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Multiwavelength variability and correlation studies of Mrk 421 during historically low X-ray and γ-ray activity in 2015-2016

Acciari VA; Ansoldi S; Antonelli LA; Asano K; Babic A; Banerjee B; Baquero A; de Almeida UB; Barrio JA; Gonzalez JB; Bednarek W; Bellizzi L; Bernardini E; Bernardos M; Berti A; Besenrieder J; Bhattacharyya W; Bigongiari C; Blanch O; Bonnoli G; Bosnjak Z; Busetto G; Carosi R; Ceribella G; Cerruti M; Chai Y; Chilingarian A; Cikota S; Colak SM; Colombo E; Contreras JL; Cortina J; Covino S; D'Amico G; D'Elia V; Da Vela P; Dazzi F; De Angelis A; De Lotto B; Delfino M; Delgado J; Mendez CD; Depaoli D; Di Girolamo T; Di Pierro F; Di Venere L; Neira EDE; Prester DD; Donini A; Doro M; Ramazani VF; Fattorini A; Ferrara G; Foffano L; Fonseca MV; Font L; Fruck C; Fukami S; Lopez RJG; Garczarczyk M; Gasparyan S; Gaug M; Giglietto N; Giordano F; Gliwny P; Green JG; Green D; Hadasch D; Hahn A; Heckmann L; Herrera J; Hoang J; Hrupec D; Hutten M; Inada T; Inoue S; Ishio K; Iwamura Y; Jormanainen J; Jouvin L; Kajiwara Y; Karjalainen M; Kerszberg D; Kobayashi Y; Kubo H; Kushida J; Lamastra A; Lelas D; Leone F; Lindfors E; Lombardi S; Longo F; Lopez M; Lopez-Coto R; Lopez-Oramas A; Loporchio S; Fraga BMD; Maggio C; Majumdar P; Makariev M; Mallamaci M; Maneva G; Manganaro M; Maraschi L; Mariotti M; Martinez M; Mazin D; Mender S; Micanovic S; Miceli D; Miener T; Minev M; Miranda JM; Mirzoyan R; Molina E; Moralejo A; Morcuende D; Moreno V; Moretti E; Munar-Adrover P; Neustroev V; Nigro C; Nilsson K; Ninci D; Nishijima K; Noda K; Nozaki S; Ohtani Y; Oka T; Otero-Santos J; Palatiello M; Paneque D; Paoletti R; Paredes JM; Pavletic L; Penil P; Perennes C; Persic M; Moroni PGP; Prandini E; Priyadarshi C; Puljak I; Rhode W; Ribo M; Rico J; Righi C; Rugliancich A; Saha L; Sahakyan N; Saito T; Sakurai S; Satalecka K; Schleicher B; Schmidt K; Schweizer T; Sitarek J; Snidaric I; Sobczynska D; Spolon A; Stamerra A; Strom D; Strzys M; Suda Y; Suric T; Takahashi M; Tavecchio F; Temnikov P; Terzic T; Teshima M; Torres-Alba N; Tosti L; Truzzi S; van Scherpenberg J; Vanzo G; Acosta MV; Ventura S; Verguilov V; Vigorito CF; Vitale V; Vovk I; Will M; Zaric D; Arbet-Engels A; Baack D; Balbo M; Beck M; Biederbeck N; Biland A; Bretz T; Bruegge K; Buss J; Dorner D; Elsaesser D; Hildebrand D; Iotov R; Klinger M; Mannheim K; Neise D; Neronov A; Noethe M; Paravac A; Rhode W; Sliusar V; Theissen F; Walter R; Valverde J; Horan D; Giroletti M; Perri M; Verrecchia F; Leto C; Sadun AC; Moody JW; Joner M; Marscher AP; Jorstad SG; Lahteenmaki A; Tornikoski M; Ramakrishnan V; Jarvela E; Vera RJC; Righini S; Lien AY

Multiwavelength variability and correlation studies of Mrk 421 during historically low X-ray and γ-ray activity in 2015-2016

Acciari VA
Ansoldi S
Antonelli LA
Asano K
Babic A
Banerjee B
Baquero A
de Almeida UB
Barrio JA
Gonzalez JB
Bednarek W
Bellizzi L
Bernardini E
Bernardos M
Berti A
Besenrieder J
Bhattacharyya W
Bigongiari C
Blanch O
Bonnoli G
Bosnjak Z
Busetto G
Carosi R
Ceribella G
Cerruti M
Chai Y
Chilingarian A
Cikota S
Colak SM
Colombo E
Contreras JL
Cortina J
Covino S
D'Amico G
D'Elia V
Da Vela P
Dazzi F
De Angelis A
De Lotto B
Delfino M
Delgado J
Mendez CD
Depaoli D
Di Girolamo T
Di Pierro F
Di Venere L
Neira EDE
Prester DD
Donini A
Doro M
Ramazani VF
Fattorini A
Ferrara G
Foffano L
Fonseca MV
Font L
Fruck C
Fukami S
Lopez RJG
Garczarczyk M
Gasparyan S
Gaug M
Giglietto N
Giordano F
Gliwny P
Green JG
Green D
Hadasch D
Hahn A
Heckmann L
Herrera J
Hoang J
Hrupec D
Hutten M
Inada T
Inoue S
Ishio K
Iwamura Y
Jormanainen J
Jouvin L
Kajiwara Y
Karjalainen M
Kerszberg D
Kobayashi Y
Kubo H
Kushida J
Lamastra A
Lelas D
Leone F
Lindfors E
Lombardi S
Longo F
Lopez M
Lopez-Coto R
Lopez-Oramas A
Loporchio S
Fraga BMD
Maggio C
Majumdar P
Makariev M
Mallamaci M
Maneva G
Manganaro M
Maraschi L
Mariotti M
Martinez M
Mazin D
Mender S
Micanovic S
Miceli D
Miener T
Minev M
Miranda JM
Mirzoyan R
Molina E
Moralejo A
Morcuende D
Moreno V
Moretti E
Munar-Adrover P
Neustroev V
Nigro C
Nilsson K
Ninci D
Nishijima K
Noda K
Nozaki S
Ohtani Y
Oka T
Otero-Santos J
Palatiello M
Paneque D
Paoletti R
Paredes JM
Pavletic L
Penil P
Perennes C
Persic M
Moroni PGP
Prandini E
Priyadarshi C
Puljak I
Rhode W
Ribo M
Rico J
Righi C
Rugliancich A
Saha L
Sahakyan N
Saito T
Sakurai S
Satalecka K
Schleicher B
Schmidt K
Schweizer T
Sitarek J
Snidaric I
Sobczynska D
Spolon A
Stamerra A
Strom D
Strzys M
Suda Y
Suric T
Takahashi M
Tavecchio F
Temnikov P
Terzic T
Teshima M
Torres-Alba N
Tosti L
Truzzi S
van Scherpenberg J
Vanzo G
Acosta MV
Ventura S
Verguilov V
Vigorito CF
Vitale V
Vovk I
Will M
Zaric D
Arbet-Engels A
Baack D
Balbo M
Beck M
Biederbeck N
Biland A
Bretz T
Bruegge K
Buss J
Dorner D
Elsaesser D
Hildebrand D
Iotov R
Klinger M
Mannheim K
Neise D
Neronov A
Noethe M
Paravac A
Rhode W
Sliusar V
Theissen F
Walter R
Valverde J
Horan D
Giroletti M
Perri M
Verrecchia F
Leto C
Sadun AC
Moody JW
Joner M
Marscher AP
Jorstad SG
Lahteenmaki A
Tornikoski M
Ramakrishnan V
Jarvela E
Vera RJC
Righini S
Lien AY
Katso/Avaa
Publisher's PDF (7.774Mb)
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OXFORD UNIV PRESS
doi:10.1093/mnras/staa3727
Näytä kaikki kuvailutiedot
Julkaisun pysyvä osoite on:
https://urn.fi/URN:NBN:fi-fe2021093048441
Tiivistelmä
We report a characterization of the multiband flux variability and correlations of the nearby (z = 0.031) blazar Markarian 421 (Mrk 421) using data from Metsahovi, Swift, Fermi-LAT, MAGIC, FACT, and other collaborations and instruments from 2014 November till 2016 June. Mrk 421 did not show any prominent flaring activity, but exhibited periods of historically low activity above 1 TeV (F->1 TeV < 1.7 x 10(-12) ph cm(-2) s(-1)) and in the 2-10 keV (X-ray) band (F2-10 keV < 3.6 x 10(-11) erg cm(-2) s(-1)), during which the Swift-BAT data suggest an additional spectral component beyond the regular synchrotron emission. The highest flux variability occurs in X-rays and very high-energy (E > 0.1 TeV) gamma-rays, which, despite the low activity, show a significant positive correlation with no time lag. The HRkeV and HRTeV show the harder-when-brighter trend observed in many blazars, but the trend flattens at the highest fluxes, which suggests a change in the processes dominating the blazar variability. Enlarging our data set with data from years 2007 to 2014, we measured a positive correlation between the optical and the GeV emission over a range of about 60 d centred at time lag zero, and a positive correlation between the optical/GeV and the radio emission over a range of about 60 d centred at a time lag of 43(-6)(+9) d. This observation is consistent with the radio-bright zone being located about 0.2 parsec downstream from the optical/GeV emission regions of the jet. The flux distributions are better described with a lognormal function in most of the energy bands probed, indicating that the variability in Mrk 421 is likely produced by a multiplicative process.
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