ODNet: A Convolutional Neural Network for Asteroid Occultation Detection
- URL: http://arxiv.org/abs/2210.16440v1
- Date: Fri, 28 Oct 2022 23:53:09 GMT
- Title: ODNet: A Convolutional Neural Network for Asteroid Occultation Detection
- Authors: Dorian Cazeneuve, Franck Marchis, Guillaume Blaclard, Paul A. Dalba,
Victor Martin, Jo\'e Asencioa
- Abstract summary: We propose to build an algorithm that will use a Convolutional Neural Network (CNN) and observations from the Unistellar network to reliably detect asteroid occultations.
The algorithm is sufficiently fast and robust so we can envision incorporating onboard the eVscopes to deliver real-time results.
- Score: 0.36700088931938835
- License: http://creativecommons.org/licenses/by/4.0/
- Abstract: We propose to design and build an algorithm that will use a Convolutional
Neural Network (CNN) and observations from the Unistellar network to reliably
detect asteroid occultations. The Unistellar Network, made of more than 10,000
digital telescopes owned by citizen scientists, and is regularly used to record
asteroid occultations. In order to process the increasing amount of
observational produced by this network, we need a quick and reliable way to
analyze occultations. In an effort to solve this problem, we trained a CNN with
artificial images of stars with twenty different types of photometric signals.
Inputs to the network consists of two stacks of snippet images of stars, one
around the star that is supposed to be occulted and a reference star used for
comparison. We need the reference star to distinguish between a true
occultation and artefacts introduced by poor atmospheric condition. Our
Occultation Detection Neural Network (ODNet), can analyze three sequence of
stars per second with 91\% of precision and 87\% of recall. The algorithm is
sufficiently fast and robust so we can envision incorporating onboard the
eVscopes to deliver real-time results. We conclude that citizen science
represents an important opportunity for the future studies and discoveries in
the occultations, and that application of artificial intelligence will permit
us to to take better advantage of the ever-growing quantity of data to
categorize asteroids.
Related papers
- Rewrite the Stars [70.48224347277014]
Recent studies have drawn attention to the untapped potential of the "star operation" in network design.
Our study attempts to reveal the star operation's ability to map inputs into high-dimensional, non-linear feature spaces.
We introduce StarNet, a simple yet powerful prototype, demonstrating impressive performance and low latency.
arXiv Detail & Related papers (2024-03-29T04:10:07Z) - Deep-learning based measurement of planetary radial velocities in the
presence of stellar variability [70.4007464488724]
We use neural networks to reduce stellar RV jitter in three years of HARPS-N sun-as-a-star spectra.
We find that the multi-line CNN is able to recover planets with 0.2 m/s semi-amplitude, 50 day period, with 8.8% error in the amplitude and 0.7% in the period.
arXiv Detail & Related papers (2023-04-10T18:33:36Z) - Photometric identification of compact galaxies, stars and quasars using
multiple neural networks [0.9894420655516565]
MargNet is a deep learning-based classifier for identifying stars, quasars and compact galaxies.
It learns classification directly from the data, minimising the need for human intervention.
MargNet is the first classifier focusing exclusively on compact galaxies.
arXiv Detail & Related papers (2022-11-15T18:37:04Z) - Semi-Supervised Domain Adaptation for Cross-Survey Galaxy Morphology
Classification and Anomaly Detection [57.85347204640585]
We develop a Universal Domain Adaptation method DeepAstroUDA.
It can be applied to datasets with different types of class overlap.
For the first time, we demonstrate the successful use of domain adaptation on two very different observational datasets.
arXiv Detail & Related papers (2022-11-01T18:07:21Z) - Discovering Faint and High Apparent Motion Rate Near-Earth Asteroids
Using A Deep Learning Program [0.5729426778193399]
We developed a convolutional neural network for detecting faint fast-moving near-Earth objects.
It was trained with artificial streaks generated from simulations and was able to find these asteroid streaks with an accuracy of 98.7%.
This approach can be adopted by any observatory for detecting fast-moving asteroid streaks.
arXiv Detail & Related papers (2022-08-19T00:16:09Z) - Optimization of Artificial Neural Networks models applied to the
identification of images of asteroids' resonant arguments [0.6449761153631166]
Recent works used Convolutional Neural Networks (CNN) models to perform such task automatically.
We compare the outcome of such models with those of some of the most advanced and publicly available CNN architectures, like the VGG, Inception and ResNet.
The VGG model, with and without regularizations, proved to be the most efficient method to predict labels of large datasets.
arXiv Detail & Related papers (2022-07-28T15:46:39Z) - Identifying outliers in astronomical images with unsupervised machine
learning [4.469071901315176]
Unpredictable astronomical outliers constantly lead to the discovery of genuinely unforeseen knowledge in astronomy.
It is a severe challenge to mine rare and unexpected targets from enormous data with human inspection.
We adopt unsupervised machine learning approaches to identify outliers in the data of galaxy images.
arXiv Detail & Related papers (2022-05-19T09:58:48Z) - DeepShadows: Separating Low Surface Brightness Galaxies from Artifacts
using Deep Learning [70.80563014913676]
We investigate the use of convolutional neural networks (CNNs) for the problem of separating low-surface-brightness galaxies from artifacts in survey images.
We show that CNNs offer a very promising path in the quest to study the low-surface-brightness universe.
arXiv Detail & Related papers (2020-11-24T22:51:08Z) - Detection of gravitational-wave signals from binary neutron star mergers
using machine learning [52.77024349608834]
We introduce a novel neural-network based machine learning algorithm that uses time series strain data from gravitational-wave detectors.
We find an improvement by a factor of 6 in sensitivity to signals with signal-to-noise ratio below 25.
A conservative estimate indicates that our algorithm introduces on average 10.2 s of latency between signal arrival and generating an alert.
arXiv Detail & Related papers (2020-06-02T10:20:11Z) - Ventral-Dorsal Neural Networks: Object Detection via Selective Attention [51.79577908317031]
We propose a new framework called Ventral-Dorsal Networks (VDNets)
Inspired by the structure of the human visual system, we propose the integration of a "Ventral Network" and a "Dorsal Network"
Our experimental results reveal that the proposed method outperforms state-of-the-art object detection approaches.
arXiv Detail & Related papers (2020-05-15T23:57:36Z) - Detection and Classification of Astronomical Targets with Deep Neural
Networks in Wide Field Small Aperture Telescopes [9.035184185881777]
We propose an astronomical targets detection and classification framework based on deep neural networks.
Our framework adopts the concept of the Faster R-CNN and uses a modified Resnet-50 as backbone network.
We propose to install our framework in embedded devices such as the Nvidia Jetson Xavier to achieve real-time astronomical targets detection and classification abilities.
arXiv Detail & Related papers (2020-02-21T10:35:31Z)
This list is automatically generated from the titles and abstracts of the papers in this site.
This site does not guarantee the quality of this site (including all information) and is not responsible for any consequences.