The Detection of Extremely Distant Galaxies

Details The Detection of Extremely Distant Galaxies The Detection of Extremely Distant Galaxies

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ap%26ss.265..561l&link_type=abstract

Astrophysics and Space Science, v. 265, Issue 1/4, p. 561-566 (1999).

Astronomy and Astrophysics

Astrophysics

Scientific paper

Very recent observations have shown that there are dusty galaxies at redshifts larger that 5. Their integrated contribution to the far-IR/submillimeter sky background is known. These galaxies are very hard to detect in the visible and in the infrared, but they will be within reach of the NGST, although it will be very difficult to recognize them without further studies. However their far-infrared emission will be detectable by FIRST and more easily by the large submillimeter interferometer (ALMA) presently under study. The ALMA, FIRST, SIRTF and the NGST will make an ideal set for investigating the formation and early evolution of galaxies.

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