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26 April 2024
 
  » arxiv » astro-ph/0407644

 Article overview



The Luminosity Function of Early-Type Galaxies at z~0.75
N. J. G. Cross ; R. Bouwens ; N. Benitez ; J. P. Blakeslee ; F. Menanteau ; H. C. Ford ; T. Goto ; B. Holden ; A. R. Martel ; R. Overzier ; C. Gronwall ; N. Homeier ; D. R. Ardila ; F. Bartko ; T. J. Broadhurst ; R. A. Brown ; C.J. Burrows ; E. S. Cheng ; M. Clampin ; P. D. Feldman ; M. Franx ; D. A. Golimowski ; G. F. Hartig ; G. D. Illingworth ; L. Infante ; R. A. Kimble ; J. E. Krist ; M. P. Lesser ; G. R. Meurer ; G. K. Miley ; M. Postman ; P. Rosati ; M. Sirianni ; W. B. Sparks ; H. D. Tran ; Z. I. Tsvetanov ; R. L. White ; W. Zheng ;
Date 30 Jul 2004
Subject astro-ph
AbstractWe measure the luminosity function of morphologically selected E/S0 galaxies from $z=0.5$ to $z=1.0$ using deep high resolution Advanced Camera for Surveys imaging data. Our analysis covers an area of $48Boxarcmin$ (8$ imes$ the area of the HDF-N) and extends 2 magnitudes deeper ($Isim24$ mag) than was possible in the Deep Groth Strip Survey (DGSS). At $0.51.7$, E/S0 galaxies at brighter luminosities ($M_B<-20.1$), but are increasingly different at fainter magnitudes where `blue’ galaxies are both smaller and have lower Sersic parameters. Fits of the colors to stellar population models suggest that most E/S0 galaxies have short star-formation time scales ($ au<1$ Gyr), and that galaxies have formed at an increasing rate from $zsim8$ until $zsim2$ after which there has been a gradual decline.
Source arXiv, astro-ph/0407644
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