Multiwavelength study of the gravitationally lensed blazar QSO B0218+357 between 2016 and 2020

Cortina J; D'Ammando F; Prester DD; Hahn A; Ferrara G; Lombardi S; Sitarek J; Perennes C; Antonelli LA; Engels AA; Strom D; Asano K; Rhode W; Rico J; Di Venere L; Acosta MV; Ansoldi S; Manganaro M; Loporchio S; Vanzo G; Ventura S; Kiehlmann S; Delfino M; Baquero A; Ceribella G; Jouvin L; Tornikoski M; Kajiwara Y; Jormanainen J; Blanch O; Gaug M; Elsaesser D; Max-Moerbeck W; Giordano F; Delgado J; Lahteenmaki A; Saito T; Kushida J; Di Pierro F; van Scherpenberg J; Lindfors E; Tosti L; Iwamura Y; Fukami S; Pearson TJ; Mannheim K; Bednarek W; Bjorklund I; de Palma F; Sobczynska D; Bonnoli G; Depaoli D; Nozaki S; Sahu DK; Artero M; Palatiello M; Kerszberg D; Schweizer T; Menchiari S; Nilsson K; Martinez M; Kobayashi Y; Bhattacharyya W; Espineira ED; Font L; Miranda JM; Mazin D; Schmidt K; Pavletic L; Strzys M; Truzzi S; Maneva G; Paoletti R; Oka T; Maraschi L; Terzic T; Mender S; Gliwny P; Da Vela P; Lelas D; Babic A; Doro M; Besenrieder J; Karjalainen M; Puljak I; Gonzalez JB; Bosnjak Z; Busetto G; Gasparyan S; Otero-Santos J; Sakurai S; Fruck C; Batkovic I; Majumdar P; Cerruti M; Nigro C; Bernardini E; Hada K; Fattorini A; Inoue S; Temnikov P; Bernardos M; Vitale V; Sahakyan N; Jimenez I; Lopez RJG; Herrera J; Satalecka K; Lopez-Moya M; Hutten M; Noda K; Mariotti M; Fraga BMD; Miceli D; Berti A; Carosi R; Paredes JM; Dorner D; Hodges M; Bellizzi L; Micanovic S; Inada T; Tavecchio F; Vigorito CF; Prandini E; Readhead ACS; Nishijima K; Moreno V; Green JG; Barnacka A; Hoang J; Ohtani Y; Wunderlich C; Longo F; Ribo M; de Almeida UB; Green D; Ramazani VF; Moralejo A; Colombo E; Neustroev V; Suda Y; Niinuma K; Kubo H; Teshima M; Lopez-Coto R; Verguilov V; Miener T; Bigongiari C; D'Elia V; Moroni PGP; Hadasch D; Baack D; Lopez-Oramas A; Suric T; Lamastra A; Dazzi F; Heckmann L; Penil P; Will M; Moretti E; Acciari VA; Hovatta T; Rugliancich A; Ubach S; Contreras JL; Paiano S; Maggio C; Mallamaci M; Garczarczyk M; Colak SM; Hrupec D; Persic M; Barrio JA; Paneque D; Suutarinen S; Donini A; Minev M; Morcuende D; Cikota S; Snidaric I; Tammi J; Spolon A; De Angelis A; Saha L; Giglietto N; Mendez CD; Saturni FG; Vovk I; Godinovic N; D'Amico G; Covino S; Zaric D; Ishio K; Reeves R; Schleicher B; Molina E; Priyadarshi C; De Lotto B; Takahashi M; Mirzoyan R; Stamerra A; Leone F; Righi C; Makariev M; Tutone A; Chilingarian A; Chai Y; Fonseca MV; Biland A

Multiwavelength study of the gravitationally lensed blazar QSO B0218+357 between 2016 and 2020

Cortina J; D'Ammando F; Prester DD; Hahn A; Ferrara G; Lombardi S; Sitarek J; Perennes C; Antonelli LA; Engels AA; Strom D; Asano K; Rhode W; Rico J; Di Venere L; Acosta MV; Ansoldi S; Manganaro M; Loporchio S; Vanzo G; Ventura S; Kiehlmann S; Delfino M; Baquero A; Ceribella G; Jouvin L; Tornikoski M; Kajiwara Y; Jormanainen J; Blanch O; Gaug M; Elsaesser D; Max-Moerbeck W; Giordano F; Delgado J; Lahteenmaki A; Saito T; Kushida J; Di Pierro F; van Scherpenberg J; Lindfors E; Tosti L; Iwamura Y; Fukami S; Pearson TJ; Mannheim K; Bednarek W; Bjorklund I; de Palma F; Sobczynska D; Bonnoli G; Depaoli D; Nozaki S; Sahu DK; Artero M; Palatiello M; Kerszberg D; Schweizer T; Menchiari S; Nilsson K; Martinez M; Kobayashi Y; Bhattacharyya W; Espineira ED; Font L; Miranda JM; Mazin D; Schmidt K; Pavletic L; Strzys M; Truzzi S; Maneva G; Paoletti R; Oka T; Maraschi L; Terzic T; Mender S; Gliwny P; Da Vela P; Lelas D; Babic A; Doro M; Besenrieder J; Karjalainen M; Puljak I; Gonzalez JB; Bosnjak Z; Busetto G; Gasparyan S; Otero-Santos J; Sakurai S; Fruck C; Batkovic I; Majumdar P; Cerruti M; Nigro C; Bernardini E; Hada K; Fattorini A; Inoue S; Temnikov P; Bernardos M; Vitale V; Sahakyan N; Jimenez I; Lopez RJG; Herrera J; Satalecka K; Lopez-Moya M; Hutten M; Noda K; Mariotti M; Fraga BMD; Miceli D; Berti A; Carosi R; Paredes JM; Dorner D; Hodges M; Bellizzi L; Micanovic S; Inada T; Tavecchio F; Vigorito CF; Prandini E; Readhead ACS; Nishijima K; Moreno V; Green JG; Barnacka A; Hoang J; Ohtani Y; Wunderlich C; Longo F; Ribo M; de Almeida UB; Green D; Ramazani VF; Moralejo A; Colombo E; Neustroev V; Suda Y; Niinuma K; Kubo H; Teshima M; Lopez-Coto R; Verguilov V; Miener T; Bigongiari C; D'Elia V; Moroni PGP; Hadasch D; Baack D; Lopez-Oramas A; Suric T; Lamastra A; Dazzi F; Heckmann L; Penil P; Will M; Moretti E; Acciari VA; Hovatta T; Rugliancich A; Ubach S; Contreras JL; Paiano S; Maggio C; Mallamaci M; Garczarczyk M; Colak SM; Hrupec D; Persic M; Barrio JA; Paneque D; Suutarinen S; Donini A; Minev M; Morcuende D; Cikota S; Snidaric I; Tammi J; Spolon A; De Angelis A; Saha L; Giglietto N; Mendez CD; Saturni FG; Vovk I; Godinovic N; D'Amico G; Covino S; Zaric D; Ishio K; Reeves R; Schleicher B; Molina E; Priyadarshi C; De Lotto B; Takahashi M; Mirzoyan R; Stamerra A; Leone F; Righi C; Makariev M; Tutone A; Chilingarian A; Chai Y; Fonseca MV; Biland A

Multiwavelength study of the gravitationally lensed blazar QSO B0218+357 between 2016 and 2020

Cortina J

D'Ammando F

Prester DD

Hahn A

Ferrara G

Lombardi S

Sitarek J

Perennes C

Antonelli LA

Engels AA

Strom D

Asano K

Rhode W

Rico J

Di Venere L

Acosta MV

Ansoldi S

Manganaro M

Loporchio S

Vanzo G

Ventura S

Kiehlmann S

Delfino M

Baquero A

Ceribella G

Jouvin L

Tornikoski M

Kajiwara Y

Jormanainen J

Blanch O

Gaug M

Elsaesser D

Max-Moerbeck W

Giordano F

Delgado J

Lahteenmaki A

Saito T

Kushida J

Di Pierro F

van Scherpenberg J

Lindfors E

Tosti L

Iwamura Y

Fukami S

Pearson TJ

Mannheim K

Bednarek W

Bjorklund I

de Palma F

Sobczynska D

Bonnoli G

Depaoli D

Nozaki S

Sahu DK

Artero M

Palatiello M

Kerszberg D

Schweizer T

Menchiari S

Nilsson K

Martinez M

Kobayashi Y

Bhattacharyya W

Espineira ED

Font L

Miranda JM

Mazin D

Schmidt K

Pavletic L

Strzys M

Truzzi S

Maneva G

Paoletti R

Oka T

Maraschi L

Terzic T

Mender S

Gliwny P

Da Vela P

Lelas D

Babic A

Doro M

Besenrieder J

Karjalainen M

Puljak I

Gonzalez JB

Bosnjak Z

Busetto G

Gasparyan S

Otero-Santos J

Sakurai S

Fruck C

Batkovic I

Majumdar P

Cerruti M

Nigro C

Bernardini E

Hada K

Fattorini A

Inoue S

Temnikov P

Bernardos M

Vitale V

Sahakyan N

Jimenez I

Lopez RJG

Herrera J

Satalecka K

Lopez-Moya M

Hutten M

Noda K

Mariotti M

Fraga BMD

Miceli D

Berti A

Carosi R

Paredes JM

Dorner D

Hodges M

Bellizzi L

Micanovic S

Inada T

Tavecchio F

Vigorito CF

Prandini E

Readhead ACS

Nishijima K

Moreno V

Green JG

Barnacka A

Hoang J

Ohtani Y

Wunderlich C

Longo F

Ribo M

de Almeida UB

Green D

Ramazani VF

Moralejo A

Colombo E

Neustroev V

Suda Y

Niinuma K

Kubo H

Teshima M

Lopez-Coto R

Verguilov V

Miener T

Bigongiari C

D'Elia V

Moroni PGP

Hadasch D

Baack D

Lopez-Oramas A

Suric T

Lamastra A

Dazzi F

Heckmann L

Penil P

Will M

Moretti E

Acciari VA

Hovatta T

Rugliancich A

Ubach S

Contreras JL

Paiano S

Maggio C

Mallamaci M

Garczarczyk M

Colak SM

Hrupec D

Persic M

Barrio JA

Paneque D

Suutarinen S

Donini A

Minev M

Morcuende D

Cikota S

Snidaric I

Tammi J

Spolon A

De Angelis A

Saha L

Giglietto N

Mendez CD

Saturni FG

Vovk I

Godinovic N

D'Amico G

Covino S

Zaric D

Ishio K

Reeves R

Schleicher B

Molina E

Priyadarshi C

De Lotto B

Takahashi M

Mirzoyan R

Stamerra A

Leone F

Righi C

Makariev M

Tutone A

Chilingarian A

Chai Y

Fonseca MV

Biland A

Katso/Avaa

stab3454.pdf (2.661Mb)

Lataukset:

OXFORD UNIV PRESS

doi:10.1093/mnras/stab3454

URI

https://academic.oup.com/mnras/article/510/2/2344/6446016

Näytä kaikki kuvailutiedot

Julkaisun pysyvä osoite on:
https://urn.fi/URN:NBN:fi-fe2022081154397

Tiivistelmä

We report multiwavelength observations of the gravitationally lensed blazar QSO B0218+357 in 2016-2020. Optical, X-ray, and GeV flares were detected. The contemporaneous MAGIC observations do not show significant very high energy (VHE; greater than or similar to 100 GeV) gamma-ray emission. The lack of enhancement in radio emission measured by The Owens Valley Radio Observatory indicates the multizone nature of the emission from this object. We constrain the VHE duty cycle of the source to be <16 2014-like flares per year (95 per cent confidence). For the first time for this source, a broad-band low-state spectral energy distribution is constructed with a deep exposure up to the VHE range. A flux upper limit on the low-state VHE gamma-ray emission of an order of magnitude below that of the 2014 flare is determined. The X-ray data are used to fit the column density of (8.10 +/- 0.93(stat)) x 10(21) cm(-2) of the dust in the lensing galaxy. VLBI observations show a clear radio core and jet components in both lensed images, yet no significant movement of the components is seen. The radio measurements are used to model the source-lens-observer geometry and determine the magnifications and time delays for both components. The quiescent emission is modelled with the high-energy bump explained as a combination of synchrotron-self-Compton and external Compton emission from a region located outside of the broad-line region. The bulk of the low-energy emission is explained as originating from a tens-of-parsecs scale jet.

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