Showing 1–20 of 37 results
/ Date/ Name
Nov 26, 2020A puzzling non-detection of [O III] and [C II] from a $z \approx 7.7$ galaxy observed with ALMAMay 16, 2013A statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveysAug 30, 2011Dissecting Photometric redshift for Active Galactic Nuclei using XMM- and Chandra-COSMOS samplesMar 6, 2009Universality of the Nf=2 Running CouplingOct 3, 2008Chasing highly obscured QSOs in the COSMOS fieldMay 16, 2007Evolution of the Frequency of Luminous (\geq L_V*) Close Galaxy Pairs at z < 1.2 in the COSMOS FieldDec 14, 2006The XMM-Newton wide-field survey in the COSMOS field. IV: X-ray spectral properties of Active Galactic NucleiApr 6, 2006The End of the Reionization Epoch Probed by Ly-alpha Emitters at z=6.5 in the Subaru Deep FieldFeb 28, 2006Ly Alpha Emitters at z=5.7 in the Subaru Deep FieldAug 31, 2005Nonperturbative $O(a)$ improvement of the Wilson quark action with the RG-improved gauge action using the Schrödinger functional methodSep 30, 2004The Subaru Deep Field: The Optical Imaging DataSep 18, 2004A scaling study of the step scaling function of quenched QCD with improved gauge actionsAug 13, 2004A Strong Lyman-alpha Emitter at z=6.33 in the Subaru Deep Field Selected as an i' DropoutAug 9, 2004A scaling study of the step scaling function in SU(3) gauge theory with improved gauge actionsJul 27, 2004The Subaru Deep Field Project: Lyman$α$ Emitters at Redshift of 6.6Apr 30, 2004Non-perturbative renormalization of meson decay constants in quenched QCD for a renormalization group improved gauge actionSep 30, 2003Non-perturbative renormalization of vector and axial vector currents in quenched QCD for a renormalization group improved gauge actionSep 24, 2003I=2 pion-pion scattering phase shift in the continuum limit calculated with two-flavor full QCDFeb 22, 2003Subaru Deep Survey. IV. Discovery of a Large-Scale Structure at Redshift \simeq 5Jan 7, 2003The Discovery of Two Lyman$α$ Emitters Beyond Redshift 6 in the Subaru Deep Field