Pith. sign in

REVIEW

Out of the Chorus Line : What Makes 1E1207.4-5209 a Unique Object?

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/0310177 v1 pith:LH5AV6W4 submitted 2003-10-07 astro-ph

A. De Luca , P.A. Caraveo , S. Mereghetti , M. Moroni , G. Bignami , R. Mignani This is my paper · ORCID
classification astro-ph
keywords e1207featuresspectralchoruslineobjectobservationx-ray
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

The discovery of deep spectral features in the X-ray spectrum of 1E1207.4-5209 has pushed this Isolated Neutron Star (INS) out of the chorus line, since no other INS has shown significant features in its X-ray continuum. On August 2002, XMM-Newton devoted a two-orbit TOO observation to this target with the aim to better understand the nature of such spectral features, using much improved statistics. Indeed, the 260 ksec observation yielded 360,000 photons from 1E1207.4-5209, allowing for a very sensitive study of the temporal and spectral behaviour of this object.

Discussion (0). Continue with ORCID to comment.

Pith tools