1. Galactic Astronomy 銀河物理学特論 I Lecture 3-3: Stellar mass function of galaxies Seminar: Perez-Gonzalez et al. 2008, ApJ, 675, 234
Lecture:
2012/01/16

2. Observed magnitude and stellar mass, current stellar mass limit of deep surveys:
Marchesini et al. 2009, ApJ, 701, 1765,

3. Evolution of Stellar Mass Function of Galaxies : Uncertainty due to stellar population synthesis model
Kajisawa et al. 2009, ApJ, 702, 1393

4. Evolution of Stellar Mass Function of Galaxies :
Kajisawa et al. 2009, ApJ, 702, 1393
Marchesini et al. 2009, ApJ, 701, 1765

5. Evolution of stellar mass density as a function of z:
Kajisawa et al. 2009, ApJ, 702, 1393
Marchesini et al. 2009, ApJ, 701, 1765

6. Evolution of stellar mass density as a function of z and stellar mass
2019/6/4
Evolution of stellar mass density as a function of z and stellar mass
Marchesini et al. 2009, ApJ, 701, 1765,
Perez-Gonzalez et al. 2008, ApJ, 675, 234

7. Luminosity function compared with semi-analytic models
Bower 2008

8. Luminosity function compared with semi-analytic models
Based on simple Cold-Dark-Matter galaxy formation model, more massive galaxies expected than observed. Formation of massive galaxies needs to be stopped with feed-back from AGNs etc.
Without AGN feedback
With AGN feedback
Without AGN feedback
With AGN feedback
Bower et al. 2006, MNRAS, 370, 645

9. Stellar mass function compared with semi-analytic models
Three semi-analytic models with AGN feedback etc.
Bower et al. 2011, arXiv:

10. The relation between stellar mass and star formation rate:
Daddi et al. 2007, ApJ, 670, 156

11. The relation between stellar mass and star formation rate:
Comparison with semi-analytic models
Z=0 observation (contour) vs.
Three semi-analytic models with AGN feedback etc.
Bower et al. 2011, arXiv:

12. 2019/6/4
Evolution of stellar mass density as a function of z and stellar mass, compared with the estimated growth curve of SMBHs
Perez-Gonzalez et al. 2008, ApJ, 675, 234
Marconi et al. 2004, MNRAS, 351, 169
Single Eddington ratio assumed, etc.