Zobrazeno 1 - 10
of 171
pro vyhledávání: '"E Hatziminaoglou"'
Autor:
A Wong, E Hatziminaoglou, A Borkar, G Popping, I Pérez-Fournon, F Poidevin, F Stoehr, H Messias
The Atacama Large Millimetre/submillimetre Array (ALMA) is the world’s most advanced radio interferometric facility, producing science data with an average rate of about 1 TB per day. After a process of calibration, imaging and quality assurance, t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2744e90ca42207205afa99def04ef9c9
Autor:
M. Sánchez-Portal, M. Castillo-Fraile, C. Ramos Almeida, P. Esquej, A. Alonso-Herrero, A. M. Pérez García, J. Acosta-Pulido, B. Altieri, A. Bongiovanni, J. M. Castro Céron, J. Cepa, D. Coia, L. Conversi, J. Fritz, J. I. Gonzalez-Serrano, E. Hatziminaoglou, M. Povic, J. M. Rodrguez Espinosa, I. Valtchanov
Publikováno v:
Acta Polytechnica CTU Proceedings, Vol 1, Iss 1, Pp 307-310 (2014)
The "Seyfert and star formation Activity in the Far-Infrared" (SAFIR) project is aimed at studying the physical nature of the nuclear IR emission and star formation properties of a small sample of nearby Seyfert galaxies observed with the PACS and SP
Externí odkaz:
https://doaj.org/article/a2bc8f29fc41463eb447b949120a12e6
Autor:
F. Salvestrini, C. Gruppioni, E. Hatziminaoglou, F. Pozzi, C. Vignali, V. Casasola, R. Paladino, S. Aalto, P. Andreani, S. Marchesi, T. Stanke
We present a multi-wavelength study of the molecular gas properties of a sample of local Seyfert 2 galaxies to assess if, and to what extent, the presence of an active galactic nucleus (AGN) can affect the Interstellar Medium (ISM) properties in a sa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cbbc33b2981d20ca12431491cf39f16b
http://arxiv.org/abs/2203.15825
http://arxiv.org/abs/2203.15825
Autor:
L. Bisigello, C. Gruppioni, F. Calura, A. Feltre, F. Pozzi, C. Vignali, L. Barchiesi, G. Rodighiero, M. Negrello, F. J. Carrera, K. M. Dasyra, J. A. Fernández-Ontiveros, M. Giard, E. Hatziminaoglou, H. Kaneda, E. Lusso, M. Pereira-Santaella, P. G. Pérez González, C. Ricci, D. Schaerer, L. Spinoglio, L. Wang
Publikováno v:
Publications of the Astronomical Society of Australia
Publications of the Astronomical Society of Australia, Cambridge University Press (CUP), In press
Publications of the Astronomical Society of Australia, In press, 38, ⟨10.1017/pasa.2021.57⟩
Publications of the Astronomical Society of Australia, 38:e064. Cambridge University Press
Digital.CSIC. Repositorio Institucional del CSIC
instname
Publications of the Astronomical Society of Australia, Cambridge University Press (CUP), In press
Publications of the Astronomical Society of Australia, In press, 38, ⟨10.1017/pasa.2021.57⟩
Publications of the Astronomical Society of Australia, 38:e064. Cambridge University Press
Digital.CSIC. Repositorio Institucional del CSIC
instname
arXiv:2111.11453v1
Mid- and far-infrared (IR) photometric and spectroscopic observations are fundamental to a full understanding of the dust-obscured Universe and the evolution of both star formation and black hole accretion in galaxies. In this
Mid- and far-infrared (IR) photometric and spectroscopic observations are fundamental to a full understanding of the dust-obscured Universe and the evolution of both star formation and black hole accretion in galaxies. In this
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ca17cd1b059cff35a8d3879de7fe3469
https://hal.archives-ouvertes.fr/hal-03454699
https://hal.archives-ouvertes.fr/hal-03454699
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
D. Rigopoulou, G. Magdis, R. J. Ivison, A. Amblard, V. Arumugam, H. Aussel, A. Blain, J. Bock, A. Boselli, V. Buat, D. Burgarella, N. Castro-Rodríguez, A. Cava, P. Chanial, D. L. Clements, A. Conley, L. Conversi, A. Cooray, C. D. Dowell, E. Dwek, S. Eales, D. Elbaz, D. Farrah, A. Franceschini, J. Glenn, M. Griffin, M. Halpern, E. Hatziminaoglou, J.-S. Huang, E. Ibar, K. Isaak, G. Lagache, L. Levenson, N. Lu, S. Madden, B. Maffei, G. Mainetti, L. Marchetti, H. T. Nguyen, B. O’Halloran, S. J. Oliver, A. Omont, M. J. Page, P. Panuzzo, A. Papageorgiou, C. P. Pearson, I. Pérez-Fournon, M. Pohlen, D. Rizzo, I. G. Roseboom, M. Rowan-Robinson, B. Schulz, Douglas Scott, N. Seymour, D. L. Shupe, A. J. Smith, J. A. Stevens, M. Symeonidis, M. Trichas, K. E. Tugwell, M. Vaccari, I. Valtchanov, L. Vigroux, L. Wang, G. Wright, C. K. Xu, M. Zemcov
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 409:L7-L12
We present first results of a study of the submillimetre (rest frame far-infrared) properties of z~3 Lyman Break Galaxies (LBGs) and their lower-redshift counterparts BX/BM galaxies, based on Herschel-SPIRE observations of the Northern field of the G
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::60ac414f01104ba01e1f0700b927584f
https://doi.org/10.1111/j.1745-3933.2010.00950.x
https://doi.org/10.1111/j.1745-3933.2010.00950.x
Autor:
M. Rowan-Robinson, I. G. Roseboom, M. Vaccari, A. Amblard, V. Arumugam, R. Auld, H. Aussel, T. Babbedge, A. Blain, J. Bock, A. Boselli, D. Brisbin, V. Buat, D. Burgarella, N. Castro-Rodriguez, A. Cava, P. Chanial, D. L. Clements, A. Conley, L. Conversi, A. Cooray, C. D. Dowell, E. Dwek, S. Dye, S. Eales, D. Elbaz, D. Farrah, M. Fox, A. Franceschini, W. Gear, J. Glenn, E. A. González Solares, M. Griffin, M. Halpern, E. Hatziminaoglou, J. Huang, E. Ibar, K. Isaak, R. J. Ivison, G. Lagache, L. Levenson, N. Lu, S. Madden, B. Maffei, G. Mainetti, L. Marchetti, A. M. J. Mortier, H. T. Nguyen, B. O'Halloran, S. J. Oliver, A. Omont, M. J. Page, P. Panuzzo, A. Papageorgiou, H. Patel, C. P. Pearson, I. Perez Fournon, M. Pohlen, J. I. Rawlings, G. Raymond, D. Rigopoulou, D. Rizzo, B. Schulz, Douglas Scott, N. Seymour, D. L. Shupe, A. J. Smith, J. A. Stevens, M. Symeonidis, M. Trichas, K. E. Tugwell, I. Valtchanov, L. Vigroux, L. Wang, R. Ward, G. Wright, C. K. Xu, M. Zemcov
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 409:2-11
We present spectral energy distributions (SEDs) for 68 Herschel sources detected at 5-sigma at 250, 350 and 500 mu in the HerMES SWIRE-Lockman field. We explore whether existing models for starbursts, quiescent star-forming galaxies and for AGN dust
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ad8f5e271b659326a3541eb71506a5a0
https://doi.org/10.1111/j.1365-2966.2010.17041.x
https://doi.org/10.1111/j.1365-2966.2010.17041.x