CaltechAUTHORS
  A Caltech Library Service

Millimetre/submillimetre-wave emission-line searches for high-redshift galaxies

Blain, A. W. and Frayer, D. T. and Bock, J. J. and Scoville, N. Z. (2000) Millimetre/submillimetre-wave emission-line searches for high-redshift galaxies. Monthly Notices of the Royal Astronomical Society, 313 (3). pp. 559-570. ISSN 0035-8711. http://resolver.caltech.edu/CaltechAUTHORS:BLAmnras00

[img]
Preview
PDF - Published Version
See Usage Policy.

713Kb

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:BLAmnras00

Abstract

The redshifted spectral line radiation emitted from both atomic fine-structure and molecular rotational transitions in the interstellar medium (ISM) of high-redshift galaxies can be detected in the centimetre, millimetre and submillimetre wavebands. Here we predict the counts of galaxies detectable in an array of molecular and atomic lines. This calculation requires a reasonable knowledge of both the surface density of these galaxies on the sky, and the physical conditions in their ISM. The surface density is constrained using the results of submillimetre-wave continuum surveys. Follow-up OVRO Millimeter Array observations of two of the galaxies detected in the dust continuum have provided direct measurements of CO rotational line emission at redshifts of 2.56 and 2.81. Based on these direct high-redshift observations and on models of the ISM that are constrained by observations of low-redshift ultraluminous infrared galaxies, we predict the surface density of line-emitting galaxies as a function of line flux density and observing frequency. We incorporate the sensitivities and mapping speeds of existing and future millimetre/submillimetre-wave telescopes and spectrographs, and so assess the prospects for blank-field surveys to detect this line emission from gas-rich high-redshift galaxies.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1046/j.1365-8711.2000.03287.xDOIUNSPECIFIED
Additional Information:© 2000 RAS. Accepted 1999 November 11. Received 1999 November 10; in original form 1999 March 24. The results in this paper are based on the properties of the SCUBA lens survey galaxies detected at the Owens Valley Millimeter Array in collaboration with Aaron Evans and Min Yun. The core of the SCUBA lens survey was carried out by Ian Smail, Rob Ivison, AWB and Jean-Paul Kneib. We thank the referee, Paul van der Werf, for his careful reading of the manuscript and valuable comments, and also Jackie Davidson, Kate Isaak, Rob Ivison, Richard Hills, Brett Kornfeld, Malcolm Longair, Phil Lubin, Kate Quirk, John Richer and Gordon Stacey for helpful conversations and comments. AWB - the Raymond & Beverly Sackler Foundation Research Fellow at the IoA, Cambridge - gratefully acknowledges generous support from the Raymond & Beverly Sackler Foundation as part of the Deep Sky Initiative programme at the IoA. AWB also thanks the Caltech AY visitors program for support while this work was conducted.
Funders:
Funding AgencyGrant Number
Raymond & Beverly Sackler FoundationUNSPECIFIED
Caltech Astronomy visitors' programUNSPECIFIED
Subject Keywords:molecules; galactic evolution; galaxy formation; cosmology; infrared galaxies; radio lines
Record Number:CaltechAUTHORS:BLAmnras00
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:BLAmnras00
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:11308
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:06 Aug 2008 03:19
Last Modified:30 Aug 2013 18:49

Repository Staff Only: item control page