Astronomy and Astrophysics – Astronomy
Scientific paper
May 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...192.5520s&link_type=abstract
American Astronomical Society, 192nd AAS Meeting, #55.20; Bulletin of the American Astronomical Society, Vol. 30, p.902
Astronomy and Astrophysics
Astronomy
Scientific paper
High--redshift quasars provide some of the earliest glimpses we have of the Universe, constrain models of structure formation, and are valuable probes of the intervening intergalactic medium. We are pursuing a program to find high--redshift, radio--loud quasars. The search technique relies upon two new large--area surveys of unprecedented depth and accuracy: the FIRST survey (Faint Images of the Radio Sky at Twenty Centimeters) --- a VLA effort mapping the Northern sky with 1.0'' positional uncertainty to a limiting flux of S_1.4 GHz = 1 mJy, and the DPOSS (digitized Second Palomar Observatory Sky Survey) --- a photographic montage of the northern sky in three pass bands: blue (g; lambda_eff ~ 4800 Angstroms), red (r; lambda_eff ~ 6500 Angstroms), and infrared (i; lambda_eff ~ 8500 Angstroms). Typical limiting magnitudes are 22.5() m, 20.8() m and 19.5() m, respectively; i.e., ~ 1 -- 1.5 magnitudes deeper than the POSS--I and with an additional redder plate. Correlating these large radio and optical catalogs, we find optical identifications for the radio sources and select red objects which are classified as stars by DPOSS for spectroscopic observation. We have found the two most distant quasars selected from the FIRST survey to date: FIRST 1410+3409 (z=4.36) and FIRST 0100-0128 (z=3.85).
Breugel Wil van
de Carvalho Reinaldo R.
Djorgovski Stanislav
Gal Roy R.
Odewahn Stephen
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