Pith. sign in

REVIEW

The Submillimetre Universe

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 1008.4159 v1 pith:ZN3PPRT4 submitted 2010-08-24 astro-ph.IM

Douglas Scott , Pauline Barmby , Pierre Bastien , Jan Cami , Edward Chapin , James Di Francesco , Michel Fich , Mark Halpern
show 14 more authors
Martin Houde Gilles Joncas Douglas Johnstone Peter Martin Gaelen Marsden Brenda Matthews David Naylor C. Barth Netterfield Els Peeters Rene Plume Alexandra Pope Gerald Schieven Tracy Webb Christine Wilson
This is my paper
classification astro-ph.IM
keywords submillimetregalaxiesallowsalmaansweringcircumstellarcoldcombination
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Submillimetre continuum radiation allows us to probe cold objects, particularly the earliest, dusty phases of star formation, high-redshift galaxies and circumstellar disks. The submillimetre window gives a unique view of the physical and dynamical conditions in the neutral and molecular interstellar medium. In the next decade a combination of wide-field surveys with single-dish telescopes and targeted follow-up with ALMA and other facilities should enable rapid progress in answering questions about the origins of planetary systems, stars and galaxies.

Discussion (0). Sign in to comment.

Pith tools