{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,10,12]],"date-time":"2025-10-12T01:51:48Z","timestamp":1760233908764,"version":"build-2065373602"},"reference-count":20,"publisher":"MDPI AG","issue":"3","license":[{"start":{"date-parts":[[2021,3,8]],"date-time":"2021-03-08T00:00:00Z","timestamp":1615161600000},"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 dataset of Stark widths for Tb II, Tb III and Tb IV is presented. To data obtained before, the results of new calculations for 62 Tb III lines from 5d to 6pj(6,j)o, a transition array, have been added. Calculations have been performed by using the simplified modified semiempirical method for temperatures from 5000 to 80,000 K for an electron density of 1017 cm\u22123. The results were also used to discuss the regularities within multiplets and a supermultiplet.<\/jats:p>","DOI":"10.3390\/data6030028","type":"journal-article","created":{"date-parts":[[2021,3,8]],"date-time":"2021-03-08T04:01:25Z","timestamp":1615176085000},"page":"28","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":0,"title":["Stark Width Data for Tb II, Tb III and Tb IV Spectral Lines"],"prefix":"10.3390","volume":"6","author":[{"ORCID":"https:\/\/orcid.org\/0000-0001-9138-8642","authenticated-orcid":false,"given":"Milan S.","family":"Dimitrijevi\u0107","sequence":"first","affiliation":[{"name":"Astronomical Observatory, 11060 Belgrade, Serbia"},{"name":"Sorbonne Universit\u00e9, Observatoire de Paris, Universit\u00e9 PSL, CNRS, LERMA, F-92190 Meudon, France"}]}],"member":"1968","published-online":{"date-parts":[[2021,3,8]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"795","DOI":"10.1051\/0004-6361:20021801","article-title":"The electron-impact broadening parameters for Co III spectral lines","volume":"399","year":"2003","journal-title":"A&A"},{"key":"ref_2","doi-asserted-by":"crossref","first-page":"375","DOI":"10.1051\/0004-6361:20034162","article-title":"Importance of collisions with charged particles for stellar UV line shapes: Cd III","volume":"417","year":"2004","journal-title":"A&A"},{"key":"ref_3","doi-asserted-by":"crossref","first-page":"871","DOI":"10.1111\/j.1365-2966.2008.13284.x","article-title":"Atomic data and electron-impact broadening effect in DO white dwarf atmospheres: SiVI","volume":"387","author":"Hamdi","year":"2008","journal-title":"MNRAS"},{"key":"ref_4","doi-asserted-by":"crossref","first-page":"133","DOI":"10.1007\/BF02743638","article-title":"Broadening and self-absorption of the resonance lines of H-like light ions in laser-produced plasmas","volume":"48","author":"Nicolosi","year":"1978","journal-title":"Nuovo Cimento B"},{"key":"ref_5","doi-asserted-by":"crossref","first-page":"4010","DOI":"10.1103\/PhysRevA.45.4010","article-title":"Measurements of line broadening of B V H\u03b1 and L\u03b4 in a laser-produced plasma","volume":"45","author":"Wang","year":"1992","journal-title":"Phys. Rev. A"},{"key":"ref_6","doi-asserted-by":"crossref","first-page":"361","DOI":"10.1016\/S0022-4073(98)00002-8","article-title":"Stark Broadening Parameters of Analogous Spectral Lines Along the Lithium and Beryllium Isoelectronic Sequences","volume":"61","year":"1999","journal-title":"J. Quant. Spectrosc. Radiat. Transf."},{"key":"ref_7","doi-asserted-by":"crossref","first-page":"327","DOI":"10.1023\/A:1001140202851","article-title":"UV Line Profiles of B IV from a 10-Ps Krf-Laser-Produced Plasma","volume":"256","author":"Iglesias","year":"1997","journal-title":"Astrophys. Space Sci."},{"key":"ref_8","doi-asserted-by":"crossref","first-page":"36","DOI":"10.1016\/j.optlastec.2015.05.012","article-title":"Laser controlled melting of H12 hot-work tool steel with B4C particles at the surface","volume":"74","author":"Yilbas","year":"2015","journal-title":"Opt. Laser Technol."},{"key":"ref_9","doi-asserted-by":"crossref","first-page":"A93","DOI":"10.1051\/0004-6361\/201423826","article-title":"High-resolution abundance analysis of very metal-poor r-I stars","volume":"565","author":"Hill","year":"2014","journal-title":"Astron. Astrophys."},{"key":"ref_10","doi-asserted-by":"crossref","first-page":"4126","DOI":"10.1093\/mnras\/stu2406","article-title":"Time resolved spectroscopy of the cool Ap star HD 213637","volume":"446","author":"Elkin","year":"2015","journal-title":"MNRAS"},{"key":"ref_11","first-page":"323","article-title":"Spectroscopic study of pulsations in the atmosphere of roAp star 10 Aql","volume":"38","author":"Sachkov","year":"2008","journal-title":"Contrib. Astron. Obs. Skalnat\u00e9 Pleso"},{"key":"ref_12","doi-asserted-by":"crossref","first-page":"299","DOI":"10.1046\/j.1365-8711.2000.03578.x","article-title":"Abundances in Przybylski\u2019s star","volume":"317","author":"Cowley","year":"2000","journal-title":"MNRAS"},{"key":"ref_13","first-page":"122","article-title":"Stark broadening data for spectral lines of rare-earth elements: Example of Tb II and Tb IV","volume":"50","year":"2020","journal-title":"Contrib. Astron. Obs. Skalnat\u00e9 Pleso"},{"key":"ref_14","doi-asserted-by":"crossref","first-page":"72","DOI":"10.5937\/univtho10-26397","article-title":"Stark broadening of Tb III spectral lines originating from 6s-6p transitions","volume":"10","year":"2020","journal-title":"University Thought"},{"key":"ref_15","first-page":"345","article-title":"Simple estimates for Stark broadening of ion lines in stellar plasma","volume":"172","year":"1987","journal-title":"Astron. Astrophys."},{"key":"ref_16","first-page":"1","article-title":"Atomic Energy Levels: The Rare-Earth Elements","volume":"60","author":"Martin","year":"1978","journal-title":"Nat. Stand. Ref. Data Ser. NSRDS-NBS"},{"key":"ref_17","unstructured":"Kramida, A., Ralchenko, Y., Reader, J., and NIST ASD Team (2021, January 21). NIST Atomic Spectra Database, ver. 5.5.1, Available online: https:\/\/physics.nist.gov\/asd."},{"key":"ref_18","doi-asserted-by":"crossref","first-page":"185","DOI":"10.1016\/0022-4073(82)90022-X","article-title":"Regularities and similarities in plasma broadened spectral line widths (Stark widths)","volume":"28","author":"Wiese","year":"1982","journal-title":"J. Quant. Spectrosc. Radiat. Transf."},{"key":"ref_19","doi-asserted-by":"crossref","first-page":"357","DOI":"10.3390\/atoms2030357","article-title":"On the Application of Stark Broadening Data Determined with a Semiclassical Perturbation Approach","volume":"2","year":"2014","journal-title":"Atoms"},{"key":"ref_20","doi-asserted-by":"crossref","unstructured":"Dimitrijevi\u0107, M.S. (2020). Forty years of the applications of Stark broadening data determined with the modified semiempirical method. Data, 5.","DOI":"10.3390\/data5030073"}],"container-title":["Data"],"original-title":[],"language":"en","link":[{"URL":"https:\/\/www.mdpi.com\/2306-5729\/6\/3\/28\/pdf","content-type":"unspecified","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2025,10,11]],"date-time":"2025-10-11T05:34:38Z","timestamp":1760160878000},"score":1,"resource":{"primary":{"URL":"https:\/\/www.mdpi.com\/2306-5729\/6\/3\/28"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2021,3,8]]},"references-count":20,"journal-issue":{"issue":"3","published-online":{"date-parts":[[2021,3]]}},"alternative-id":["data6030028"],"URL":"https:\/\/doi.org\/10.3390\/data6030028","relation":{},"ISSN":["2306-5729"],"issn-type":[{"type":"electronic","value":"2306-5729"}],"subject":[],"published":{"date-parts":[[2021,3,8]]}}}