|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| BPS BS 17569-0049 , the SIMBAD biblio (40 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST04:26:19 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 2000AJ....120.1516A | 349 | 22 | The INT search for metal-poor stars: spectroscopic observations and classification via artificial neural networks. | ALLENDE PRIETO C., REBOLO R., GARCIA LOPEZ R.J., et al. | |||||
|
2004A&A...416.1117C |
8 | 37 | 976 | First stars. V - Abundance patterns from C to Zn and supernova yields in the early Galaxy. | CAYREL R., DEPAGNE E., SPITE M., et al. | ||||
| 2005A&A...430..655S | 3 | 35 | 361 | First stars VI - Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements. | SPITE M., CAYREL R., PLEZ B., et al. | ||||
|
2005AJ....130.2804R |
166 | 34 | Estimation of carbon abundances in metal-poor stars. I. Application to the strong G-band stars of Beers, Preston, and Shectman. | ROSSI S., BEERS T.C., SNEDEN C., et al. | |||||
| 2006A&A...455..291S | 1 | 35 | 138 | First stars IX - Mixing in extremely metal-poor giants. Variation of the 12C/13C, [Na/Mg] and [Al/Mg] ratios. | SPITE M., CAYREL R., HILL V., et al. | ||||
|
2007ApJS..168..128B |
15 | D | 1852 | 38 | Broadband UBVRCIC photometry of horizontal-branch and metal-poor candidates from the HK and Hamburg/ESO surveys. I. | BEERS T.C., FLYNN C., ROSSI S., et al. | |||
| 2007A&A...464.1081A | 55 | 100 | NLTE determination of the sodium abundance in a homogeneous sample of extremely metal-poor stars. | ANDRIEVSKY S.M., SPITE M., KOROTIN S.A., et al. | |||||
| 2007A&A...476..935F | 239 | D | X C | 6 | 34 | 252 | First stars. VIII. Enrichment of the neutron-capture elements in the early Galaxy. | FRANCOIS P., DEPAGNE E., HILL V., et al. | |
| 2008A&A...481..481A | 16 | D | 1 | 52 | 114 | NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars. | ANDRIEVSKY S.M., SPITE M., KOROTIN S.A., et al. | ||
| 2009A&A...494.1083A | 90 | D | C | 2 | 41 | 57 | Evolution of the barium abundance in the early galaxy from a NLTE analysis of the Ba lines in a homogeneous sample of EMP stars. | ANDRIEVSKY S.M., SPITE M., KOROTIN S.A., et al. | |
| 2009PASJ...61..563T | 15 | D | 1 | 42 | 15 | Potassium abundances in red giants of mildly to very metal-poor globular clusters. | TAKEDA Y., KANEKO H., MATSUMOTO N., et al. | ||
|
2009A&A...501..519B |
16 | D | 2 | 58 | 187 | First stars. XII. Abundances in extremely metal-poor turnoff stars, and comparison with the giants. | BONIFACIO P., SPITE M., CAYREL R., et al. | ||
| 2010A&A...509A..88A | 15 | D | 1 | 54 | 90 | Non-LTE abundances of Mg and K in extremely metal-poor stars and the evolution of [O/Mg], [Na/Mg], [Al/Mg], and [K/Mg] in the Milky way. | ANDRIEVSKY S.M., SPITE M., KOROTIN S.A., et al. | ||
|
2010A&A...509A..93M |
15 | D | 2 | 181 | 196 | A holistic approach to carbon-enhanced metal-poor stars. | MASSERON T., JOHNSON J.A., PLEZ B., et al. | ||
|
2010A&A...515A.111S |
15 | D | 1 | 17230 | 227 | The PASTEL catalogue of stellar parameters. | SOUBIRAN C., LE CAMPION J.-F., CAYREL DE STROBEL G., et al. | ||
|
2010ApJ...724..975R |
15 | D | 1 | 197 | 141 | The ubiquity of the rapid neutron-capture process. | ROEDERER I.U., COWAN J.J., KARAKAS A.I., et al. | ||
| 2011A&A...528A...9S | 15 | D | 2 | 55 | 39 | First stars. XIV. Sulfur abundances in extremely metal-poor stars. | SPITE M., CAFFAU E., ANDRIEVSKY S.M., et al. | ||
| 2011A&A...530A.105A | 15 | D | 1 | 60 | 49 | NLTE strontium abundance in a sample of extremely metal poor stars and the Sr/Ba ratio in the early Galaxy. | ANDRIEVSKY S.M., SPITE F., KOROTIN S.A., et al. | ||
|
2012A&A...541A.143S |
15 | D | 1 | 55 | 38 | NLTE determination of the calcium abundance and 3D corrections in extremely metal-poor stars. | SPITE M., ANDRIEVSKY S.M., SPITE F., et al. | ||
|
2013ApJ...762...26Y |
15 | D | 1 | 198 | 263 | The most metal-poor stars. II. Chemical abundances of 190 metal-poor stars including 10 new stars with [Fe/H] ≤ -3.5. | YONG D., NORRIS J.E., BESSELL M.S., et al. | ||
| 2013A&A...551A..57H | 15 | D | O | 1 | 73 | 63 | LTE or non-LTE, that is the question. The NLTE chemical evolution of strontium in extremely metal-poor stars. | HANSEN C.J., BERGEMANN M., CESCUTTI G., et al. | |
|
2014ApJ...788..180C |
15 | D | 1 | 329 | 52 | Carbon-enhanced metal-poor stars: CEMP-s and CEMP-no subclasses in the halo system of the Milky Way. | CAROLLO D., FREEMAN K., BEERS T.C., et al. | ||
|
2014ApJ...797...21P |
15 | D | 2 | 606 | 226 | Carbon-enhanced metal-poor star frequencies in the galaxy: corrections for the effect of evolutionary status on carbon abundances. | PLACCO V.M., FREBEL A., BEERS T.C., et al. | ||
|
2016A&A...591A.118S |
16 | D | 1 | 31408 | 141 | The PASTEL catalogue: 2016 version. | SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al. | ||
| 2018A&A...611A..30S | 241 | X C | 5 | 21 | 14 | Abundance patterns of the light neutron-capture elements in very and extremely metal-poor stars. | SPITE F., SPITE M., BARBUY B., et al. | ||
|
2018MNRAS.478.4513B |
16 | D | 1 | 342691 | 271 | The GALAH Survey: second data release. | BUDER S., ASPLUND M., DUONG L., et al. | ||
|
2018AJ....156..179R |
16 | D | 1 | 90 | 63 | Kinematics of highly r-process-enhanced field stars: evidence for an accretion origin and detection of several groups from disrupted satellites. | ROEDERER I.U., HATTORI K. and VALLURI M. | ||
|
2019A&A...627A.177R |
41 | X | 1 | 109 | 34 | Non-LTE analysis of K I in late-type stars. | REGGIANI H., AMARSI A.M., LIND K., et al. | ||
|
2019ApJ...882...40J |
16 | D | 2 | 210 | 41 | The lanthanide fraction distribution in metal-poor stars: a test of neutron star mergers as the dominant r-process site. | JI A.P., DROUT M.R. and HANSEN T.T. | ||
|
2020A&A...641A.135S |
41 | X | 1 | 19 | ~ | A wide angle view of the Sagittarius dwarf spheroidal galaxy. II. A CEMP-r/s star in the Sagittarius dwarf spheroidal galaxy. | SBORDONE L., HANSEN C.J., MONACO L., et al. | ||
|
2021MNRAS.506..150B |
17 | D | 1 | 588596 | 276 | The GALAH+ survey: Third data release. | BUDER S., SHARMA S., KOS J., et al. | ||
|
2021ApJ...923..183L |
17 | D | 1 | 147 | ~ | Fuzzy cluster analysis: application to determining metallicities for very metal-poor stars. | LI H. | ||
| 2022ApJ...930...47H | 17 | D | 2 | 72 | 6 | The GALAH Survey: A New Sample of Extremely Metal-poor Stars Using a Machine-learning Classification Algorithm. | HUGHES A.C.N., SPITLER L.R., ZUCKER D.B., et al. | ||
|
2023ApJ...943...23S |
17 | D | 1 | 1792 | 5 | The R-Process Alliance: Chemodynamically Tagged Groups. II. An Extended Sample of Halo r-process-enhanced Stars. | SHANK D., BEERS T.C., PLACCO V.M., et al. | ||
|
2023ApJ...946...48H |
17 | D | 2 | 181 | 5 | Finding r-II Sibling Stars in the Milky Way with the Greedy Optimistic Clustering Algorithm. | HATTORI K., OKUNO A. and ROEDERER I.U. | ||
|
2023ApJ...947...23Z |
17 | D | 1 | 647 | 14 | Chemodynamically Tagged Groups of CEMP Stars in the Halo of the Milky Way. I. Untangling the Origins of CEMP-s and CEMP-no Stars. | ZEPEDA J., BEERS T.C., PLACCO V.M., et al. | ||
|
2023A&A...679A.110G |
17 | D | 3 | 52 | ~ | TITANS metal-poor reference stars II. Red giants and CEMP stars. | GIRIBALDI R.E., VAN ECK S., MERLE T., et al. | ||
| 2024ApJ...971..158R | 18 | D | 1 | 48 | ~ | The R-Process Alliance: 2MASS J22132050-5137385, the Star with the Highest-known r-process Enhancement at [Eu/Fe] = +2.45. | ROEDERER I.U., BEERS T.C., HATTORI K., et al. | ||
| 2025A&A...698A..11G | 19 | D | 2 | 63 | ~ | The most metal-poor tail of the Galactic halo: Hypothesis for its origin from precise spectral analysis. | GIRIBALDI R.E., MAGRINI L., ROSSI M., et al. | ||
| 2025ApJ...992...36V | 19 | D | 1 | 42 | ~ | Classifying Metal-poor Stars with Machine Learning Using Nucleosynthesis Calculations. | VASSH N., WANG Y., WOLOSHYN R.M., et al. |