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The γ-ray sky seen at X-ray energies I. Searching for the connection between X-rays and y-rays in <i>Fermi</i> BL Lac objects
| Indexado |
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| DOI | 10.1051/0004-6361/201936285 | ||||
| Año | 2019 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Results. We did not find any correlation or clear trend between X-ray and gamma-ray fluxes and/or spectral shapes, but we discovered a correlation between the X-ray flux and the mid-infrared color. Finally, we discuss on a possible interpretation of our results in the SSC framework.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Marchesini, E. J. | Hombre |
Univ Torino - Italia
UNIV NACL LA PLATA - Argentina Ist Nazl Fis Nucl - Italia UNLP - Argentina INAF Osservatorio Astrofis & Sci Spazio - Italia Università degli Studi di Torino - Italia Universidad Nacional de La Plata - Argentina Istituto Nazionale di Fisica Nucleare, Sezione di Torino - Italia Instituto de Astrofísica de La Plata (CONICET- Universidad Nacional de La Plata) - Argentina INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia Instituto de Astrofisica de La Plata - Argentina |
| 2 | Paggi, A. | Hombre |
Univ Torino - Italia
Università degli Studi di Torino - Italia |
| 3 | Massaro, Francesco | Hombre |
Univ Torino - Italia
Università degli Studi di Torino - Italia |
| 4 | Masetti, N. | Mujer |
INAF Osservatorio Astrofis & Sci Spazio - Italia
Universidad Nacional Andrés Bello - Chile INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia |
| 5 | D'Abrusco, R. | Hombre |
Harvard & Smithsonian - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos |
| 6 | Andruchow, I. | Mujer |
UNIV NACL LA PLATA - Argentina
UNLP - Argentina Universidad Nacional de La Plata - Argentina Instituto de Astrofísica de La Plata (CONICET- Universidad Nacional de La Plata) - Argentina Instituto de Astrofisica de La Plata - Argentina |
| 7 | Santos, W. A. | Hombre |
Univ Torino - Italia
UNIV SAO PAULO - Brasil Università degli Studi di Torino - Italia Universidade de Sao Paulo - USP - Brasil Universidade de São Paulo - Brasil |
| Fuente |
|---|
| National Science Foundation |
| Australian Research Council |
| Ministry of Science and Technology |
| National Aeronautics and Space Administration |
| Ministero dell’Istruzione, dell’Università e della Ricerca |
| NASA's Goddard Space Flight Center |
| Ministero dell’Istruzione, dell’Università e della Ricerca |
| Horizon 2020 Framework Programme |
| Ministry of Science and Technology, Taiwan |
| Italian Ministry of Education, University and Research |
| Italian Ministry of Education, University and Research (MIUR) |
| Consorzio Interuniversitario per la fisica Spaziale (CIFS) |
| Ministry of Education, Universities and Research |
| Compagnia di San Paolo |
| University of Sydney |
| Science Foundation for Physics within the University of Sydney - National Aeronautics and Space Administration |
| Molonglo Observatory Synthesis Telescope (MOST) |
| European Union's Horizon 2020 Research and Innovation Programme under the Marie Slodowska-Curie Grant |
| Consorzio Interuniversitario per la Fisica Spaziale |
| Science Foundation for Physics |
| Marie Słodowska-Curie |
| Agradecimiento |
|---|
| E. J. Marchesini would like to thank Rocio I. Paez and M. Victoria Reynaldi for useful discussions on this work. This work is supported by the "Departments of Excellence 2018 2022" Grant awarded by the Italian Ministry of Education, University and Research (MIUR) (L. 232/2016). This research has made use of resources provided by the Compagnia di San Paolo for the grant awarded on the BLENV project (S1618_L1_MASF_01) and by the Ministry of Education, Universities and Research for the grant MASF_FFABR_17_01. F. M. acknowledges financial contribution from the agreement ASI-INAF n.2017-14-H.0 A. P. acknowledges financial support from the Consorzio Interuniversitario per la fisica Spaziale (CIFS) under the agreement related to the grant MASF_CONTR_FIN_18_02. This research has made use of data obtained from the high-energy Astrophysics Science Archive Research Center (HEASARC) provided by NASA's Goddard Space Flight Center. This work is part of a project that has received funding from the European Union's Horizon 2020 Research and Innovation Programme under the Marie Slodowska-Curie Grant Agreement No. 664931. Part of this work is based on the NVSS (NRAO VLA Sky Survey). The National Radio Astronomy Observatory is operated by Associated Universities, Inc., under contract with the National Science Foundation. The Molonglo Observatory site manager, Duncan CampbellWilson, and the staff, Jeff Webb, Michael White, and John Barry, are responsible for the smooth operation of the Molonglo Observatory Synthesis Telescope (MOST) and the day-to-day observing program of SUMSS. SUMSS is dedicated to Michael Large, whose expertise and vision made the project possible. The MOST is operated by the School of Physics with the support of the Australian Research Council and the Science Foundation for Physics within the University of Sydney. This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. TOPCAT (http://www.star.bris.ac.uk/~mbt/topcat/) (Taylor 2005) and STILTS (Taylor 2006) were used for the preparation and manipulation of the images and the tabular data. |
| Acknowledgements. E. J. Marchesini would like to thank Rocío I. Páez and M. Victoria Reynaldi for useful discussions on this work. This work is supported by the “Departments of Excellence 2018−2022” Grant awarded by the Italian Ministry of Education, University and Research (MIUR) (L. 232/2016). This research has made use of resources provided by the Compagnia di San Paolo for the grant awarded on the BLENV project (S1618_L1_MASF_01) and by the Ministry of Education, Universities and Research for the grant MASF_FFABR_17_01. F. M. acknowledges financial contribution from the agreement ASI-INAF n.2017-14-H.0 A. P. acknowledges financial support from the Consorzio Interuniversitario per la fisica Spaziale (CIFS) under the agreement related to the grant MASF_CONTR_FIN_18_02. This research has made use of data obtained from the high-energy Astrophysics Science Archive Research Center (HEASARC) provided by NASA’s Goddard Space Flight Center. This work is part of a project that has received funding from the European Union’s Horizon 2020 Research and Innovation Programme under the Marie Słodowska-Curie Grant Agreement No. 664931. Part of this work is based on the NVSS (NRAO VLA Sky Survey). The National Radio Astronomy Observatory is operated by Associated Universities, Inc., under contract with the National Science Foundation. The Molonglo Observatory site manager, Duncan Campbell-Wilson, and the staff, Jeff Webb, Michael White, and John Barry, are responsible for the smooth operation of the Molonglo Observatory Synthesis Telescope (MOST) and the day-to-day observing program of SUMSS. SUMSS is dedicated to Michael Large, whose expertise and vision made the project possible. The MOST is operated by the School of Physics with the support of the Australian Research Council and the Science Foundation for Physics within the University of Sydney. This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. TOPCAT (http://www.star.bris.ac.uk/~mbt/topcat/) (Taylor 2005) and STILTS (Taylor 2006) were used for the preparation and manipulation of the images and the tabular data. |
