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Machine learning methods for the search for L&T brown dwarfs in the data of modern sky surveys
DOI: 10.1016/j.ascom.2023.100744 Bibcode: 2023A&C....4500744A

Avdeeva, A.

According to various estimates, brown dwarfs (BD) should account for up to 25 percent of all objects in the Galaxy. However, few of them are discovered and well-studied, both individually and as a population. Homogeneous and complete samples of brown dwarfs are needed for these kinds of studies. Due to their weakness, spectral studies of brown dwa…

2023 Astronomy and Computing
Gaia 4
HILIGT, upper limit servers I-Overview
DOI: 10.1016/j.ascom.2021.100531 Bibcode: 2022A&C....3800531S

Gabriel, C.; Kretschmar, P.; Kuulkers, E. +10 more

The advent of all-sky facilities, such as the Neil Gehrels Swift observatory, the All Sky Automated Search for Supernovae (ASAS-SN), eROSITA and Gaia has led to a new appreciation of the importance of transient sources in solving outstanding astrophysical questions. Identification and catalogue cross-matching of transients has been eased over the …

2022 Astronomy and Computing
Exosat INTEGRAL XMM-Newton 27
HILIGT, Upper Limit Servers II - Implementing the data servers
DOI: 10.1016/j.ascom.2021.100529 Bibcode: 2022A&C....3800529K

Freyberg, M. J.; Wilms, J.; Savchenko, V. +7 more

The High-Energy Lightcurve Generator (HILIGT) is a new web-based tool which allows the user to generate long-term lightcurves of X-ray sources. It provides historical data and calculates upper limits from image data in real-time. HILIGT utilizes data from twelve satellites, both modern missions such as XMM-Newton and Swift, and earlier facilities …

2022 Astronomy and Computing
Exosat INTEGRAL XMM-Newton 19
Using multiple instance learning for explainable solar flare prediction
DOI: 10.1016/j.ascom.2022.100668 Bibcode: 2022A&C....4100668H

Melchior, M.; Huwyler, C.

In this work we leverage a weakly-labeled dataset of spectral data from NASA's IRIS satellite for the prediction of solar flares using the Multiple Instance Learning (MIL) paradigm. While standard supervised learning models expect a label for every instance, MIL relaxes this and only considers bags of instances to be labeled. This is ideally suite…

2022 Astronomy and Computing
IRIS 6
1-DREAM: 1D Recovery, Extraction and Analysis of Manifolds in noisy environments
DOI: 10.1016/j.ascom.2022.100658 Bibcode: 2022A&C....4100658C

Smith, R.; Peletier, R.; Mastropietro, M. +7 more

Filamentary structures (one-dimensional manifolds) are ubiquitous in astronomical data sets. Be it in particle simulations or observations, filaments are always tracers of a perturbation in the equilibrium of the studied system and hold essential information on its history and future evolution. However, the recovery of such structures is often com…

2022 Astronomy and Computing
Gaia 6
Sensitivity estimation for dark matter subhalos in synthetic Gaia DR2 using deep learning
DOI: 10.1016/j.ascom.2022.100667 Bibcode: 2022A&C....4100667B

Benito, M.; Bazarov, A.; Hütsi, G. +3 more

The abundance of dark matter subhalos orbiting a host galaxy is a generic prediction of the cosmological framework, and is a promising way to constrain the nature of dark matter. In this paper, we investigate the use of machine learning-based tools to quantify the magnitude of phase-space perturbations caused by the passage of dark matter subhalos…

2022 Astronomy and Computing
Gaia 5
The Gaia AVU-GSR parallel solver: Preliminary studies of a LSQR-based application in perspective of exascale systems
DOI: 10.1016/j.ascom.2022.100660 Bibcode: 2022A&C....4100660C

Lattanzi, M. G.; Becciani, U.; Bucciarelli, B. +6 more

The Gaia Astrometric Verification Unit-Global Sphere Reconstruction (AVU-GSR) Parallel Solver aims to find the astrometric parameters for ∼ 108 stars in the Milky Way, the attitude and the instrumental specifications of the Gaia satellite, and the global parameter γ of the post Newtonian formalism. The code iteratively solves a system o…

2022 Astronomy and Computing
Gaia 2
Solar activity classification based on Mg II spectra: Towards classification on compressed data
DOI: 10.1016/j.ascom.2021.100473 Bibcode: 2021A&C....3600473I

Ivanov, S.; Tsizh, M.; Ullmann, D. +2 more

Although large volumes of solar data are available for investigation and study, the vast majority of these data remain unlabeled and are therefore not amenable to modern supervised machine learning methods. Having a way to accurately and automatically classify spectra into categories related to the degree of solar activity is highly desirable and …

2021 Astronomy and Computing
IRIS 4
The Open Universe VOU-Blazars tool
DOI: 10.1016/j.ascom.2019.100350 Bibcode: 2020A&C....3000350C

Giommi, P.; Chang, Y. -L.; Brandt, C. H.

Blazars are a remarkable type of Active Galactic Nuclei (AGN) that are playing an important and rapidly growing role in today's multi-frequency and multi-messenger astrophysics. In the past several years, blazars have been discovered in relatively large numbers in radio, microwave, X-ray and gamma-ray surveys, and more recently have been associate…

2020 Astronomy and Computing
XMM-Newton 29
Data Lab-A community science platform
DOI: 10.1016/j.ascom.2020.100411 Bibcode: 2020A&C....3300411N

Nikutta, R.; Fitzpatrick, M.; Scott, A. +1 more

Data Lab is an open-access science platform developed and operated by the Community and Science Data Center (CSDC) at NSF's National Optical-Infrared Astronomy Research Laboratory (NOIRLab). It serves public photometric survey datasets, provides interactive and programmatic data access, and SQL/ADQL query capabilities via TAP. Users also receive g…

2020 Astronomy and Computing
Gaia 24