Publication:
Science goals for Antarctic infrared telescopes

dc.contributor.author Burton, Michael en_US
dc.contributor.author Storey, John en_US
dc.contributor.author Ashley, Michael en_US
dc.date.accessioned 2021-11-25T12:56:40Z
dc.date.available 2021-11-25T12:56:40Z
dc.date.issued 2001 en_US
dc.description.abstract Over the past few years, site-testing at the South Pole has revealed conditions that are uniquely favorable for IR astronomy. In particular, the exceptionally low sky brightness throughout the near- and mid-IR leads to the possibility of a modest-sized telescope achieving comparable sensitivity to that of existing 8-10 meter class telescopes. An 8m Antarctic telescope, if constructed, would yield performance that would be unrivaled until the advent of the NGST. In this paper we review the scientific potential of IR telescopes in Antarctica, and discuss their complementarity with existing 8-10m class telescopes. en_US
dc.identifier.issn 1323-3580 en_US
dc.identifier.uri http://hdl.handle.net/1959.4/38617
dc.language English
dc.language.iso EN en_US
dc.rights CC BY-NC-ND 3.0 en_US
dc.rights.uri https://creativecommons.org/licenses/by-nc-nd/3.0/au/ en_US
dc.source Legacy MARC en_US
dc.title Science goals for Antarctic infrared telescopes en_US
dc.type Journal Article en
dcterms.accessRights metadata only access
dspace.entity.type Publication en_US
unsw.accessRights.uri http://purl.org/coar/access_right/c_14cb
unsw.relation.faculty Science
unsw.relation.ispartofjournal Publications of the Astronomical Society of Australia en_US
unsw.relation.ispartofpagefrompageto 158-165 en_US
unsw.relation.ispartofvolume 18 en_US
unsw.relation.originalPublicationAffiliation Burton, Michael, Physics, Faculty of Science, UNSW en_US
unsw.relation.originalPublicationAffiliation Storey, John, Physics, Faculty of Science, UNSW en_US
unsw.relation.originalPublicationAffiliation Ashley, Michael, Physics, Faculty of Science, UNSW en_US
unsw.relation.school School of Physics *
Files
Resource type