The End of the Reionization Epoch Probed by Lyα Emitters at z = 6.5 in the Subaru Deep Field
- N. KashikawaK. Shimasaku M. Umemura
- 6 April 2006
Physics
We report an extensive search for Lyα emitters (LAEs) at z = 6.5 in the Subaru Deep Field. Subsequent spectroscopy with Subaru and Keck identified eight more LAEs, giving a total of 17…
Lyα Emitters at z = 5.7 in the Subaru Deep Field
- K. ShimasakuN. Kashikawa Y. Taniguchi
- 28 February 2006
Physics
PASJ: Publ. Astron. Soc. Japan , 1–??, c 2008. Astronomical Society of Japan. Lyα Emitters at z = 5.7 in the Subaru Deep Field Kazuhiro Shimasaku, 1,2 Nobunari Kashikawa, 3,4 Mamoru Doi, 5,2 Chun Ly,…
Gas metallicity diagnostics in star-forming galaxies
- T. NagaoR. MaiolinoAlessandro Marconi Arcetri ObservatoryN. A. O. Japan
- 21 March 2006
Physics
Generally the gas metallicity in distant galaxies can only be inferred by using a few prominent emission lines. Various theoretical models have been used to predict the relationship between emission…
The Luminosity Function and Star Formation Rate between Redshifts of 0.07 and 1.47 for Narrowband Emitters in the Subaru Deep Field
- C. LyM. Malkan K. Motohara
- 1 June 2006
Physics
SDF line-emitting galaxies in four narrowband filters at low and intermediate redshifts are presented. Broadband colors, follow-up optical spectroscopy, and multiple NB filters are used to…
The First Release COSMOS Optical and Near-IR Data and Catalog
- P. CapakH. Aussel G. Zamorani
- 19 April 2007
Physics
Panchromatic number counts are constructed which confirm that both the geometry of the universe and the galaxy population are evolving and that both Stellar and galaxy colors and counts agree well with the expected values.
A Subaru Search for Lyα Blobs in and around the Protocluster Region At Redshift z = 3.1
- Y. MatsudaT. Yamada Y. Taniguchi
- 12 May 2004
Physics
We report the properties of 35 robust candidate Lyα blobs (LABs), which are larger than 16 arcsec2 in isophotal area and brighter than 0.7 × 10-16 ergs s-1 cm-2, located in and around the…
The HI content of star-forming galaxies at z = 0.24
- Philip LahJ. Chengalur S. Okamura
- 24 January 2007
Physics
We use observations from the Giant Metrewave Radio Telescope (GMRT) to measure the atomic hydrogen gas content of star-forming galaxies at z = 0.24 (i.e. a look-back time of ∼3 Gyr). The sample of…
COMPLETING THE CENSUS OF Lyα EMITTERS AT THE REIONIZATION EPOCH
- N. KashikawaK. Shimasaku J. Toshikawa
- 12 April 2011
Physics
We carried out extended spectroscopic confirmations of Lyα emitters (LAEs) at z = 6.5 and 5.7 in the Subaru Deep Field. Now, the total number of spectroscopically confirmed LAEs is 45 and 54 at z =…
Metallicity evolution, metallicity gradients, and gas fractions at z ~ 3.4
- P. TroncosoR. Maiolino L. Pentericci
- 18 November 2013
Physics
This work was funded by the Marie Curie Initial Training Network ELIXIR 214227 of the European Commission. We also acknowledge partial support by INAF. Alessandro Marconi acknowledges support from…
The SUBARU Deep Field Project: Lymanα Emitters at a Redshift of 6.6
- Y. TaniguchiM. Ajiki Michitoshi Yoshida
- 27 July 2004
Physics
We present new results of a deep optical imaging survey using a narrow band filter (NB921) centered at λ = 9196 u A together with B, V, R, i � ,a ndzbroadband filters in the sky area of the Subaru…
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