Revised Bolometric Corrections and Interstellar Extinction Coefficients for the ACS and WFPC2 Photometric Systems

Bibcode
2008PASP..120..583G
DOI
10.1086/588526
Girardi, Léo; Dalcanton, Julianne; Williams, Benjamin; de Jong, Roelof; Gallart, C.; Monelli, M.; Groenewegen, Martin A. T.; Holtzman, Jon A.; Olsen, Knut A. G.; Seth, Anil C.; Weisz, Daniel R.; ANGST/ANGRRR Collaboration
Referencia bibliográfica

The Publications of the Astronomical Society of the Pacific, Volume 120, Issue 867, pp. 583-591.

Fecha de publicación:
5
2008
Número de autores
12
Número de autores del IAC
2
Número de citas
130
Número de citas referidas
127
Descripción
We present extensive tables of bolometric corrections and interstellar extinction coefficients for the WFPC2 and ACS (both WFC and HRC) photometric systems. They are derived from synthetic photometry applied to a database of spectral energy distributions covering a large range of effective temperatures, surface gravity, and metal content. Carbon stars are also considered. The zero points take into consideration the new high-accuracy Vega fluxes from Bohlin. These tables are employed to transform Padova isochrones into WFPC2 and ACS photometric systems using interstellar extinction coefficients on a star-to-star basis. All data are available either in tabular form or via an interactive web interface in the case of the isochrones. Preliminary tables for the WFC3 camera are also included in the database.
Proyectos relacionados
Cúmulo Globular NGC 2808
Vía Láctea y galaxias cercanas
El objetivo general del Proyecto es el estudio de la estructura, historia evolutiva y proceso de formación de galaxias a través de sus poblaciones estelares resueltas, tanto a partir de fotometría como espectroscopia. El proyecto puede dividirse en cuatro líneas principales: I. Historia de formación estelar en el Grupo Local. El objetivo de esta
Martín
López Corredoira
Cerrado
Tipo
Con árbitro
La Vía Láctea y el Grupo Local (MWLG)

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