Search for very high energy gamma-rays from the z = 0.896 quasar 4C +55.17 with the MAGIC telescopes

The bright gamma-ray quasar 4C+55.17 is a distant source (z=0.896) with a hard spectrum atGeV energies as observed by the Large Area Telescope (LAT) on board the Fermi satellite. Thissource is identified as a good source candidate for very high energy (VHE; >30 GeV) gammarays.In general, VHE...

Full description

Bibliographic Details
Main Authors:	Aleksic, J., Ansoldi, S., Antonelli, L., Antoranz, P., Babic, A., Bangale, P., Barres de Almeida, U., Barrio, J., Becerra, J., Bednarek, W., Berger, K., Bernardini, E., Biland, A., Blanch, O., Bock, R., Bonnefoy, S., Bonnoli, G., Borracci, F., Bretz, T., Carmona, E., Carosi, A., Carreto Fidalgo, D., Colin, P., Colombo, E., Contreras, J., Cortina, J., Covino, S., Da Vela, P., Dazzi, F., de Angelis, A., De Caneva, G., De Lotto, B., Mendez, D., Doert, M., Dominguez, A., Dominis Prester, D., Dorner, D., Doro, M., Einecke, S., Eisenacher, D., Elsaesser, D., Farina, E., Ferenc, D., Fonseca, M., Font, L., Frantzen, K., Fruck, C., Garcia López, R., Garczarczyk, M., Garrido Terrats, D., Gaug, M., Giavitto, G., Godinovic, N., González Muñoz, A., Gozzini, S., Hadasch, D., Hayashida, M., Herrero, A., Hildebrand, D., Hose, J., Hrupec, D., Idec, W., Kadenius, V., KELLERMANN, K., Knoetig, M., Kodani, K., Konno, Y., Krause, J., Kubo, H., Kushida, J., La Barbera, A., Lelas, D., Lewandowska, N., Lindfors, E., Lombardi, S., López, M., López-Coto, R., López-Oramas, A., Lorenz, E., Lozano, I., Makariev, M., Mallot, K., Maneva, G., Mankuzhiyil, N., Mannheim, K., Maraschi, L., Marcote, B., Mariotti, M., Martínez, M., Mazin, D., Menzel, U., Meucci, M., Miranda, J., Mirzoyan, R., Moralejo, A., Munar-Adrover, P., Nakajima, D., Niedzwiecki, A., Nilsson, K., Nishijima, K., Nowak, N., Orito, R., Overkemping, A., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J., Paredes-Fortuny, X., Partini, S., Persic, M., Prada, F., Prada Moroni, P., Prandini, E., Preziuso, S., Puljak, I., Reinthal, R., Rhode, W., Ribo, M., Rico, J., Rodriguez Garcia, J., Rugamer, S., Saggion, A., Saito, T., Saito, K., Salvati, M., Satalecka, K., Scalzotto, V., Scapin, V., Schultz, C., Schweizer, T., Shore, S., Sillanpää, A., Sitarek, J., Snidaric, I., Sobczynska, D., Spanier, F., Stamatescu, V., Stamerra, A., Steinbring, T., Storz, J., Sun, S., Suric, T., Takalo, L., Takami, H., Tavecchio, F., Temnikov, P., Terzic, T., Tescaro, D., Teshima, M., Thaele, J., Tibolla, Omar, Torres, D., Toyama, T., Treves, A., Vogler, P., Wagner, R., Zandanel, F., Zanin, R.
Format:	Journal Article
Published:	Oxford University Press 2014
Subjects:	Key words: radiation mechanisms: non-thermal – galaxies: active – galaxies: nuclei – - quasars: individual: 4C +55.17 – gamma-rays: galaxies
Online Access:	http://hdl.handle.net/20.500.11937/33203

_version_	1848753880007966720
author	Aleksic, J. Ansoldi, S. Antonelli, L. Antoranz, P. Babic, A. Bangale, P. Barres de Almeida, U. Barrio, J. Becerra, J. Bednarek, W. Berger, K. Bernardini, E. Biland, A. Blanch, O. Bock, R. Bonnefoy, S. Bonnoli, G. Borracci, F. Bretz, T. Carmona, E. Carosi, A. Carreto Fidalgo, D. Colin, P. Colombo, E. Contreras, J. Cortina, J. Covino, S. Da Vela, P. Dazzi, F. de Angelis, A. De Caneva, G. De Lotto, B. Mendez, D. Doert, M. Dominguez, A. Dominis Prester, D. Dorner, D. Doro, M. Einecke, S. Eisenacher, D. Elsaesser, D. Farina, E. Ferenc, D. Fonseca, M. Font, L. Frantzen, K. Fruck, C. Garcia López, R. Garczarczyk, M. Garrido Terrats, D. Gaug, M. Giavitto, G. Godinovic, N. González Muñoz, A. Gozzini, S. Hadasch, D. Hayashida, M. Herrero, A. Hildebrand, D. Hose, J. Hrupec, D. Idec, W. Kadenius, V. KELLERMANN, K. Knoetig, M. Kodani, K. Konno, Y. Krause, J. Kubo, H. Kushida, J. La Barbera, A. Lelas, D. Lewandowska, N. Lindfors, E. Lombardi, S. López, M. López-Coto, R. López-Oramas, A. Lorenz, E. Lozano, I. Makariev, M. Mallot, K. Maneva, G. Mankuzhiyil, N. Mannheim, K. Maraschi, L. Marcote, B. Mariotti, M. Martínez, M. Mazin, D. Menzel, U. Meucci, M. Miranda, J. Mirzoyan, R. Moralejo, A. Munar-Adrover, P. Nakajima, D. Niedzwiecki, A. Nilsson, K. Nishijima, K. Nowak, N. Orito, R. Overkemping, A. Paiano, S. Palatiello, M. Paneque, D. Paoletti, R. Paredes, J. Paredes-Fortuny, X. Partini, S. Persic, M. Prada, F. Prada Moroni, P. Prandini, E. Preziuso, S. Puljak, I. Reinthal, R. Rhode, W. Ribo, M. Rico, J. Rodriguez Garcia, J. Rugamer, S. Saggion, A. Saito, T. Saito, K. Salvati, M. Satalecka, K. Scalzotto, V. Scapin, V. Schultz, C. Schweizer, T. Shore, S. Sillanpää, A. Sitarek, J. Snidaric, I. Sobczynska, D. Spanier, F. Stamatescu, V. Stamerra, A. Steinbring, T. Storz, J. Sun, S. Suric, T. Takalo, L. Takami, H. Tavecchio, F. Temnikov, P. Terzic, T. Tescaro, D. Teshima, M. Thaele, J. Tibolla, Omar Torres, D. Toyama, T. Treves, A. Vogler, P. Wagner, R. Zandanel, F. Zanin, R.
author_facet	Aleksic, J. Ansoldi, S. Antonelli, L. Antoranz, P. Babic, A. Bangale, P. Barres de Almeida, U. Barrio, J. Becerra, J. Bednarek, W. Berger, K. Bernardini, E. Biland, A. Blanch, O. Bock, R. Bonnefoy, S. Bonnoli, G. Borracci, F. Bretz, T. Carmona, E. Carosi, A. Carreto Fidalgo, D. Colin, P. Colombo, E. Contreras, J. Cortina, J. Covino, S. Da Vela, P. Dazzi, F. de Angelis, A. De Caneva, G. De Lotto, B. Mendez, D. Doert, M. Dominguez, A. Dominis Prester, D. Dorner, D. Doro, M. Einecke, S. Eisenacher, D. Elsaesser, D. Farina, E. Ferenc, D. Fonseca, M. Font, L. Frantzen, K. Fruck, C. Garcia López, R. Garczarczyk, M. Garrido Terrats, D. Gaug, M. Giavitto, G. Godinovic, N. González Muñoz, A. Gozzini, S. Hadasch, D. Hayashida, M. Herrero, A. Hildebrand, D. Hose, J. Hrupec, D. Idec, W. Kadenius, V. KELLERMANN, K. Knoetig, M. Kodani, K. Konno, Y. Krause, J. Kubo, H. Kushida, J. La Barbera, A. Lelas, D. Lewandowska, N. Lindfors, E. Lombardi, S. López, M. López-Coto, R. López-Oramas, A. Lorenz, E. Lozano, I. Makariev, M. Mallot, K. Maneva, G. Mankuzhiyil, N. Mannheim, K. Maraschi, L. Marcote, B. Mariotti, M. Martínez, M. Mazin, D. Menzel, U. Meucci, M. Miranda, J. Mirzoyan, R. Moralejo, A. Munar-Adrover, P. Nakajima, D. Niedzwiecki, A. Nilsson, K. Nishijima, K. Nowak, N. Orito, R. Overkemping, A. Paiano, S. Palatiello, M. Paneque, D. Paoletti, R. Paredes, J. Paredes-Fortuny, X. Partini, S. Persic, M. Prada, F. Prada Moroni, P. Prandini, E. Preziuso, S. Puljak, I. Reinthal, R. Rhode, W. Ribo, M. Rico, J. Rodriguez Garcia, J. Rugamer, S. Saggion, A. Saito, T. Saito, K. Salvati, M. Satalecka, K. Scalzotto, V. Scapin, V. Schultz, C. Schweizer, T. Shore, S. Sillanpää, A. Sitarek, J. Snidaric, I. Sobczynska, D. Spanier, F. Stamatescu, V. Stamerra, A. Steinbring, T. Storz, J. Sun, S. Suric, T. Takalo, L. Takami, H. Tavecchio, F. Temnikov, P. Terzic, T. Tescaro, D. Teshima, M. Thaele, J. Tibolla, Omar Torres, D. Toyama, T. Treves, A. Vogler, P. Wagner, R. Zandanel, F. Zanin, R.
author_sort	Aleksic, J.
building	Curtin Institutional Repository
collection	Online Access
description	The bright gamma-ray quasar 4C+55.17 is a distant source (z=0.896) with a hard spectrum atGeV energies as observed by the Large Area Telescope (LAT) on board the Fermi satellite. Thissource is identified as a good source candidate for very high energy (VHE; >30 GeV) gammarays.In general, VHE gamma-rays from distant sources provide a unique opportunity to studythe extragalactic background light (EBL) and underlying astrophysics. The flux intensity ofthis source in the VHE range is investigated. Then, constraints on the EBL are derived fromthe attenuation of gamma-ray photons coming from the distant blazar. We searched for agamma-ray signal from this object using the 35 h observations taken by the MAGIC (MajorAtmospheric Gamma-ray Imaging Cherenkov) telescopes between 2010 November and 2011January. No significant VHE gamma-ray signal was detected. We computed the upper limitsof the integrated gamma-ray flux at the 95 per cent confidence level of 9.4 × 10-12 and2.5 × 10-12 cm-2 s-1 above 100 and 200 GeV, respectively. The differential upper limitsin four energy bins in the range from 80 to 500 GeV are also derived. The upper limits areconsistent with the attenuation predicted by low-flux EBL models on the assumption of asimple power-law spectrum extrapolated from LAT data.
first_indexed	2025-11-14T08:31:32Z
format	Journal Article
id	curtin-20.500.11937-33203
institution	Curtin University Malaysia
institution_category	Local University
last_indexed	2025-11-14T08:31:32Z
publishDate	2014
publisher	Oxford University Press
recordtype	eprints
repository_type	Digital Repository
spelling	curtin-20.500.11937-332032017-09-13T15:29:12Z Search for very high energy gamma-rays from the z = 0.896 quasar 4C +55.17 with the MAGIC telescopes Aleksic, J. Ansoldi, S. Antonelli, L. Antoranz, P. Babic, A. Bangale, P. Barres de Almeida, U. Barrio, J. Becerra, J. Bednarek, W. Berger, K. Bernardini, E. Biland, A. Blanch, O. Bock, R. Bonnefoy, S. Bonnoli, G. Borracci, F. Bretz, T. Carmona, E. Carosi, A. Carreto Fidalgo, D. Colin, P. Colombo, E. Contreras, J. Cortina, J. Covino, S. Da Vela, P. Dazzi, F. de Angelis, A. De Caneva, G. De Lotto, B. Mendez, D. Doert, M. Dominguez, A. Dominis Prester, D. Dorner, D. Doro, M. Einecke, S. Eisenacher, D. Elsaesser, D. Farina, E. Ferenc, D. Fonseca, M. Font, L. Frantzen, K. Fruck, C. Garcia López, R. Garczarczyk, M. Garrido Terrats, D. Gaug, M. Giavitto, G. Godinovic, N. González Muñoz, A. Gozzini, S. Hadasch, D. Hayashida, M. Herrero, A. Hildebrand, D. Hose, J. Hrupec, D. Idec, W. Kadenius, V. KELLERMANN, K. Knoetig, M. Kodani, K. Konno, Y. Krause, J. Kubo, H. Kushida, J. La Barbera, A. Lelas, D. Lewandowska, N. Lindfors, E. Lombardi, S. López, M. López-Coto, R. López-Oramas, A. Lorenz, E. Lozano, I. Makariev, M. Mallot, K. Maneva, G. Mankuzhiyil, N. Mannheim, K. Maraschi, L. Marcote, B. Mariotti, M. Martínez, M. Mazin, D. Menzel, U. Meucci, M. Miranda, J. Mirzoyan, R. Moralejo, A. Munar-Adrover, P. Nakajima, D. Niedzwiecki, A. Nilsson, K. Nishijima, K. Nowak, N. Orito, R. Overkemping, A. Paiano, S. Palatiello, M. Paneque, D. Paoletti, R. Paredes, J. Paredes-Fortuny, X. Partini, S. Persic, M. Prada, F. Prada Moroni, P. Prandini, E. Preziuso, S. Puljak, I. Reinthal, R. Rhode, W. Ribo, M. Rico, J. Rodriguez Garcia, J. Rugamer, S. Saggion, A. Saito, T. Saito, K. Salvati, M. Satalecka, K. Scalzotto, V. Scapin, V. Schultz, C. Schweizer, T. Shore, S. Sillanpää, A. Sitarek, J. Snidaric, I. Sobczynska, D. Spanier, F. Stamatescu, V. Stamerra, A. Steinbring, T. Storz, J. Sun, S. Suric, T. Takalo, L. Takami, H. Tavecchio, F. Temnikov, P. Terzic, T. Tescaro, D. Teshima, M. Thaele, J. Tibolla, Omar Torres, D. Toyama, T. Treves, A. Vogler, P. Wagner, R. Zandanel, F. Zanin, R. Key words: radiation mechanisms: non-thermal – galaxies: active – galaxies: nuclei – - quasars: individual: 4C +55.17 – gamma-rays: galaxies The bright gamma-ray quasar 4C+55.17 is a distant source (z=0.896) with a hard spectrum atGeV energies as observed by the Large Area Telescope (LAT) on board the Fermi satellite. Thissource is identified as a good source candidate for very high energy (VHE; >30 GeV) gammarays.In general, VHE gamma-rays from distant sources provide a unique opportunity to studythe extragalactic background light (EBL) and underlying astrophysics. The flux intensity ofthis source in the VHE range is investigated. Then, constraints on the EBL are derived fromthe attenuation of gamma-ray photons coming from the distant blazar. We searched for agamma-ray signal from this object using the 35 h observations taken by the MAGIC (MajorAtmospheric Gamma-ray Imaging Cherenkov) telescopes between 2010 November and 2011January. No significant VHE gamma-ray signal was detected. We computed the upper limitsof the integrated gamma-ray flux at the 95 per cent confidence level of 9.4 × 10-12 and2.5 × 10-12 cm-2 s-1 above 100 and 200 GeV, respectively. The differential upper limitsin four energy bins in the range from 80 to 500 GeV are also derived. The upper limits areconsistent with the attenuation predicted by low-flux EBL models on the assumption of asimple power-law spectrum extrapolated from LAT data. 2014 Journal Article http://hdl.handle.net/20.500.11937/33203 10.1093/mnras/stu227 Oxford University Press unknown
spellingShingle	Key words: radiation mechanisms: non-thermal – galaxies: active – galaxies: nuclei – - quasars: individual: 4C +55.17 – gamma-rays: galaxies Aleksic, J. Ansoldi, S. Antonelli, L. Antoranz, P. Babic, A. Bangale, P. Barres de Almeida, U. Barrio, J. Becerra, J. Bednarek, W. Berger, K. Bernardini, E. Biland, A. Blanch, O. Bock, R. Bonnefoy, S. Bonnoli, G. Borracci, F. Bretz, T. Carmona, E. Carosi, A. Carreto Fidalgo, D. Colin, P. Colombo, E. Contreras, J. Cortina, J. Covino, S. Da Vela, P. Dazzi, F. de Angelis, A. De Caneva, G. De Lotto, B. Mendez, D. Doert, M. Dominguez, A. Dominis Prester, D. Dorner, D. Doro, M. Einecke, S. Eisenacher, D. Elsaesser, D. Farina, E. Ferenc, D. Fonseca, M. Font, L. Frantzen, K. Fruck, C. Garcia López, R. Garczarczyk, M. Garrido Terrats, D. Gaug, M. Giavitto, G. Godinovic, N. González Muñoz, A. Gozzini, S. Hadasch, D. Hayashida, M. Herrero, A. Hildebrand, D. Hose, J. Hrupec, D. Idec, W. Kadenius, V. KELLERMANN, K. Knoetig, M. Kodani, K. Konno, Y. Krause, J. Kubo, H. Kushida, J. La Barbera, A. Lelas, D. Lewandowska, N. Lindfors, E. Lombardi, S. López, M. López-Coto, R. López-Oramas, A. Lorenz, E. Lozano, I. Makariev, M. Mallot, K. Maneva, G. Mankuzhiyil, N. Mannheim, K. Maraschi, L. Marcote, B. Mariotti, M. Martínez, M. Mazin, D. Menzel, U. Meucci, M. Miranda, J. Mirzoyan, R. Moralejo, A. Munar-Adrover, P. Nakajima, D. Niedzwiecki, A. Nilsson, K. Nishijima, K. Nowak, N. Orito, R. Overkemping, A. Paiano, S. Palatiello, M. Paneque, D. Paoletti, R. Paredes, J. Paredes-Fortuny, X. Partini, S. Persic, M. Prada, F. Prada Moroni, P. Prandini, E. Preziuso, S. Puljak, I. Reinthal, R. Rhode, W. Ribo, M. Rico, J. Rodriguez Garcia, J. Rugamer, S. Saggion, A. Saito, T. Saito, K. Salvati, M. Satalecka, K. Scalzotto, V. Scapin, V. Schultz, C. Schweizer, T. Shore, S. Sillanpää, A. Sitarek, J. Snidaric, I. Sobczynska, D. Spanier, F. Stamatescu, V. Stamerra, A. Steinbring, T. Storz, J. Sun, S. Suric, T. Takalo, L. Takami, H. Tavecchio, F. Temnikov, P. Terzic, T. Tescaro, D. Teshima, M. Thaele, J. Tibolla, Omar Torres, D. Toyama, T. Treves, A. Vogler, P. Wagner, R. Zandanel, F. Zanin, R. Search for very high energy gamma-rays from the z = 0.896 quasar 4C +55.17 with the MAGIC telescopes
title	Search for very high energy gamma-rays from the z = 0.896 quasar 4C +55.17 with the MAGIC telescopes
title_full	Search for very high energy gamma-rays from the z = 0.896 quasar 4C +55.17 with the MAGIC telescopes
title_fullStr	Search for very high energy gamma-rays from the z = 0.896 quasar 4C +55.17 with the MAGIC telescopes
title_full_unstemmed	Search for very high energy gamma-rays from the z = 0.896 quasar 4C +55.17 with the MAGIC telescopes
title_short	Search for very high energy gamma-rays from the z = 0.896 quasar 4C +55.17 with the MAGIC telescopes
title_sort	search for very high energy gamma-rays from the z = 0.896 quasar 4c +55.17 with the magic telescopes
topic	Key words: radiation mechanisms: non-thermal – galaxies: active – galaxies: nuclei – - quasars: individual: 4C +55.17 – gamma-rays: galaxies
url	http://hdl.handle.net/20.500.11937/33203

Search for very high energy gamma-rays from the z = 0.896 quasar 4C +55.17 with the MAGIC telescopes

Similar Items