Some Prospects for High Redshift Galaxy Observations with the Submillimeter Array

Details Some Prospects for High Redshift Galaxy Observations with the Submillimeter Array Some Prospects for High Redshift Galaxy Observations with the Submillimeter Array

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001dms..conf...55w&link_type=abstract

DEEP MILLIMETER SURVEYS Implications for Galaxy Formation and Evolution. Held 19-21 June 2000 in University of Massachusetts, Am

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Submillimeter Array, being built near the summit of Mauna Kea by the Smithsonian Astrophysical Observatory and the Institute of Astronomy and Astrophysics (Taiwan), has the potential to make unique observations of the newly recognized population of luminous high redshift dusty galaxies. Prospects for submillimeter continuum observations include (1) accurate position determinations for improved associations at optical/infrared/radio wavelengths, (2) deep integrations that probe beyond the confusion limit of single dish telescopes, and (3) imaging the detailed morphologies of the stronger sources at kiloparsec size scales.

Affiliated with

Also associated with

No associations

Rating

Some Prospects for High Redshift Galaxy Observations with the Submillimeter Array does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Some Prospects for High Redshift Galaxy Observations with the Submillimeter Array, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Some Prospects for High Redshift Galaxy Observations with the Submillimeter Array will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1104873