Stellar masses and star formation histories for 105 galaxies from the Sloan Digital Sky Survey
We develop a new method to constrain the star formation histories, dust attenuation and
stellar masses of galaxies. It is based on two stellar absorption-line indices, the 4000-Å …
stellar masses of galaxies. It is based on two stellar absorption-line indices, the 4000-Å …
[HTML][HTML] Stellar masses and star formation histories for 105 galaxies from the Sloan Digital Sky Survey
G Kauffmann, TM Heckman, SDM White… - Monthly Notice of the …, 2003 - adsabs.harvard.edu
We develop a new method to constrain the star formation histories, dust attenuation and
stellar masses of galaxies. It is based on two stellar absorption-line indices, the 4000-Å …
stellar masses of galaxies. It is based on two stellar absorption-line indices, the 4000-Å …
Stellar masses and star formation histories for 105 galaxies from the Sloan Digital Sky Survey
G Kauffmann, TM Heckman, DM Simon… - Monthly Notices of the …, 2003 - elibrary.ru
We develop a new method to constrain the star formation histories, dust attenuation and
stellar masses of galaxies. It is based on two stellar absorption-line indices, the 4000-A …
stellar masses of galaxies. It is based on two stellar absorption-line indices, the 4000-A …
Stellar Masses and Star Formation Histories for Galaxies from the Sloan Digital Sky Survey
G Kauffmann, TM Heckman, SDM White… - Mon. Not. Roy. Astron …, 2003 - inspirehep.net
We develop a new method to constrain the star formation histories, dust attenuation and
stellar masses of galaxies. It is based on two stellar absorption line indices, the 4000 …
stellar masses of galaxies. It is based on two stellar absorption line indices, the 4000 …
[PDF][PDF] Stellar Masses and Star Formation Histories for 10 5 Galaxies from the Sloan Digital Sky Survey
G Kauffmann, TM Heckman, SDM White… - arXiv preprint astro-ph … - academia.edu
We develop a new method to constrain the star formation histories, dust attenuation and
stellar masses of galaxies. It is based on two stellar absorption line indices, the 4000 Å …
stellar masses of galaxies. It is based on two stellar absorption line indices, the 4000 Å …
[引用][C] Stellar masses and star formation histories for 10⁵ galaxies from the Sloan Digital Sky Survey
G Kauffmann, TM Heckman, SDM White… - Monthly Notices of the …, 2003 - pure.mpg.de
Stellar masses and star formation histories for 105 galaxies from the Sloan Digital Sky Survey
G Kauffmann, TM Heckman, SDM White… - Monthly Notices of …, 2003 - Wiley Online Library
We develop a new method to constrain the star formation histories, dust attenuation and
stellar masses of galaxies. It is based on two stellar absorption‐line indices, the 4000‐Å …
stellar masses of galaxies. It is based on two stellar absorption‐line indices, the 4000‐Å …
Stellar masses and star formation histories for 105 galaxies from the Sloan Digital Sky Survey
G Kauffmann, TM Heckman, SDM White… - Monthly Notices of …, 2003 - ieeexplore.ieee.org
We develop a new method to constrain the star formation histories, dust attenuation and
stellar masses of galaxies. It is based on two stellar absorption-line indices, the 4000-Å …
stellar masses of galaxies. It is based on two stellar absorption-line indices, the 4000-Å …
Stellar masses and star formation histories for 105 galaxies from the Sloan Digital Sky Survey
G Kauffmann, TM Heckman, SDM White… - Monthly Notices of …, 2003 - nyuscholars.nyu.edu
We develop a new method to constrain the star formation histories, dust attenuation and
stellar masses of galaxies. It is based on two stellar absorption-line indices, the 4000-Å …
stellar masses of galaxies. It is based on two stellar absorption-line indices, the 4000-Å …
