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1
Implicit Likelihood Inference of Reionization Parameters from the 21 cm Power Spectrum
Implicit Likelihood Inference of Reionization Parameters from the 21 cm Power Spectrum
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Implicit Likelihood Inference of Reionization Parameters from the 21 cm Power Spectrum

The Astrophysical journal, 2022-07, Vol.933 (2), p.236 [Peer Reviewed Journal]

2022. The Author(s). Published by the American Astronomical Society. ;2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;Attribution ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac778e

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2
A Framework for Obtaining Accurate Posteriors of Strong Gravitational Lensing Parameters with Flexible Priors and Implicit Likelihoods Using Density Estimation
A Framework for Obtaining Accurate Posteriors of Strong Gravitational Lensing Parameters with Flexible Priors and Implicit Likelihoods Using Density Estimation
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A Framework for Obtaining Accurate Posteriors of Strong Gravitational Lensing Parameters with Flexible Priors and Implicit Likelihoods Using Density Estimation

The Astrophysical journal, 2023-01, Vol.943 (1), p.4 [Peer Reviewed Journal]

2023. The Author(s). Published by the American Astronomical Society. ;2023. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aca7c2

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3
Temperature and Differential Emission Measure Profiles in Turbulent Solar Active Region Loops
Temperature and Differential Emission Measure Profiles in Turbulent Solar Active Region Loops
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Temperature and Differential Emission Measure Profiles in Turbulent Solar Active Region Loops

The Astrophysical journal, 2022-11, Vol.939 (1), p.19 [Peer Reviewed Journal]

2022. The Author(s). Published by the American Astronomical Society. ;2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac961b

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4
Structure in the Rotation Measure Sky
Structure in the Rotation Measure Sky
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Structure in the Rotation Measure Sky

The Astrophysical journal, 2011-01, Vol.726 (1), p.4-jQuery1323912087536='47' [Peer Reviewed Journal]

2015 INIST-CNRS ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/726/1/4 ;CODEN: ASJOAB

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5
A ROBUST MEASURE OF DARK MATTER HALO ELLIPTICITIES
A ROBUST MEASURE OF DARK MATTER HALO ELLIPTICITIES
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A ROBUST MEASURE OF DARK MATTER HALO ELLIPTICITIES

Astrophysical journal. Letters, 2016-08, Vol.826 (2), p.L23-L23 [Peer Reviewed Journal]

2016. The American Astronomical Society. All rights reserved. ;ISSN: 2041-8205 ;EISSN: 2041-8213 ;DOI: 10.3847/2041-8205/826/2/L23

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6
High-frequency-peaked BL Lacertae Objects as Spectral Candles to Measure the Extragalactic Background Light in the Fermi and Air Cherenkov Telescopes Era
High-frequency-peaked BL Lacertae Objects as Spectral Candles to Measure the Extragalactic Background Light in the Fermi and Air Cherenkov Telescopes Era
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High-frequency-peaked BL Lacertae Objects as Spectral Candles to Measure the Extragalactic Background Light in the Fermi and Air Cherenkov Telescopes Era

Astrophysical journal. Letters, 2010-05, Vol.715 (1), p.L16-L20 [Peer Reviewed Journal]

ISSN: 2041-8205 ;EISSN: 2041-8213 ;DOI: 10.1088/2041-8205/715/1/L16

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7
Radiation-hydrodynamical Modeling of Core-collapse Supernovae: Light Curves and the Evolution of Photospheric Velocity and Temperature
Radiation-hydrodynamical Modeling of Core-collapse Supernovae: Light Curves and the Evolution of Photospheric Velocity and Temperature
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Radiation-hydrodynamical Modeling of Core-collapse Supernovae: Light Curves and the Evolution of Photospheric Velocity and Temperature

The Astrophysical journal, 2011-11, Vol.741 (1), p.41-jQuery1323902170911='48' [Peer Reviewed Journal]

2015 INIST-CNRS ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/741/1/41 ;CODEN: ASJOAB

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8
Are Coronae of Magnetically Active Stars Heated by Flares? II. Extreme Ultraviolet and X-Ray Flare Statistics and the Differential Emission Measure Distribution
Are Coronae of Magnetically Active Stars Heated by Flares? II. Extreme Ultraviolet and X-Ray Flare Statistics and the Differential Emission Measure Distribution
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Are Coronae of Magnetically Active Stars Heated by Flares? II. Extreme Ultraviolet and X-Ray Flare Statistics and the Differential Emission Measure Distribution

The Astrophysical journal, 2003-01, Vol.582 (1), p.423-442 [Peer Reviewed Journal]

ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1086/344614

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9
Markov-Chain Monte Carlo Reconstruction of Emission Measure Distributions: Application to Solar Extreme-Ultraviolet Spectra
Markov-Chain Monte Carlo Reconstruction of Emission Measure Distributions: Application to Solar Extreme-Ultraviolet Spectra
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Markov-Chain Monte Carlo Reconstruction of Emission Measure Distributions: Application to Solar Extreme-Ultraviolet Spectra

The Astrophysical journal, 1998-08, Vol.503 (1), p.450-466 [Peer Reviewed Journal]

ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1086/305964

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10
A Spectroscopic Model of the Type Ia Supernova–Host-galaxy Mass Correlation from SALT3
A Spectroscopic Model of the Type Ia Supernova–Host-galaxy Mass Correlation from SALT3
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A Spectroscopic Model of the Type Ia Supernova–Host-galaxy Mass Correlation from SALT3

The Astrophysical journal, 2023-07, Vol.951 (1), p.22 [Peer Reviewed Journal]

2023. The Author(s). Published by the American Astronomical Society. ;2023. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;ISSN: 1538-4357 ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/acd195

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11
Supernova Simulations with Boltzmann Neutrino Transport: A Comparison of Methods
Supernova Simulations with Boltzmann Neutrino Transport: A Comparison of Methods
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Supernova Simulations with Boltzmann Neutrino Transport: A Comparison of Methods

The Astrophysical journal, 2005-02, Vol.620 (2), p.840-860 [Peer Reviewed Journal]

2005 INIST-CNRS ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1086/427203 ;CODEN: ASJOAB

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12
Stellar Winds, Dead Zones, and Coronal Mass Ejections
Stellar Winds, Dead Zones, and Coronal Mass Ejections
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Stellar Winds, Dead Zones, and Coronal Mass Ejections

The Astrophysical journal, 2000-02, Vol.530 (2), p.1036-1048 [Peer Reviewed Journal]

ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1086/308395

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13
Thermal and Non-thermal Properties of Active Region Recurrent Coronal Jets
Thermal and Non-thermal Properties of Active Region Recurrent Coronal Jets
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Thermal and Non-thermal Properties of Active Region Recurrent Coronal Jets

The Astrophysical journal, 2022-08, Vol.935 (2), p.172 [Peer Reviewed Journal]

2022. The Author(s). Published by the American Astronomical Society. ;2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac80fb

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14
Neutrino Losses in Type I Thermonuclear X-Ray Bursts: An Improved Nuclear Energy Generation Approximation
Neutrino Losses in Type I Thermonuclear X-Ray Bursts: An Improved Nuclear Energy Generation Approximation
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Neutrino Losses in Type I Thermonuclear X-Ray Bursts: An Improved Nuclear Energy Generation Approximation

The Astrophysical journal, 2019-01, Vol.870 (2), p.64 [Peer Reviewed Journal]

2019. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jan 10, 2019 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aaeed2

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15
MAGNETIC NULL POINTS IN KINETIC SIMULATIONS OF SPACE PLASMAS
MAGNETIC NULL POINTS IN KINETIC SIMULATIONS OF SPACE PLASMAS
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MAGNETIC NULL POINTS IN KINETIC SIMULATIONS OF SPACE PLASMAS

The Astrophysical journal, 2016-03, Vol.819 (1), p.52 [Peer Reviewed Journal]

2016. The American Astronomical Society. All rights reserved. ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-637X ;ISSN: 1538-4357 ;EISSN: 1538-4357 ;DOI: 10.3847/0004-637X/819/1/52

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16
RADIATION-HYDRODYNAMICAL MODELING OF CORE-COLLAPSE SUPERNOVAE: LIGHT CURVES AND THE EVOLUTION OF PHOTOSPHERIC VELOCITY AND TEMPERATURE
RADIATION-HYDRODYNAMICAL MODELING OF CORE-COLLAPSE SUPERNOVAE: LIGHT CURVES AND THE EVOLUTION OF PHOTOSPHERIC VELOCITY AND TEMPERATURE
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RADIATION-HYDRODYNAMICAL MODELING OF CORE-COLLAPSE SUPERNOVAE: LIGHT CURVES AND THE EVOLUTION OF PHOTOSPHERIC VELOCITY AND TEMPERATURE

The Astrophysical journal, 2011-11, Vol.741 (1) [Peer Reviewed Journal]

ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/741/1/41;COUNTRYOFINPUT:INTERNATIONALATOMICENERGYAGENCY(IAEA)

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17
The Variability of Star Formation Rate in Galaxies. II. Power Spectrum Distribution on the Main Sequence
The Variability of Star Formation Rate in Galaxies. II. Power Spectrum Distribution on the Main Sequence
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The Variability of Star Formation Rate in Galaxies. II. Power Spectrum Distribution on the Main Sequence

The Astrophysical journal, 2020-05, Vol.895 (1), p.25 [Peer Reviewed Journal]

2020. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing May 01, 2020 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab8b5e

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18
The Spatial Energy Spectrum of Magnetic Fields in Our Galaxy
The Spatial Energy Spectrum of Magnetic Fields in Our Galaxy
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The Spatial Energy Spectrum of Magnetic Fields in Our Galaxy

The Astrophysical journal, 2004-08, Vol.610 (2), p.820-826 [Peer Reviewed Journal]

2004 INIST-CNRS ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1086/421760 ;CODEN: ASJOAB

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19
V-FASTR: The VLBA Fast Radio Transients Experiment
V-FASTR: The VLBA Fast Radio Transients Experiment
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V-FASTR: The VLBA Fast Radio Transients Experiment

The Astrophysical journal, 2011-07, Vol.735 (2), p.97-jQuery1323906554489='48' [Peer Reviewed Journal]

2015 INIST-CNRS ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/735/2/97 ;CODEN: ASJOAB

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20
How to Obtain the Redshift Distribution from Probabilistic Redshift Estimates
How to Obtain the Redshift Distribution from Probabilistic Redshift Estimates
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How to Obtain the Redshift Distribution from Probabilistic Redshift Estimates

The Astrophysical journal, 2022-04, Vol.928 (2), p.127 [Peer Reviewed Journal]

2022. The Author(s). Published by the American Astronomical Society. ;2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac062f

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