activity
20172022
most citedThe MUSE Extremely Deep Field: the Cosmic Web in Emission at High Redshift

77 citations · 314 across the 9 of their papers we have counts for

collaborators

24 papers

astro-ph.GA202244 cited

Equivalent widths of Lyman emitters in MUSE-Wide and MUSE-Deep

J. Kerutt, L. Wisotzki, A. Verhamme +15

The aim of this study is to better understand the connection between the Lyman rest-frame equivalent width (EW) and spectral properties as well as ultraviolet (UV) continuu…

astro-ph.GA2021

Catch Me if You Can: Biased Distribution of Ly-emitting Galaxies according to the Viewing Direction

Rieko Momose, Kazuhiro Shimasaku, Kentaro Nagamine +4

We report that Ly-emitting galaxies (LAEs) may not faithfully trace the cosmic web of neutral hydrogen (HI), but their distribution is likely biased depending on the viewing dir…

astro-ph.GA2021

SILVERRUSH X: Machine Learning-Aided Selection of LAEs at , , , , , and from the HSC SSP and CHORUS Survey Data

Yoshiaki Ono, Ryohei Itoh, Takatoshi Shibuya +25

We present a new catalog of Ly emitter (LAE) candidates at , , , , , and that are photometrically selected by the SILVERRUSH program wi…

astro-ph.GA202116 cited

Constraining the cosmic UV background at z>3 with MUSE Lyman-α emission observations

Sofia G. Gallego, Sebastiano Cantalupo, Saeed Sarpas +10

The intensity of the Cosmic UV background (UVB), coming from all sources of ionising photons such as star-forming galaxies and quasars, determines the thermal evolution and ionizat…

astro-ph.CO202111 cited

Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1

Rhythm Shimakawa, Yuichi Higuchi, Masato Shirasaki +8

Subaru Strategic Program with the Hyper-Suprime Cam (HSC-SSP) has proven to be successful with its extremely-wide area coverage in past years. Taking advantages of this feature, we…

astro-ph.CO202177 cited

The MUSE Extremely Deep Field: the Cosmic Web in Emission at High Redshift

Roland Bacon, David Mary, Thibault Garel +29

We report the discovery of diffuse extended Ly-alpha emission from redshift 3.1 to 4.5, tracing cosmic web filaments on scales of 2.5-4 comoving Mpc. These structures have been obs…