TANAMI: Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry - II. Additional Sources
aut.relation.journal | Astronomy and Astrophysics | en_NZ |
aut.researcher | Weston, Stuart | |
dc.contributor.author | Muller, C | en_NZ |
dc.contributor.author | Kadler, M | en_NZ |
dc.contributor.author | Ojha, R | en_NZ |
dc.contributor.author | Schulz, R | en_NZ |
dc.contributor.author | Trustedt, J | en_NZ |
dc.contributor.author | Edwards, PG | en_NZ |
dc.contributor.author | Ros, E | en_NZ |
dc.contributor.author | Carpenter, B | en_NZ |
dc.contributor.author | Angioni, R | en_NZ |
dc.contributor.author | Blanchard, J | en_NZ |
dc.contributor.author | Bock, M | en_NZ |
dc.contributor.author | Burd, PR | en_NZ |
dc.contributor.author | Dorr, M | en_NZ |
dc.contributor.author | Dutka, MS | en_NZ |
dc.contributor.author | Eberl, T | en_NZ |
dc.contributor.author | Gulyaev, S | en_NZ |
dc.contributor.author | Hase, H | en_NZ |
dc.contributor.author | Horiuchi, S | en_NZ |
dc.contributor.author | Katz, U | en_NZ |
dc.contributor.author | Krauss, F | en_NZ |
dc.contributor.author | Lovell, JEJ | en_NZ |
dc.contributor.author | Natusch, T | en_NZ |
dc.contributor.author | Nesci, R | en_NZ |
dc.contributor.author | Phillips, C | en_NZ |
dc.contributor.author | Plotz, C | en_NZ |
dc.contributor.author | Pursimo, T | en_NZ |
dc.contributor.author | Quick, JFH | en_NZ |
dc.contributor.author | Stevens, J | en_NZ |
dc.contributor.author | Thompson, DJ | en_NZ |
dc.contributor.author | Tingay, SJ | en_NZ |
dc.contributor.author | Tzioumis, AK | en_NZ |
dc.contributor.author | Weston, S | en_NZ |
dc.contributor.author | Wilms, J | en_NZ |
dc.contributor.author | Zensus, JA | en_NZ |
dc.date.accessioned | 2017-10-10T22:29:43Z | |
dc.date.available | 2017-10-10T22:29:43Z | |
dc.date.copyright | 2017-09-10 | en_NZ |
dc.date.issued | 2017-09-10 | en_NZ |
dc.description.abstract | Context. TANAMI is a multiwavelength program monitoring active galactic nuclei (AGN) south of −30◦ declination including highresolution Very Long Baseline Interferometry (VLBI) imaging, radio, optical/UV, X-ray and γ-ray studies. We have previously published first-epoch 8.4 GHz VLBI images of the parsec-scale structure of the initial sample. In this paper, we present images of 39 additional sources. The full sample comprises most of the radio- and γ-ray brightest AGN in the southern quarter of the sky, overlapping with the region from which high-energy (> 100 TeV) neutrino events have been found. Aims. We characterize the parsec-scale radio properties of the jets and compare with the quasi-simultaneous Fermi/LAT γ-ray data. Furthermore, we study the jet properties of sources which are in positional coincidence with high-energy neutrino events as compared to the full sample. We test the positional agreement of high-energy neutrino events with various AGN samples. Methods. TANAMI VLBI observations at 8.4 GHz are made with Southern-Hemisphere radio telescopes located in Australia, Antarctica, Chile, New Zealand, and South Africa. Results. Our observations yield the first images of many jets below −30◦ declination at milliarcsecond resolution. We find that γ-ray loud TANAMI sources tend to be more compact on parsec-scales and have higher core brightness temperatures than γ-ray faint jets, indicating higher Doppler factors. No significant structural difference is found between sources in positional coincidence with high-energy neutrino events and other TANAMI jets. The 22 γ-ray brightest AGN in the TANAMI sky show only a weak positional agreement with high-energy neutrinos demonstrating that the > 100 TeV IceCube signal is not simply dominated by a small number of the γ-ray brightest blazars. Instead, a larger number of sources have to contribute to the signal with each individual source having only a small Poisson probability for producing an event in multi-year integrations of current neutrino detectors. | |
dc.identifier.citation | arXiv preprint arXiv:1709.03091. | |
dc.identifier.issn | 0004-6361 | en_NZ |
dc.identifier.uri | https://hdl.handle.net/10292/10858 | |
dc.publisher | EDP Sciences | en_NZ |
dc.relation.uri | http://arxiv.org/abs/1709.03091 | en_NZ |
dc.rights | arXiv.org Open access to e-prints in Physics, Mathematics, Computer Science, Quantitative Biology, Quantitative Finance, Statistics, Electrical Engineering and Systems Science, and Economics | |
dc.rights.accessrights | OpenAccess | en_NZ |
dc.subject | galaxies: active -– galaxies: jets -– galaxies: nuclei -– radio continuum: galaxies – techniques: high angular resolution | |
dc.title | TANAMI: Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry - II. Additional Sources | en_NZ |
dc.type | Journal Article | |
pubs.elements-id | 311116 | |
pubs.organisational-data | /AUT | |
pubs.organisational-data | /AUT/Design & Creative Technologies | |
pubs.organisational-data | /AUT/Design & Creative Technologies/Engineering, Computer & Mathematical Sciences | |
pubs.organisational-data | /AUT/Design & Creative Technologies/Engineering, Computer & Mathematical Sciences/ISASR | |
pubs.organisational-data | /AUT/PBRF | |
pubs.organisational-data | /AUT/PBRF/PBRF Design and Creative Technologies | |
pubs.organisational-data | /AUT/PBRF/PBRF Design and Creative Technologies/PBRF ECMS |
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