VLBI and γ-ray studies of TANAMI radio galaxies. Roberto Angioni, MPIfR Bonn EVN symposium, September 2016 St. Petersburg, Russia

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VLBI and γ-ray studies of TANAMI radio galaxies Roberto Angioni, MPIfR Bonn EVN symposium, 20-23 September 2016 St. Petersburg, Russia

11/10/2016 R. Angioni - TANAMI radio galaxies 2 Collaborators Eduardo Ros MPIfR Bonn, Uni. Valencia Matthias Kadler Uni. Würzburg Roopesh Ojha NASA Goddard Space Flight Center Cornelia Müller Radboud Uni. Nijmegen Felicia Krauss GRAPPA & API, Uni. Amsterdam Anton Zensus MPIfR Bonn TANAMI collaboration Fermi-LAT collaboration (graduate member)

11/10/2016 R. Angioni - TANAMI radio galaxies 3 Outline TANAMI program and science VLBI monitoring The highest-resolution view of the closest AGN: Centaurus A VLBI sample study of TANAMI radio galaxies: Pictor A Dual frequency imaging Spectral index mapping Kinematics γ-ray studies of radio galaxies

11/10/2016 R. Angioni - TANAMI radio galaxies 4 The TANAMI program Tracking Active Nuclei with Austral Milliarcsecond Interferometry ~90 jets at θ < 30 declination at mas resolution since 2007 Array: LBA + New Zealand, South Africa, Antarctica, Chile Dual frequency 8.4 GHz and 22.3 GHz, 3-4 epochs/yr

11/10/2016 R. Angioni - TANAMI radio galaxies The TANAMI program 5

11/10/2016 R. Angioni - TANAMI radio galaxies 6 The TANAMI program First-epoch images Ojha et al. 2010

11/10/2016 R. Angioni - TANAMI radio galaxies 7 The TANAMI program New sources Müller et al. in prep.

11/10/2016 R. Angioni - TANAMI radio galaxies 8 The TANAMI program Centaurus A Highest-resolution view of the closest AGN jet Müller et al. 2011,14 Comp. speeds 0.1 c to 0.3c, downstream acceleration Intrinsic jet parameters θ~12 45 β~0.24 0.37 Tuning fork ~0.4 pc from core revealed by stacked images, most likely jet-start interaction

11/10/2016 R. Angioni - TANAMI radio galaxies 9 TANAMI radio galaxies B1950 IAU Alt. name RA Dec Class z γ-ray det. 0518-458 Pictor A 79.96-45.78 FR II 0.035 Y 0521-365 PKS 0521-36 80.74-36.46 RG/SSRQ 0.057 Y 0625-354 PKS 0625-35 96.78-35.49 FRI/BLL 0.055 Y 1258-321 PKS 1258-321 195.25-32.44 FR I 0.017 N 1333-337 IC 4296 204.16-33.97 FR I 0.013 N 1343-601 Centaurus B 206.70-60.41 FR I 0.013 Y 1549-790 PKS 1549-79 239.25-79.23 RG/CSO 0.15 N 1718-649 NGC 6328 260.92-65.01 GPS/CSO 0.014 Y 1733-565 PKS 1733-56 264.40-56.57 FR II 0.099 N 1814-637 PKS 1814-63 274.90-63.76 CSS/CSO 0.065 N 1934-638 PKS 1934-63 294.85-63.71 GPS 0.18 N 2027-308 PKS 2027-308 307.41-30.66 RG 0.54 N 2152-699 PKS 2153-69 329.28-69.69 FR II 0.028 N

11/10/2016 R. Angioni - TANAMI radio galaxies 10 VLBI dual frequency imaging VLBI imaging of southern hemisphere radio galaxies (FR I, FR II, compact objects) at 3.6 cm and 1.3 cm 13 sources in total Pictor A Pictor A Perley+ 1997, VLA 1.4 GHz Angioni+ in prep., TANAMI 8.4 GHz

11/10/2016 R. Angioni - TANAMI radio galaxies 11 Spectral index mapping 8.4 GHz Pictor A No previous study on spectral morphology on VLBI scales Pictor A Angioni+ in prep. 22 GHz Pictor A Preliminary map indicates inverted core

11/10/2016 R. Angioni - TANAMI radio galaxies 12 Jet kinematics Pictor A Previous VLBI study (Tingay et al. 2000) 2 epochs at 8.4 GHz (SHEVE 1993 + VLBA 1999) Jet bend at ~5 mas from core Subluminal motion of inner components β 1 Preliminary TANAMI features 5 epochs at 8.4 GHz Jet bend looks persistent App. speed for innermost moving component β = 1.8 ± 0.4 Angioni+ in prep.

11/10/2016 R. Angioni - TANAMI radio galaxies 13 TANAMI radio galaxies Current progress on sample study: Imaging completed for 10/13 sources, ~80 maps in total 16 spix maps 3 preliminary kinematic analyses

11/10/2016 R. Angioni - TANAMI radio galaxies 14 Radio galaxies with Fermi-LAT Alternative high-energy view of relativistic jets (w.r.t. blazars) Smaller bias from strong Doppler effects Test for unified models, emission models, acceleration models Simultaneous obs. of accretion and jet origin of radio-loudness Abdo et al. 2010 GeV γ-rays from RG lobes Energetic particles far from central engine Core/lobes and impact on variability Uncl. 28% FSRQ 29% Nonblazar 1% BL Lac 42% Cen A Fornax A Ackermann et al. 2016 γ-ray RGs provide crucial information, but we have only few sources...new detections with Pass8 analysis?

11/10/2016 R. Angioni - TANAMI radio galaxies 15 Multi-wavelength and Fermi-LAT Pass8 Fermi-LAT data analysis for RGs and γ-ray undetected quasars: new detections or better ULs SEDs: why are these sources not detected by the LAT? Pictor A

11/10/2016 R. Angioni - TANAMI radio galaxies 16 Thank you for your attention!

11/10/2016 R. Angioni - TANAMI radio galaxies 17 γ-ray-faint TANAMI sources There is a strong connection between radio and γ-ray emission in radio-loud AGN... Correlations (Arshakian+ 2012) Variability behavior (e.g. Fuhrmann+ 2014, Casadio+ 2015, Rani+ 2014, 2015, Karamanavis+ 2015, 2016)...but there are bright radio-loud sources without a γ-ray detection (Lister+ 2015) Lower SED peak? Doppler factor?

11/10/2016 R. Angioni - TANAMI radio galaxies 18 Multi-wavelength and Fermi-LAT Analysis of Pass8 LAT data for γ-ray-faint TANAMI sources (radio galaxies and quasars)

11/10/2016 R. Angioni - TANAMI radio galaxies 19 γ-ray-faint sample Source RA(J2000) Dec(J2000) Redshift Class PKS 0438-43 70.07167-43.5525 2.863 Q PMN J0529-3555 82.406958-35.921222 * U PKS 1257-326 195.17678-32.886697 1.256 Q PKS 1258-321 195.25334-32.441456 0.017042 G IC 4296 204.1625-33.96583 0.012465 G PKS 1549-79 239.24542-79.23444 0.1501 G PKS 1716-771 260.96042-77.23056 * U PKS 1733-56 264.39917-56.5675 0.098 G PKS 1814-63 274.89583-63.76333 0.0627 G PKS 1915-458 289.81950-45.727389 2.47 Q PKS 1934-63 294.85428-63.71267 0.539 G PKS 2027-308 307.74125-30.65667 0.539 G PKS 2106-413 317.38833-41.1725 1.058 Q PKS 2153-69 329.275-69.69 0.028273 G

11/10/2016 R. Angioni - TANAMI radio galaxies 20 Multi-wavelength and Fermi-LAT Analysis of Pass8 LAT data for γ-ray-faint TANAMI sources (radio galaxies and quasars) No detections yet, but significantly improved upper limits w.r.t. previously published work (TANAMI paper on 1 st year of LAT data, Böck et al. 2016) B1950 IAU name P7 UL (erg cm^-2 s^-1) P8 UL (erg cm^-2 s^-1) 0438-436 7.92e-12 2.34e-12 1257-326 1.55e-11 2.15e-12 1258-321 1.73e-11 3.43e-12 1333-337 6.48e-12 1.88e-13 1549-790 1.59e-11 1.54e-12 2106-413 4.32e-12 1.55e-12 2152-699 1.23e-11 1.61e-12

11/10/2016 R. Angioni - TANAMI radio galaxies 21 TANAMI highlights: multi-messenger

11/10/2016 R. Angioni - TANAMI radio galaxies 22 TANAMI highlights: multi-messenger Long γ-ray outburst from blazar PKS B1424-418 coincident with highest energy IceCube neutrino event TANAMI sees strongest outburst ever from VLBI core, starting before γ-ray flare (1.5 to 6 Jy) Chance coincidence probabiliity estimated in ~5%

11/10/2016 R. Angioni - TANAMI radio galaxies 23 TANAMI highlights: time resolved Krauss et al. 2016 Dynamic SED catalog: 81 SEDs for 22 brightest TANAMI γ-ray blazars

11/10/2016 R. Angioni - TANAMI radio galaxies 24 TANAMI highlights: multi-wavelength Müller et al. 2014,15,16 Identification of the peculiar γ-ray source PMN J1603-4904 with a MPS radio galaxy