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Items where Person is "Feruglio-C"

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Number of items: 13.

2015

Feruglio, C. and Fiore, F. and Carniani, S. et al. (2015) The multi-phase winds of Markarian 231: from the hot, nuclear, ultra-fast wind to the galaxy-scale, molecular outflow. Astronomy and Astrophysics, 583 . A99. ISSN 0004-6361. http://resolver.caltech.edu/CaltechAUTHORS:20160201-105807048

Miettinen, O. and Smolčić, V. and Novak, M. et al. (2015) (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. I. Multiwavelength identifications and redshift distribution. Astronomy and Astrophysics, 577 . Art. No. A29. ISSN 0004-6361. http://resolver.caltech.edu/CaltechAUTHORS:20150605-105722803

2014

Cicone, C. and Maiolino, R. and Sturm, E. et al. (2014) Massive molecular outflows and evidence for AGN feedback from CO observations. Astronomy and Astrophysics, 562 . Art. No. A21. ISSN 0004-6361. http://resolver.caltech.edu/CaltechAUTHORS:20140428-104758132

2012

Smolčić, V. and Aravena, M. and Navarrete, F. et al. (2012) Millimeter imaging of submillimeter galaxies in the COSMOS field: redshift distribution. Astronomy and Astrophysics, 548 . Art. No. A4. ISSN 0004-6361. http://resolver.caltech.edu/CaltechAUTHORS:20130115-134253660

2010

Feruglio, C. and Aussel, H. and Le Floc'h, E. et al. (2010) Obscured Star Formation and Environment in the COSMOS Field. Astrophysical Journal, 721 (1). pp. 607-614. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20101025-134444339

Piconcelli, E. and Lanzuisi, G. and Fiore, F. et al. (2010) Type 2 Quasars at the heart of dust-obscured galaxies (DOGs) at high z. In: X-Ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives. AIP Conference Proceedings. No.1248. American Institute of Physics , Melville, NY, pp. 493-494. ISBN 978-0-7354-0795-4. http://resolver.caltech.edu/CaltechAUTHORS:20160420-140504600

2009

Sacchi, N. and La Franca, F. and Feruglio, C. et al. (2009) Spectroscopic Identifications of Spitzer Sources in the SWIRE/XMM-Newton/ELAIS-S1 Field: A Large Fraction of Active Galactic Nucleus with High F(24 μm)/F(R) Ratio. Astrophysical Journal, 703 (2). pp. 1778-1790. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20091013-111837503

Le Floc'h, Emeric and Aussel, Hervé and Ilbert, Olivier et al. (2009) Deep Spitzer 24 μm COSMOS Imaging. I. The Evolution of Luminous Dusty Galaxies—Confronting the Models. Astrophysical Journal, 703 (1). pp. 222-239. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20091001-151003670

Piconcelli, E. and Lanzuisi, G. and Fiore, F. et al. (2009) High-z X-ray Obscured Quasars in Galaxies with Extreme Mid-IR/Optical Colors. In: Simbol-X: Focusing on the Hard X-ray Universe. AIP Conference Proceedings. No.1126. American Institute of Physics , Melville, NY, pp. 231-234. ISBN 978-0-07354-0662-9. http://resolver.caltech.edu/CaltechAUTHORS:20160505-161131765

Lanzuisi, G. and Piconcelli, E. and Fiore, F. et al. (2009) Revealing X-ray obscured quasars in SWIRE sources with extreme mid-IR/optical flux ratios. Astronomy and Astrophysics, 498 (1). pp. 67-81. ISSN 0004-6361. http://resolver.caltech.edu/CaltechAUTHORS:20090901-091448170

Fiore, F. and Puccetti, S. and Brusa, M. et al. (2009) Chasing highly obscured QSOs in the COSMOS field. Astrophysical Journal, 693 (1). pp. 447-462. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20090604-115049653

2008

Berta, S. and Rubele, S. and Franceschini, A. et al. (2008) The ESO-Spitzer Imaging extragalactic Survey (ESIS) II. VIMOS I, z wide field imaging of ELAIS-S1 and selection of distant massive galaxies. Astronomy and Astrophysics, 488 (2). pp. 533-548. ISSN 0004-6361. http://resolver.caltech.edu/CaltechAUTHORS:BERaanda08

2007

Berta, S. and Lonsdale, C. J. and Polletta, M. et al. (2007) The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function. Astronomy and Astrophysics, 476 (1). pp. 151-175. ISSN 0004-6361. http://resolver.caltech.edu/CaltechAUTHORS:20091016-143908375

This list was generated on Tue Jun 18 19:42:25 2019 PDT.