Shedding light on the dark side of galaxy formation: submillimetre surveys through lensing clusters

Simple item page
dc.creatorIvison, Rob
dc.date2000-07-12
dc.date.accessioned2026-07-07T01:54:22Z
dc.date.available2026-07-07T01:54:22Z
dc.descriptionMost new sub-mm/mm surveys, both deep and shallow, are being targeted at rich cluster fields. I explain why, comparing surveys that have exploited weak lensing by massive foreground clusters with those done in blank fields.
dc.description6 pages, 2 colour figures. Proceedings of the XXth Moriond Astrophysics Meeting, `Cosmological Physics with Gravitational Lensing', eds J.-P. Kneib, Y. Mellier, M. Moniez, J. Tran Thanh Van
dc.identifierhttps://arxiv.org/abs/astro-ph/0007162
dc.identifierhttp://arxiv.org/abs/astro-ph/0007162
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1322
dc.subjectAstrophysics
dc.titleShedding light on the dark side of galaxy formation: submillimetre surveys through lensing clusters
dc.typetext

Files

Collections

arXiv