Blakesley Burkhart
#116,286
Most Influential Person
American astrophysicist
Blakesley Burkhart's AcademicInfluence.com Rankings
Physics
#4955
World Rank
#6883
Historical Rank
Cosmology
#338
World Rank
#367
Historical Rank
Astrophysics
#805
World Rank
#900
Historical Rank
Why Is Blakesley Burkhart Influential?
(Suggest an Edit or Addition)According to Wikipedia, Blakesley Burkhart is an astrophysicist. She is the winner of the 2017 Robert J. Trumpler Award awarded by the Astronomical Society of the Pacific, which recognizes a Ph.D. thesis that is "particularly significant to astronomy." She also is the winner of the 2019 Annie Jump Cannon Award in Astronomy and the 2022 winner of The American Physical Society's Maria Goeppert-Mayer Award. The awards both cited her work on magnetohydrodynamic turbulence, and for developing innovative techniques for comparing observable astronomical phenomena with theoretical models.
Blakesley Burkhart's Published Works
Number of citations in a given year to any of this author's works
Total number of citations to an author for the works they published in a given year. This highlights publication of the most important work(s) by the author
Published Papers
- CMB-S4 Science Case, Reference Design, and Project Plan (2019) (327)
- DENSITY STUDIES OF MHD INTERSTELLAR TURBULENCE: STATISTICAL MOMENTS, CORRELATIONS AND BISPECTRUM (2008) (155)
- A unified model for galactic discs: star formation, turbulence driving, and mass transport (2017) (125)
- Low-Mach-number turbulence in interstellar gas revealed by radio polarization gradients (2011) (120)
- CHARACTERIZING MAGNETOHYDRODYNAMIC TURBULENCE IN THE SMALL MAGELLANIC CLOUD (2009) (102)
- Is turbulence in the interstellar medium driven by feedback or gravity? An observational test (2015) (97)
- PROPERTIES OF INTERSTELLAR TURBULENCE FROM GRADIENTS OF LINEAR POLARIZATION MAPS (2011) (66)
- Unveiling the Role of the Magnetic Field at the Smallest Scales of Star Formation (2017) (61)
- The CARMA-NRO Orion Survey (2018) (60)
- The Star Formation Rate in the Gravoturbulent Interstellar Medium (2018) (59)
- Moving-mesh Simulations of Star-forming Cores in Magneto-gravo-turbulence (2017) (58)
- The CAMELS Project: Cosmology and Astrophysics with Machine-learning Simulations (2020) (57)
- The Interaction of Relativistic Spacecrafts with the Interstellar Medium (2016) (52)
- OBSERVATIONAL DIAGNOSTICS OF SELF-GRAVITATING MHD TURBULENCE IN GIANT MOLECULAR CLOUDS (2015) (51)
- MEASURING THE ALFVÉNIC NATURE OF THE INTERSTELLAR MEDIUM: VELOCITY ANISOTROPY REVISITED (2014) (45)
- THE GALFA-H i COMPACT CLOUD CATALOG (2012) (45)
- THE TURBULENCE VELOCITY POWER SPECTRUM OF NEUTRAL HYDROGEN IN THE SMALL MAGELLANIC CLOUD (2015) (45)
- CMB-S4 Decadal Survey APC White Paper (2019) (44)
- THE TURBULENCE POWER SPECTRUM IN OPTICALLY THICK INTERSTELLAR CLOUDS (2013) (38)
- HIERARCHICAL STRUCTURE OF MAGNETOHYDRODYNAMIC TURBULENCE IN POSITION-POSITION-VELOCITY SPACE (2012) (38)
- Galactic interstellar turbulence across the southern sky seen through spatial gradients of the polarization vector (2014) (37)
- The H i-to-H2 Transition in a Turbulent Medium (2017) (37)
- INTERSTELLAR SONIC AND ALFVÉNIC MACH NUMBERS AND THE TSALLIS DISTRIBUTION (2011) (33)
- Statistical Tracing of Magnetic Fields: Comparing and Improving the Techniques (2018) (32)
- THE LOGNORMAL PROBABILITY DISTRIBUTION FUNCTION OF THE PERSEUS MOLECULAR CLOUD: A COMPARISON OF HI AND DUST (2015) (32)
- The Anatomy of the Column Density Probability Distribution Function (N-PDF) (2017) (26)
- THE COLUMN DENSITY VARIANCE– RELATIONSHIP (2012) (26)
- ALFVÉNIC TURBULENCE BEYOND THE AMBIPOLAR DIFFUSION SCALE (2014) (25)
- RADIO SYNCHROTRON FLUCTUATION STATISTICS AS A PROBE OF MAGNETIZED INTERSTELLAR TURBULENCE (2016) (24)
- Star formation from dense shocked regions in supersonic isothermal magnetoturbulence (2018) (23)
- The Effect of AGN Heating on the Low-redshift Lyα Forest (2016) (21)
- THE RAZOR’S EDGE OF COLLAPSE: THE TRANSITION POINT FROM LOGNORMAL TO POWER-LAW DISTRIBUTIONS IN MOLECULAR CLOUDS (2016) (21)
- Multi-phase Turbulence Density Power Spectra in the Perseus Molecular Cloud (2018) (20)
- The Supersonic Project: Shining Light on SIGOs—A New Formation Channel for Globular Clusters (2019) (20)
- THE EFFECTS OF RADIATIVE TRANSFER ON THE PROBABILITY DISTRIBUTION FUNCTIONS OF MOLECULAR MAGNETOHYDRODYNAMIC TURBULENCE (2013) (20)
- The Self-gravitating Gas Fraction and the Critical Density for Star Formation (2018) (19)
- Massive-star Formation via the Collapse of Subvirial and Virialized Turbulent Massive Cores (2019) (19)
- Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations (2021) (17)
- Developing the 3-point Correlation Function for the Turbulent Interstellar Medium (2017) (17)
- Chemical Abundances in a Turbulent Medium–H2, OH+, H2O+, ArH+ (2019) (17)
- Efficient early stellar feedback can suppress galactic outflows by reducing supernova clustering (2020) (16)
- TurbuStat: Turbulence Statistics in Python (2019) (16)
- Advanced Diagnostics for the Study of Linearly Polarized Emission. II. Application to Diffuse Interstellar Radio Synchrotron Emission (2018) (15)
- The Detectability of Radio Auroral Emission from Proxima b (2017) (15)
- THE H i PROBABILITY DISTRIBUTION FUNCTION AND THE ATOMIC-TO-MOLECULAR TRANSITION IN MOLECULAR CLOUDS (2016) (15)
- Classification of Magnetohydrodynamic Simulations Using Wavelet Scattering Transforms (2020) (15)
- Velocity centroid gradients for absorbing media (2017) (14)
- The Driving Scale–Density Decorrelation Scale Relation in a Turbulent Medium (2020) (14)
- Probes of turbulent driving mechanisms in molecular clouds from fluctuations in synchrotron intensity (2016) (13)
- Do Androids Dream of Magnetic Fields? Using Neural Networks to Interpret the Turbulent Interstellar Medium (2019) (13)
- THE PHASE COHERENCE OF INTERSTELLAR DENSITY FLUCTUATIONS (2015) (13)
- CHARACTERIZING THE TURBULENT PROPERTIES OF THE STARLESS MOLECULAR CLOUD MBM 16 (2013) (13)
- PREDICTED SIZES OF PRESSURE-SUPPORTED HI CLOUDS IN THE OUTSKIRTS OF THE VIRGO CLUSTER (2016) (12)
- PRINCIPAL COMPONENT ANALYSIS STUDIES OF TURBULENCE IN OPTICALLY THICK GAS (2015) (12)
- Observational diagnostics for two-fluid turbulence in molecular clouds as suggested by simulations (2013) (12)
- First Results from SMAUG: The Need for Preventative Stellar Feedback and Improved Baryon Cycling in Semianalytic Models of Galaxy Formation (2020) (11)
- Turbulence and Energetic Particles in Radiative Shock Waves in the Cygnus Loop. I. Shock Properties (2020) (10)
- OPACITY BROADENING OF 13CO LINEWIDTHS AND ITS EFFECT ON THE VARIANCE–SONIC MACH NUMBER RELATION (2014) (9)
- The relative orientation between the magnetic field and gradients of surface brightness within thin velocity slices of 12CO and 13CO emission from the Taurus molecular cloud (2020) (8)
- The Column Density Variance-Sonic Mach Number Relationship (2012) (8)
- Winds in Star Clusters Drive Kolmogorov Turbulence (2020) (8)
- Turbulence and Energetic Particles in Radiative Shock Waves in the Cygnus Loop. II. Development of Postshock Turbulence (2020) (7)
- The Catalogue for Astrophysical Turbulence Simulations (CATS) (2020) (7)
- An In-depth Investigation of Faraday Depth Spectrum Using Synthetic Observations of Turbulent MHD Simulations (2019) (6)
- The Effects of Radiative Transfer on the PDFs of Molecular MHD Turbulence (2013) (6)
- The Next Decade of Astroinformatics and Astrostatistics (2019) (6)
- The Simons Observatory: Galactic Science Goals and Forecasts (2021) (6)
- Magnetic field orientation in self-gravitating turbulent molecular clouds (2021) (6)
- The Supersonic Project: To Cool or Not to Cool Supersonically Induced Gas Objects (SIGOs)? (2020) (5)
- Bursting Bubbles: Feedback from Clustered Supernovae and the Trade-off Between Turbulence and Outflows (2021) (5)
- Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies (2021) (5)
- A Markov Model for Non-lognormal Density Distributions in Compressive Isothermal Turbulence (2019) (5)
- The Dense Gas Fraction and The Critical Density Required for Star Formation (2018) (5)
- The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses? (2021) (5)
- The Effects of Magnetic Fields and Outflow Feedback on the Shape and Evolution of the Density Probability Distribution Function in Turbulent Star-forming Clouds (2021) (4)
- The Supersonic Project: SIGOs, A Proposed Progenitor to Globular Clusters, and Their Connections to Gravitational-wave Anisotropies (2021) (4)
- Astrophysical MHD turbulence: confluence of observations, simulations, and theory (2012) (3)
- The Low-redshift Lyα Forest as a Constraint for Models of AGN Feedback (2022) (3)
- sígame v3: Gas Fragmentation in Postprocessing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling (2021) (3)
- The CAMELS Project: Public Data Release (2022) (3)
- Bursting Bubbles: Clustered Supernova Feedback in Local and High-redshift Galaxies (2021) (3)
- Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations (2023) (2)
- PICO : Probe of Inflation and Cosmic Origins Thematic Area : Space Based Projects-Medium Lead (2019) (2)
- CMB foreground measurements through broad-band radio spectro-polarimetry: prospects of the SKA-MPG telescope (2019) (2)
- First extragalactic measurement of the turbulence driving parameter: ALMA observations of the star-forming region N159E in the Large Magellanic Cloud (2021) (2)
- Statistical tools of interstellar turbulence: connecting observations with theory (2010) (1)
- The CARMA-NRO Orion Survey—Data Release (2021) (1)
- On the impact of runaway stars on dwarf galaxies with resolved interstellar medium (2022) (1)
- The Supersonic Project: The Early Evolutionary Path of Supersonically Induced Gas Objects (2023) (1)
- Studying Interstellar Turbulence Driving Scales Using the Bispectrum (2022) (1)
- Active galactic nucleus jet feedback in hydrostatic halos (2022) (1)
- Understanding biases in measurements of molecular cloud kinematics using line emission (2020) (0)
- Astro2020: Training the Future Generation of Computational Researchers (2019) (0)
- Code Comparison in Galaxy Scale Simulations with Resolved Supernova Feedback: Lagrangian vs. Eulerian Methods (2022) (0)
- Probing turbulent, magnetized star formation with ALMA observations and next-generation AREPO simulations (2017) (0)
- The Supersonic Project: The Early Evolutionary Path of SIGOs (2022) (0)
- Measuring the turbulent ISM via polarised radio-emission (2012) (0)
- The Supersonic Project: The Eccentricity and Rotational Support of SIGOs and DM GHOSts (2022) (0)
- TurbuStat: Turbulence statistics in spectral-line data cubes (2019) (0)
- The Bane of Column Density Analysis and What Good It Can Do for Us (2016) (0)
- Spatially Resolved Gas-phase Metallicity in FIRE-2 Dwarfs: Late-Time Evolution of Metallicity Relations in Simulations with Feedback and Mergers (2022) (0)
- Chapter VI CRITICAL PHYSICAL INGREDIENTS FOR DYNAMOS: TURBULENCE AND INSTABILITIES (2013) (0)
- Topology in Synthetic Column Density Maps for Interstellar Turbulence (2013) (0)
- Astro2020 Science White Paper: The Next Decade of Astroinformatics and Astrostatistics (2019) (0)
- Gauging the Turbulent Mach Numbers in Optically Thick Clouds (2012) (0)
- Gas Accretion Can Drive Turbulence in Galaxies (2022) (0)
- Hyperion: the origin of the stars. A far UV space telescope for high-resolution spectroscopy over wide fields (2022) (0)
- Using the Velocity Anisotropy Technique to Investigate Interstellar Magnetohydrodynamic Turbulence (2016) (0)
- Statistical Tools of Interstellar Turbulence: Bridging the Gap Between Numerics and Observations (2011) (0)
- What Sets the Star Formation Rate of Molecular Clouds? The Density Distribution as a Fingerprint of Compression and Expansion Rates (2023) (0)
- Efficient Long-range Active Galactic Nuclei (AGNs) Feedback Affects the Low-redshift Lyα Forest (2023) (0)
- Spiral arms are metal freeways: Azimuthal gas-phase metallicity variations in flocculent disks in the FIRE-2 cosmological zoom-in simulations (2022) (0)
- Statistical Tools of ISM turbulence (2011) (0)
- CARMA-NRO Orion Survey: Unbiased Survey of Dense Cores and Core Mass Functions in Orion A (2022) (0)
- The energy spectrum and geometrical structure of Galactic turbulent magnetic field (2012) (0)
- JWST constraints on the UV luminosity density at cosmic dawn: implications for 21-cm cosmology (2023) (0)
- The GALFA-HI Survey: Extracting New Clouds From a Complex Medium (2011) (0)
- X-ray Absorption Lines in the Warm-Hot Intergalactic Medium: Probing Chandra observations with the CAMEL simulations (2022) (0)
- Turbulence in the WIM: The Sonic Mach Number Revealed Using Gradients of Linear Radio Polarization Maps (2012) (0)
- Efficient long-range AGN feedback affects the low redshift Lyman-$\alpha$ forest (2022) (0)
- The Relationship Between the Turbulence-Driving-Length and the Length-Scale of Density Structures in Magnetohydrodynamic Turbulence (2020) (0)
- ERRATUM: “THE GALFA-HI COMPACT CLOUD CATALOG” (2012, ApJ, 758, 44) (2015) (0)
- The Column Density Distribution of the Low-Redshift Lyman-Alpha Forest in Illustris (2016) (0)
- Evidence for efficient long-range AGN jet feedback from the low redshift Lyman- α forest (2022) (0)
- Bursting Bubbles: Clustered SNe Feedback in Local and High-redshift Galaxies (2021) (0)
- New Frontiers for Diagnosing the Turbulent Nature of the Multiphase Magnetized Interstellar Medium (2016) (0)
- Molecular gas and star formation in nearby starburst galaxy mergers (2023) (0)
- Training the Future Generation of Computational Researchers (2019) (0)
- COMPARING CAF AND MPI-3 AND SIMULATING MOLECULAR CLOUD TURBULENCE WITH TWO-FLUID MHD (2017) (0)
- The Origin of Turbulence in Galactic Disks (2016) (0)
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