Name | Abs no. | Title |
Aisha Alowais | 713 | Neural Networks for Meteorite and
Meteor Recognition |
Amelia Yu | 1360 | Deep learning proves to be an effective
tool for detecting previously undiscovered exoplanets in Kepler data |
Anupam Bhardwaj | 760 | Predicting Physical Parameters of
Cepheid and RR Lyrae variables in an Instant with Machine Learning |
Atila Poro | 2845 | Investigation of the orbital period
and mass relations for W UMa-type contact systems |
Atrideb Chatterjee | 1529 | ANN based MCMC pipeline for
constraining cosmological and astrophysical parameters using EoR
observations |
Connor Bottrell | 1921 | Unraveling galaxy merger
histories with deep learning |
Dominic Adams | 2801 | Combining citizen science and
machine learning strategies to enable Galaxy Zoo: Clump Scout
science |
Dongjin Lee | 2605 | How and why TDA improves CNN:
Transient vs Bogus classifications |
Eunsu Park | 2553 | Application of image translation
methods based on deep learning to denoising solar magnetograms |
Garreth Martin | 2514 | Versatile morphological
classification for the next generation of large surveys |
Gor Mikayelyan | 888 | Astronomical objects classification
based on the Digitized First Byurakan Survey low-dispersion spectra |
Guillermo Torralba Elipe | 1676 | A Machine Learning-based
DPAC algorithm for Gaia RVS spectra parameterization |
Hanwool Koo | 334 | Bayesian vs frequentist: comparing
Bayesian model selection with a frequentist approach using the iterative
smoothing method |
Jaehan Bae | 670 | KPSFinder: a machine learning-based
exoplanet searching tool |
Jinkoo Yim | 2549 | 3-day Forecasting of Global TEC Maps
Using a Deep Learning Model |
Joeri Van Leeuwen | 2470 | CORTEX - the Center for
Optimal, Real-Time Machine Studies of the Explosive Universe |
Johan Knapen | 2784 | Deep Learning and numerical
simulations to infer the evolution of MaNGA galaxies |
John Eduard Martínez Fernández | 3162 | Clustering
analysis with stellar photometric data |
John Hefele | 3283 | Machine Learning for Hazardous Small
Solar System Body Detection |
Josef Durech | 2415 | Machine-learning detection of
false-positive solutions in the inversion of asteroid sparse-in time
photometry |
Kakeru Fukumitsu | 3306 | Image Restoration based on Deep
Learning for High-Resolution Solar Images |
Krisztián Vida | 1260 | Flare detection with different
machine learning methods |
Kyungmin Kim | 557 | Deep Learning-based Search for Lensed
Gravitational-Wave Signals from Binary Black Hole Events in GWTC-1 and
-2 |
Laurent Eyer | 2489 | Revealing celestial variable sources
with Gaia DR3 |
Marco Álvarez | 1730 | Unsupervised clustering
visualisation tool for Gaia DR3 |
Marc Huertas-Company | 2857 | Unveiling the morphologies
of z>3 with JWST and self-supervised learning |
Margherita Grespan | 1299 | A study on representation of
Gravitational Waves Data for Convolutional Neural Network |
Maria Luisa Buzzo | 1405 | A survey of stellar populations
in Ultra-Diffuse Galaxies (UDGs) in the era of LSST and JWST: the role of
machine learning in finding and characterising UDGs. |
Marian Douspis | 2053 | Retrieving cosmological
information from clusters and hot diffuse gas in CMB small scales using
machine learning emulator of power spectrum |
Mark Birkinshaw | 2276 | Radio image segmentation with
variational autoencoders: application to SKA Data Challenge 1 |
Michel Cure | 1678 | Bayesian deconvolution of a rotating
spectral line profile to a non-rotating one |
Monika Soraisam | 2563 | A classification algorithm for
time-domain novelties in preparation for LSST alerts |
Médéric Boquien | 1551 | Accelerating spectro-photometric
modeling for next-generation massive surveys |
Nahathai Tanakul | 2637 | Searching for Globular Cluster
Candidates around M81, M82, NGC3077 Using Machine Learning
Techniques |
Nahathai Tanakul | 1177 | Features Selection and Imbalance
Learning in Automatic Variable Star Classification |
Nicolás Vásquez | 998 | Computational techniques for high
energy astrophysics and medical image processing |
Oliver Boersma | 1701 | Efficient neural network emulation
of complex physical models for gamma-ray burst afterglows |
Pablo Manuel Sánchez Alarcón | 2643 | Fully Adaptive
Bayesian Algorithm for Data Analysis. FABADA |
Rodrigo Calderon | 2580 | Joint reconstructions of growth
and expansion histories with Gaussian Processes: Dark Energy beyond
Λ |
Ryohtaroh Ishikawa | 2614 | Multi-scale deep learning for
estimating horizontal velocity fields on the solar surface |
SYED NAJAMUL HASAN | 1692 | Is GMM effective in membership
determination of Open Clusters? |
Sandor Pinter | 2250 | High-redshift galaxy cluster
candidates from Subaru HSC photometric redshifts |
Sandor Pinter | 2248 | Can the distance of GRBs be
estimated using machine learning? |
SangHoon Oh | 3384 | Deep Learning Classification of Noise
Transients using Multi-Scale Neural Networks applied to LIGO’s Auxiliary
Channel Data |
Satadru Bag | 3265 | Detecting Strong Lensed Quasars and
Measuring their Time Delays from the Unresolved Light Curves |
Se Yeon Hwang | 3055 | Deep Learning Approaches to Large
Scale Structure Cosmology |
Seong-Heon Lee | 2670 | CNN-TDA Net : Focus adjustment
toward persistent topological signal of point-source. |
Sergen Ozdemir | 3161 | Searching for similar stars in
large spectroscopic datasets with machine learning |
Simon Anghel | 1437 | Machine Learning Tools Applied to
All-Sky Astroclimate Analysis in Romania |
Sirinrat Sithajan | 912 | Applied Machine Learning Models
for Identifying Spectral Sub-Types of M Dwarfs from Photometric
Surveys |
Suk Kim | 3307 | Development of an image similarity
retrieval engine using Convolutional Neural Network for automating galaxy
morphology classification |
Sumi Kim | 1380 | Cosmological Information from Higher
Order Clustering Statistics |
Tomasz Różański | 2348 | Stellar spectra classification
and clustering using deep learning |
Vitor Cernic | 1043 | Stellar Population Photometric
Synthesis with AI of S-PLUS galaxies |
William Pearson | 2124 | Data pre-extraction for better
classification of galaxy mergers |
Wuhyun Sohn | 2582 | Reconstructing the early universe
using CMB temperature and polarization |