activity
20062009
most citedA calibration of the relation between the abundance of close galaxy pairs and the rate of galaxy mergers

208 citations · 658 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.CO20091 cited

HST/ACS Morphology of Lyman Alpha Emitters at Redshift 5.7 in the COSMOS Field

Y. Taniguchi, T. Murayama, N. Z. Scoville +28

We present detailed morphological properties of Lyman alpha emitters (LAEs) at z~ 5.7 in the COSMOS field, based on {\it Hubble Space Telescope} Advanced Camera for Surveys (ACS) d…

astro-ph2008208 cited

A calibration of the relation between the abundance of close galaxy pairs and the rate of galaxy mergers

Manfred G. Kitzbichler, Simon D. M. White

Estimates of galaxy merger rates based on counts of close pairs typically assume that most of the observed systems will merge within a few hundred Myr (for projected pair separatio…

astro-ph2007117 cited

The Dependence of Galaxy Formation on Cosmological Parameters: Can we distinguish the WMAP1 and WMAP3 Parameter Sets?

Jie Wang, Gabriella De Lucia, Manfred G. Kitzbichler +1

We combine N-body simulations of structure growth with physical modelling of galaxy evolution to investigate whether the shift in cosmological parameters between the 1-year and 3-y…

astro-ph200764 cited

The angular correlations of galaxies in the COSMOS field

H. J. McCracken, J. A. Peacock, L. Guzzo +21

We present measurements of the two-point galaxy angular correlation function w(θ) in the COSMOS field. Independent determinations of w(θ) as a function of magnitude limit are prese…

astro-ph200755 cited

The [OII]3727 Luminosity function and Star Formation Rate at z~1.2 in the COSMOS 2 Square-degree Field and the Subaru Deep Field

M. I. Takahashi, Y. Shioya, Y. Taniguchi +31

We have carried out a wide-field imaging survey for [OII]3727 emitting galaxies at z~1.2 in the HST COSMOS 2 square degree field using the Suprime-Cam on the Subaru Telescope. The…

astro-ph2007107 cited

Lyman Alpha Emitters at Redshift 5.7 in the COSMOS Field

T. Murayama, Y. Taniguchi, N. Z. Scoville +24

We present results from a narrow-band optical survey of a contiguous area of 1.95 deg^2, covered by the Cosmic Evolution Survey (COSMOS). Both optical narrow-band (lambda_c = 8150…