activity
20182026
most citedSIGNALS: I. Survey Description

64 citations · 239 across the 18 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2026

JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf

Tamás Szalai, Dan Milisavljevic, Noah Zimmer +22

Supernova (SN) 2026sqf recently appeared in the nearby face-on spiral galaxy NGC 3310 and has shown signs of strong interaction with a circumstellar medium (CSM). Such intense inte…

astro-ph.GA2026

An automated method for planetary nebula detection with SIGNALS: first applications to NGC 4214 and NGC 4449

Nancy Yang, Johanna Hartke, Martin Bureau +11

Utilising the optical imaging Fourier transform spectrograph SITELLE, the Star-formation, Ionized Gas and Nebular Abundances Legacy Survey (SIGNALS) is designed to study the connec…

astro-ph.GA2026

WISDOM Project -- XXVIII. Molecular gas measurement of the supermassive black hole mass of the galaxy NGC 1387

Pandora Dominiak, Martin Bureau, Fu-Heng Liang +6

Supermassive black hole (SMBH) masses can be measured using molecular gas kinematics. Here we present high angular resolution ( arcsec or pc) Atacama Large Millim…

astro-ph.GA2026

Stellar-mass black holes on the millimetre fundamental plane of black hole accretion

Jacob S. Elford, Ilaria Ruffa, Timothy A. Davis +5

Recent work revealed the existence of a galaxy "millimetre fundamental plane of black hole accretion", a tight correlation between nuclear mm luminosity, intrinsic - keV…

astro-ph.GA2025

Neural Deprojection of Galaxy Stellar Mass Profiles

M. J. Yantovski-Barth, Hengyue Zhang, Nolan Smyth +4

We introduce a neural approach to dynamical modeling of galaxies that replaces traditional imaging-based deprojections with a differentiable mapping. Specifically, we train a neura…

astro-ph.GA2025

WISDOM Project -- XXV. Improving the CO-dynamical supermassive black hole mass measurement in the galaxy NGC 1574 using high spatial resolution ALMA observations

Hengyue Zhang, Martin Bureau, Ilaria Ruffa +5

We present a molecular gas dynamical supermassive black hole (SMBH) mass measurement in the nearby barred lenticular galaxy NGC 1574, using Atacama Large Millimeter/sub-millimeter…

astro-ph.GA2025

WISDOM project -- XXIII. Star-formation efficiencies of eight early-type galaxies and bulges observed with SITELLE and ALMA

Anan Lu, Daryl Haggard, Martin Bureau +18

Early-type galaxies (ETGs) are known to harbour dense spheroids of stars with scarce star formation (SF). Approximately a quarter of these galaxies have rich molecular gas reservoi…

astro-ph.GA2025

The resolved star-formation efficiency of early-type galaxies

Thomas G. Williams, Francesco Belfiore, Martin Bureau +19

Understanding how and why star formation varies between galaxies is fundamental to our comprehension of galaxy evolution. In particular, the star-formation efficiency (SFE; star-fo…

astro-ph.GA2025★ 5 cited

WISDOM Project -- XXII. A 5% precision CO-dynamical supermassive black hole mass measurement in the galaxy NGC 383

Hengyue Zhang, Martin Bureau, Ilaria Ruffa +8

We present a measurement of the supermassive black hole (SMBH) mass of the nearby lenticular galaxy NGC 383, based on Atacama Large Millimeter/sub-millimeter Array (ALMA) observati…

astro-ph.GA2024★ 1 cited

WISDOM project XX -- Strong shear tearing molecular clouds apart in NGC 524

Anan Lu, Daryl Haggard, Martin Bureau +17

Early-type galaxies (ETGs) are known to harbour dense spheroids of stars but scarce star formation (SF). Approximately a quarter of these galaxies have rich molecular gas reservoir…

astro-ph.GA2024

WISDOM Project -- XXI. Giant molecular clouds in the central region of the barred spiral galaxy NGC 613: a steep size -- linewidth relation

Woorak Choi, Martin Bureau, Lijie Liu +9

NGC~613 is a nearby barred spiral galaxy with a nuclear ring. Exploiting high spatial resolution ( pc) Atacama Large Millimeter/sub-millimeter Array CO(1-0) obser…

astro-ph.GA2024★ 5 cited

WISDOM Project -- XIX. Figures of merit for supermassive black hole mass measurements using molecular gas and/or megamaser kinematics

Hengyue Zhang, Martin Bureau, Mark D. Smith +7

The mass () of a supermassive black hole (SMBH) can be measured using spatially-resolved kinematics of the region where the SMBH dominates gravitationally. The most…

astro-ph.GA2024

WISDOM Project -- XXVI. Cross-checking supermassive black hole mass estimates from ALMA CO gas kinematics and SINFONI stellar kinematics in the galaxy NGC 4751

Pandora Dominiak, Michele Cappellari, Martin Bureau +6

We present high angular resolution ( or pc) ALMA observations of the CO(3-2) line emission of the galaxy NGC 4751. The data provide evidence for the pres…

astro-ph.GA2020★ 51 cited

JINGLE -- IV. Dust, HI gas and metal scaling laws in the local Universe

I. De Looze, I. Lamperti, A. Saintonge +29

Scaling laws of dust, HI gas and metal mass with stellar mass, specific star formation rate and metallicity are crucial to our understanding of the buildup of galaxies through thei…

astro-ph.GA2019★ 64 cited

SIGNALS: I. Survey Description

L. Rousseau-Nepton, R. P. Martin, C. Robert +60

SIGNALS, the Star formation, Ionized Gas, and Nebular Abundances Legacy Survey, is a large observing program designed to investigate massive star formation and HII regions in a sam…

astro-ph.GA2019★ 38 cited

The MBHBM* Project -- I: Measurement of the Central Black Hole Mass in Dwarf Galaxy NGC 3504 Using Molecular Gas Kinematics

Dieu D. Nguyen, Mark den Brok, Anil C. Seth +19

We present the first measurement of the mass of a supermassive black hole (SMBH) in the nearby double-barred spiral galaxy NGC 3504 as part of the Measuring Black Holes Below the M…

astro-ph.GA2018★ 24 cited

Dust properties in the cold and hot gas phases of the ATLAS3D early-type galaxies as revealed by AKARI

T. Kokusho, H. Kaneda, M. Bureau +6

The properties of the dust in the cold and hot gas phases of early-type galaxies (ETGs) are key to understand ETG evolution. We thus conducted a systematic study of the dust in a l…