Pith. sign in

REVIEW

Identifying variable gamma-ray sources through radio observations

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/0407454 v1 pith:CJGDKDHU submitted 2004-07-21 astro-ph

J.M. Paredes , J. Marti , D.F. Torres , G.E. Romero , J.A. Combi , V. Bosch-Ramon , J. Garcia-Sanchez This is my paper · ORCID
classification astro-ph
keywords radiogamma-raysourcesvariableemissiontimeappearcampaign
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We present preliminary results of a campaign undertaken with different radio interferometers to observe a sample of the most variable unidentified EGRET sources. We expect to detect which of the possible counterparts of the gamma-ray sources (any of the radio emitters in the field) varies in time with similar timescales as the gamma-ray variation. If the gamma-rays are produced in a jet-like source, as we have modelled theoretically, synchrotron emission is also expected at radio wavelengths. Such radio emission should appear variable in time and correlated with the gamma-ray variability.

Discussion (0). Continue with ORCID to comment.

Pith tools