The "Large Millimeter Telescop&' and its potential for high-z studies

Olmi, L. and Mauskopf, Philip Daniel ORCID: https://orcid.org/0000-0001-6397-5516 1998. The "Large Millimeter Telescop&' and its potential for high-z studies. Presented at: The young universe : galaxy formation and evolution at intermediate and high redshift, Monteporzio, Italy, 29 Sept - 3 Oct 1997. Published in: D'Odorico, S., Fontana, A. and Giallongo, E. eds. The young universe : galaxy formation and evolution at intermediate and high redshift : proceedings from a meeting held at Rome Astronomical Observatory, Monteporzio, 29 September - 3 October 1997. Astronomical Society of the Pacific conference series (146) Astronomical Society of the Pacific conference series: San Francisco, CA, pp. 371-375.

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Abstract

The "Large Millimeter Telescope" (LMT) is a joint U.S.A. and Mexico Project and will be the world's largest millimeter-wavelength radio telescope, equipped with the state-of-the-art heterodyne and bolometric focal plane arrays. We show that CO lines (and also CS) will be able to be detected in unlensed galaxies. Furthermore, the continuum camera will allow measurements of the Sunyaev-Zel'dovich effect, as well as enabling deep surveys of dust emission from protogalaxies.

Item Type:	Conference or Workshop Item (Paper)
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Publisher:	San Francisco, CA
ISBN:	9781583814826
Related URLs:	Publisher
Last Modified:	27 Oct 2022 10:20
URI:	https://orca.cardiff.ac.uk/id/eprint/69748

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