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20112026
most citedCOSMOS2020: A panchromatic view of the Universe to from two complementary catalogs

485 citations · 3.2k across the 61 of their papers we have counts for

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7 papers · 1 filter

astro-ph.GA2022★ 147 cited

EIGER I. a large sample of [OIII]-emitting galaxies at and direct evidence for local reionization by galaxies

Daichi Kashino, Simon J. Lilly, Jorryt Matthee +4

We present a first sample of 117 [OIII]4960,5008-selected star-forming galaxies at detected in JWST/NIRCam 3.5m slitless spectroscopy of a …

astro-ph.GA2022★ 51 cited

EIGER III. JWST/NIRCam observations of the ultra-luminous high-redshift quasar J0100+2802

Anna-Christina Eilers, Robert A. Simcoe, Minghao Yue +6

We present the first rest-frame optical spectrum of a high-redshift quasar observed with JWST/NIRCam in Wide Field Slitless (WFSS) mode. The observed quasar, J0100+2802, is the mos…

astro-ph.GA2022★ 162 cited

EIGER II. first spectroscopic characterisation of the young stars and ionised gas associated with strong H and [OIII] line-emission in galaxies at z=5-7 with JWST

Jorryt Matthee, Ruari Mackenzie, Robert A. Simcoe +4

We present emission-line measurements and physical interpretations for a sample of 117 [OIII] emitting galaxies at , using the first deep JWST/NIRCam wide field slitle…

astro-ph.GA2022★ 4 cited

Galaxy Manifold: Characterizing and understanding galaxies with two parameters

Suchetha Cooray, Tsutomu T. Takeuchi, Daichi Kashino +3

We report the discovery of a two-dimensional Galaxy Manifold within the multi-dimensional luminosity space of local galaxies. The multi-dimensional luminosity space is constructed…

astro-ph.GA2022★ 5 cited

Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering

Shogo Masaki, Daichi Kashino, Shogo Ishikawa +1

We propose a novel subhalo abundance matching (SHAM) model that uses the virial mass of the main progenitor of each (sub)halo as a proxy of the galaxy stellar mass $…

astro-ph.GA2022★ 18 cited

The physical origin for spatially large scatter of IGM opacity at the end of reionization: the IGM Ly opacity-galaxy density relation

Rikako Ishimoto, Nobunari Kashikawa, Daichi Kashino +9

The large opacity fluctuations in the Ly forest may indicate inhomogeneous progress of reionization. To explain the observed large scatter of the effective Ly optic…

astro-ph.CO2022★ 32 cited

Predicted future fate of COSMOS galaxy protoclusters over 11 Gyr with constrained simulations

Metin Ata, Khee-Gan Lee, Claudio Dalla Vecchia +5

Cosmological simulations are crucial tools in studying the Universe, but they typically do not directly match real observed structures. Constrained cosmological simulations, on the…