activity
20072023
most citedAT2018cow: a luminous millimeter transient

146 citations · 837 across the 31 of their papers we have counts for

collaborators

32 papers

astro-ph.IM2023★ 70 cited

The ALMA Interferometric Pipeline Heuristics

Todd R. Hunter, Remy Indebetouw, Crystal L. Brogan +25

We describe the calibration and imaging heuristics developed and deployed in the ALMA interferometric data processing pipeline, as of ALMA Cycle 9. The pipeline software framework…

astro-ph.GA2023★ 12 cited

A Candidate Dual QSO at Cosmic Noon

Eilat Glikman, Rachel Langgin, Makoto A. Johnstone +6

We report the discovery of a candidate dual QSO at z=1.889, a redshift that is in the era known as "cosmic noon" where most of the Universe's black hole and stellar mass growth occ…

astro-ph.GA2023★ 11 cited

The SUPERCOLD-CGM survey: \\ I. Probing the extended CO(4-3) Emission of the Circumglactic medium in a sample of 10 Enormous Ly Nebulae at

Jianrui Li, Bjorn H. C. Emonts, Zheng Cai +10

To understand how massive galaxies at high- co-evolve with enormous reservoirs of halo gas, it is essential to study the coldest phase of the circum-galactic medium (CGM), which…

astro-ph.GA2023★ 29 cited

A cosmic stream of atomic carbon gas connected to a massive radio galaxy at redshift 3.8

Bjorn H. C. Emonts, Matthew D. Lehnert, Ilsang Yoon +7

The growth of galaxies in the early Universe is driven by accretion of circum- and inter-galactic gas. Simulations predict that steady streams of cold gas penetrate the dark matter…

astro-ph.GA2022★ 5 cited

ALMA FIR View of Ultra High-redshift Galaxy Candidates at 11-17: Blue Monsters or Low- Red Interlopers?

Seiji Fujimoto, Steven L. Finkelstein, Denis Burgarella +50

We present ALMA Band~7 observations of a remarkably bright galaxy candidate at = (=), S5-z17-1, identified in JWST Early Releas…

astro-ph.GA2022★ 22 cited

ALMA Observation of a Galaxy Candidate Discovered with JWST

Ilsang Yoon, Christopher L. Carilli, Seiji Fujimoto +12

We report the ALMA observation of a galaxy candidate (GHZ1) discovered from the GLASS-JWST Early Release Science Program. Our ALMA program aims to detect the [OIII] em…