The int search for metal-poor stars: spectroscopic observations and classification via artificial neural networks (2000)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA ESTELAR; ASTROFÍSICA; GALÁXIAS; ESTRELAS (CLASSIFICAÇÃO); ESPECTROSCOPIA
- Language: Inglês
- Imprenta:
- Source:
- Título: Astronomical Journal
- ISSN: 0004-6256
- Volume/Número/Paginação/Ano: v. 120, n. 3, p. 1516-1531, 2000
-
ABNT
PRIETO, Carlos Allende et al. The int search for metal-poor stars: spectroscopic observations and classification via artificial neural networks. Astronomical Journal, v. 120, n. 3, p. 1516-1531, 2000Tradução . . Acesso em: 13 fev. 2026. -
APA
Prieto, C. A., Rebolo, R., López, R. J. G., Serra-Ricart, M., Beers, T. C., Rossi, S. C. F., et al. (2000). The int search for metal-poor stars: spectroscopic observations and classification via artificial neural networks. Astronomical Journal, 120( 3), 1516-1531. -
NLM
Prieto CA, Rebolo R, López RJG, Serra-Ricart M, Beers TC, Rossi SCF, Bonifacio P, Molaro P. The int search for metal-poor stars: spectroscopic observations and classification via artificial neural networks. Astronomical Journal. 2000 ; 120( 3): 1516-1531.[citado 2026 fev. 13 ] -
Vancouver
Prieto CA, Rebolo R, López RJG, Serra-Ricart M, Beers TC, Rossi SCF, Bonifacio P, Molaro P. The int search for metal-poor stars: spectroscopic observations and classification via artificial neural networks. Astronomical Journal. 2000 ; 120( 3): 1516-1531.[citado 2026 fev. 13 ] - Broadband UBVRcIc photometry of horizontal-branch and metal-poor candidates from the HK and Hamburg/ESO surveys. I.
- Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H] <= -3,5
- The Hamburg/ESO R-process enhanced star survey (HERES): II. Spectroscopic analysis of the survey sample
- Metal abundance estimates for F- and G-type stars from Edinburgh-cape blue object survey
- Estimativas de precisão de temperaturas efetivas estelares e avermelhamento interestelar utilizando o índice de linha de Balmer baseado em espectroscopia de média resolução
- Bright metal-poor stars from the Hamburg/ESO survey: I. Selection and follow-up observations from 329 fields
- The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey
- Elemental abundances and classification of carbon-enhanced metal-poor stars
- Additional emission-line candidates from the hk survey
- Spectroscopic validation of low-metallicity stars from RAVE
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