Results 21 to 30 of about 29,249,487 (323)

AstroEBSD: exploring new space in pattern indexing with methods launched from an astronomical approach [PDF]

open access: yesJournal of Applied Crystallography, 2018
Electron backscatter diffraction (EBSD) is a technique used to measure crystallographic features in the scanning electron microscope. The technique is highly automated and readily accessible in many laboratories.
T. B. Britton   +4 more
semanticscholar   +1 more source

An Astronomical Image Content-based Recommendation System Using Combined Deep Learning Models in a Fully Unsupervised Mode [PDF]

open access: yesAstronomical Journal, 2021
We have developed a method that maps large astronomical images onto a two-dimensional map and clusters them. A combination of various state-of-the-art machine-learning algorithms is used to develop a fully unsupervised image-quality assessment and ...
H. Teimoorinia   +6 more
semanticscholar   +1 more source

The Statistical Uncertainties on X-Ray Flux and Spectral Parameters from Chandra ACIS-I Observations of Faint Sources: Application to the Cygnus OB2 Association

open access: yesThe Astrophysical Journal Supplement Series, 2023
We investigate the uncertainties of fitted X-ray model parameters and fluxes for relatively faint Chandra ACIS-I source spectra. Monte Carlo (MC) simulations are employed to construct a large set of 150,000 fake X-ray spectra in the low photon count ...
J. F. Albacete-Colombo   +5 more
doaj   +1 more source

Self-supervised Representation Learning for Astronomical Images [PDF]

open access: yesAstrophysical Journal Letters, 2020
Sky surveys are the largest data generators in astronomy, making automated tools for extracting meaningful scientific information an absolute necessity.
Md. Abul Hayat   +4 more
semanticscholar   +1 more source

Fast and Scalable Gaussian Process Modeling with Applications to Astronomical Time Series [PDF]

open access: yes, 2017
The growing field of large-scale time domain astronomy requires methods for probabilistic data analysis that are computationally tractable, even with large data sets. Gaussian processes (GPs) are a popular class of models used for this purpose, but since
D. Foreman-Mackey   +3 more
semanticscholar   +1 more source

Detecting outliers in astronomical images with deep generative networks [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2020
With the advent of future big-data surveys, automated tools for unsupervised discovery are becoming ever more necessary. In this work, we explore the ability of deep generative networks for detecting outliers in astronomical imaging data sets. The main
B. Margalef-Bentabol   +7 more
semanticscholar   +1 more source

Incorporating Measurement Error in Astronomical Object Classification [PDF]

open access: yesAstronomical Journal, 2021
Most general-purpose classification methods, such as support-vector machine (SVM) and random forest (RF), fail to account for an unusual characteristic of astronomical data: known measurement error uncertainties. In astronomical data, this information is
Sarah Shy   +4 more
semanticscholar   +1 more source

The LAEX and NASA portals for CoRoT public data [PDF]

open access: yes, 2009
* Aims. We describe here the main functionalities of the LAEX (Laboratorio de Astrofisica Estelar y Exoplanetas/Laboratory for Stellar Astrophysics and Exoplanets) and NASA portals for CoRoT Public Data.
A. C. Laity   +39 more
core   +2 more sources

An analysis of feature relevance in the classification of astronomical transients with machine learning methods [PDF]

open access: yes, 2016
The exploitation of present and future synoptic (multiband and multi-epoch) surveys requires an extensive use of automatic methods for data processing and data interpretation.
Antonio D'Isanto   +6 more
semanticscholar   +1 more source

The Data Big Bang and the Expanding Digital Universe: High-Dimensional, Complex and Massive Data Sets in an Inflationary Epoch [PDF]

open access: yes, 2010
Recent and forthcoming advances in instrumentation, and giant new surveys, are creating astronomical data sets that are not amenable to the methods of analysis familiar to astronomers.
McCollum, Bruce   +2 more
core   +4 more sources

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