activity
20142023
most citedPrime Focus Spectrograph (PFS) for the Subaru Telescope: Overview, recent progress, and future perspectives

149 citations · 598 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR20231 cited

Semi-analytic calculations for extended mid-Infrared emission associated with FU Ori-type objects

Michihiro Takami, Pin-Gao Gu, Gilles Otten +4

(Aims) Near-infrared imaging polarimetry at high-angular resolutions has revealed intriguing distribution of circumstellar dust towards FU Ori-type objects (FUors). These dust grai…

astro-ph.GA202364 cited

Quasar Luminosity Function at z = 7

Yoshiki Matsuoka, Masafusa Onoue, Kazushi Iwasawa +41

We present the quasar luminosity function (LF) at , measured with 35 spectroscopically confirmed quasars at . The sample of 22 quasars from the Subaru High-…

astro-ph.EP202357 cited

The two rings of (50000) Quaoar

C. L. Pereira, B. Sicardy, B. E. Morgado +66

Quaoar is a classical Trans-Neptunian Object (TNO) with an area equivalent diameter of 1,100 km and an orbital semi-major axis of 43.3 astronomical units. Based on stellar occultat…

astro-ph.CO20238 cited

Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Emulator Based Halo Model

Hironao Miyatake, Sunao Sugiyama, Masahiro Takada +31

We present cosmology results from a blinded joint analysis of cosmic shear, , galaxy-galaxy weak lensing, , and projected galaxy clustering, $w_{\rm p}…

astro-ph.SR202213 cited

Investigating the stability of mass transfer in neutron star-helium white dwarf binaries

Hai-Liang Chen, Thomas M. Tauris, Xuefei Chen +1

Neutron star-helium white dwarf (NS+He WD) binaries are important evolutionary products of close-orbit binary star systems. They are often observed as millisecond pulsars and may c…

astro-ph.EP2021

Col-OSSOS: Probing Ice Line/Color Transitions within the Kuiper Belt's Progenitor Populations

Laura E. Buchanan, Megan E. Schwamb, Wesley C. Fraser +15

Dynamically excited objects within the Kuiper belt show a bimodal distribution in their surface colors, and these differing surface colors may be a tracer of where these objects fo…