Radio and Gamma Properties of the 2 cm Survey and MOJAVE Samples
Eduardo Ros (Univ. Valencia & MPIfR) (for the MOJAVE collaboration)

TL;DR
This paper compares radio and gamma-ray properties of AGN samples from the 2 cm VLBA Survey and MOJAVE project, revealing higher gamma-ray detection rates in MOJAVE sources with faster jets and a preference for BL Lac objects.
Contribution
It provides a comparative analysis of gamma-ray detection rates between two well-defined AGN samples, highlighting the correlation with jet speed and object type.
Findings
MOJAVE sources have higher gamma-ray detection rates.
Faster jets correlate with increased gamma-ray detection.
BL Lac objects are more frequently detected in gamma-rays than QSOs.
Abstract
The 2 cm VLBA Survey observed since 1994 a set of ~170 Quasars, BL Lac objects, and radio galaxies, selected to be representative of the compact AGN radio population. This effort was continued as the MOJAVE project, where a statistically complete set of radio sources being monitored was defined. A comparison of the gamma-detection rates between the members of both samples shows that the MOJAVE-I sources, hosting generally faster jets, have a much higher detection rate than the sources not belonging to this sample. BL Lac objects are more favourably detected than QSOs in gamma-rays, in the same rate for both samples.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Gamma-ray bursts and supernovae
