Search Results - "Haggard, Daryl"
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The Analogous Structure of Accretion Flows in Supermassive and Stellar Mass Black Holes: New Insights from Faded Changing-look Quasars
Published in The Astrophysical journal (20-09-2019)“…Despite their factor of ∼108 difference in black hole mass, several lines of evidence suggest possible similarities between black hole accretion flows in…”
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Chandra Study of the Proper Motion of HST-1 in the Jet of M87
Published in The Astrophysical journal (01-07-2024)“…Abstract The radio galaxy M87 is well known for its jet, which features a series of bright knots observable from radio to X-ray wavelengths. We analyze the…”
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KilonovAE: Exploring Kilonova Spectral Features with Autoencoders
Published in The Astrophysical journal (01-01-2024)“…Abstract Kilonovae are likely a key site of heavy r -process element production in the Universe, and their optical/infrared spectra contain insights into both…”
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Simulation-based Inference of Radio Millisecond Pulsars in Globular Clusters
Published in The Astrophysical journal (01-10-2024)“…Abstract Millisecond pulsars (MSPs) are abundant in globular clusters (GCs), which offer favorable environments for their creation. While the advent of recent,…”
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Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations. I. Unique Galaxy Morphologies in Imaging
Published in The Astrophysical journal (01-01-2024)“…Abstract Low-frequency gravitational-wave experiments such as the Laser Interferometer Space Antenna and pulsar timing arrays are expected to detect individual…”
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Spectroscopic r-process Abundance Retrieval for Kilonovae. II. Lanthanides in the Inferred Abundance Patterns of Multicomponent Ejecta from the GW170817 Kilonova
Published in The Astrophysical journal (01-02-2024)“…Abstract In kilonovae, freshly synthesized r -process elements imprint features on optical spectra, as observed in AT2017gfo, the counterpart to the GW170817…”
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Spectroscopic r-Process Abundance Retrieval for Kilonovae. I. The Inferred Abundance Pattern of Early Emission from GW170817
Published in The Astrophysical journal (01-02-2023)“…Abstract Freshly synthesized r -process elements in kilonovae ejecta imprint absorption features on optical spectra, as observed in the GW170817 binary neutron…”
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A Deep CFHT Optical Search for a Counterpart to the Possible Neutron Star-Black Hole Merger GW190814
Published in The Astrophysical journal (01-06-2020)“…We present a wide-field optical imaging search for electromagnetic counterparts to the likely neutron star-black hole (NS-BH) merger GW190814/S190814bv. This…”
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Explaining the GWSkyNet-Multi Machine Learning Classifier Predictions for Gravitational-wave Events
Published in The Astrophysical journal (01-03-2024)“…Abstract GWSkyNet-Multi is a machine learning model developed for the classification of candidate gravitational-wave events detected by the LIGO and Virgo…”
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Multistructured Accretion Flow of Sgr A. II. Signatures of a Cool Accretion Disk in Hydrodynamic Simulations of Stellar Winds
Published in The Astrophysical journal (01-10-2024)“…Abstract Hydrodynamic simulations of the stellar winds from Wolf–Rayet stars within the Galactic center can provide predictions for the X-ray spectrum of the…”
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Multistructured Accretion Flow of Sgr A. I. Examination of a Radiatively Inefficient Accretion Flow Model
Published in The Astrophysical journal (01-10-2024)“…Abstract The extreme low-luminosity supermassive black hole Sgr A* provides a unique laboratory in which to test models of radiatively inefficient accretion…”
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Radio Scrutiny of the X-Ray-weak Tail of Low-mass Active Galactic Nuclei: A Novel Signature of High-Eddington Accretion?
Published in The Astrophysical journal (01-10-2024)“…Abstract The supermassive black holes ( M BH ∼ 10 6 –10 10 M ⊙ ) that power luminous active galactic nuclei (AGNs), i.e., quasars, generally show a correlation…”
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GWSkyNet. II. A Refined Machine-learning Pipeline for Real-time Classification of Public Gravitational Wave Alerts
Published in The Astrophysical journal (01-09-2024)“…Electromagnetic follow-up observations of gravitational wave events offer critical insights and provide significant scientific gain from this new class of…”
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Chandra Spectral and Timing Analysis of Sgr A's Brightest X-Ray Flares
Published in The Astrophysical journal (01-12-2019)“…We analyze the two brightest Chandra X-ray flares detected from Sagittarius A*, with peak luminosities more than 600× and 245× greater than the quiescent X-ray…”
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Monitoring observations of SMC X-1’s excursions (MOOSE) – II. A new excursion accompanies spin-up acceleration
Published in Monthly notices of the Royal Astronomical Society (15-02-2023)“…ABSTRACT SMC X-1 is a high-mass X-ray binary showing superorbital modulation with an unstable period. Previous monitoring shows three excursion events in…”
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Gemini Imaging of the Host Galaxies of Changing-look Quasars
Published in The Astrophysical journal (01-05-2019)“…Changing-look (CL) quasars are a newly discovered class of luminous active galactic nuclei that undergo rapid ( 10 yr) transitions between Type 1 and Type…”
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Simultaneous Monitoring of X-Ray and Radio Variability in Sagittarius A
Published in The Astrophysical journal (10-08-2017)“…Monitoring of Sagittarius A* from X-ray to radio wavelengths has revealed structured variability-including X-ray flares-but it is challenging to establish…”
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Prospects for Time-Domain and Multi-Messenger Science with AXIS
Published in Universe (Basel) (01-08-2024)“…The Advanced X-ray Imaging Satellite (AXIS) promises revolutionary science in the X-ray and multi-messenger time domain. AXIS will leverage excellent spatial…”
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Speedy stars blow the cover of hidden black hole
Published in Nature (London) (11-07-2024)“…Fast-moving stars have been discovered in the middle of the nearby star cluster ω Centauri using two decades of Hubble Space Telescope imaging. The stars offer…”
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Black hole goes with the flow
Published in Nature (London) (10-01-2019)“…First you would hear the sound of each drip, and then you would hear an echo when each sound bounces off the cave walls. The authors found that particular…”
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