Combined spatial and retrospective analysis of fluoroalkyl chemicals in fluvial sediments reveal changes in levels and patterns over the last 40 years

Autor: J. Raux, Pierre Labadie, Marc Desmet, Marc Babut, Hélène Budzinski, Cécile Grosbois, Yoann Copard, Patrick Pardon, Brice Mourier, Maxime Debret

Publikováno v: Environmental Pollution
Environmental Pollution, Elsevier, 2019, 253 (253), pp.1117-1125. ⟨10.1016/j.envpol.2019.07.079⟩
Environmental Pollution, Elsevier, 2019, 253, pp.1117-1125. ⟨10.1016/j.envpol.2019.07.079⟩

International audience; Bed sediments and a dated sediment core were collected upstream and downstream from the city of Lyon (France) to assess the spatial and temporal trends of contamination by per- and polyfluoroalkyl substances (PFASs) in this se

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::396bd93250d39793c3964658219b8cb6
https://hal.archives-ouvertes.fr/hal-02282820/document

Supernova photometric data analysis and reduction details

Autor: J. Raux

Publikováno v: New Astronomy Reviews. 48:641-645

This paper presents reduction methods in photometric analysis, currently used for type Ia supernova surveys.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::778366fd269fd8f1ba824decaffff75d
https://doi.org/10.1016/j.newar.2003.12.041

Discovery of Very-High-Energy Gamma-Rays from the Galactic Centre Ridge

Autor: V. Sahakian, Conor Masterson, Michael Punch, D. Hauser, M. Beilicke, A. Djannati-Ataï, C. Stegmann, Stefan Gillessen, G. Fontaine, Christo Venter, B. Degrange, Wystan Benbow, J. L. Osborne, F. Feinstein, Luigi Costamante, L. O'c. Drury, F. Breitling, Dieter Horns, M. Lemoine-Goumard, M. Tluczykont, A. M. Brown, Helene Sol, P. Espigat, N. Leroy, Gavin Rowell, Konrad Bernlöhr, R. Le Gallou, J.-P. Tavernet, P. M. Chadwick, M. Panter, L. Rolland, G. Pühlhofer, G. Heinzelmann, I. J. Latham, A. Reimer, Olaf Reimer, A. Lemiere, M. de Naurois, Nu. Komin, R. Cornils, S. J. Nolan, Martin Raue, M. Hauser, Ullrich Schwanke, P. Goret, A. G. Akhperjanian, S. M. Rayner, R. Steenkamp, C. G. Théoret, Jim Hinton, Guy Pelletier, Ilana M. Braun, Sven Klages, J. Raux, K. J. Orford, M. Siewert, C. van Eldik, O. Bolz, M. Holleran, A. Noutsos, P. Vincent, S. Schlenker, Werner Hofmann, Y. Fuchs, Felix Aharonian, T. J. L. McComb, A. Jacholkowska, A. Konopelko, Heinrich J. Völk, Gilles Henri, Reinhard Schlickeiser, Dimitrios Emmanoulopoulos, V. Borrel, Hugh Dickinson, A. R. Bazer-Bachi, B. Giebels, O. C. de Jager, Stefan Wagner, J. Ripken, L. Saugé, Stefan Funk, Jean Michel Martin, David Berge, Thomas Lohse, D. Spangler, Catherine Boisson, S. Pita, B. Khélifi, G. Hermann, Regis Terrier, Y. A. Gallant, C. Schuster, B. C. Raubenheimer, J. F. Glicenstein, O. Martineau-Huynh, L. Rob, M. Ouchrif, G. Vasileiadis, C. Hadjichristidis, Guillaume Dubus, L.-M. Chounet, A. Marcowith

Publikováno v: Nature
Nature, Nature Publishing Group, 2006, 439, pp.695-698. ⟨10.1038/nature04467⟩
Nature, 2006, 439, pp.695-698. ⟨10.1038/nature04467⟩
Nature, 2006, Vol.439(7077), pp.695-698 [Peer Reviewed Journal]

The origin of Galactic cosmic rays (with energies up to 10^15 eV) remains unclear, though it is widely believed that they originate in the shock waves of expanding supernova remnants. Currently the best way to investigate their acceleration and propa

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7dfef5d58a7fdb8b3c871dbee7df2b6
http://hal.in2p3.fr/in2p3-00025901

Spectroscopic confirmation of high-redshift supernovae with the ESO VLT ***

Autor: Vallery Stanishev, Peter Nugent, Nobunari Kashikawa, Alex Conley, Chris Lidman, A. G. Kim, Mamoru Doi, Bradley E. Schaefer, D. A. Howell, Vitaliy Fadeyev, W. M. Wood-Vasey, A. L. Spadafora, J. Raux, Tomoki Morokuma, Nicholas A. Walton, I. M. Hook, Naoki Yasuda, K. Schahmaneche, P. Antilogus, Greg Aldering, G. Goldhaber, V. Prasad, Robert Quimby, Kentaro Motohara, R. A. Knop, R. Gibbons, S. Nobili, Reynald Pain, Pierre Astier, Brian C. Lee, Guillermo A. Blanc, M. S. Burns, Saul Perlmutter, Eric P. Smith, Sebastien Fabbro, Nicolas Regnault, Ariel Goobar, G. Sainton, Lifan Wang, S. E. Deustua, Gastón Folatelli, Richard S. Ellis, Javier Méndez, Rahman Amanullah, Donald E. Groom, G. Garavini, Pilar Ruiz-Lapuente

Publikováno v: Astronomy & Astrophysics, vol 430, iss 3
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2005, 430, pp.843-851. ⟨10.1051/0004-6361:20041504⟩
Astronomy and Astrophysics, vol 430, iss 3
Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 430, pp.843-851. ⟨10.1051/0004-6361:20041504⟩
Lidman, C; Howell, DA; Folatelli, G; Garavini, G; Nobili, S; Aldering, G; et al.(2005). Spectroscopic confirmation of high-redshift supernovae with the ESO VLT. Astronomy and Astrophysics, 430(3), 843-851. doi: 10.1051/0004-6361:20041504. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/2vx7q9f0

We present VLT FORS1 and FORS2 spectra of 39 candidate high-redshift supernovae that were discovered as part of a cosmological study using Type Ia supernovae (SNe Ia) over a wide range of redshifts. From the spectra alone, 20 candidates are spectrall

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::93f4d055c1e70883e121aef7f6eed715
https://escholarship.org/uc/item/2vx7q9f0

A search for very high energy gamma-ray emission from the starburst galaxy NGC 253 with H.E.S.S

Autor: F. Aharonian, A. G. Akhperjanian, A. R. Bazer-Bachi, M. Beilicke, W. Benbow, D. Berge, K. Bernlöhr, C. Boisson, O. Bolz, V. Borrel, I. Braun, F. Breitling, A. M. Brown, P. M. Chadwick, L.-M. Chounet, R. Cornils, L. Costamante, B. Degrange, H. J. Dickinson, A. Djannati-Ataï, null L. O'C. Drury, G. Dubus, D. Emmanoulopoulos, P. Espigat, F. Feinstein, G. Fontaine, Y. Fuchs, S. Funk, Y. A. Gallant, B. Giebels, S. Gillessen, J. F. Glicenstein, P. Goret, C. Hadjichristidis, M. Hauser, G. Heinzelmann, G. Henri, G. Hermann, J. A. Hinton, W. Hofmann, M. Holleran, D. Horns, A. Jacholkowska, O. C. de Jager, B. Khélifi, Nu. Komin, A. Konopelko, I. J. Latham, R. Le Gallou, A. Lemière, M. Lemoine-Goumard, N. Leroy, T. Lohse, J. M. Martin, O. Martineau-Huynh, A. Marcowith, C. Masterson, T. J. L. McComb, M. de Naurois, S. J. Nolan, A. Noutsos, K. J. Orford, J. L. Osborne, M. Ouchrif, M. Panter, G. Pelletier, S. Pita, G. Pühlhofer, M. Punch, B. C. Raubenheimer, M. Raue, J. Raux, S. M. Rayner, A. Reimer, O. Reimer, J. Ripken, L. Rob, L. Rolland, G. Rowell, V. Sahakian, L. Saugé, S. Schlenker, R. Schlickeiser, C. Schuster, U. Schwanke, M. Siewert, H. Sol, D. Spangler, R. Steenkamp, C. Stegmann, J.-P. Tavernet, R. Terrier, C. G. Théoret, M. Tluczykont, G. Vasileiadis, C. Venter, P. Vincent, H. J. Völk, S. J. Wagner

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2005, 442, pp.177-183. ⟨10.1051/0004-6361:20053521⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 442, pp.177-183. ⟨10.1051/0004-6361:20053521⟩
Astrophysics & Astronomy

We present the result of 28 hours of observations of the nearby starburst galaxy NGC 253 with the H.E.S.S. detector in 2003. We find no evidence for very high energy gamma-ray emission from this object. Gamma-ray emission above 400 GeV from NGC 253 h

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::238fcc36948301c6f383fa2bc6f7df3a
https://hal.in2p3.fr/in2p3-00024438