A calibrant-free drift compensation method for gas sensor arrays

Autor: Maho, Pierre, Herrier, Cyril, Livache, Thierry, Comon, Pierre, Barthelmé, Simon

Publikováno v: In Chemometrics and Intelligent Laboratory Systems 15 June 2022 225

A calibrant-free drift compensation method for gas sensor arrays

Autor: Maho, Pierre, Herrier, Cyril, Livache, Thierry, Comon, Pierre, Barthelme, Simon

Gas sensors lack repeatability over time. They are affected by drift, the result of changes at the sensor level and in the environment. A solution is to design software methods that compensate for the drift. Existing methods are often based on calibr

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b6a86d5037fb6b2389be14ab00392c35
https://hal.archives-ouvertes.fr/hal-03409223/document

Signal Processing for Artificial Olfaction

Autor: Maho, Pierre

Publikováno v: Signal and Image processing. Université Grenoble Alpes [2020-..], 2020. English. ⟨NNT : 2020GRALT040⟩

In Nature, olfaction is a key sense used by most species of animals for detecting, tracking and recognizing odors in the environment. An electronic nose is an instrument that takes inspiration from natural olfaction in order to detect volatile compou

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::e2d6d73068472f48db654573219ad297
https://tel.archives-ouvertes.fr/tel-03276312/document

Tracking the Lyman alpha emission line in the CircumGalactic Medium in MUSE data

Autor: Bacher, Raphael, Maho, Pierre, Chatelain, Florent, Michel, Olivier

Publikováno v: Mathematical Tools for Instrumentation & Signal Processing in Astronomy
D. Mary; R. Flamary; C. Theys and C. Aime. Mathematical Tools for Instrumentation & Signal Processing in Astronomy, 78-79, EDP Sciences, pp.233-245, 2016, EAS Publications Series, 978-2-7598-9006-4. ⟨10.1051/eas/1678011⟩

International audience; Since 2014, the Multi Unit Spectroscopic Explorer (MUSE) instrument generates hyperspectral datacubes (300 by 300 pixels by 3600 wavelength in the visible range) of the deep Universe. One of the main purposes of the wide field

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::b7107560e5d024cfabaa5dd41d215dd5
https://hal.archives-ouvertes.fr/hal-01503524