Search Results - "Speagle(沈佳士), Joshua S"
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A New Census of the 0.2 < z < 3.0 Universe. II. The Star-forming Sequence
Published in The Astrophysical journal (01-09-2022)“…Abstract We use the panchromatic spectral energy distribution (SED)-fitting code Prospector to measure the galaxy log M *–logSFR relationship (the star-forming…”
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2
Making the sum greater than its parts
Published in Nature astronomy (01-10-2021)“…Without a proper accounting of known and unknown systematics and uncertainties, combining information across multiple surveys, wavelengths, and detectors may…”
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3
Photometric Completeness Modelled with Neural Networks
Published in The Astronomical journal (01-07-2024)“…Abstract In almost any study involving optical/near-infrared photometry, understanding the completeness of detection and recovery is an essential part of the…”
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4
The outer stellar mass of massive galaxies: a simple tracer of halo mass with scatter comparable to richness and reduced projection effects
Published in Monthly notices of the Royal Astronomical Society (13-08-2022)“…ABSTRACT Using the weak gravitational lensing data from the Hyper Suprime-Cam Subaru Strategic Program (HSC survey), we study the potential of different…”
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5
The Stellar Halo of the Galaxy is Tilted and Doubly Broken
Published in The Astronomical journal (01-12-2022)“…Abstract Modern Galactic surveys have revealed an ancient merger that dominates the stellar halo of our galaxy (Gaia–Sausage–Enceladus, GSE). Using chemical…”
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6
The Mass of the Milky Way from the H3 Survey
Published in The Astrophysical journal (01-01-2022)“…Abstract The mass of the Milky Way is a critical quantity that, despite decades of research, remains uncertain within a factor of two. Until recently, most…”
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7
Evidence from Disrupted Halo Dwarfs that r-process Enrichment via Neutron Star Mergers is Delayed by ≳500 Myr
Published in Astrophysical journal. Letters (24-02-2022)“…Abstract The astrophysical origins of r -process elements remain elusive. Neutron star mergers (NSMs) and special classes of core-collapse supernovae (rCCSNe)…”
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Searching for the extra-tidal stars of globular clusters using high-dimensional analysis and a core particle spray code
Published in Monthly notices of the Royal Astronomical Society (01-01-2023)“…ABSTRACT Three-body interactions can eject stars from the core of a globular cluster, causing them to enter the Galactic halo as extra-tidal stars. While…”
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Should Zeros Count? Modeling the Galaxy–Globular Cluster Scaling Relation with(out) Zero-inflated Count Models
Published in The Astrophysical journal (01-09-2024)“…Abstract The scaling relation between the size of a galaxy’s globular cluster (GC) population ( N GC ) and the galaxy’s stellar mass ( M * ) is usually…”
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10
A Tilt in the Dark Matter Halo of the Galaxy
Published in The Astrophysical journal (01-07-2022)“…Abstract Recent observations of the stellar halo have uncovered the debris of an ancient merger, Gaia–Sausage–Enceladus (GSE), estimated to have occurred ≳8…”
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11
Characterizing the 3D Kinematics of Young Stars in the Radcliffe Wave
Published in The Astrophysical journal (01-09-2022)“…Abstract We present an analysis of the kinematics of the Radcliffe Wave, a 2.7 kpc long sinusoidal band of molecular clouds in the solar neighborhood recently…”
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SBI++: Flexible, Ultra-fast Likelihood-free Inference Customized for Astronomical Applications
Published in Astrophysical journal. Letters (01-07-2023)“…Abstract Flagship near-future surveys targeting 10 8 –10 9 galaxies across cosmic time will soon reveal the processes of galaxy assembly in unprecedented…”
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13
On the Robustness of the Velocity Anisotropy Parameter in Probing the Stellar Kinematics in Milky Way–Like Galaxies: Takeaway from TNG50 Simulation
Published in The Astrophysical journal (01-09-2022)“…Abstract We analyze the velocity anisotropy of stars in real and energy space for a sample of Milky Way–like galaxies in the TNG50 simulation. We employ…”
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14
Stochastic Modeling of Star Formation Histories. III. Constraints from Physically Motivated Gaussian Processes
Published in The Astrophysical journal (01-01-2024)“…Abstract Galaxy formation and evolution involve a variety of effectively stochastic processes that operate over different timescales. The extended regulator…”
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15
The First Catalog of Candidate White Dwarf–Main-sequence Binaries in Open Star Clusters: A New Window into Common Envelope Evolution
Published in The Astrophysical journal (01-11-2024)“…Abstract Close binary systems are the progenitors to both Type Ia supernovae and the compact object mergers that can be detected via gravitational waves. To…”
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16
Improving Power Spectrum Estimation Using Multitapering: Efficient Asteroseismic Analyses for Understanding Stars, the Milky Way, and Beyond
Published in The Astronomical journal (01-11-2024)“…Abstract Asteroseismic time series data have imprints of stellar oscillation modes, whose detection and characterization through time series analysis allows us…”
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The Dark Energy Camera Plane Survey 2 (DECaPS2): More Sky, Less Bias, and Better Uncertainties
Published in The Astrophysical journal. Supplement series (01-02-2023)“…Abstract Deep optical and near-infrared imaging of the entire Galactic plane is essential for understanding our Galaxy’s stars, gas, and dust. The second data…”
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The HERBAL Model: A Hierarchical Errors-in-variables Bayesian Lognormal Hurdle Model for Galactic Globular Cluster Populations
Published in The Astrophysical journal (01-09-2023)“…Abstract Galaxy stellar mass is known to be monotonically related to the size of the galaxy’s globular cluster (GC) population for Milky Way sized and larger…”
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Disentangling Stellar Age Estimates from Galactic Chemodynamical Evolution
Published in The Astrophysical journal (01-01-2024)“…Abstract Stellar ages are key for determining the formation history of the Milky Way, but are difficult to measure precisely. Furthermore, methods that use…”
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As Simple as Possible but No Simpler: Optimizing the Performance of Neural Net Emulators for Galaxy SED Fitting
Published in The Astrophysical journal (01-09-2023)“…Abstract Artificial neural network emulators have been demonstrated to be a very computationally efficient method to rapidly generate galaxy spectral energy…”
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