Pith. sign in

REVIEW

XMM-Newton Survey of a Distance-limited Sample of Seyfert Galaxies: Preliminary Spectral Results

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/0303367 v1 pith:I6IKP6OW submitted 2003-03-17 astro-ph

M.Cappi , G.Di Cocco , F.Panessa , L. Bassani , E. Caroli , M. Dadina , A. Comastri , R.Della Ceca
show 14 more authors
A.V.Filippenko L. Foschini F. Gianotti L.C.Ho K.Makishima G.Malaguti J.S.Mulchaey G.G.C.Palumbo E.Piconcelli W.L.W.Sargent J.Stephen M.Trifoglio K.Weaver G.Zamorani
This is my paper · ORCID
classification astro-ph
keywords galaxiesseyfertmodelspreliminaryresultssamplex-rayxmm-newton
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

An unbiased estimate of the average intrinsic X-ray properties and column density distribution of Seyfert galaxies in the local Universe is crucial to validate unified models of active galactic nuclei (AGNs) and to synthesis models for the X-ray background. We present here preliminary results obtained from an on-going XMM-Newton study (~250 ks awarded in the EPIC GT) on a well-defined, statistically complete, and significant sample of nearby Seyfert galaxies.

Discussion (0). Continue with ORCID to comment.

Pith tools