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The era of high-precision astrometry has dawned upon us. The potential of Gaia $\mu$as-level precision in positional measurements is about to be unleashed in the field of extrasolar planetary systems. The Gaia data hold the promise for much…

Earth and Planetary Astrophysics · Physics 2015-02-13 A. Sozzetti

Gaia's readout window strategy is challenged by very dense fields in the sky. Therefore, in addition to standard Gaia observations, full Sky Mapper (SM) images were recorded for nine selected regions in the sky. A new software pipeline…

Solar and Stellar Astrophysics · Physics 2023-12-13 Gaia Collaboration , K. Weingrill , A. Mints , J. Castañeda , Z. Kostrzewa-Rutkowska , M. Davidson , F. De Angeli , J. Hernández , F. Torra , M. Ramos-Lerate , C. Babusiaux , M. Biermann , C. Crowley , D. W. Evans , L. Lindegren , J. M. Martín-Fleitas , L. Palaversa , D. Ruz Mieres , K. Tisanić , A. G. A. Brown , A. Vallenari , T. Prusti , J. H. J. de Bruijne , F. Arenou , A. Barbier , O. L. Creevey , C. Ducourant , L. Eyer , R. Guerra , A. Hutton , C. Jordi , S. A. Klioner , U. Lammers , X. Luri , F. Mignard , S. Randich , P. Sartoretti , R. Smiljanic , P. Tanga , N. A. Walton , C. A. L. Bailer-Jones , U. Bastian , M. Cropper , R. Drimmel , D. Katz , C. Soubiran , F. van Leeuwen , M. Audard , J. Bakker , R. Blomme , C. Fabricius , M. Fouesneau , Y. Frémat , L. Galluccio , A. Guerrier , E. Masana , R. Messineo , C. Nicolas , K. Nienartowicz , F. Pailler , P. Panuzzo , F. Riclet , W. Roux , G. M. Seabroke , R. Sordo , F. Thévenin , G. Gracia-Abril , J. Portell , D. Teyssier , M. Altmann , K. Benson , J. Berthier , P. W. Burgess , D. Busonero , G. Busso , H. Cánovas , B. Carry , N. Cheek , G. Clementini , Y. Damerdji , P. de Teodoro , L. Delchambre , A. DellÓro , E. Fraile Garcia , D. Garabato , P. García-Lario , N. Garralda Torres , P. Gavras , R. Haigron , N. C. Hambly , D. L. Harrison , D. Hatzidimitriou , S. T. Hodgkin , B. Holl , S. Jamal , S. Jordan , A. Krone-Martins , A. C. Lanzafame , W. Löffler , A. Lorca , O. Marchal , P. M. Marrese , A. Moitinho , K. Muinonen , M. Nuñez Campos , I. Oreshina-Slezak , P. Osborne , E. Pancino , T. Pauwels , A. Recio-Blanco , M. Riello , L. Rimoldini , A. C. Robin , T. Roegiers , L. M. Sarro , M. Schultheis , C. Siopis , M. Smith , A. Sozzetti , E. Utrilla , M. van Leeuwen , U. Abbas , P. Ábrahám , A. Abreu Aramburu , C. Aerts , G. Altavilla , M. A. Álvarez , J. Alves , F. Anders , R. I. Anderson , T. Antoja , D. Baines , S. G. Baker , Z. Balog , C. Barache , D. Barbato , M. Barros , M. A. Barstow , S. Bartolomé , D. Bashi , N. Bauchet , N. Baudeau , U. Becciani , L. R. Bedin , I. Bellas-Velidis , M. Bellazzini , W. Beordo , A. Berihuete , M. Bernet , C. Bertolotto , S. Bertone , L. Bianchi , A. Binnenfeld , A. Blazere , T. Boch , A. Bombrun , S. Bouquillon , A. Bragaglia , J. Braine , L. Bramante , E. Breedt , A. Bressan , N. Brouillet , E. Brugaletta , B. Bucciarelli , A. G. Butkevich , R. Buzzi , E. Caffau , R. Cancelliere , S. Cannizzo , T. Cantat-Gaudin , R. Carballo , T. Carlucci , M. I. Carnerero , J. M. Carrasco , J. Carretero , S. Carton , L. Casamiquela , M. Castellani , A. Castro-Ginard , V. Cesare , P. Charlot , L. Chemin , V. Chiaramida , A. Chiavassa , N. Chornay , R. Collins , G. Contursi , W. J. Cooper , T. Cornez , M. Crosta , C. Dafonte , P. de Laverny , F. De Luise , R. De March , R. de Souza , A. de Torres , E. F. del Peloso , M. Delbo , A. Delgado , T. E. Dharmawardena , S. Diakite , C. Diener , E. Distefano , C. Dolding , K. Dsilva , J. Durán , H. Enke , P. Esquej , C. Fabre , M. Fabrizio , S. Faigler , M. Fatović , G. Fedorets , J. Fernández-Hernández , P. Fernique , F. Figueras , Y. Fournier , C. Fouron , M. Gai , M. Galinier , A. Garcia-Gutierrez , M. García-Torres , A. Garofalo , E. Gerlach , R. Geyer , P. Giacobbe , G. Gilmore , S. Girona , G. Giuffrida , R. Gomel , A. Gomez , J. González-Núñez , I. González-Santamaría , E. Gosset , M. Granvik , V. Gregori Barrera , R. Gutiérrez-Sánchez , M. Haywood , A. Helmer , A. Helmi , K. Henares , S. L. Hidalgo , T. Hilger , D. Hobbs , C. Hottier , H. E. Huckle , M. Jabłońska , F. Jansen , Ó. Jiménez-Arranz , J. Juaristi Campillo , S. Khanna , G. Kordopatis , Á Kóspál , M. Kun , S. Lambert , A. F. Lanza , J. -F. Le Campion , Y. Lebreton , T. Lebzelter , S. Leccia , I. Lecoeur-Taibi , G. Lecoutre , S. Liao , L. Liberato , E. Licata , H. E. P. Lindstrøm , T. A. Lister , E. Livanou , A. Lobel , C. Loup , L. Mahy , R. G. Mann , M. Manteiga , J. M. Marchant , M. Marconi , D. Marín Pina , S. Marinoni , D. J. Marshall , J. Martín Lozano , G. Marton , N. Mary , A. Masip , D. Massari , A. Mastrobuono-Battisti , T. Mazeh , P. J. McMillan , J. Meichsner , S. Messina , D. Michalik , N. R. Millar , D. Molina , R. Molinaro , L. Molnár , G. Monari , M. Monguió , P. Montegriffo , A. Montero , R. Mor , A. Mora , R. Morbidelli , T. Morel , D. Morris , N. Mowlavi , D. Munoz , T. Muraveva , C. P. Murphy , I. Musella , Z. Nagy , S. Nieto , L. Noval , A. Ogden , C. Ordenovic , C. Pagani , I. Pagano , P. A. Palicio , L. Pallas-Quintela , A. Panahi , C. Panem , S. Payne-Wardenaar , L. Pegoraro , A. Penttilä , P. Pesciullesi , A. M. Piersimoni , M. Pinamonti , F. -X. Pineau , E. Plachy , G. Plum , E. Poggio , D. Pourbaix , A. Prša , L. Pulone , E. Racero , M. Rainer , C. M. Raiteri , P. Ramos , M. Ratajczak , P. Re Fiorentin , S. Regibo , C. Reylé , V. Ripepi , A. Riva , H. -W. Rix , G. Rixon , N. Robichon , C. Robin , M. Romero-Gómez , N. Rowell , F. Royer , K. A. Rybicki , G. Sadowski , A. Sáez Núñez , A. Sagristà Sellés , J. Sahlmann , V. Sanchez Gimenez , N. Sanna , R. Santoveña , M. Sarasso , C. Sarrate Riera , E. Sciacca , J. C. Segovia , D. Ségransan , S. Shahaf , A. Siebert , L. Siltala , E. Slezak , R. L. Smart , O. N. Snaith , E. Solano , F. Solitro , D. Souami , J. Souchay , L. Spina , E. Spitoni , F. Spoto , L. A. Squillante , I. A. Steele , H. Steidelmüller , J. Surdej , L. Szabados , F. Taris , M. B. Taylor , R. Teixeira , L. Tolomei , G. Torralba Elipe , M. Trabucchi , M. Tsantaki , A. Ulla , N. Unger , O. Vanel , A. Vecchiato , D. Vicente , S. Voutsinas , M. Weiler , Ł. Wyrzykowski , H. Zhao , J. Zorec , T. Zwitter , L. Balaguer-Núñez , N. Leclerc , S. Morgenthaler , G. Robert , S. Zucker

The {\Gaia} astrometric mission was approved by the European Space Agency in 2000 and the construction of the spacecraft and payload is on-going for a launch in late 2012. {\Gaia} will continuously scan the entire sky for 5 years, yielding…

Instrumentation and Methods for Astrophysics · Physics 2011-06-01 C. Jordi

To use libraries of observed stellar spectra, one needs to know the atmospheric parameters of the stars associated to those spectra. It is, however, hard to know what are the real levels of precision and accuracy of these parameters. To…

Solar and Stellar Astrophysics · Physics 2017-09-18 R. Smiljanic , A. J. Korn , A. R. Casey , the Gaia-ESO Survey consortium

Currently, most machine learning models are trained by centralized teams and are rarely updated. In contrast, open-source software development involves the iterative development of a shared artifact through distributed collaboration using a…

Spectral Toolkit of Algorithms for Graphs (STAG) is an open-source library for efficient graph algorithms. This technical report presents the newly implemented component on locality sensitive hashing, kernel density estimation, and fast…

Data Structures and Algorithms · Computer Science 2024-07-11 Peter Macgregor , He Sun

The most valuable asset of a space mission like Euclid are the data. Due to their huge volume, the automatic quality control becomes a crucial aspect over the entire lifetime of the experiment. Here we focus on the design strategy for the…

We present SkyCURTAINs, a data driven and model agnostic method to search for stellar streams in the Milky Way galaxy using data from the Gaia telescope. SkyCURTAINs is a weakly supervised machine learning algorithm that builds a background…

Astrophysics of Galaxies · Physics 2024-05-22 Debajyoti Sengupta , Stephen Mulligan , David Shih , John Andrew Raine , Tobias Golling

The NASA Exoplanet Archive and the Exoplanet Follow-up Observing Program service are two widely used resources for the exoplanet community. The NASA Exoplanet Archive provides a complete and accurate accounting of exoplanetary systems…

Automated text scoring (ATS) tasks, such as automated essay scoring and readability assessment, are important educational applications of natural language processing. Due to their interpretability of models and predictions, traditional…

Computation and Language · Computer Science 2021-04-09 Hitoshi Manabe , Masato Hagiwara

The Euclid satellite is an ESA mission scheduled for launch in September 2023. To optimally perform critical stages of the data reduction, such as object detection and morphology determination, a new and modern software package was…

Instrumentation and Methods for Astrophysics · Physics 2022-12-06 M. Kümmel , A. Álvarez-Ayllón , E. Bertin , P. Dubath , R. Gavazzi , W. Hartley , M. Schefer

The increased amount of high precision seismic data for solar-like stars calls for the existence of tools that can extract information from such data. In the case of the study of acoustic glitches there are no publicly available tools and…

Solar and Stellar Astrophysics · Physics 2017-11-08 L. F. R. Pereira , J. P. Faria , M. J. P. F. G. Monteiro

The Gaia satellite will survey the entire celestial sphere down to 20th magnitude, obtaining astrometry, photometry, and low resolution spectrophotometry on one billion astronomical sources, plus radial velocities for over one hundred…

New surveys such as ESA's Euclid mission are planned to map with unprecedented precision the large-scale structure of the Universe by measuring the 3D positions of tens of millions of galaxies. It is necessary to develop theoretically…

Context. Gaia is an ESA cornerstone mission launched on 19 December 2013 aiming to obtain the most complete and precise 3D map of our Galaxy by observing more than one billion sources. This paper is part of a series of documents explaining…

We present a sub-arcsecond cross-match of Gaia Data Release 3 (DR3) against the INT Galactic Plane Surveys (IGAPS) and the United Kingdom Infrared Deep Sky Survey (UKIDSS). The resulting cross-match of Galactic Plane Surveys (XGAPS)…

Astrophysics of Galaxies · Physics 2022-11-30 S. Scaringi , M. Monguio , C. Knigge , M. Fratta , B. Gaensicke , P. J. Groot , A. Rebassa-Mansergas , O. Toloza

The rapid growth of imaging and spectroscopic surveys has intensified the need for efficient tools that support visual inspection, a practice that remains essential for tasks such as classification, catalog refinement, and validation of…

Spatiotemporal techniques for signal coordination with actively transmitting extraterrestrial civilizations, without the need for prior communication, can constrain technosignature searches to a significantly smaller coordinate space. With…

Instrumentation and Methods for Astrophysics · Physics 2023-08-02 Andy Nilipour , James R. A. Davenport , Steve Croft , Andrew P. V. Siemion

This contribution to the Stellar Clusters & Associations: A RIA Workshop on Gaia deals with surveys of stars, in particular spectroscopic surveys, with attention to their impact on cluster studies, and their connectionwith Gaia. I review…

Astrophysics of Galaxies · Physics 2011-07-12 Sofia Feltzing

MOTIVATION: Microarray technology makes it possible to measure thousands of variables and to compare their values under hundreds of conditions. Once microarray data are quantified, normalized and classified, the analysis phase is…

Quantitative Methods · Quantitative Biology 2007-09-11 Claude Pasquier , Fabrice Girardot , Karim Jevardat De Fombelle , Richard Christen