{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,10,10]],"date-time":"2025-10-10T01:40:38Z","timestamp":1760060438526,"version":"build-2065373602"},"reference-count":20,"publisher":"MDPI AG","issue":"9","license":[{"start":{"date-parts":[[2025,8,31]],"date-time":"2025-08-31T00:00:00Z","timestamp":1756598400000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Data"],"abstract":"<jats:p>A data set on Stark broadening parameters defining the Lorentzian line profile (spectral line widths and shifts) for 31 multiplets of four-times-charged nitrogen ion (N V), with lines broadened by impacts with electrons (e), protons (p), He II ions, \u03b1 particles (He III), and B III, B IV, B V, and B VI ions, is given. The above-mentioned data have been calculated within the frame of the semiclassical perturbation theory, for temperatures from 50,000 K to 1,000,000 K, and densities of perturbers from 1015 cm\u22123 up to 1021 cm\u22123. These data are, first of all, of interest for diagnostics and modeling of laser-driven plasma in experiments and investigations of proton\u2013boron fusion, especially when the target is boron nitride (BN). Data on Stark broadening by collisions with e, p, He II ions, and \u03b1 particles are useful for the investigation of stellar plasma, in particular for white dwarf atmospheres and subphotospheric layer modeling.<\/jats:p>","DOI":"10.3390\/data10090140","type":"journal-article","created":{"date-parts":[[2025,9,1]],"date-time":"2025-09-01T08:28:15Z","timestamp":1756715295000},"page":"140","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":0,"title":["Data on Stark Broadening of N V Spectral Lines"],"prefix":"10.3390","volume":"10","author":[{"ORCID":"https:\/\/orcid.org\/0000-0001-9138-8642","authenticated-orcid":false,"given":"Milan S.","family":"Dimitrijevi\u0107","sequence":"first","affiliation":[{"name":"Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia"},{"name":"LUX (Laboratoire d\u2019\u00e9tude de l\u2019Univers et des Ph\u00e9nom\u00e8nes Extr\u00e8mes) Observatoire de Paris, Universit\u00e9 PSL (Paris Sciences & Lettres), CNRS (Centre National de la Recherche Scientifique), Sorbonne Universit\u00e9, F-92190 Meudon, France"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-6851-5436","authenticated-orcid":false,"given":"Magdalena D.","family":"Christova","sequence":"additional","affiliation":[{"name":"Department of Applied Physics, Technical University of Sofia, 1000 Sofia, Bulgaria"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-2348-2044","authenticated-orcid":false,"given":"Sylvie","family":"Sahal-Br\u00e9chot","sequence":"additional","affiliation":[{"name":"LUX (Laboratoire d\u2019\u00e9tude de l\u2019Univers et des Ph\u00e9nom\u00e8nes Extr\u00e8mes) Observatoire de Paris, Universit\u00e9 PSL (Paris Sciences & Lettres), CNRS (Centre National de la Recherche Scientifique), Sorbonne Universit\u00e9, F-92190 Meudon, France"}],"role":[{"role":"author","vocabulary":"crossref"}]}],"member":"1968","published-online":{"date-parts":[[2025,8,31]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"C09012","DOI":"10.1088\/1748-0221\/18\/09\/C09012","article-title":"Perspectives on research on laser driven proton-boron fusion and applications","volume":"18","author":"Batani","year":"2023","journal-title":"J. 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