Multiwavelength observations of the blazar BL Lacertae: a new fast TeV gamma-ray flare
|
|
- Ralph Bruce
- 6 years ago
- Views:
Transcription
1 Multiwavelength observations of the blazar BL Lacertae: a new fast TeV gamma-ray flare Qi Feng1 for the VERITAS Collaboration, S.G. JORSTAD, A.P. MARSCHER, M.L. Lister,Y.Y. Kovalev, A.B. Pushkarev, T. Savolainen, I. AGUDO, S.N. MOLINA, J.L. GOMEZ, V.M. Larionov, G.A. Borman, A.A. Mokrushina, and P.S. Smith 1McGill University 1 ICRC July 13, 2017, Busan
2 Radio-loud AGN + beaming = blazar AGN: active (accreting) galactic nuclei; Radio loud: ~10% of AGN have a relativistic jet; Blazar: ~10% of radio-loud AGN point their jet toward us. High luminosity & compact central region: extreme physics! Urry & Padovani
3 Radio-loud AGN + beaming = blazar AGN: active (accreting) galactic nuclei; Radio loud: ~10% of AGN have a relativistic jet; Blazar: ~10% of radio-loud AGN point their jet toward us. High luminosity & compact central region: extreme physics! blazar Urry & Padovani
4 Radio-loud AGN + beaming = blazar AGN: active (accreting) galactic nuclei; Radio loud: ~10% of AGN have a relativistic jet; Blazar: ~10% of radio-loud AGN point their jet toward us. High luminosity & compact central region: extreme physics! blazar Urry & Padovani
5 What s to learn from fast TeV flare of blazars Causality: fast flare (minutes) => small size Flux R Δtint=0 Flux Time Δtobs R (1+z)/(δc) Δtobs R (1+z)/(δc) when Δtint is unknown => upper limit on R Time Gamma rays escaped pair-production: - the emitting location is far away from BLR - large doppler factor to escape synchrotron photons Ɣ e + Ɣ e - 3
6 What s to learn from fast TeV flare of blazars For BL Lac: A radio core, stationary radio knots, and many superluminal knots A coincident superluminal radio knot after the first fast TeV flare in 2011; implication on the location of the emitting region Flux (10-6 m -2 s -1 ) m -2 s >200 GeV Minutes The first TeV flare from BL Lac on 2011 Jun 28 decay time ~13 minutes Cohen et al GHz GHz Arlen et al
7 A new TeV flare from BL Lac on 2016 Oct 5 Peak flux ~180% Crab Avg flux ~90% Crab I(t) = ( I peak e (t t peak)/t rise, t 6 t peak ; I peak e (t t peak)/t decay, t > t peak ; 5 rise time = 140 ( ) minutes decay time = 36 (+ 8-7) minutes
8 Markov-Chain Monte Carlo: To get posterior probability distribution of the parameters. Ensemble sampling: 100 random walkers 1000 steps after 1000 burning steps 100,000 sims Peak flux 6 Peak time Rise time Decay time
9 Adding a constant baseline makes the best-fit variability time much faster Motivation: 1. BL Lac is known for its multiple radio cores 2. A concurrent 1-week GeV flare was observed red χ 2 = 1.18 I(t) = ( I base + I 0 e (t t peak)/t rise, t 6 t peak ; I base + I 0 e (t t peak)/t decay, t > t peak ; Considering the statistical and systematic uncertainties, we can t significantly reject either model. 7 rise time = 65 (+19-8) minutes decay time = 2.6 ( ) minutes I_base = (1.2 ± 0.1) x 10-6 ph m -2 s -1
10 Baseline constraints from observations Integral flux upper limit TeV at 99% confidence level assuming a photon index of -3.3 Peak ~180% Crab On Oct 6 (live time 37.6 min) the UL is 2x10-7 m -2 s -1 Avg ~90% Crab On Oct 22 - Nov 19 (live time min) the UL is 2.8x10-8 m -2 s -1 ~8% Crab +1 day ~1% Crab +3 weeks 8
11 Higher order exponential fit with a constant baseline can fit the ULs measured later Soft L1 loss function I_base = ± I_0 = 9.7 ± 5.6 t_peak = ± 1.1 t_rise = 7.7 ± 18 t_decay= 1.9 ± 4.4 k = 0.21 ± 0.06 red χ 2 = 73.7/42 = 1.75 I(t) = ( I base + I 0 e [ t t peak /t rise ] k, t 6 t peak ; I base + I 0 e [ t t peak /t decay ] k, t > t peak ; +1 day +3 weeks No single model can explain both the flare and the upper limits. Two components are most likely required. 9
12 while fails to fit the flare I(t) = ( I base + I 0 e [ t t peak /t rise ] k, t 6 t peak ; I base + I 0 e [ t t peak /t decay ] k, t > t peak ; Overfit No single model can explain both the flare and the upper limits. Two components are most likely required. 10
13 Spectral energy distribution (SED) 1.83 ± ± 0.07 VHE spec: Power law: index = ; red χ 2 = 34 Log-parabola: alpha = ; beta = ; red χ 2 =
14 MWL light curves Concurrent LAT flare: rise time 2.1 ± 0.2 days decay time 6.9 ± 1.8 days Drop in polarization fraction Change in polarization angle 12
15 Swift XRT observations on Oct 6, 7, 8 Oct 6 Oct 7 Oct 8 13
16 Swift XRT SED - exclusion region has no effect on the spectral results Except statistics! 14
17 VLBA 43 GHz Marscher & Jorstad 0.2 mas 1.3 pc/mas A potential new knot (K16) travelling at ~6c. 15
18 VLBA 43 GHz Marscher & Jorstad 0.2 mas 1.3 pc/mas A potential new knot (K16) travelling at ~6c. K11 at ~3.6c Arlen et al The first TeV flare from BL Lac on 2016 Jun 28 15
19 MOJAVE VLBA 15 GHz Lister, Pushkarev, Kovalev, Savolainen VLBA 15 GHz VLBA 43 GHz 1.3 pc/mas Radio knot K16/VHE gamma-ray flare 16
20 VLBA 15 GHz 17
21 Single-dish light curve at 37 and 15 GHz Merja, Kiehlmann, Hovatta+ Metsahovi OVRO 15 GHz vs 37 GHz 18 Zero lag between 15 GHz and 37 GHz indicates they are both measuring the jet outside the 15 GHz radio core.
22 Interpretation Fast flare => small size of emission region Fast decay => abrupt stop of injection R apple ct decay 1+z Gaussian injection The upper limit of the size of emission region is: ~12 Rs (Schwarzschild radius; ~1 Rs for the model with a baseline), or 1.39x10 13 m, or 4.5x10-4 pc on-off injection MBH = 3.8x10 8 M ; Doppler Factor δ= 24; Wu et al. (2009) Hervet et al. (2016) Katarzynski et al. (2003) 19
23 Interpretation Association between TeV and radio: Turbulent Extrem Multi-Zone model: Particle acceleration Radio core/knot Marscher et al. (2014) Fast gamma-ray flare Figure 1. Sketch of the geometry employed to carry out calculations withi Multiple recollimation shock + carried-away shock model: Magnetic dominated jet Class I/II Faster flow of plasma/perturbation Particle dominated jet Hervet et al. (2016) E Radio core/ stationary knot Stationary knot Superluminal knot Magnetic reconnection - gamma-ray flare 20
24 Summary VERITAS detected a fast TeV flare from BL Lac peaking at ~180% Crab. The decay time is about 36 minutes, and faster than the rise time. Size of the emitting region constrained to be 12Rs. Correlated GeV/optical flare at the time of the TeV flare, but slower. Polarization activities observed in R band and radio frequencies. VLBA 43 GHz images can be interpreted with a superluminal radio knot passing the core around the time of the TeV flare (but the interpretation s likely not unique). Such observations can potentially locate the TeV gamma-ray emitting region (a difficult task)! 21
Millimeter-Wave and Optical Polarimetric Behavior of Blazars
Millimeter-Wave and Optical Polarimetric Behavior of Blazars Iván Agudo Instituto de Astrofísica de Andalucía Granada (Spain) with: Clemens Thum José L. Gómez Sol Molina Carolina Casadio Helmut Wiesemeyer
More information10 Years. of TeV Extragalactic Science. with VERITAS. Amy Furniss California State University East Bay
55 555 56 565 57 55 555 56 565 57 55 555 56 565 57 572 574 576 578 57 5712 5714 5716 572 574 576 578 57 5712 5714 5716 5712 5713 5714 5715 5716 5712 5713 5714 5715 5716 5712 5713 5714 5715 5716 5712 5713
More informationParsec-Scale Jet Properties of Fermi-detected AGN
Parsec-Scale Jet Properties of Fermi-detected AGN Matthew Lister (Purdue) for the MOJAVE Team Montage by M. Kadler et al. MOJAVE Collaboration M. Lister (P.I.), N. Cooper, B. Hogan, T. Hovatta S. Kuchibhotla
More informationMultiwavelength observations of the blazar BL Lacertae: a new fast TeV γ-ray flare
Boston University OpenBU Astronomy http://open.bu.edu BU Open Access Articles Multiwavelength observations of the blazar BL Lacertae: a new fast TeV γ-ray flare Feng, Q. Q. Feng, for the VERITAS Collaboration,
More informationThe Extragalactic Gamma-Ray View of AGILE and Fermi
INAF, Osservatorio Astronomico di Capodimonte 22 February 2012 The Extragalactic Gamma-Ray View of AGILE and Fermi Elena Pian INAF, Trieste Astronomical Observatory & Scuola Normale Superiore di Pisa UNIFIED
More informationThe connection between millimeter and gamma-ray emission in AGNs
The connection between millimeter and gamma-ray emission in AGNs Marcello Giroletti INAF Istituto di Radioastronomia Secondo Workshop sull'astronomia millimetrica e submillimetrica in Italia Bologna, 2-3
More informationInvestigating the jet structure and its link with the location of the high-energy emitting region in radio-loud AGN
Investigating the jet structure and its link with the location of the high-energy emitting region in radio-loud AGN Filippo D Ammando (INAF-IRA and DIFA Bologna) Monica Orienti (INAF-IRA) Marcello Giroletti
More informationRadio activity of BL Lacertae during gamma-ray outbursts
Radio activity of BL Lacertae during gamma-ray outbursts Daewon Kim (SNU) S. Trippe, S. Lee, J. Park, J. Oh, T. Lee,, G. Zhao, S. Kang, M. Kino, J. Kim, K. Wajima, and J. Algaba The 10th East Asian Meeting
More informationAGILE and Blazars: the Unexpected, the Unprecedented, and the Uncut
AGILE and Blazars: the Unexpected, the Unprecedented, and the Uncut Rome, AGILE γ-ray Symposium 2017.12.12 Stefano Vercellone (INAF-OAB) 1 Rationale A review of the whole set of AGILE results on extra-galactic
More informationSIMILARITY AND DIVERSITY OF BLACK HOLE SYSTEMS View from the Very High Energies
SIMILARITY AND DIVERSITY OF BLACK HOLE SYSTEMS View from the Very High Energies 1 Symp. 324, 12-16 September, 2016 Classical view Spinning black hole Accretion disk Collimated jets of particles 2 Looking
More informationGlobal evlbi observations of the first gamma-ray RL NLS1
Global evlbi observations of the first gamma-ray RL NLS1 Marcello Giroletti (INAF/IRA), Akihiro Doi (ISAS/JAXA) and Z. Paragi, H. Bignall, L. Foschini, K. Gabanyi, C. Reynolds, and many others Outline
More informationLong term multi-wavelength variability studies of the blazar PKS
52nd Rencontres de Moriond 2017 Very High Energy Phenomena in the Universe Long term multi-wavelength variability studies of the blazar PKS 2155-304 Jill Chevalier D. Sanchez, P. Serpico, J-P. Lenain,
More informationNon-Blazar Gamma-ray Active Galactic Nuclei seen by Fermi-LAT. C.C. Teddy Cheung Naval Research Lab/NRC on behalf of the Fermi-LAT Collaboration
Non-Blazar Gamma-ray Active Galactic Nuclei seen by Fermi-LAT C.C. Teddy Cheung Naval Research Lab/NRC on behalf of the Fermi-LAT Collaboration 1 st LAT AGN Catalog (1LAC) Summary FmJ 2010 Entire 1LAC:
More informationObservations of Active Galactic Nuclei at very high energies with H.E.S.S.
Observations of Active Galactic Nuclei at very high energies with H.E.S.S. Robert Wagner for the H.E.S.S. Collaboration http://www.mpi-hd.mpg.de/hess/ @hesstelescopes 1 H.E.S.S. High Energy Stereoscopic
More informationPolarization Swings Reveal Magnetic Energy Dissipation in Blazars
Polarization Swings Reveal Magnetic Energy Dissipation in Blazars Xuhui Chen Most of this work is done by : Haocheng Zhang (Ohio University & LANL, USA) Other Collaborators: Markus Boettcher (North-West
More informationMWL. A Brief Advertisement Before Your Regularly Scheduled Program
MWL A Brief Advertisement Before Your Regularly Scheduled Program PKS 1441+25 PKS 1441+25 z=0.939! VHE detection over more than a single day! PKS 1441+25 37.7% polarization! PKS 1441+25 Continues optical
More informationarxiv: v1 [astro-ph.he] 24 Jan 2013
arxiv:1301.5751v1 [astro-ph.he] 24 Jan 2013 1, Tuomas Savolainen 1, Alexander B. Pushkarev 2,3,1, Yuri Y. Kovalev 4,1, Matthew L. Lister 5 1 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121
More informationPoS(SWIFT 10)142. The Swift-XRT observations of HBL Source 1ES
The Swift-XRT observations of HBL Source 1ES 199+ ab, Patrizia Romano b, Stefano Vercellone b, Sergo Kapanadze a, Grigol Kharshiladze c a E. Kharadze Abastumani Astrophysical Observatory, Ilia State University,
More informationarxiv: v1 [astro-ph.he] 20 Sep 2016
galaxies Article Radiative Transfer Modeling of Radio-band Linear Polarization Observations as a Probe of the Physical Conditions in the Jets of γ-ray Flaring Blazars Margo F. Aller 1, Philip A. Hughes
More informationRadio Loud Black Holes. An observational perspective
Radio Loud Black Holes An observational perspective Tiziana Venturi INAF, Istituto di Radioastronomia, Bologna Overview of the first lesson 1) Synchrotron emission and radio spectra of AGN 2) Classification
More informationVery High Energy gamma-ray radiogalaxies and blazars
Very High Energy gamma-ray radiogalaxies and blazars Hélène Sol Paris Observatory, CNRS JD6, The connection between radio properties and High-Energy emission in AGNs Outline The sample of AGN currently
More informationarxiv: v1 [astro-ph.he] 27 Feb 2018
Draft version March 1, 2018 Typeset using L A TEX preprint2 style in AASTeX61 MULTIWAVELENGTH OBSERVATIONS OF THE BLAZAR BL LACERTAE: A NEW FAST TEV GAMMA-RAY FLARE arxiv:1802.10113v1 [astro-ph.he] 27
More informationFrom EGRET to Fermi: mm-radio data and the origin of gamma-ray emission
From EGRET to Fermi: mm-radio data and the origin of gamma-ray emission FmJ 2010 Esko Valtaoja Merja Tornikoski, Jonathan León-Tavares, Elina Nieppola, Anne Lähteenmäki, Joni Tammi, Talvikki Hovatta Metsähovi-Tuorla
More informationBlazar science with mm-vlbi. Marcello Giroletti, Monica Orienti, Filippo D Ammando on behalf of the Fermi-LAT collaboration
Blazar science with mm-vlbi Marcello Giroletti, Monica Orienti, Filippo D Ammando on behalf of the Fermi-LAT collaboration Outline Why are blazars interesting? mm-vlbi & blazar sampler 7mm, 3mm, 1.3mm
More informationNot only typical flaring blazars in the Fermi gamma-ray sky. The strange cases of SBS and PKS
Not only typical flaring blazars in the Fermi gamma-ray sky. The strange cases of SBS 0846+513 and PKS 0521-36 Filippo D Ammando (University of Perugia and INFN) and M. Orienti (Univ. of Bologna and INAF-IRA)
More informationTwo exceptional γ-ray flares of PKS and their implications on blazar and fundamental physics
Two exceptional γ-ray flares of PKS 2155-304 and their implications on blazar and fundamental physics Rolf Bühler MPIK Heidelberg KIPAC Tea Talk SLAC 9th December 2008 H.E.S.S. Telescopes Located in Namibia
More informationPolarization Studies of Extragalactic Relativistic Jets from Supermassive Black Holes. Iván Agudo
Polarization Studies of Extragalactic Relativistic Jets from Supermassive Black Holes Iván Agudo What is an active galactic nuclei (AGN)? Compact regions at the centre of galaxies with much higher than
More informationFermi Source Analyses and Identifying VERITAS Candidates
Fermi Source Analyses and Identifying VERITAS Candidates 1 1 1. University of California, Berkeley 2 Overview Introduction VERITAS Fermi Analysis Likelihood Doppler Factor Estimation Motivations Blazars
More informationThe ALMA contribution to the
The ALMA contribution to the study of the blazar jets M. Orienti (Bologna University, INAF-IRA) Outline The extragalactic γ-ray sky and relativistic jets The Atacama Large Millimeter Array Relativistic
More informationDiversity of Multi-wavelength Behavior of Relativistic Jet in 3C 279 Discovered During the Fermi Era
Diversity of Multi-wavelength Behavior of Relativistic Jet in 3C 279 Discovered During the Fermi Era Rapid Variability of Blazar 3C 279 during Flaring States in 2013-2014 with Joint Fermi-LAT, NuSTAR,
More informationGamma-ray emitting narrow-line Seyfert 1 galaxies and their place in the AGN zoo
Gamma-ray emitting narrow-line Seyfert 1 galaxies and their place in the AGN zoo Filippo D Ammando (DIFA and INAF-IRA Bologna) Monica Orienti, Justin Finke, Marcello Giroletti, Josefin Larsson on behalf
More informationDetermining the TeV Gamma-Ray Emission Region in the Relativistic Jet of M87 using TeV and Radio Monitoring
Determining the TeV Gamma-Ray Emission Region in the Relativistic Jet of M87 using TeV and Radio Monitoring R. M. Wagner Max-Planck-Institut für Physik, München and Excellence Cluster Origin and Structure
More informationCan blazar flares be triggered by the VHE gamma-rays from the surrounding of a supermassive black hole?
Can blazar flares be triggered by the VHE gamma-rays from the surrounding of a supermassive black hole? Department of Astrophysics, University of Lodz, Lodz, Poland E-mail: p.banasinski@uni.lodz.pl Wlodek
More informationThe extreme ends of the spectrum: the radio/gamma connection
The extreme ends of the spectrum: the radio/gamma connection Monica Orienti INAF IRA Bologna Astronomy Department, Bologna University This research has made used of data from the MOJAVE database that is
More informationThe First Full-Polarimetric 3.5 & 1.3mm Monitoring Program of Bright Gamma-Ray Blazars Iván Agudo
The First Full-Polarimetric 3.5 & 1.3mm Monitoring Program of Bright Gamma-Ray Blazars Iván Agudo Instituto de Astrofísica de Andalucía Granada (Spain) Clemens Thum José L. Gómez Sol Molina Carolina Casadio
More informationVERITAS detection of VHE emission from the optically bright quasar OJ 287
VERITAS detection of VHE emission from the optically bright quasar OJ 287 S. Zola & NASA/JPL S. O Brien For The VERITAS Collaboration Outline 1. OJ 287 2. Historical Observations and Monitoring Programs
More informationMultiwavelength Observations of 3C 66A in
Blazar Variability Workshop II: Entering the GLAST Era ASP Conference Series, Vol. 350, 2006 H. R. Miller, K. Marshall, J. R. Webb, and M. F. Aller Multiwavelength Observations of 3C 66A in 2003 2004 M.
More informationThe first detection of the blazar S at VHE with the MAGIC Telescopes during an exceptionally high optical state
The first detection of the blazar S4 0954+65 at VHE with the MAGIC Telescopes during an exceptionally high optical state Giovanna Pedaletti on behalf of the MAGIC and Fermi collaborations and the MWL team
More informationPhysical Properties of Jets in AGN. Dan Homan Denison University
Physical Properties of Jets in AGN Dan Homan Denison University Probes of Physical Properties (Part 1) Long Time Baseline Kinematics Distribution of Apparent Speeds in Blazar Population Lorentz Factor/Viewing
More informationDoppler boosting as the generator of the blazar sequence
Doppler boosting as the generator of the blazar sequence, 1 Esko Valtaoja, 2,3 Merja Tornikoski, 1 Talvikki Hovatta 1 and Mikko Kotiranta 1 1 Metsähovi Radio Observatory Metsähovintie 114, 02540 Kylmälä,
More informationExtreme high-energy variability of Markarian 421
Extreme high-energy variability of Markarian 421 Mrk 421 an extreme blazar Previous observations outstanding science issues 2001 Observations by VERITAS/Whipple 10 m 2001 Light Curve Energy spectrum is
More informationModelling the Variability of Blazar Jets
Modelling the Variability of Blazar Jets A Selfconsistent SSC Model Matthias Weidinger Institut für Theoretische Physik und Astrophysik, Universität Würzburg GRK Tage: 24. Juli 2009 M. Weidinger (Uni Wü)
More informationMonitoring of Blazars for variability from MIRO. Kiran S Baliyan Physical Research Laboratory, Ahmedabad, India
Monitoring of Blazars for variability from MIRO Kiran S Baliyan Physical Research Laboratory, Ahmedabad, India Black-holes, Jets and Outflows, Kathmandu, Nepal, October 14, 2013 Enigmatic AGNs AGNs- Huge
More informationarxiv: v1 [astro-ph] 8 Dec 2008
Studying the continuum spectrum of the parsec scale jets by multi-frequency VLBI measurements arxiv:0812.1486v1 [astro-ph] 8 Dec 2008 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn,
More informationEnergy-dependent variability in blazars SSC simulations
Energy-dependent variability in blazars SSC simulations David Sanchez Laboratoire Leprince-Ringuet, CNRS/IN2P3, Ecole Polytechnique, 91128 Palaiseau, France E-mail: dsanchez@llr.in2p3.fr Berrie Giebels
More informationPAGaN II: The evolution of AGN jets on sub-parsec scales Junghwan Oh Seoul National University East-Asia AGN Workshop 2016
PAGaN II: The evolution of AGN jets on sub-parsec scales Junghwan Oh Seoul National University East-Asia AGN Workshop 2016 S. Trippe, S. Kang, D. Kim, M. Kino, SS. Lee, T. Lee, J. Park, B. Sohn AGN at
More informationRadio and gamma-ray emission in Faint BL Lacs
AGN X ROMA, 10-13/09/2012 Radio and gamma-ray emission in Faint BL Lacs E. Liuzzo, B. Boccardi, M. Giroletti, G. Giovannini, F. Massaro, M. Orienti, S. Tamburri, C. Casadio 3EG Catalog γ sky EGRET (3EG,
More informationUNDERSTANDING POWERFUL JETS AT DIFFERENT SCALES IN THE FERMI ERA. B. THE KPC SCALE: X-RAY EMISSION MECHANISM AND JET SPEED
UNDERSTANDING POWERFUL JETS AT DIFFERENT SCALES IN THE FERMI ERA. A. THE PC SCALE: LOCATING THE Γ-RAY EMISSION SITE B. THE KPC SCALE: X-RAY EMISSION MECHANISM AND JET SPEED Markos Georganopoulos 1,2 Eileen
More informationTotal intensity radio variations in blazars. Talvikki Hovatta, Anne Lähteenmäki, Elina Nieppola, Ilona Torniainen, Merja Tornikoski
Total intensity radio variations in blazars Esko 1, Markku Lainela, Elina Lindfors, Pia-Maria Saloranta, Kaj Wiik Tuorla Observatory and Department of Physics, University of Turku Väisäläntie 20, FI-21500
More informationBlazars in gamma-ray views
Blazars in gamma-ray views Challenges of AGN jets@naoj, Mitaka 19 January 2017 Masaaki Hayashida M.Hayashida et al. 2015, ApJ, in press (Institute Cosmic-ray research, (arxiv:1502.04699) the Univ. of Tokyo)
More informationM87 in context: the radio gamma-ray connection in misaligned AGNs
M87 in context: the radio gamma-ray connection in misaligned AGNs M. Giroletti and F. D'Ammando on behalf of the Fermi-LAT collaboration, and C. Casadio, P. Grandi, K. Hada M87 Workshop: Towards the 100th
More informationActive Galactic Nuclei
Active Galactic Nuclei Optical spectra, distance, line width Varieties of AGN and unified scheme Variability and lifetime Black hole mass and growth Geometry: disk, BLR, NLR Reverberation mapping Jets
More informationarxiv: v1 [astro-ph.he] 2 Jul 2010
Fermi meets Jansky AGN in Radio and Gamma-Rays Savolainen, T., Ros, E., Porcas, R.W., & Zensus, J.A. (eds.) June 21 23, 2010, Bonn, Germany Recent multi-wavelength campaigns in the Fermi-GST era Lars Fuhrmann
More informationPoS(Extremesky 2011)055
Aalto University Metsähovi Radio Observatory, P.O.Box 13000, FI-00076 Aalto, FINLAND E-mail: joni.tammi@iki.fi I discuss the role of radio observations and modelling of the low-frequency emission in active
More informationThe third Fermi LAT AGN catalogue and beyond
The third Fermi LAT AGN catalogue and beyond Filippo D Ammando (DIFA and INAF-IRA Bologna) on behalf of the Fermi LAT Collaboration dammando@ira.inaf.it 1 Different classes of AGN Quasars Radio-quiet or
More informationHubble Space Telescope ultraviolet spectroscopy of blazars: emission lines properties and black hole masses. E. Pian, R. Falomo, A.
Hubble Space Telescope ultraviolet spectroscopy of blazars: emission lines properties and black hole masses E. Pian, R. Falomo, A. Treves 1 Outline Extra Background Introduction Sample Selection Data Analysis
More informationPoS(11th EVN Symposium)022
The connection between radio and Very High Energy in Active Galactic Nuclei: perspectives with CTA, the Cherenkov Telescope Array 1 Observatoire de Paris, CNRS, LUTH Place J. Janssen, 92195 Meudon, France
More informationStudies on the VHE γ-ray/x-ray correlation in high-synchrotron peak BL Lacs
Studies on the VHE γ-ray/x-ray correlation in high-synchrotron peak BL Lacs Magda Gonzalez Instituto de Astronomía, UNAM, México Nissim Fraija 1, Barbara Patricelli 2, José Andrés García 3 & Simone Dichiara
More informationScientific Highlights from AGN Observations with the MAGIC Telescope
Scientific Highlights from AGN Observations with the MAGIC Telescope Robert Marcus WAGNER Max-Planck-Institut für Physik, München on behalf of the MAGIC COLLABORATION MAGIC Major Atmospheric Gamma-ray
More informationCorrelation between γ -ray and radio emissions in Fermi blazars
Publ. Astron. Soc. Japan (2014) 66 (6), 117 (1 11) doi: 10.1093/pasj/psu111 Advance Access Publication Date: 2014 December 11 117-1 Correlation between γ -ray and radio emissions in Fermi blazars De-Xiang
More informationStatus of the MAGIC telescopes
SNOWPAC 2010 Status of the MAGIC telescopes Pierre Colin for the MAGIC collaboration Max-Planck-Institut für physik (Munich) Status of the MAGIC telescopes MAGIC-1 MAGIC-2 Outline: Recent results of the
More informationActive Galactic Nuclei in the MeV-GeV band (first results from Fermi)
Active Galactic Nuclei in the MeV-GeV band (first results from Fermi) Gino Tosti University & INFN Perugia On behalf of the Fermi-LAT Collaboration 1 Active Galactic Nuclei (AGN) EGRET showed that AGN
More informationTeV γ-ray observations with VERITAS and the prospects of the TeV/radio connection
TeV γ-ray observations with VERITAS and the prospects of the TeV/radio connection Matthias Beilicke for the VERITAS collaboration Washington University in St.Louis, Physics Department and McDonnell Center
More informationBlazars as the Astrophysical Counterparts of the IceCube Neutrinos
Blazars as the Astrophysical Counterparts of the IceCube Neutrinos Maria Petropoulou Department of Physics & Astronomy, Purdue University, West Lafayette, USA Einstein Fellows Symposium Harvard-Smithsonian
More informationFlaring Active Galactic Nuclei: the view from Fermi-LAT
Flaring Active Galactic Nuclei: the view from Fermi-LAT INAF-IASF IASF Palermo On behalf of the Fermi-LAT Collaboration and many multi-wavelength collaborators SciNeGHE 2010 1 The EGRET Era AGN dominate
More informationMarkus Boettcher Centre for Space Research, North-West University, Potchefstroom, 2520, South Africa
Time-Dependence of VHE γ-ray induced Pair Cascades in AGN Environments Department of Physics and Astronomy, Rice University, Houston, TX 77005, USA Department of Physics and Astronomy, Ohio University,
More informationVariability of Extragalactic VHE γ-ray Emitters
Variability of Extragalactic VHE γ-ray Emitters Wystan Benbow Harvard-Smithsonian Center for Astrophysics APS April 2011 Meeting, Anaheim, CA Very High Energy (VHE) γ-ray Astronomy VHE: ~100 GeV to ~100
More informationOrigin of X-rays in blazars
Origin of X-rays in blazars Greg Madejski, Stanford / KIPAC With much of the work presented here done by Amy Furniss, Masaaki Hayashida, Krzysztof Nalewajko, Marek Sikora, Jim Chiang, David Paneque, Mislav
More informationAlan Marscher Boston University
The Relationship between Radio and Higher Frequency Emission in AGNs Alan Marscher Boston University Research Web Page: www.bu.edu/blazars Sketch of an AGN 10 6 to > 10 9 M sun black hole + accretion disk
More informationMAGIC detection of very-high-energy gamma-ray emission from the z = 0.94 blazar PKS
MAGIC detection of very-high-energy gamma-ray emission from the z = 0.94 blazar PKS 1441+25 Miguel Nievas Rosillo Co-authors: J. Becerra, M. Manganaro, F. Tavecchio MW Collaborators: E. Lindfors, J. Sitarek,
More informationINTRINSIC BRIGHTNESS TEMPERATURES OF COMPACT RADIO JETS
Journal of the Korean Astronomical Society http://dx.doi.org/10.5303/jkas.2014.47.6.303 47: 303 309, 2014 December pissn: 1225-4614 eissn: 2288-890X c 2014. The Korean Astronomical Society. All rights
More informationObserving TeV Gamma Rays from the Jet Interaction Regions of SS 433 with HAWC
Observing TeV Gamma Rays from the Jet Interaction Regions of SS 433 with HAWC Chang Dong Rho University of Rochester TeVPA 2018 Berlin, Germany 08/28/2018 Overview 2 Microquasars as sources of TeV gamma
More informationACCRETION JET CONNECTION τ α MBH
Radio Observations ACCRETION JET CONNECTION τ α MBH 1 hr in GRS 1915+105 = 30 yr in SgrA* Mirabel et al. 1998 THE TRIGGERS OF JETS ARE INSTABILITIES IN THE ACCRETION DISK (TRANSITION LOW HARD TO HIGH THE
More informationRecent Results from VERITAS
Recent Results from VERITAS Physics Department, McGill University, Montreal, Canada E-mail: hanna@physics.mcgill.ca VERITAS (Very Energetic Radiation Imaging Telescope Array System) is an array of four
More informationarxiv: v1 [astro-ph] 20 Aug 2008
arxiv:0808.2733v1 [astro-ph] 20 Aug 2008, 1 Merja Tornikoski, 1 Harry J. Lehto, 2,3 Elina Nieppola, 1 Esko Valtaoja, 2,3 Markku Lainela, 2 Ilona Torniainen, 1 Anne Lähteenmäki 1 Margo F. Aller 4 and Hugh
More informationRadio sources. P. Charlot Laboratoire d Astrophysique de Bordeaux
Radio sources Laboratoire d Astrophysique de Bordeaux Outline Introduction Continuum and spectral line emission processes The radio sky: galactic and extragalactic History of radioastronomy The first 50
More informationVERITAS Observations of Relativistic Jets
VERITAS Observations of Relativistic Jets 1 for the VERITAS Collaboration 1Barnard College, Columbia University Sensitivity improvement: 1% Crab in ~25 hr Sensitive energy range: 100 GeV to 30 TeV Spectral
More informationAnalysis of Five Fermi-LAT LBL/IBL BL Lac Objects: Examining the June 2011 Gamma-ray Flare of BL Lacertae
Analysis of Five Fermi-LAT LBL/IBL BL Lac Objects: Examining the June 2011 Gamma-ray Flare of BL Lacertae Valerie Marchenko 3 August 2012, Nevis Labs, Columbia University https://news.slac.stanford.edu/sites/default/files/images/image/blazar-search-st.jpg
More informationThe RoboPol project: Rotations of polarization plane in optical emission of blazars
The RoboPol project: Rotations of polarization plane in optical emission of blazars Dmitry Blinov for the RoboPol collaboration Univ. of Crete, Heraklion, Greece http://robopol.org Kikuchi et al., 1988,
More informationHigh Energy Emission. Brenda Dingus, LANL HAWC
High Energy Emission from GRBs Brenda Dingus, LANL HAWC What are GRBs? Cosmological distance Typical observed z>1 Energy released is up to few times the rest mass of Sun (if isotropic) in a few seconds
More informationNEUTRINOS ON ICE THE SEARCH FOR THE COSMIC-RAY SOURCES FE KRAUSS, J. WILMS, M. KADLER, M. KRETER
NEUTRINOS ON ICE THE SEARCH FOR THE COSMIC-RAY SOURCES FE KRAUSS, J. WILMS, M. KADLER, M. KRETER FELICIA.KRAUSS@UVA.NL COSMIC RAYS 2a COSMIC RAYS 1896: Henri Becquerel discovery of radioactivity 1909:
More informationTeV Observations of Extragalactic Sources
TeV Observations of Extragalactic Sources Henric Krawczynski (Washington University in St. Louis), Oct. 2, 2009 Plan of Talk: Status of Experiments Key-Results: Radio Galaxies Blazars Starburst Galaxies
More informationCTA / ALMA synergies. C. Boisson. Zech
CTA / ALMA synergies C. Boisson LUTh, Observatoire de Paris Zech thanks to H. Sol & A. Particle acceleration is a wide-spread phenomena in the Universe CTA Key Science Cosmic Rays Origin of cosmic rays
More informationOBSERVATIONS OF VERY HIGH ENERGY GAMMA RAYS FROM M87 BY VERITAS
OBSERVATIONS OF VERY HIGH ENERGY GAMMA RAYS FROM M87 BY VERITAS 1 Tülün Ergin (U. of Massachusetts Amherst, MA) on behalf of the VERITAS Collaboration (http://veritas.sao.arizona.edu) APOD, 2004 December
More informationGamma-ray observations of blazars with the Whipple 10 m telescope
Gamma-ray observations of blazars with the Whipple 1 m telescope, presented on behalf of the VERITAS collaboration. E-mail: edward.collins.hughes@gmail.com This paper presents a status update of the current
More informationThe radio/gamma-ray connection in Active Galactic Nuclei in the Fermi era
The radio/gamma-ray connection in Active Galactic Nuclei in the Fermi era M. Giroletti INAF Istituto di Radioastronomia and V. Pavlidou, A. Reimer on behalf of the Fermi-LAT collaboration Roma, X Congresso
More informationMisaligned AGN with Fermi-Lat:
Misaligned AGN with Fermi-Lat: a different perspective on relativistic jets PAOLA GRANDI INAF/IASF BOLOGNA, ITALY on behalf of the FERMI LAT Collaboration Many thanks to : Torresi E., Migliori G., P. Malaguti,
More informationTheoretical Study of the Effects of Magnetic Field Geometry on the High-Energy Emission of Blazars
Article Theoretical Study of the Effects of Magnetic Field Geometry on the High-Energy Emission of Blazars Manasvita Joshi 1, *, Alan Marscher 1 and Markus Böttcher 2,3 1 Insitute for Astrophysical Research,
More informationGuiding Questions. Active Galaxies. Quasars look like stars but have huge redshifts
Guiding Questions Active Galaxies 1. Why are quasars unusual? How did astronomers discover that they are extraordinarily distant and luminous? 2. What evidence showed a link between quasars and galaxies?
More informationDepartment of Physics and Astronomy, Purdue University, 525 Northwestern Avenue, West Lafayette, IN 47907, USA;
galaxies Article AGN Jet Kinematics on Parsec-Scales: The MOJAVE Program Matthew Lister and the MOJAVE Collaboration Department of Physics and Astronomy, Purdue University, 525 Northwestern Avenue, West
More informationThe University of Michigan Centimeter-Band All Stokes Blazar Monitoring Program: Single-dish Polarimetry as a Probe of Parsec-scale Magnetic Fields
galaxies Article The University of Michigan Centimeter-Band All Stokes Blazar Monitoring Program: Single-dish Polarimetry as a Probe of Parsec-scale Magnetic Fields Margo F. Aller 1 ID, Hugh D. Aller 1
More informationarxiv: v2 [astro-ph.co] 19 Jan 2010
Astronomy & Astrophysics manuscript no. savolainen v4 c ESO 2018 November 5, 2018 Relativistic beaming and gamma-ray brightness of blazars T. Savolainen 1, D. C. Homan 2, T. Hovatta 3,4, M. Kadler 5,6,7,
More informationThe X-Ray Universe. The X-Ray Universe
The X-Ray Universe The X-Ray Universe Potsdam University Dr. Lidia Oskinova Sommersemester 2017 lida@astro.physik.uni-potsdam.de astro.physik.uni-potsdam.de ~lida/vorlesungxrayso17.html Chandra X-ray,
More informationTHE STORY OF STRONGLY LENSED JETS AND COSMOLOGY. Anna Barnacka Einstein Fellow at Harvard
Berenice Abbott THE STORY OF STRONGLY LENSED JETS AND COSMOLOGY Anna Barnacka Einstein Fellow at Harvard EXTRAGALACTIC JETS - M87 Increased x-ray emission by a factor of 50 from HST-1 knot (Harris et al.
More informationStatus of TeV AGN Studies
Status of TeV AGN Studies Wystan Benbow Harvard-Smithsonian Center for Astrophysics AGN Physics in the CTA Era Workshop, Toulouse, France, May 16, 2011 The Extragalactic VHE Gamma-ray Sky May 1, 2011:
More informationr = A g / A opt > 2 or more, that is,
Name Affiliation A. Bulgarelli INAF-IASF Bologna A.W. Chen INAF-IASF Milano I. Donnarumma INAF-IASF Roma P. Giommi ASDC Roma A. Giuliani INAF-IASFMilano F. Longo INFN Trieste C. Pittori ASDC Roma L. Pacciani
More informationKinematics of AGN jets
Journal of Physics: Conference Series Kinematics of AGN jets To cite this article: Eduardo Ros 2008 J. Phys.: Conf. Ser. 131 012061 View the article online for updates and enhancements. This content was
More informationarxiv: v1 [astro-ph.he] 8 Jul 2014
Constraining the Physical Conditions in the Jets of γ-ray Flaring Blazars using Centimeter-Band Polarimetry and Radiative Transfer Simulations. I. Data and Models for 0420-014, OJ 287, & 1156+295 arxiv:1407.2194v1
More informationNEAR-INFRARED PHOTOMETRY OF BLAZARS
NEAR-INFRARED PHOTOMETRY OF BLAZARS C. Chapuis 1,2,S.Corbel 1, P. Durouchoux 1,T.N.Gautier 3, and W. Mahoney 3 1) Service d Astrophysique DAPNIA, CEA Saclay F-91191 Gif sur Yvette cedex 2) Département
More informationModels for the Spectral Energy Distributions and Variability of Blazars
Models for the Spectral Energy Distributions and Variability of Blazars Markus Böttcher Ohio University, Athens, OH, USA Fermi Meets Jansky Bonn, Germany, June 21, 2010 Outline: 1) Introduction to leptonic
More information