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J/A+A/610/A1        TANAMI II. Additional sources               (Mueller+, 2018)

TANAMI: Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry. II. Additional sources Mueller C., Kadler M., Ojha R., Schulz R., Truestedt J., Edwards P.G., Ros E., Carpenter B., Angioni R., Blanchard J., Boeck M., Burd P.R., Doerr M., Dutka M.S., Eberl T., Gulyaev S., Hase H., Horiuchi S., Katz U., Krauss F., Lovell J.E.J., Natusch T., Nesci R., Phillips C., Ploetz C., Pursimo T., Quick J.F.H., Stevens J., Thompson D.J., Tingay S.J., Tzioumis A.K., Weston S., Wilms J., Zensus J.A. <Astron. Astrophys. 610, A1 (2018)> =2018A&A...610A...1M (SIMBAD/NED BibCode)
ADC_Keywords: Active gal. nuclei ; VLBI Keywords: galaxies: active - galaxies: jets - galaxies: nuclei - radio continuum: galaxies - techniques: high angular resolution - neutrinos Abstract: TANAMI is a multiwavelength program monitoring active galactic nuclei (AGN) south of -30° declination including high-resolution Very Long Baseline Interferometry (VLBI) imaging, radio, optical/UV, X-ray and γ-ray studies. We have previously published first-epoch 8.4GHz 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 (>100TeV) neutrino events have been found. 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. TANAMI VLBI observations at 8.4GHz are made with Southern-Hemisphere radio telescopes located in Australia, Antarctica, Chile, New Zealand, and South Africa. 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 >100TeV 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. Description: Very Long Baseline Interferometry (VLBI) images of 39 active galactic nuclei from the TANAMI sample (Figs. 1-5). TANAMI VLBI observations at 8.4 GHz are made with southern hemisphere radio telescopes located in Australia, Antarctica, Chile, New Zealand, and South Africa. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file list.dat 102 39 List of FITS images fits/* 0 39 Individual VLBI FITS images of 39 sources at 8.4GHz
See also: J/A+A/591/A130 : Dynamic SEDs of southern blazars - DSSB (Krauss+, 2016) Byte-by-byte Description of file: list.dat
Bytes Format Units Label Explanations
1- 9 F9.5 deg RAdeg Right ascension of center (J2000) 11- 19 F9.5 deg DEdeg Declination of center (J2000) 21- 24 F4.2 mas/pix Scale Scale of the image 26- 29 I4 --- Nx Number of pixels along X-axis 30 A1 --- --- [x] 31- 34 I4 --- Ny Number of pixels along Y-axis 36- 42 F7.5 GHz Freq Frequency 44- 53 A10 "YYYY-MM-DD" ObsDate Observation date 55- 59 I5 Kibyte size Size of FITS file 61- 74 A14 --- FileName Name of FITS file in subdirectory fits 76-102 A27 --- Title Title of the file
Acknowledgements: Cornelia Mueller, c.mueller(at) References: Krauss et al., Paper I 2016A&A...591A.130K, Cat. J/A+A/591/A130
(End) Patricia Vannier [CDS] 22-Sep-2017
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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