Increasing the Number of TeV Blazars with Parsec-Scale Kinematics
Vivian C. Tiet, B. Glenn Piner, and Philip G. Edwards

TL;DR
This study provides new VLBA observations of five TeV-detected blazars, revealing their jet speeds and properties, and roughly doubles the known sample of TeV HBLs with detailed kinematic data.
Contribution
It presents the first multi-epoch VLBA imaging of five TeV blazars, expanding the sample of TeV HBLs with parsec-scale kinematic measurements.
Findings
TeV HBLs have slower apparent jet speeds than radio-selected blazars.
The jets likely have modest Lorentz factors, indicating a gradient in jet speeds.
The study roughly doubles the number of TeV HBLs with detailed kinematic data.
Abstract
We report on our observations of the parsec-scale radio jet structures of five blazars that have been detected by ground-based TeV gamma-ray telescopes. These five blazars all belong to the class of high-frequency peaked BL Lac objects (HBLs), which are the most common blazar type detected at the TeV energy range. Because of their relative faintness in the radio, these HBLs are not well represented in other radio blazar surveys. Our observations consist of five epochs of Very Long Baseline Array (VLBA) imaging from 2006 to 2009, of each of the five blazars 1ES 1101-232, Markarian 180, 1ES 1218+304, PG 1553+113, and H 2356-309, at frequencies from 5 to 22 GHz. Fundamental jet properties, including the apparent jet speeds, that can be measured from these multi-epoch series of VLBA images are presented and compared with other gamma-ray blazars. Confirming prior work, we find that the TeV…
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Astrophysics and Cosmic Phenomena · Computational Physics and Python Applications
