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dc.contributor.authorHolmbeck, EM
dc.contributor.authorHansen, TT
dc.contributor.authorBeers, TC
dc.contributor.authorPlacco, VM
dc.contributor.authorWhitten, DD
dc.contributor.authorRasmussen, KC
dc.contributor.authorRoederer, IU
dc.contributor.authorEzzeddine, R
dc.contributor.authorSakari, CM
dc.contributor.authorFrebel, A
dc.contributor.authorDrout, MR
dc.contributor.authorSimon, JD
dc.contributor.authorThompson, IB
dc.contributor.authorBland-Hawthorn, J
dc.contributor.authorGibson, BK
dc.contributor.authorGrebel, EK
dc.contributor.authorKordopatis, G
dc.contributor.authorKunder, A
dc.contributor.authorMeléndez, J
dc.contributor.authorNavarro, JF
dc.contributor.authorReid, WA
dc.contributor.authorSeabroke, G
dc.contributor.authorSteinmetz, M
dc.contributor.authorWatson, F
dc.contributor.authorWyse, RFĠ
dc.date.accessioned2021-09-20T18:22:23Z
dc.date.available2021-09-20T18:22:23Z
dc.identifier.urihttps://hdl.handle.net/1721.1/132439
dc.description.abstract© 2020. The American Astronomical Society. All rights reserved. This compilation is the fourth data release from the R-Process Alliance (RPA) search for r-process-enhanced stars and the second release based on "snapshot"high-resolution (R ∼ 30,000) spectra collected with the du Pont 2.5 m Telescope. In this data release, we propose a new delineation between the r-I and r-II stellar classes at, instead of the empirically chosen level previously in use, based on statistical tests of the complete set of RPA data released to date. We also statistically justify the minimum level of [Eu/Fe] for definition of the r-I stars, [Eu/Fe] > +0.3. Redefining the separation between r-I and r-II stars will aid in the analysis of the possible progenitors of these two classes of stars and determine whether these signatures arise from separate astrophysical sources at all. Applying this redefinition to previous RPA data, the number of identified r-II and r-I stars changes to 51 and 121, respectively, from the initial set of data releases published thus far. In this data release, we identify 21 new r-II, 111 new r-I (plus 3 re-identified), and 7 new (plus 1 re-identified) limited-r stars out of a total of 232 target stars, resulting in a total sample of 72 new r-II stars, 232 new r-I stars, and 42 new limited-r stars identified by the RPA to date.en_US
dc.language.isoen
dc.publisherAmerican Astronomical Societyen_US
dc.relation.isversionof10.3847/1538-4365/ab9c19en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceThe American Astronomical Societyen_US
dc.titleThe R-Process Alliance: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Haloen_US
dc.typeArticleen_US
dc.relation.journalAstrophysical Journal, Supplement Seriesen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2020-10-23T16:12:48Z
dspace.orderedauthorsHolmbeck, EM; Hansen, TT; Beers, TC; Placco, VM; Whitten, DD; Rasmussen, KC; Roederer, IU; Ezzeddine, R; Sakari, CM; Frebel, A; Drout, MR; Simon, JD; Thompson, IB; Bland-Hawthorn, J; Gibson, BK; Grebel, EK; Kordopatis, G; Kunder, A; Meléndez, J; Navarro, JF; Reid, WA; Seabroke, G; Steinmetz, M; Watson, F; Wyse, RFĠen_US
dspace.date.submission2020-10-23T16:13:00Z
mit.journal.volume249en_US
mit.journal.issue2en_US
mit.licensePUBLISHER_POLICY
mit.metadata.statusAuthority Work and Publication Information Needed


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