activity
20152026
most citedGravitational Lensing Size Scales for Quasars

78 citations · 261 across the 35 of their papers we have counts for

collaborators

39 papers

astro-ph.GA2026

Cool Embeddings: Predicting Galaxy Cluster Cooling Times in IllustrisTNG and TNG-Cluster with AstroCLIP

Rawan Karam, Carter Lee Rhea, Julie Hlavacek-Larrondo +4

Foundation models trained on optical astronomical data have not previously been applied to X-ray cluster thermodynamics. We show that embeddings from AstroCLIP, a contrastive visio…

astro-ph.IM2026

Simultaneous PSF Matching via Dual Kernel Optimization

Carter Lee Rhea, Pieter Van Dokkum, Roberto Abraham +6

Standard point spread function (PSF) matching algorithms consider one image as the reference and aim to find a convolution kernel such that, when applied to the reference image, th…

astro-ph.HE2026

Using CFHT's SITELLE to Probe the Long-Sought Supernova Remnant Shell in the Crab Nebula

Lucas V. da Conceição, Janette Suherli, Samar Safi-Harb +3

We present deep, wide-field integral field spectroscopy of the Crab nebula obtained with the imaging Fourier transform spectrometer SITELLE at the Canada--France--Hawaii Telescope…

astro-ph.GA2026

High-spectral-resolution Observations of the [S II] Emission-line Doublet in the Filamentary Nebula Surrounding NGC 1275

Benjamin Vigneron, Julie Hlavacek-Larrondo, Carter Lee Rhea +10

We analyze new high-spectral resolution SITELLE observations (R = = 7000) of the filamentary nebula surrounding NGC 1275, central galaxy of the Perseus cluster. We present h…

astro-ph.SR2026

Numerous bow shocks in the outer Helix Nebula

Pieter van Dokkum, Roberto Abraham, William P. Bowman +5

Near the end of their lives, low- and intermediate-mass stars expel metal-enriched material in winds and outflows, ultimately producing planetary nebulae (PNe). The ejected materia…

astro-ph.GA2026

Mapping Gas Accretion and Stellar Kinematics to Sub-kiloparsec Scales in NGC 4696 with JWST/NIRSpec

Mathieu Marquis, Julie Hlavacek-Larrondo, Olivia Pereira +35

We present JWST/NIRSpec IFU spectroscopy of the central pc () of NGC 4696, the BCG in the Centaurus cluster. Leveraging the (…

astro-ph.GA2026

JWST reveals how black holes are fed: kiloparsec-scale multiphase filaments feed sub-kiloparsec circumnuclear disks

Julie Hlavacek-Larrondo, Hyunseop Choi, Minghao Guo +35

The Centaurus cluster is one of the most important archetypes of radio-mode AGN feedback, with its central galaxy, NGC 4696, launching powerful jets that inflate X-ray cavities and…

astro-ph.IM2026

dfcosmic: A Python package for cosmic ray removal

Carter Lee Rhea, Pieter van Dokkum, Steven R. Janssens +5

Astronomical images often show sharp features that are caused by cosmic ray (CR) hits, hot pixels, or non-Gaussian noise. L.A.Cosmic (van Dokkum 2001) is a widely used edge detecti…

astro-ph.CO2025

Discovery of Diffuse Radio Emission in a Massive z=1.709 Cool Core Cluster: A Candidate Radio Mini-Halo

Julie Hlavacek-Larrondo, Roland Timmerman, Christoph Pfrommer +10

Clusters of galaxies host spectacular diffuse radio sources, extending over scales from 100 kpc to several Mpcs. These sources, with extremely faint surface brightness (Jy/arcse…

astro-ph.IM2025

dfreproject: A Python package for astronomical reprojection

Carter Lee Rhea, Pieter Van Dokkum, Steven R. Janssens +5

Deep astronomical images are often constructed by digitially stacking many individual sub-exposures. Each sub-exposure is expected to show small differences in the positions of sta…

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

Mapping the Filamentary Nebula of NGC 1275 with Multiwavelength SITELLE Observations

Carter Lee Rhea, Julie Hlavacek-Larrondo, Marie-Lou Gendron-Marsolais +11

The filamentary nebula encompassing the central galaxy of the Perseus Cluster, NGC 1275, is a complex structure extending dozens of kiloparsecs from NGC 1275. Decades of previous w…

astro-ph.GA2025

HST Observations within the Sphere of Influence of the Powerful Supermassive Black Hole in PKS0745-191

Julie Hlavacek-Larrondo, Hyunseop Choi, Minghao Guo +18

We present Space Telescope Imaging Spectrograph observations from the Hubble Space Telescope of the supermassive black hole (SMBH) at the center of PKS0745-191, a brightest cluster…

astro-ph.GA2024

A novel approach to understanding the link between supermassive black holes and host galaxies

Gabriel Sasseville, Julie Hlavacek-Larrondo, Samantha C. Berek +5

The strongest and most universal scaling relation between a supermassive black hole and its host galaxy is known as the relation, where is the mass of the…

astro-ph.GA2024

Deconvolving X-ray Galaxy Cluster Spectra Using a Recurrent Inference Machine

Carter Rhea, Julie Hlavacek-Larrondo, Alexandre Adam +4

Recent advances in machine learning algorithms have unlocked new insights in observational astronomy by allowing astronomers to probe new frontiers. In this article, we present a m…

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

Reconstructing Robust Background IFU spectra using Machine Learning

Carter Lee Rhea, Julie Hlavacek-Larrondo, Justine Giroux +6

In astronomy, spectroscopy consists of observing an astrophysical source and extracting its spectrum of electromagnetic radiation. Once extracted, a model is fit to the spectra to…

astro-ph.GA2023★ 1 cited

Unraveling the Mysteries of Galaxy Clusters: Recurrent Inference Deconvolution of X-ray Spectra

Carter Rhea, Julie Hlavacek-Larrondo, Ralph Kraft +3

In the realm of X-ray spectral analysis, the true nature of spectra has remained elusive, as observed spectra have long been the outcome of convolution between instrumental respons…

astro-ph.GA2023★ 13 cited

High-Spectral Resolution Observations of the Optical Filamentary Nebula in NGC 1275

Benjamin Vigneron, Julie Hlavacek-Larrondo, Carter Lee Rhea +18

We present new high-spectral resolution observations (R = = 7000) of the filamentary nebula surrounding NGC 1275, the central galaxy of the Perseus cluster. These observatio…

astro-ph.IM2023★ 3 cited

Rapid Spectral Parameter Prediction for Black Hole X-Ray Binaries using Physicalised Autoencoders

Ethan Tregidga, James Steiner, Cecilia Garraffo +2

Black hole X-ray binaries (BHBs) offer insights into extreme gravitational environments and the testing of general relativity. The X-ray spectrum collected by NICER offers valuable…

astro-ph.GA2023

A Machine Learning Approach to Galactic Emission-Line Region Classification

Carter Lee Rhea, Laurie Rousseau-Nepton, Ismael Moumen +13

Diagnostic diagrams of emission-line ratios have been used extensively to categorize extragalactic emission regions; however, these diagnostics are occasionally at odds with each o…

astro-ph.GA2023★ 9 cited

Constraining the LyC escape fraction from LEGUS star clusters with SIGNALS HII region observations: A pilot study of NGC 628

J. W. Teh, K. Grasha, M. R. Krumholz +23

The ionising radiation of young and massive stars is a crucial form of stellar feedback. Most ionising (Lyman-continuum; LyC, ) photons are absorbed close to the stars tha…

astro-ph.GA2023★ 6 cited

Extended Line Emission in the BCG of Abell 2390

Leo Y. Alcorn, H. K. C Yee, Laurent Drissen +10

We report CFHT/SITELLE imaging Fourier Transform Spectrograph observations of the Brightest Cluster Galaxy (BCG) of galaxy cluster Abell 2390 at z=0.228. The BCG displays a promine…

astro-ph.EP2022★ 5 cited

The First High-Contrast Images of X-Ray Binaries: Detection of Candidate Companions in the Cas Analog RX J1744.72713

M. Prasow-Émond, J. Hlavacek-Larrondo, K. Fogarty +16

X-ray binaries provide exceptional laboratories for understanding the physics of matter under the most extreme conditions. Until recently, there were few, if any, observational con…