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 keywords = {galaxies: formation, galaxies: individual: NGC 6155, galaxies: spiral, galaxies: stellar content, galaxies: structure},
     year = 2010,
    month = jun,
   volume = 716,
    pages = {L4-L8},
      doi = {10.1088/2041-8205/716/1/L4},
   adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...716L...4Y},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{quil08,
   author = {{Quillen}, A.~C. and {Bland-Hawthorn}, J.},
    title = "{When is star formation episodic? A delay differential equation `negative feedback' model}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {0801.3469},
 keywords = {ISM: evolution , galaxies: ISM},
     year = 2008,
    month = jun,
   volume = 386,
    pages = {2227-2234},
      doi = {10.1111/j.1365-2966.2008.13193.x},
   adsurl = {http://adsabs.harvard.edu/abs/2008MNRAS.386.2227Q},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{perez13,
   author = {{P{\'e}rez}, E. and {Cid Fernandes}, R. and {Gonz{\'a}lez Delgado}, R.~M. and
	{Garc{\'{\i}}a-Benito}, R. and {S{\'a}nchez}, S.~F. and {Husemann}, B. and
	{Mast}, D. and {Rod{\'o}n}, J.~R. and {Kupko}, D. and {Backsmann}, N. and
	{de Amorim}, A.~L. and {van de Ven}, G. and {Walcher}, J. and
	{Wisotzki}, L. and {Cortijo-Ferrero}, C. and {collaboration6}, C.
	},
    title = "{The Evolution of Galaxies Resolved in Space and Time: A View of Inside-out Growth from the CALIFA Survey}",
  journal = {\apjl},
archivePrefix = "arXiv",
   eprint = {1301.1679},
 primaryClass = "astro-ph.CO",
 keywords = {galaxies: bulges, galaxies: evolution, galaxies: fundamental parameters, galaxies: stellar content, galaxies: structure },
     year = 2013,
    month = feb,
   volume = 764,
      eid = {L1},
    pages = {L1},
      doi = {10.1088/2041-8205/764/1/L1},
   adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...764L...1P},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{jest05,
   author = {{Jester}, S. and {Schneider}, D.~P. and {Richards}, G.~T. and
	{Green}, R.~F. and {Schmidt}, M. and {Hall}, P.~B. and {Strauss}, M.~A. and
	{Vanden Berk}, D.~E. and {Stoughton}, C. and {Gunn}, J.~E. and
	{Brinkmann}, J. and {Kent}, S.~M. and {Smith}, J.~A. and {Tucker}, D.~L. and
	{Yanny}, B.},
    title = "{The Sloan Digital Sky Survey View of the Palomar-Green Bright Quasar Survey}",
  journal = {\aj},
   eprint = {arXiv:astro-ph/0506022},
 keywords = {Catalogs, Galaxies: Active, Galaxies: Quasars: Emission Lines, Galaxies: Quasars: General, Surveys},
     year = 2005,
    month = sep,
   volume = 130,
    pages = {873-895},
      doi = {10.1086/432466},
   adsurl = {http://adsabs.harvard.edu/abs/2005AJ....130..873J},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{thilk02,
   author = {{Thilker}, D.~A. and {Walterbos}, R.~A.~M. and {Braun}, R. and
	{Hoopes}, C.~G.},
    title = "{H II Regions and Diffuse Ionized Gas in 11 Nearby Spiral Galaxies}",
  journal = {\aj},
 keywords = {Galaxies: Spiral, ISM: H II Regions, ISM: General, Techniques: Photometric},
     year = 2002,
    month = dec,
   volume = 124,
    pages = {3118-3134},
      doi = {10.1086/344303},
   adsurl = {http://adsabs.harvard.edu/abs/2002AJ....124.3118T},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{naka12,
   author = {{Nakajima}, K. and {Ouchi}, M. and {Shimasaku}, K. and {Ono}, Y. and
	{Lee}, J.~C. and {Foucaud}, S. and {Ly}, C. and {Dale}, D.~A. and
	{Salim}, S. and {Finn}, R. and {Almaini}, O. and {Okamura}, S.
	},
    title = "{Average Metallicity and Star Formation Rate of Ly{$\alpha$} Emitters Probed by a Triple Narrowband Survey}",
  journal = {\apj},
archivePrefix = "arXiv",
   eprint = {1105.2824},
 primaryClass = "astro-ph.CO",
 keywords = {galaxies: abundances, galaxies: evolution, galaxies: formation, galaxies: high-redshift, galaxies: star formation},
     year = 2012,
    month = jan,
   volume = 745,
      eid = {12},
    pages = {12},
      doi = {10.1088/0004-637X/745/1/12},
   adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...745...12N},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{magr12,
   author = {{Magrini}, L. and {Hunt}, L. and {Galli}, D. and {Schneider}, R. and
	{Bianchi}, S. and {Maiolino}, R. and {Romano}, D. and {Tosi}, M. and
	{Valiante}, R.},
    title = "{Scaling relations of metallicity, stellar mass and star formation rate in metal-poor starbursts - II. Theoretical models}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {1209.1103},
 primaryClass = "astro-ph.CO",
 keywords = {galaxies: abundances, galaxies: dwarf, galaxies: evolution, galaxies: high-redshift, galaxies: starburst, galaxies: star formation},
     year = 2012,
    month = dec,
   volume = 427,
    pages = {1075-1088},
      doi = {10.1111/j.1365-2966.2012.22055.x},
   adsurl = {http://adsabs.harvard.edu/abs/2012MNRAS.427.1075M},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{cres12,
   author = {{Cresci}, G. and {Mannucci}, F. and {Sommariva}, V. and {Maiolino}, R. and
	{Marconi}, A. and {Brusa}, M.},
    title = "{The metallicity properties of zCOSMOS galaxies at 0.2 {\lt} z {\lt} 0.8}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {1110.4408},
 primaryClass = "astro-ph.CO",
 keywords = {galaxies: abundances, galaxies: formation, galaxies: high-redshift},
     year = 2012,
    month = mar,
   volume = 421,
    pages = {262-269},
      doi = {10.1111/j.1365-2966.2011.20299.x},
   adsurl = {http://adsabs.harvard.edu/abs/2012MNRAS.421..262C},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{rich11,
   author = {{Richard}, J. and {Jones}, T. and {Ellis}, R. and {Stark}, D.~P. and
	{Livermore}, R. and {Swinbank}, M.},
    title = "{The emission line properties of gravitationally lensed 1.5 {\lt} z {\lt} 5 galaxies}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {1011.6413},
 primaryClass = "astro-ph.CO",
 keywords = {gravitational lensing: strong, galaxies: abundances, galaxies: evolution, galaxies: high-redshift, galaxies: kinematics and dynamics},
     year = 2011,
    month = may,
   volume = 413,
    pages = {643-658},
      doi = {10.1111/j.1365-2966.2010.18161.x},
   adsurl = {http://adsabs.harvard.edu/abs/2011MNRAS.413..643R},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{long09,
   author = {{Longhetti}, M. and {Saracco}, P.},
    title = "{Stellar mass estimates in early-type galaxies: procedures, uncertainties and models dependence}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {0811.4041},
 keywords = {galaxies: elliptical and lenticular, cD , galaxies: fundamental parameters , galaxies: stellar content},
     year = 2009,
    month = apr,
   volume = 394,
    pages = {774-794},
      doi = {10.1111/j.1365-2966.2008.14375.x},
   adsurl = {http://adsabs.harvard.edu/abs/2009MNRAS.394..774L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@INPROCEEDINGS{skill92,
   author = {{Skillman}, E.~D.},
    title = "{The Mass-Metallicity Relationship for Dwarf Irregular Galaxies}",
booktitle = {Elements and the Cosmos},
     year = 1992,
   editor = {{Edmunds}, M.~G. and {Terlevich}, R.},
    pages = {246},
   adsurl = {http://adsabs.harvard.edu/abs/1992eatc.conf..246S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{skill89,
   author = {{Skillman}, E.~D. and {Kennicutt}, R.~C. and {Hodge}, P.~W.},
    title = "{Oxygen abundances in nearby dwarf irregular galaxies}",
  journal = {\apj},
 keywords = {ABUNDANCE, DWARF GALAXIES, H II REGIONS, INTERSTELLAR GAS, IRREGULAR GALAXIES, OXYGEN, ELLIPTICAL GALAXIES, GALACTIC EVOLUTION, LUMINOSITY, PLANETARY NEBULAE},
     year = 1989,
    month = dec,
   volume = 347,
    pages = {875-882},
 abstract = "{Oxygen abundances are obtained by optical spectrophotometry of H II
regions in seven nearby dwarf irregular galaxies. All of these yield
oxygen abundances of less than 1/10 of the solar value, and most are in
the range of 3-5 percent of the solar value. This suggests that
observations of nearby dwarf galaxies may provide an effective means for
studying the chemical evolution of low-mass galaxies and, possibly, the
primordial helium abundance. A strong correlation is found between the
oxygen abundances and absolute magnitudes for nearby irregular galaxies.
This correlation will be useful for estimating abundances of irregular
galaxies without observable H II regions, and possibly as a distance
indicator for irregular galaxies with known abundances. It is inferred
from this relationship that infall is no more important in irregular
galaxies with extremely large H I halos than in typical irregular
galaxies.
}",
      doi = {10.1086/168178},
   adsurl = {http://adsabs.harvard.edu/abs/1989ApJ...347..875S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2006ApJ...647..970L,
   author = {{Lee}, H. and {Skillman}, E.~D. and {Cannon}, J.~M. and {Jackson}, D.~C. and
	{Gehrz}, R.~D. and {Polomski}, E.~F. and {Woodward}, C.~E.},
    title = "{On Extending the Mass-Metallicity Relation of Galaxies by 2.5 Decades in Stellar Mass}",
  journal = {\apj},
   eprint = {arXiv:astro-ph/0605036},
 keywords = {Galaxies: Dwarf, Galaxies: Evolution, Galaxies: Irregular, Infrared: Galaxies},
     year = 2006,
    month = aug,
   volume = 647,
    pages = {970-983},
 abstract = "{We report 4.5 {$\mu$}m luminosities for 27 nearby (D{\lt}\~{}5 Mpc) dwarf
irregular galaxies measured with the Spitzer Infrared Array Camera. We
have constructed the 4.5 {$\mu$}m luminosity-metallicity (L-Z) relation for
25 dwarf galaxies with secure distance and interstellar medium oxygen
abundance measurements. The 4.5 {$\mu$}m L-Z relation is
12+log(O/H)=(5.78+/-0.21)+(-0.122+/-0.012)M$_{[4.5]}$, where
M$_{[4.5]}$ is the absolute magnitude at 4.5 {$\mu$}m. The dispersion
in the near-infrared L-Z relation is smaller than the corresponding
dispersion in the optical L-Z relation. The subsequently derived stellar
mass-metallicity (M$_{*}$-Z) relation is
12+log(O/H)=(5.65+/-0.23)+(0.298+/-0.030)logM$_{*}$, and extends
the SDSS M$_{*}$- Z relation to lower mass by about 2.5 dex. We
find that the dispersion in the M$_{*}$-Z relation is similar over
5 orders of magnitude in stellar mass, and that the relationship between
stellar mass and interstellar medium metallicity is similarly tight from
high-mass to low-mass systems. We find a larger scatter at low mass in
the relation between effective yield and total baryonic mass. In fact,
there are a few dwarf galaxies with large yields, which is difficult to
explain if galactic winds are ubiquitous in dwarf galaxies. The low
scatter in the L-Z and M$_{*}$-Z relationships are difficult to
understand if galactic superwinds or blowout are responsible for the low
metallicities at low mass or luminosity. Naively, one would expect an
ever increasing scatter at lower masses, which is not observed.
}",
      doi = {10.1086/505573},
   adsurl = {http://adsabs.harvard.edu/abs/2006ApJ...647..970L},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2011MNRAS.410.2203S,
   author = {{Sakstein}, J. and {Pipino}, A. and {Devriendt}, J.~E.~G. and
	{Maiolino}, R.},
    title = "{The origin and evolution of the mass-metallicity relation at high redshift using GalICS}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {1008.4158},
 primaryClass = "astro-ph.CO",
 keywords = {methods: numerical, galaxies: evolution, galaxies: formation, galaxies: haloes, galaxies: high-redshift, galaxies: star formation},
     year = 2011,
    month = feb,
   volume = 410,
    pages = {2203-2216},
 abstract = "{The Galaxies in Cosmological Simulations (GalICS) semi-analytical model
of hierarchical galaxy formation is used to investigate the effects of
different galactic properties, including star formation rate (SFR) and
outflows, on the shape of the mass-metallicity relation and to predict
the relation for galaxies at redshift z= 2.27 and 3.54. Our version of
GalICS has the chemical evolution implemented in great detail and is
less heavily reliant on approximations, such as instantaneous recycling.
We vary the model parameters controlling both the efficiency and
redshift dependence of the SFR as well as the efficiency of supernova
feedback. We find that the factors controlling the SFR influence the
relation significantly at all redshifts and require a strong redshift
dependence, proportional to 1 +z, in order to reproduce the observed
relation at the low-mass end. Indeed, at any redshift, the predicted
relation flattens out at the high-mass end resulting in a poorer
agreement with observations in this regime. We also find that variation
in the parameters associated with outflows has a minimal effect on the
relation at high redshift but does serve to alter its shape in the more
recent past. We thus conclude that the relation is one between the SFR
and mass and that outflows are only important in shaping the relation at
late times. When the relation is stratified by the SFR, it is apparent
that the predicted galaxies with increasing stellar masses have higher
SFRs, supporting the view that galaxy downsizing is the origin of the
relation. Attempting to reproduce the observed relation, we vary the
parameters controlling the efficiency of star formation and its redshift
dependence and compare the predicted relations with those of Erb et al.
at z= 2.27 and Maiolino et al. at z= 3.54 in order to find the
best-fitting parameters. We succeed in fitting the relation at z= 3.54
reasonably well; however, we fail at z= 2.27, our relation lying on
average below the observed one at the one standard deviation level. We
do, however, predict the observed evolution between z= 3.54 and 0.
Finally, we discuss the reasons for the above failure and the flattening
at high masses, with regards to both the comparability of our
predictions with observations and the possible lack of underlying
physics. Several of these problems are common to many
semi-analytic/hybrid models and so we discuss possible improvements and
set the stage for future work by considering how the predictions and
physics in these models can be made more robust in light of our results.
}",
      doi = {10.1111/j.1365-2966.2010.17593.x},
   adsurl = {http://adsabs.harvard.edu/abs/2011MNRAS.410.2203S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{kudri12,
   author = {{Kudritzki}, R.-P. and {Urbaneja}, M.~A. and {Gazak}, Z. and
	{Bresolin}, F. and {Przybilla}, N. and {Gieren}, W. and {Pietrzy{\'n}ski}, G.
	},
    title = "{Quantitative Spectroscopy of Blue Supergiant Stars in the Disk of M81: Metallicity, Metallicity Gradient, and Distance}",
  journal = {\apj},
archivePrefix = "arXiv",
   eprint = {1112.3643},
 primaryClass = "astro-ph.CO",
 keywords = {galaxies: distances and redshifts, galaxies: individual: M81, stars: abundances, stars: early-type},
     year = 2012,
    month = mar,
   volume = 747,
      eid = {15},
    pages = {15},
      doi = {10.1088/0004-637X/747/1/15},
   adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...747...15K},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{ferr92,
   author = {{Ferrini}, F. and {Matteucci}, F. and {Pardi}, C. and {Penco}, U.
	},
    title = "{Evolution of spiral galaxies. I - Halo-disk connection for the evolution of the solar neighborhood}",
  journal = {\apj},
 keywords = {GALACTIC EVOLUTION, GALACTIC STRUCTURE, HALOS, SOLAR NEIGHBORHOOD, SPIRAL GALAXIES, CHEMICAL EVOLUTION, DWARF STARS, G STARS, METALLICITY, NUCLEAR ASTROPHYSICS, STAR FORMATION RATE},
     year = 1992,
    month = mar,
   volume = 387,
    pages = {138-151},
      doi = {10.1086/171066},
   adsurl = {http://adsabs.harvard.edu/abs/1992ApJ...387..138F},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{ferr88,
   author = {{Ferrini}, F. and {Galli}, D.},
    title = "{A model of spiral-galaxy evolution. I - Galaxy morphology and star formation rate}",
  journal = {\aap},
 keywords = {GALACTIC EVOLUTION, HUBBLE DIAGRAM, SPIRAL GALAXIES, STAR FORMATION RATE, STELLAR EVOLUTION, H ALPHA LINE, STELLAR MASS},
     year = 1988,
    month = apr,
   volume = 195,
    pages = {27-37},
   adsurl = {http://adsabs.harvard.edu/abs/1988A%26A...195...27F},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{woos95,
   author = {{Woosley}, S.~E. and {Weaver}, T.~A.},
    title = "{The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis}",
  journal = {\apjs},
 keywords = {HYDRODYNAMICS, NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES, STARS: EVOLUTION, STARS: INTERIORS, STARS: SUPERNOVAE: GENERAL},
     year = 1995,
    month = nov,
   volume = 101,
    pages = {181},
      doi = {10.1086/192237},
   adsurl = {http://adsabs.harvard.edu/abs/1995ApJS..101..181W},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{molla05,
   author = {{Moll{\'a}}, M. and {D{\'{\i}}az}, A.~I.},
    title = "{A grid of chemical evolution models as a tool to interpret spiral and irregular galaxies data}",
  journal = {\mnras},
   eprint = {arXiv:astro-ph/0501370},
 keywords = {galaxies: abundances, galaxies: evolution, galaxies: spiral, galaxies: stellar content},
     year = 2005,
    month = apr,
   volume = 358,
    pages = {521-543},
      doi = {10.1111/j.1365-2966.2005.08782.x},
   adsurl = {http://adsabs.harvard.edu/abs/2005MNRAS.358..521M},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{ellis05,
   author = {{Ellis}, S.~C. and {Driver}, S.~P. and {Allen}, P.~D. and {Liske}, J. and
	{Bland-Hawthorn}, J. and {De Propris}, R.},
    title = "{The Millennium Galaxy Catalogue: on the natural subdivision of galaxies}",
  journal = {\mnras},
   eprint = {arXiv:astro-ph/0508365},
 keywords = {galaxies: evolution, galaxies: fundamental parameters},
     year = 2005,
    month = nov,
   volume = 363,
    pages = {1257-1271},
      doi = {10.1111/j.1365-2966.2005.09521.x},
   adsurl = {http://adsabs.harvard.edu/abs/2005MNRAS.363.1257E},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{pasq12,
   author = {{Pasquali}, A. and {Gallazzi}, A. and {van den Bosch}, F.~C.
	},
    title = "{The gas-phase metallicity of central and satellite galaxies in the Sloan Digital Sky Survey}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {1206.3458},
 primaryClass = "astro-ph.CO",
 keywords = {galaxies: abundances, galaxies: evolution, galaxies: fundamental parameters, galaxies: groups: general, galaxies: star formation },
     year = 2012,
    month = sep,
   volume = 425,
    pages = {273-286},
      doi = {10.1111/j.1365-2966.2012.21454.x},
   adsurl = {http://adsabs.harvard.edu/abs/2012MNRAS.425..273P},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{pasq10,
   author = {{Pasquali}, A. and {Gallazzi}, A. and {Fontanot}, F. and {van den Bosch}, F.~C. and
	{De Lucia}, G. and {Mo}, H.~J. and {Yang}, X.},
    title = "{Ages and metallicities of central and satellite galaxies: implications for galaxy formation and evolution}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {0912.1853},
 primaryClass = "astro-ph.CO",
 keywords = {galaxies: clusters: general, galaxies: evolution, galaxies: general, galaxies: statistics, galaxies: stellar content, dark matter},
     year = 2010,
    month = sep,
   volume = 407,
    pages = {937-954},
      doi = {10.1111/j.1365-2966.2010.17074.x},
   adsurl = {http://adsabs.harvard.edu/abs/2010MNRAS.407..937P},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{wuyt12,
   author = {{Wuyts}, E. and {Rigby}, J.~R. and {Sharon}, K. and {Gladders}, M.~D.
	},
    title = "{Constraints on the Low-mass End of the Mass-Metallicity Relation at z = 1-2 from Lensed Galaxies}",
  journal = {\apj},
archivePrefix = "arXiv",
   eprint = {1202.5267},
 primaryClass = "astro-ph.CO",
 keywords = {galaxies: evolution, galaxies: high-redshift, gravitational lensing: strong },
     year = 2012,
    month = aug,
   volume = 755,
      eid = {73},
    pages = {73},
      doi = {10.1088/0004-637X/755/1/73},
   adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...755...73W},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{renz93,
   author = {{Renzini}, A. and {Ciotti}, L. and {D'Ercole}, A. and {Pellegrini}, S.
	},
    title = "{Production and Circulation of Iron in Elliptical Galaxies and Clusters of Galaxies}",
  journal = {\apj},
 keywords = {GALAXIES: ABUNDANCES, GALAXIES: CLUSTERING, GALAXIES: ELLIPTICAL AND LENTICULAR, CD, GALAXIES: EVOLUTION, GALAXIES: INTERGALACTIC MEDIUM, STARS: SUPERNOVAE: GENERAL},
     year = 1993,
    month = dec,
   volume = 419,
    pages = {52},
      doi = {10.1086/173458},
   adsurl = {http://adsabs.harvard.edu/abs/1993ApJ...419...52R},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{PeMo12,
   author = {{P\'erez-Montero}, E. and {Contini}, T. and {Lamareille}, F. and
	{Maier}, C. and {Carollo}, C.~M. and {Kneib}, J.~P. and {Le Fevre}, O. and
	{Lilly}, S. and {Mainieiri}, V. and {Renzini}, A. and {Scodeggio}, M. and
	{Zamorani}, G. and {Bardelli}, S. and {Bolzonella}, M. and {Bongiorno}, A. and
	{Caputi}, K. and {Cucciati}, O. and {de la Torre}, S. and {de Ravel}, L. and
	{Franzetti}, P. and {Garilli}, B. and {Iovino}, A. and {Kampczyk}, P. and
	{Knobel}, C. and {Kovac}, K. and {Le Borgne}, J.~F. and {Le Brun}, V. and
	{Mignoli}, M. and {Pello}, R. and {Peng}, Y. and {Presotto}, V. and
	{Ricciardelli}, E. and {Silverman}, J.~D. and {Tanaka}, M. and
	{Tasca}, L.~A.~M. and {Tresse}, L. and {Vergani}, D. and {Zucca}, E.
	},
    title = "{The cosmic evolution of oxygen and nitrogen abundances in star-forming galaxies over the last 10 Gyrs}",
  journal = {ArXiv e-prints},
archivePrefix = "arXiv",
   eprint = {1210.0334},
 primaryClass = "astro-ph.CO",
 keywords = {Astrophysics - Cosmology and Extragalactic Astrophysics},
     year = 2012,
    month = oct,
   adsurl = {http://adsabs.harvard.edu/abs/2012arXiv1210.0334P},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{pala05,
   author = {{Palacios}, A. and {Meynet}, G. and {Vuissoz}, C. and {Kn{\"o}dlseder}, J. and
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%% Created for Jakob Walcher at 2012-05-08 00:14:34 +0200
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%% Saved with string encoding Unicode (UTF-8)
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license: MIT

license_type: permissive

branch_name: refs/heads/master

extension: bib