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- publication . Article . 2020Open AccessAuthors:Thomas Arnold; Georg Boehm; Faezeh Kazemi;Persistent IdentifiersPublisher: EDP Sciences
Atmospheric pressure plasma jet machining technology provides a flexible and efficient way to fabricate precise freeform optics. Due to the pure chemical material removal mechanism based on a dry etching process using fluorine containing gas, the choice of materials tha...
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You have already added works in your ORCID record related to the merged research outcome. - publication . Article . Preprint . 2016Open Access EnglishAuthors:Mancini, Mattia; Schneider, Raffaella; Graziani, Luca; Valiante, Rosa; Dayal, Pratika; Maio, Umberto; Ciardi, Benedetta;Persistent IdentifiersCountries: Netherlands, ItalyProject: EC | FIRST (306476)
We attempt to interpret existing data on the evolution of the UV luminosity function and UV colours, $\beta$, of galaxies at $5 \leq z \leq 8$, to improve our understanding of their dust content and ISM properties. To this aim, we post-process the results of a cosmologi...
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You have already added works in your ORCID record related to the merged research outcome. - publication . Article . Preprint . 2018Open AccessAuthors:Ehlert, K; Weinberger, R; Pfrommer, C; Pakmor, R; Springel, V;Persistent IdentifiersProject: EC | EXAGAL (308037), EC | CRAGSMAN (646955)
Feedback processes by active galactic nuclei in the centres of galaxy clusters appear to prevent large-scale cooling flows and impede star formation. However, the detailed heating mechanism remains uncertain. One promising heating scenario invokes the dissipation of Alf...
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You have already added works in your ORCID record related to the merged research outcome. - publication . Preprint . Other literature type . Article . 2021Open Access EnglishAuthors:A. Ansmann; K. Ohneiser; R.-E. Mamouri; R.-E. Mamouri; D. A. Knopf; I. Veselovskii; H. Baars; R. Engelmann; A. Foth; C. Jimenez; ...Persistent IdentifiersPublisher: Copernicus PublicationsCountry: CyprusProject: EC | ACTRIS-2 (654109), EC | ACTRIS PPP (739530)
Abstract. We present retrievals of tropospheric and stratospheric height profiles of particle mass, volume, surface area, and number concentrations in the case of wildfire smoke layers as well as estimates of smoke-related cloud condensation nuclei (CCN) and ice-nucleat...
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You have already added works in your ORCID record related to the merged research outcome. - publication . Article . 2020Open Access EnglishAuthors:Nenad Manojlovic; Igor Salom;Persistent Identifiers
doi: 10.3390/sym12030352
handle: 10400.1/13816
Publisher: MDPICountry: PortugalIn this paper we deal with the trigonometric Gaudin model, generalized using a nontrivial triangular reflection matrix (corresponding to non-periodic boundary conditions in the case of anisotropic XXZ Heisenberg spin-chain). In order to obtain the generating function of...
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You have already added works in your ORCID record related to the merged research outcome. - publication . Article . Preprint . 2017Open Access EnglishAuthors:Timothy R. White; Othman Benomar; V. Silva Aguirre; Warrick H. Ball; Timothy R. Bedding; William J. Chaplin; Jørgen Christensen-Dalsgaard; Rafael A. García; Laurent Gizon; Dennis Stello; ...Persistent IdentifiersPublisher: HAL CCSDCountries: France, United Kingdom, DenmarkProject: EC | ASTERISK (267864), ANR | IDEE (ANR-12-BS05-0008), EC | STELLARAGES (338251)
Binary star systems are important for understanding stellar structure and evolution, and are especially useful when oscillations can be detected and analysed with asteroseismology. However, only four systems are known in which solar-like oscillations are detected in bot...
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You have already added works in your ORCID record related to the merged research outcome. - publication . Article . Preprint . 2019Open AccessAuthors:Ikonnikova, N P; Parthasarathy, M; Dodin, A V; Hubrig, S; Sarkar, G;Persistent IdentifiersPublisher: Oxford University Press (OUP)
The high-resolution ($R\sim48\,000$) optical spectrum of the B-type supergiant LS 5112, identified as the optical counterpart of the post-AGB candidate IRAS 18379-1707, is analysed. We report the detailed identifications of the observed absorption and emission features ...
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You have already added works in your ORCID record related to the merged research outcome. - publication . Article . Preprint . 2016Open AccessAuthors:Adriá n Martí nez, S; Ageron, M; Aharonian, F; Aiello, S; Albert, A; Ameli, F; Anassontzis, E; Andre, M; ...Persistent IdentifiersCountries: Spain, Spain, Netherlands, United Kingdom, Spain, Germany, France, France, Italy, Italy ...Project: EC | KM3NET-PP (212525), ANR | UnivEarthS (ANR-10-LABX-0023), ANR | USPC (ANR-11-IDEX-0005)
The main objectives of the KM3NeT Collaboration are (i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and (ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly motivated by two recent importan...
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You have already added works in your ORCID record related to the merged research outcome. - publication . Article . 2019Open Access EnglishAuthors:Roza Timakova; Sergey Tikhonov; Nataliya Tikhonova; Sergey V. Shikhalev;Persistent IdentifiersPublisher: MDPI AG
The aim of this article is to develop a method for determining the dose of radiation in the processing of chilled fish and its effect on the antioxidant activity and thermophysical characteristics of muscle tissue. Radiation processing of chilled fish was performed usin...
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You have already added works in your ORCID record related to the merged research outcome. - publication . Article . Preprint . 2016Open Access EnglishAuthors:Gonneau, A.; Lançon, A.; Trager, S.C.; Aringer, B.; Lyubenova, M.; Nowotny, Walter; Peletier, R.F.; Prugniel, P.; Chen, Y.-P.; Dries, M.; ...Persistent IdentifiersCountries: France, Spain, United Kingdom, NetherlandsProject: FWF | Tracing the origins of co... (P 21988), EC | STARKEY (615604)
We provide a new collection of spectra of 35 carbon stars obtained with the ESO/VLT X-shooter instrument as part of the X-shooter Spectral Library project. The spectra extend from 0.3$\mu$m to 2.4$\mu$m with a resolving power above $\sim$ 8000. The sample contains stars...
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You have already added works in your ORCID record related to the merged research outcome.