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orvara: An Efficient Code to Fit Orbits Using Radial Velocity, Absolute, and/or Relative Astrometry

The Astronomical journal, 2021-11, Vol.162 (5), p.186

2021

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The First Dynamical Mass Measurement in the HR 8799 System

Astrophysical journal. Letters, 2021-07, Vol.915 (1), p.L16

2021

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Precise Masses and Orbits for Nine Radial-velocity Exoplanets

The Astronomical journal, 2021-12, Vol.162 (6), p.266

2021

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SCExAO CHARIS Direct Imaging Discovery of a 20 au Separation, Low-mass Ratio Brown Dwarf Companion to an Accelerating Sun-like Star

Astrophysical journal. Letters, 2020-12, Vol.904 (2), p.L25

2020

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Study of persistent luminescence and thermoluminescence in SrSi2N2O2:Eu2+,M3+ (M = Ce, Dy, and Nd)

Physical chemistry chemical physics : PCCP, 2020-01, Vol.22 (30), p.17152-17159

2020

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Identification and Validation of a Sickle Cell Disease Cohort Within Electronic Health Records

Academic pediatrics, 2017-04, Vol.17 (3), p.283-287

2017

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Synthesis and Photoluminescence Properties of Pr3+-Doped Ba0.5Ca0.5TixZr(1-x)O3 Perovskite Diphasic Ceramics Obtained by the Modified Pechini Method

Materials, 2022-01, Vol.15 (3), p.1058

2022

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The Tycho - Gaia astrometric solution: How to get 2.5 million parallaxes with less than one year of Gaia data

Astronomy and astrophysics (Berlin), 2015-02, Vol.574, p.A115

2015

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The Tycho-Gala astrometric solution. How to get 2.5 million parallaxes with less than one year of Gala data

Astronomy and astrophysics (Berlin), 2015-02, Vol.574

2015

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The effect of Al–O substitution for Si–N on the luminescence properties of YAG:Ce phosphor

Journal of the European Ceramic Society, 2012-06, Vol.32 (7), p.1383-1387

2012

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Vestibular schwannoma

InnovAiT, 2023-01, Vol.16 (1), p.34-38

Michalik, Daniel

2023

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Penicillamine-induced elastosis perforans serpiginosa and pseudo-pseudoxanthoma elasticum

International journal of women's dermatology, 2021-12, Vol.7 (5), p.822-823

2021

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Quasars can be used to verify the parallax zero-point of the Tycho-Gaia Astrometric Solution

Astronomy and astrophysics (Berlin), 2016-02, Vol.586, p.A26

2016

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Dopant Concentration Induced Optical Changes in Ca,Eu-α-Sialon

Crystals (Basel), 2017-11, Vol.7 (11), p.342

2017

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htof: A New Open-source Tool for Analyzing Hipparcos, Gaia, and Future Astrometric Missions

The Astronomical journal, 2021-12, Vol.162 (6), p.230

2021

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Joint astrometric solution of HIPPARCOS and Gaia: A recipe for the Hundred Thousand Proper Motions project

Astronomy and astrophysics (Berlin), 2014-11, Vol.571, p.A85

2014

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Precise Dynamical Masses and Orbital Fits for β Pic b and β Pic c

The Astronomical journal, 2021-04, Vol.161 (4), p.179

2021

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Mapping the Milky Way disc kinematics

Astronomy and astrophysics (Berlin), 2018, Vol.616

2018

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Shedding light on subungual digital mucous cysts

Cleveland Clinic journal of medicine, 2021-08, Vol.88 (8), p.426-427

2021

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Gaia astrometry for stars with too few observations. A Bayesian approach

Astronomy and astrophysics (Berlin), 2015-11, Vol.583, p.A68

2015

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Predictors of extensive subclinical spread in squamous cell carcinoma

Journal of clinical oncology, 2020-05, Vol.38 (15_suppl), p.e22093-e22093

2020

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Study of persistent luminescence and thermoluminescence in SrSi 2 N 2 O 2 :Eu 2+ ,M 3+ (M = Ce, Dy, and Nd)

Physical chemistry chemical physics : PCCP, 2020-08, Vol.22 (30), p.17152-17159

2020

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Mechanism of the Luminescence Enhancement of SrSi2N2O2:Eu2+ Phosphor via Manganese Addition

Journal of physical chemistry. C, 2022-03, Vol.126 (11), p.5292-5301

2022

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Synthesis and Photoluminescence Properties of Pr 3+ -Doped Ba 0.5 Ca 0.5 Ti x Zr (1-x) O 3 Perovskite Diphasic Ceramics Obtained by the Modified Pechini Method

Materials, 2022-01, Vol.15 (3)

2022

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Improving distance estimates to nearby bright stars: Combining astrometric data from Hipparcos, Nano-JASMINE and Gaia

Proceedings of the International Astronomical Union, 2012-08, Vol.8 (S289), p.414-417

2012

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orvara: An Efficient Code to Fit Orbits Using Radial Velocity, Absolute, and/or Relative Astrometry

The First Dynamical Mass Measurement in the HR 8799 System

Precise Masses and Orbits for Nine Radial-velocity Exoplanets

SCExAO CHARIS Direct Imaging Discovery of a 20 au Separation, Low-mass Ratio Brown Dwarf Companion to an Accelerating Sun-like Star

Study of persistent luminescence and thermoluminescence in SrSi2N2O2:Eu2+,M3+ (M = Ce, Dy, and Nd)

Identification and Validation of a Sickle Cell Disease Cohort Within Electronic Health Records

Synthesis and Photoluminescence Properties of Pr3+-Doped Ba0.5Ca0.5TixZr(1-x)O3 Perovskite Diphasic Ceramics Obtained by the Modified Pechini Method

The Tycho - Gaia astrometric solution: How to get 2.5 million parallaxes with less than one year of Gaia data

The Tycho-Gala astrometric solution. How to get 2.5 million parallaxes with less than one year of Gala data

The effect of Al–O substitution for Si–N on the luminescence properties of YAG:Ce phosphor

Vestibular schwannoma

Penicillamine-induced elastosis perforans serpiginosa and pseudo-pseudoxanthoma elasticum

Quasars can be used to verify the parallax zero-point of the Tycho-Gaia Astrometric Solution

Dopant Concentration Induced Optical Changes in Ca,Eu-α-Sialon

htof: A New Open-source Tool for Analyzing Hipparcos, Gaia, and Future Astrometric Missions

Joint astrometric solution of HIPPARCOS and Gaia: A recipe for the Hundred Thousand Proper Motions project

Precise Dynamical Masses and Orbital Fits for β Pic b and β Pic c

Mapping the Milky Way disc kinematics

Shedding light on subungual digital mucous cysts

Gaia astrometry for stars with too few observations. A Bayesian approach

Predictors of extensive subclinical spread in squamous cell carcinoma

Study of persistent luminescence and thermoluminescence in SrSi 2 N 2 O 2 :Eu 2+ ,M 3+ (M = Ce, Dy, and Nd)

Mechanism of the Luminescence Enhancement of SrSi2N2O2:Eu2+ Phosphor via Manganese Addition

Synthesis and Photoluminescence Properties of Pr 3+ -Doped Ba 0.5 Ca 0.5 Ti x Zr (1-x) O 3 Perovskite Diphasic Ceramics Obtained by the Modified Pechini Method

Improving distance estimates to nearby bright stars: Combining astrometric data from Hipparcos, Nano-JASMINE and Gaia

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