The luminosity–metallicity relation in the local Universe from the 2dF Galaxy Redshift Survey

By F. Lamareille, M. Mouhcine, Thierry Contini, Ian Lewis, S. Maddox. 2004

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We investigate the Luminosity ‐ Metallicity (L Z) relation in the local universe (0 0.3) galaxies. Oxygen-to-hydrogen (O/H) abundance ratios are estimated using the ”strong-line” method, which relates the strength of following bright emission lines [O II] �3727, [O III] �5007, and H� (parametersR23 andO32)

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/d40c716e0e9b4922438681c830b717848ef59c4d

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Citations in the corpus

• The Mass-Metallicity Relation at z≳2 (2006, background): “…CB3 0HA, UK 7 Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101 Skillman et al. 1989; Zaritsky et al. 1994; Garnett et al. 1997; Lamareille et al. 2004; Salzer et al. 2005, to name only a few), though others have studied correlations between metallicity and rotational velocity…”
• THE MASS–METALLICITY AND LUMINOSITY–METALLICITY RELATIONS FROM DEEP2 AT z ∼ 0.8 (2010, background): “…subsequent efforts have focused on the relation between luminosity and metallicity (Skillman et al. 1989; Zaritsky et al. 1994; Garnett et al. 1997; Lamareille et al. 2004; Salzer et al. 2005) where luminosity is taken as a proxy for mass because of the difficulty in inferring galaxy masses from…”
• The Host Galaxy of GRB 031203: Implications of Its Low Metallicity, Low Redshift, and Starburst Nature (2004, background): “Finally, HG 031203 exhibits a lower metallicity than > 99% of all galaxies with MB < −19.3mag (Melbourne & Salzer 2002; Lamareille et al. 2004).”
• Velocity-metallicity correlation for high-z DLA galaxies: evidence of a mass-metallicity relation? (2006, background): “…suggested that,if a galaxy luminosity-metallicity relation similar to that observed at 0 <∼ z <∼ 1 (e.g., Garnett 2002; Kobulnicky et al. 2003; Lamareille et al. 2004; Tremonti et al. 2004) was already in place at high redshifts, then it would be possible to significantly increase the DLA…”
• The K20 survey. VII. The spectroscopic catalogue: spectral properties and evolution of the galaxy population ⋆, ⋆⋆ (2005, methodology): “…of the underlying stellar component in absorption is accounted for by applying an “ad hoc” correction to the rest-frame EWs (see Kennicutt 1992; Lamareille et al. 2004), but since these correction values are determined from local galaxy samples we preferred to leave the equivalent widths…”
• The impact of the nitrogen-to-oxygen ratio on ionized nebula diagnostics based on [N ii] emission lines (2009, methodology): “This is the case of the blue diagnostic diagram, proposed by Lamareille et al. (2004), which involves the [Oiii] and [Oii] lines or the red diagnostic, which relates empirically the [Nii]/Hα and [Sii]/Hα ratios.”
• Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies (2012, methodology): “We have used the diagnostic diagram [O III]/Hβ versus [O II]/Hβ (Rola, Terlevich & Terlevich 1997; Lamareille et al. 2004, the ‘blue’ diagram) to extend the selection to higher redshifts (0.5 < z < 0.92).”
• Aperture Effects on Star Formation Rate, Metallicity, and Reddening (2005, methodology): “These complex metallicity gradients may introduce random and/or systematic errors into the luminosity-metallicity relation found in fiber surveys (Tremonti et al. 2004; Lamareille et al. 2004; Maier, Meisenheimer, & Hippelein 2004).”
• Gas metallicity diagnostics in star-forming galaxies (2006, unknown): “Lamareille et al. (2004) also reported that AGNs and star-forming galaxies can be distinguished by using diagnostic diagrams using only the blue part of the spectrum, i.e., O32 versus R23 and F ([Oiii]λ5007)/F (Hβ) versus F ([Oii]λ3727)/F (Hβ) (see also Rola et al. 1997).”
• An extreme [O III] emitter at z = 3.2: a low metallicity Lyman continuum source (2015, methodology): “Other diagnostic diagrams have been proposed, like the [O iii]λ5007/Hβ vs. [O ii]λ3727/Hβ (Lamareille et al. 2004).”
• Feedback and metal enrichment in cosmological smoothed particle hydrodynamics simulations ¿ I. A model for chemical enrichment (2005, background): “…Kennicutt & Hodge 1989; Brodie & Huchra 1991; Zaritsky, Kennicutt & Huchra 1994; Mushotzky et al. 1996; Ettori et al. 2002; Tremonti et al. 2004; Lamareille et al. 2004) as well as at intermediate and high redshifts (e.g. Prochaska & Wolfe 2002; Adelberger ⋆ E-mail: cecilia@iafe.uba.ar (CS);…”
• Metallicity Calibrations and the Mass-Metallicity Relation for Star-forming Galaxies (2008, unknown): “…relation has recently been obtained with large spectroscopic surveys such as the Sloan Digital Sky Survey (SDSS) and the 2 degree Field Galaxy Redshift Survey (2dF- 2 GRS) (e.g., Baldry et al. 2002; Schulte-Ladbeck et al. 2003; Lamareille et al. 2004; Tremonti et al. 2004; Gallazzi et al. 2005).”
• Semi‐empirical analysis of Sloan Digital Sky Survey galaxies – III. How to distinguish AGN hosts (2006, methodology): “The fourth one, [O III]/Hβ versus [O II]/Hβ (panel a), has been used e.g. by Tresse et al. (1996) or Lamareille et al. (2004).”
• A NEW DIAGNOSTIC OF ACTIVE GALACTIC NUCLEI: REVEALING HIGHLY ABSORBED SYSTEMS AT REDSHIFT >0.3 (2011, methodology): “COMPARISON WITH THE BLUE DIAGRAM The blue diagram discussed in §7.1 was developed in Lamareille et al. (2004) and recently improved in Lamareille (2010).”
• The Rest-Frame Optical Spectra of SCUBA Galaxies (2004, background): “The correlation is in the sense that more massive (and luminous) galaxies exhibit a higher degree of metal enrichment (Garnett et al. 1997; Zaritsky et al. 1994; Garrett 2002; Lilly et al. 2003; Lamareille et al. 2004).”
• Evidence for Solar Metallicities in Massive Star-forming Galaxies at z ≳ 2 (2004, background): “…a strong correlation between their H ii region oxygen abundances and optical luminosities, according to which more luminous and massive galaxies exhibit a higher degree of metal enrichment (Garnett & Shields 1987; Garnett 2002; Zaritsky et al. 1994; Lamareille et al. 2004; Tremonti et al. 2004).”