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19982026
most citedThe Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample

1.7k citations · 19k across the 253 of their papers we have counts for

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Showing 2009 · astro-ph.COShow all

5 papers · 2 filters

astro-ph.CO2009★ 20 cited

Subaru FOCAS Spectroscopic Observations of High-Redshift Supernovae

Tomoki Morokuma, Kouichi Tokita, Christopher Lidman +30

We present spectra of high-redshift supernovae (SNe) that were taken with the Subaru low resolution optical spectrograph, FOCAS. These SNe were found in SN surveys with Suprime-Cam…

astro-ph.CO2009★ 292 cited

Large Area Survey for z=7 Galaxies in SDF and GOODS-N: Implications for Galaxy Formation and Cosmic Reionization

Masami Ouchi, Bahram Mobasher, Kazuhiro Shimasaku +10

We present results of our large-area survey for z'-band dropout galaxies at z=7 in a 1568 arcmin^2 sky area covering the SDF and GOODS-N fields. Combining our ultra-deep Subaru/Sup…

astro-ph.CO2009★ 36 cited

Lyman Break Galaxies at z~1.8-2.8: GALEX/NUV Imaging of the Subaru Deep Field

Chun Ly, Matthew A. Malkan, Tommaso Treu +7

Abridged: A photometric sample of ~7100 V<25.3 Lyman break galaxies (LBGs) has been selected by combining Subaru/Suprime-Cam BVRci'z' data with deep GALEX/NUV imaging of the Subaru…

astro-ph.CO2009★ 59 cited

Subaru Mid-infrared Imaging of the Quadruple Lenses. II. Unveiling Lens Structure of MG0414+0534 and Q2237+030

Takeo Minezaki, Masashi Chiba, Nobunari Kashikawa +2

We present mid-infrared imaging at 11.7 m for the quadruple lens systems, MG0414+0534 and Q2237+030, using the cooled mid-infrared camera and spectrometer (COMICS) attached on t…

astro-ph.CO2009★ 5 cited

Photometric H alpha and [O II] Luminosity Function of SDF and SXDF Galaxies: Implications for Future Baryon Oscillation Surveys

Masanao Sumiyoshi, Tomonori Totani, Shunsuke Oshige +9

Efficient selection of emission line galaxies at z > 1 by photometric information in wide field surveys is one of the keys for future spectroscopic surveys to constrain dark energy…