Pith. sign in

REVIEW

The extended counterpart of submm source Lockman850.1

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/0108131 v1 pith:YRUJRKNQ submitted 2001-08-08 astro-ph

D. Lutz , J.S. Dunlop , O. Almaini , P. Andreani , A. Blain , A. Efstathiou , M. Fox , R. Genzel
show 12 more authors
G. Hasinger D. Hughes R.J. Ivison A. Lawrence R.G. Mann S. Oliver J.A. Peacock D. Rigopoulou M. Rowan-Robinson S. Scott S. Serjeant L. Tacconi
This is my paper
classification astro-ph
keywords counterpartextendedformationlockman850objectsourcestarsubmm
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

The IRAM Plateau de Bure mm interferometer and deep K-band imaging have been used to identify the brightest submm source detected in the Lockman field of the UK 8mJy SCUBA survey. The near infrared counterpart is an extended (20-30kpc), clumpy, and extremely red object. The spectral energy distribution suggests it to be a dusty star forming object at a redshift of about 3 (2-4). Its star formation rate and near-infrared properties are consistent with Lockman850.1 being a massive elliptical in formation.

Discussion (0). Sign in to comment.

Pith tools