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Large scale relative protein ligand binding affinities using non-equilibrium alchemy
ISSN: 2041-6520, 2041-6539Published: Cambridge Royal Society of Chemistry 2020Published in Chemical science (Cambridge) (2020)“…Ligand binding affinity calculations based on molecular dynamics (MD) simulations and non-physical (alchemical) thermodynamic cycles have shown great promise…”
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Extragalactic Magnetism with SOFIA (SALSA Legacy Program). III. First Data Release and On-the-fly Polarization Mapping Characterization The SOFIA Legacy Program for Magnetic Fields in Galaxies (SALSA) provides a software repository at https://github.com/galmagfields/hawc and publicly available data at http://galmagfields.com
ISSN: 0004-637X, 1538-4357Published: The American Astronomical Society 01.09.2022Published in The Astrophysical journal (01.09.2022)Get full text
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AutoWISP: Automated Processing of Wide-field Color Images https://github.com/kpenev/AutoWISP
ISSN: 0004-6256, 1538-3881, 1538-3881Published: Madison The American Astronomical Society 01.10.2025Published in The Astronomical journal (01.10.2025)“…We have developed a software pipeline, AutoWISP, for extracting high-precision photometry from citizen scientists’ observations made with consumer-grade color…”
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An Interpretable Machine-learning Framework for Modeling High-resolution Spectroscopic Data Open-source code at https://github.com/gully/blase
ISSN: 0004-637X, 1538-4357Published: The American Astronomical Society 01.12.2022Published in The Astrophysical journal (01.12.2022)Get full text
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MC-BLOS: Automated Software for Determining the Line-of-sight Component of Magnetic Fields Associated with Molecular Clouds∗ ∗Software available at https://github.com/MehrnooshTahani/MC-BLOS, DOI: 10.5281/zenodo.15338512
ISSN: 0004-637X, 1538-4357, 1538-4357Published: Philadelphia The American Astronomical Society 10.10.2025Published in The Astrophysical journal (10.10.2025)“…While plane-of-sky magnetic field observations in molecular clouds are now common, observations of their line-of-sight magnetic field remain limited. To…”
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Katachi (形): Decoding the Imprints of Past Star Formation on Present-day Morphology in Galaxies with Interpretable CNNs https://github.com/juanpabloalfonzo/Katachi
ISSN: 0004-637X, 1538-4357Published: The American Astronomical Society 29.05.2024Published in The Astrophysical journal (29.05.2024)Get full text
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Extragalactic Magnetism with SOFIA (SALSA Legacy Program). IV. Program Overview and First Results on the Polarization Fraction SALSA provides a software repository at https://github.com/galmagfields/hawc and publicly available data at http://galmagfields.com
ISSN: 0004-637X, 1538-4357Published: The American Astronomical Society 05.09.2022Published in The Astrophysical journal (05.09.2022)Get full text
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Extragalactic Magnetism with SOFIA (Legacy Program). I. The Magnetic Field in the Multiphase Interstellar Medium of M51 The SOFIA Legacy Group for Magnetic Fields in Galaxies software repository is available at https://github.com/galmagfields/hawc via the official project website, http://galmagfields.com/, and Zenodo/GitHub, https://doi.org/10.5281/zenodo.5116134
ISSN: 0004-637X, 1538-4357Published: The American Astronomical Society 09.11.2021Published in The Astrophysical journal (09.11.2021)Get full text
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Prediction of Astrometric-microlensing Events from Gaia eDR3 Proper Motions The results of the predicted microlensing events is available in electronic form via the GAVO Data Center https://dc.g-vo.org/amlensing/q3/q/form. † †The source code for this study is made publicly available https://github.com/jkluter/amlensing
ISSN: 0004-6256, 1538-3881Published: The American Astronomical Society 17.03.2022Published in The Astronomical journal (17.03.2022)Get full text
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Extragalactic Magnetism with SOFIA (SALSA Legacy Program): The Magnetic Fields in the Multiphase Interstellar Medium of the Antennae Galaxies SALSA provides a software repository at https://github.com/galmagfields/hawc, and publicly available data at http://galmagfields.com
ISSN: 2041-8205, 2041-8213Published: The American Astronomical Society 30.12.2022Published in Astrophysical journal. Letters (30.12.2022)Get full text
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Extragalactic Magnetism with SOFIA (Legacy Program) - II: A Magnetically Driven Flow in the Starburst Ring of NGC 1097 The SOFIA Legacy Program for Magnetic Fields in Galaxies provides a software repository at https://github.com/galmagfields/hawc and publicly available data at http://galmagfields.com
ISSN: 0004-637X, 1538-4357Published: The American Astronomical Society 17.12.2021Published in The Astrophysical journal (17.12.2021)Get full text
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A formalism for sequential estimation of neural membrane time constant and input–output curve towards selective and closed-loop transcranial magnetic stimulation Matlab Code is available at https://github.com/smmalavi/TMS-tau-IOC-estim-fixed-tp
ISSN: 1741-2560, 1741-2552Published: IOP Publishing 01.10.2022Published in Journal of neural engineering (01.10.2022)Get full text
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The Evolving Interstellar Medium of Star-forming Galaxies, as Traced by Stardust https://github.com/VasilyKokorev/stardust
ISSN: 0004-637X, 1538-4357Published: The American Astronomical Society 28.10.2021Published in The Astrophysical journal (28.10.2021)Get full text
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DRACON: disconnected graph neural network for atom mapping in chemical reactions
ISSN: 1463-9084, 1463-9084Published: 25.11.2020Published in Physical chemistry chemical physics : PCCP (25.11.2020)“…Machine learning solved many challenging problems in computer-assisted synthesis prediction (CASP). We formulate a reaction prediction problem in terms of…”
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IGRINS RV: A Precision Radial Velocity Pipeline for IGRINS Using Modified Forward Modeling in the Near-infrared https://github.com/shihyuntang/igrins_rv
ISSN: 0004-6256, 1538-3881Published: The American Astronomical Society 26.05.2021Published in The Astronomical journal (26.05.2021)Get full text
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Reproducing High-energy Neutrino Emission from Short Gamma-Ray Bursts: Validation and Application to GRB 170817A Detailed code for this work is available at https://doi.org/10.5281/zenodo.17569170 and https://github.com/svamshi-9384/sgrb_neutrino_replication
ISSN: 2515-5172Published: The American Astronomical Society 18.11.2025Published in Research notes of the AAS (18.11.2025)“…I reproduce the analytical framework of S. S. Kimura et al. for high-energy neutrino emission from short gamma-ray bursts. After verifying the model against S…”
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Interfacial nanomechanical heterogeneity of the E. coli biofilm matrix
ISSN: 2040-3372, 2040-3372Published: England 20.08.2020Published in Nanoscale (20.08.2020)“…The interface between bacterial biofilms and their environment plays a vital role in the recalcitrance of biofilms to biological, chemical, and mechanical…”
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End-to-end neuromorphic speech enhancement with PDM microphonesSource code will be available at https://github.com/NECOTIS/PDM-DNS
ISSN: 2634-4386Published: IOP Publishing 30.07.2025Published in Neuromorphic computing and engineering (30.07.2025)Get full text
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Machine learning dihydrogen activation in the chemical space surrounding Vaska's complex (The dataset is publicly available at Dataverse and GitHub (https://doi.org/10.5683/SP2/CJS7QA and https://github.com/pascalfriederich/vaskas-space, respectively). It includes the xyz files containing the coordinates of all complexes and transition states and the calculated energies and features used to train our machine learning models in a .csv file.)
ISSN: 2041-6520, 2041-6539Published: Cambridge Royal Society of Chemistry 01.01.2020Published in Chemical science (Cambridge) (01.01.2020)“…Homogeneous catalysis using transition metal complexes is ubiquitously used for organic synthesis, as well as technologically relevant in applications such as…”
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Debris of Asteroid Disruptions Close to the Sun∗ ∗ Data and codes that generate the figures and main results of this work are publicly available on Zenodo (doi:10.5281/zenodo.2547298) and GitHub (https://github.com/Yeqzids/near-sun-disruptions)
ISSN: 0004-637X, 1538-4357Published: The American Astronomical Society 11.03.2019Published in The Astrophysical journal (11.03.2019)“…The under-abundance of asteroids on orbits with small perihelion distances suggests that thermally driven disruption may be an important process in the removal…”
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