The O3N2 and N2 abundance indicators revisited: improved calibrations based on CALIFA and T e-based literature data
Autor (es)
Marino, R. A.; Sánchez, Sebastián F.; Gil De Paz, Armando; Miralles-Caballero, Daniel; Kehrig, Carolina; Pérez Montero, Enrique; Stanishev, Vallery; Díaz Beltrán, Ángeles Isabel; Castillo-Morales, África; López-Sánchez, Ángel R.; Galbany, Lluís; García-Benito, Rubén; Mast, Damián; Méndez-Abreu, Jairo; Monreal-Ibero, Ana; Husemann, Bernd; Walcher, Carl Jakob; Másegosa, Josefa; Del Olmo Orozco, A.; Mour̃ão, Ana M.; Papaderos, Polychronis; Sánchez-Blázquez, Patricia; Falcón-Barroso, Jesús; Roth, Martin M.; Van De Ven, Glenn; Team, Califa; Rosales Ortega, F. Fabián; Vílchez, José; Iglesias-Páramo, Jorge; Kennicutt, Robert; García-Lorenzo, Begoña; Ziegler, B.; Mollá, Mercedes; González Delgado, Rosa M.Entidad
UAM. Departamento de Física TeóricaEditor
ESOFecha de edición
2013-11-01Cita
10.1051/0004-6361/201321956
Astronomy and Astrophysics 559 (2013): A114
ISSN
0004-6361 (print); 1432-0746 (online)DOI
10.1051/0004-6361/201321956Financiado por
R.A. Marino is funded by the Spanish program of International Campus of Excellence Moncloa (CEI). D. Mast thank the Plan Nacional de Investigación y Desarrollo funding programs, AYA2012-31935 of the Spanish Ministerio de Economía y Competitividad, for the support given to this project. S.F.S thanks the the Ramón y Cajal project RyC-2011-07590 of the spanish Ministerio de Economía y Competitividad, for the support giving to this project. F.F.R.O. acknowledges the Mexican National Council for Science and Technology (CONACYT) for financial support under the program Estancias Postdoctorales y Sabáticas al Extranjero para la Consolidación de Grupos de Investigación, 2010-2012. We acknowledge financial support for the ESTALLIDOS collaboration by the Spanish Ministerio de Ciencia e Innovación under grant AYA2010- 21887-C04-03. BG-L also acknowledges support from the Spanish Ministerio de Economía y Competitividad (MINECO) under grant AYA2012- 39408-C02-02. J.F.-B. acknowledges financial support from the Ramón y Cajal Program and grant AYA2010-21322-C03-02 from the Spanish Ministry of Economy and Competitiveness (MINECO), as well as to the DAGAL network from the People’s Program (Marie Curie Actions) of the European Union’s Seventh Framework Program FP7/2007-2013/ under REA grant agreement number PITN-GA-2011-289313. CK has been funded by project AYA2010-21887 from the Spanish PNAYA. P.P. acknowledges support by the Fundação para a Ciência e a Tecnologia (FCT) under project FCOMP-01-0124-FEDER-029170 (Reference FCT PTDC/FIS-AST/3214/2012), funded by FCT-MEC (PIDDAC) and FEDER (COMPETE). R.M.G.D. and R.G.B. also acknowledge support from the Spanish Ministerio de Economía y Competitividad (MINECO) under grant AyA2010-15081. V.S., L.G., and A.M.M. acknowledge financial support from the Fundação para a Ciência e a Tecnologia (FCT) under program Ciência 2008 and the research grant PTDC/CTE-AST/112582/2009Proyecto
info:eu-repo/grantAgreement/EC/FP7/289313Versión del editor
http://dx.doi.org/10.1051/0004-6361/201321956Materias
Galaxy: abundances; Galaxy: evolution; HII regions; ISM: abundances; Techniques: spectroscopic; FísicaNota
Astronomy and Astrophysics 559 (2013): A114 reproduced with permission from Astronomy and AstrophysicsDerechos
© 2013 ESOResumen
The use of integral field spectroscopy is since recently allowing to measure the emission line fluxes of an increasingly large number of star-forming galaxies, both locally and at high redshift. Many studies have used these fluxes to derive the gas-phase metallicity of the galaxies by applying the so-called strong-line methods. However, the metallicity indicators that these datasets use were empirically calibrated using few direct abundance data points (Te-based measurements). Furthermore, a precise determination of the prediction intervals of these indicators is commonly lacking in these calibrations. Such limitations might lead to systematic errors in determining the gas-phase metallicity, especially at high redshift, which might have a strong impact on our understanding of the chemical evolution of the Universe. The main goal of this study is to review the most widely used empirical oxygen calibrations, O3N2 and N2, by using newdirect abundance measurements. We pay special attention to (1) the expected uncertainty of these calibrations as a function of the index value or abundance derived and (2) the presence of possible systematic offsets. This is possible thanks to the analysis of the most ambitious compilation of Te-based H ii regions to date. This new dataset compiles the Te-based abundances of 603 H ii regions extracted from the literature but also includes new measurements from the CALIFA survey. Besides providing new and improved empirical calibrations for the gas abundance, we also present a comparison between our revisited calibrations with a total of 3423 additional CALIFA H ii complexes with abundances derived using the ONS calibration from the literature. The combined analysis of T e-based and ONS abundances allows us to derive their most accurate calibration to date for both the O3N2 and N2 single-ratio indicators, in terms of all statistical significance, quality, and coverage of the parameters space. In particular, we infer that these indicators show shallower abundance dependencies and statistically significant offsets compared to others'. The O3N2 and N2 indicators can be empirically applied to derive oxygen abundances calibrations from either direct abundance determinations with random errors of 0.18 and 0.16, respectively, or from indirect ones (but based on a large amount of data), reaching an average precision of 0.08 and 0.09 dex (random) and 0.02 and 0.08 dex (systematic; compared to the direct estimations), respectively
Lista de ficheros
Google Scholar:Marino, R. A.
-
Sánchez, Sebastián F.
-
Gil De Paz, Armando
-
Miralles-Caballero, Daniel
-
Kehrig, Carolina
-
Pérez Montero, Enrique
-
Stanishev, Vallery
-
Díaz Beltrán, Ángeles Isabel
-
Castillo-Morales, África
-
López-Sánchez, Ángel R.
-
Galbany, Lluís
-
García-Benito, Rubén
-
Mast, Damián
-
Méndez-Abreu, Jairo
-
Monreal-Ibero, Ana
-
Husemann, Bernd
-
Walcher, Carl Jakob
-
Másegosa, Josefa
-
Del Olmo Orozco, A.
-
Mour̃ão, Ana M.
-
Papaderos, Polychronis
-
Sánchez-Blázquez, Patricia
-
Falcón-Barroso, Jesús
-
Roth, Martin M.
-
Van De Ven, Glenn
-
Team, Califa
-
Rosales Ortega, F. Fabián
-
Vílchez, José
-
Iglesias-Páramo, Jorge
-
Kennicutt, Robert
-
García-Lorenzo, Begoña
-
Ziegler, B.
-
Mollá, Mercedes
-
González Delgado, Rosa M.
Lista de colecciones del ítem
Registros relacionados
Mostrando ítems relacionados por título, autor, creador y materia.
-
The effects of spatial resolution on integral field spectrograph surveys at different redshifts - The CALIFA perspective
Mast, Damián; Rosales Ortega, F. Fabián; Sánchez, Sebastián F.; Vílchez, José M.; Walcher, Carl Jakob; Husemann, Bernd; Márquez, Isabel; Marino, R. A.; Kennicutt, Robert C.; Monreal-Ibero, Ana; Galbany, Lluís; De Lorenzo-Cáceres, Adriana; Méndez-Abreu, Jairo; Kehrig, Carolina; Del Olmo, Ascensión; Relaño, Mónica; Wisotzki, Lutz; Mármol-Queraltó, Esther; Papaderos, Polychronis; Wild, Vivienne; Aguerri, J. Alfonso L; Falcón-Barroso, Jesús; Bomans, Dominik J.; Bland-Hawthorn, Joss; López-Sánchez, Ángel R.; Van De Ven, Glenn; Iglesias-Páramo, Jorge; Bekeraitè, Simona; Ziegler, B.; García-Lorenzo, Begoña
2014-01-01 -
Ionized gas kinematics of galaxies in the CALIFA survey: I. Velocity fields, kinematic parameters of the dominant component, and presence of kinematically distinct gaseous systems
García-Lorenzo, B.; Márquez, I.; Barrera-Ballesteros, J. K.; Masegosa, J.; Husemann, B.; Falcón-Barroso, J.; Lyubenova, M.; Sánchez, S. F.; Walcher, J.; Mast, D.; García-Benito, R.; Méndez-Abreu, Jairo; Van De Ven, Glenn; Spekkens, K.; Holmes, L.; Monreal-Ibero, Ana; Del Olmo, A.; Ziegler, B.; Bland-Hawthorn, J.; Sánchez-Blázquez, Patricia; Iglesias-Páramo, J.; Aguerri, J. Alfonso L; Papaderos, P.; Gomes, J. M.; Marino, R. A.; González Delgado, R. M.; Cortijo-Ferrero, C.; López-Sánchez, A. R.; Bekeraite, S.; Wisotzki, L.; Bomans, D.; CALIFA team
2015-01-01 -
Imprints of galaxy evolution on H II regions. Memory of the past uncovered by the CALIFA survey
Sánchez, S. F.; Pérez, E.; Rosales Ortega, F. Fabián; Miralles-Caballero, D.; López-Sánchez, A. R.; Iglesias-Páramo, J.; Marino, R. A.; Sánchez-Menguiano, L.; García-Benito, R.; Mast, D.; Mendoza, M. A.; Papaderos, P.; Ellis, S.; Galbany, L.; Kehrig, C.; Monreal-Ibero, Ana; Mollá, M.; Ziegler, B.; De Lorenzo-Cáceres, A.; Méndez-Abreu, Jairo; Bland-Hawthorn, J.; Bekeraitė, S.; Roth, M. M.; Pasquali, A.; Díaz Beltrán, Ángeles Isabel; Bomans, D.; Van De Ven, Glenn; Wisotzki, L.; González Delgado, R.
2015-01-01