxies. Our objective is to define an evolutionary method that can be used for low and high redshift objects. We esti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c8407459c6c0a72291b962108acc9507
https://doi.org/10.1007/0-306-48570-2_16
https://doi.org/10.1007/0-306-48570-2_16
Publikováno v:
The Evolution of Galaxies ISBN: 9789048160204
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7bee7df5ea5af8ef4f529412edaa3e4d
https://doi.org/10.1007/978-94-017-3311-3_125
https://doi.org/10.1007/978-94-017-3311-3_125
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.