activity
19942023
most citedThe Cosmic Evolution Survey (COSMOS) -- Overview

2k citations · 32.5k across the 221 of their papers we have counts for

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8 papers · 1 filter

astro-ph.IM2022★ 879 cited

The MUSE second-generation VLT instrument

Bacon R., Accardo M., Adjali L. +65

The Multi Unit Spectroscopic Explorer (MUSE) is a second-generation VLT panoramic integral-field spectrograph currently in manufacturing, assembly and integration phase. MUSE has a…

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

Searching for Spectroscopic Signatures of Ongoing Quenching in SDSS Galaxies

Andrea D. Weibel, Enci Wang, Simon J. Lilly

In this paper we estimate the "star formation change parameter", SFR, which characterizes the current SFR relative to the average during the last 800 Myr, for 300'000…

astro-ph.GA2022★ 10 cited

The Similar Signatures of Coplanar Gas Inflow and Disk Warps in Galactic Gas Kinematic Maps

Enci Wang, Simon J. Lilly

Hydrodynamic simulations suggest that galactic gas disks form when coplanar gas spirals into the inner regions of the disk. We recently presented a simple "modified accretion disk"…