271 citations · 1.4k across the 17 of their papers we have counts for
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The stellar content of the COSMOS field as derived from morphological and SED based gtar/galaxy Separation
A. C. Robin, R. M. Rich, H. Aussel +12
We report on the stellar content of the COSMOS two degree field, as derived from a rigorous star/galaxy separation approach developed for using stellar sources to define the point…
SDSSp J104433.04012502.2 at is Gravitationally Magnified by an Intervening Galaxy
Yasuhiro Shioya, Yoshiaki Taniguchi, Takashi Murayama +15
During the course of our optical deep survey program on L emitters at in the sky area surrounding the quasar SDSSp J104433.04012502.2 at , we found th…
A New High-Redshift Lyman alpha Emitter: Possible Superwind Galaxy at z = 5.69
M. Ajiki, Y. Taniguchi, T. Murayama +33
During the course of our deep optical imaging survey for Ly alpha emitters at z approximately 5.7 in the field around the z=5.74 quasar SDSSp J104433.04-012502.2, we have found a c…
Effects of a burst of formation of first-generation stars on the evolution of galaxies
Yasuhiro Shioya, Yoshiaki Taniguchi, Takashi Murayama +3
First-generation (Population III) stars in the universe play an important role inearly enrichment of heavy elements in galaxies and intergalactic medium and thus affect the history…
The Nature of the faint far-infrared extragalactic source population: Optical/NIR and radio follow-up observations of ISOPHOT deep-field sources using Keck, Subaru, and VLA telescopes
Yuko Kakazu, D. B. Sanders, R. D. Joseph +11
We report on optical and near-infrared (NIR) follow-up spectroscopy of faint far-infrared (FIR) sources found in our deep FIR survey by Kawara et al.
On the Origin of Lyman Blobs at High Redshift: Submillimetric Evidence for a Hyperwind Galaxy at z=3.1
Yoshiaki Taniguchi, Yasuhiro Shioya, Yuko Kakazu
The most remarkable class of high-redshift objects observed so far is extended Ly emission-line blobs found in an over-density region at redshift 3.1. They may be either a dust-…
A Shock-Induced Pair of Superbubbles in the High-Redshift Powerful Radio Galaxy MRC 0406-244
Yoshiaki Taniguchi, Youichi Ohyama, Takashi Murayama +26
We present new optical spectroscopy of the high-redshift powerful radio galaxy MRC 0406244 at redshift of 2.429. We find that the two extensions toward NW and SE probed in the r…