G. Feulner

发表

On the constraining observations of the dark GRB 001109 and the properties of a z = 0.398 radio selected starburst galaxy contained in its error box

E. Rol, N. R. Tanvir, J. P. U. Fynbo, 2004, astro-ph/0406414.

The Stellar Mass Function of Galaxies to z ~ 5 in the FORS Deep and GOODS-South Fields

M. Salvato, N. Drory, A. Gabasch, 2004, astro-ph/0412167.

The Munich Near-Infrared Cluster Survey ( MUNICS ) – II . The K-band luminosity function of field galaxies to z ∼ 1 . 2

N. Drory, Garching, U. Hopp, 2022 .

The impact of Spitzer infrared data on stellar mass estimates – and a revised galaxy stellar mass function at 0 < z < 5

Garching, G. Feulner, M. F. Physik, 2007, 0711.0384.

The extraordinarily bright optical afterglow of GRB 991208 and its host galaxy

S. B. Pandey, J. M. Paredes, E. Rol, 2001, astro-ph/0102177.

The evolution of the luminosity functions in the FORS deep field from low to high redshift. II. The red bands

S. Noll, N. Drory, S. Seitz, 2004 .

The Star Formation Rate History in the FORS Deep and GOODS-South Fields

M. Salvato, N. Drory, M. Pannella, 2004 .

The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: I. The blue bands

S. Noll, N. Drory, S. Seitz, 2004, astro-ph/0403535.

Looking for obscured QSOs in the X-ray emitting ERO population

F. Mannucci, R. Della Ceca, P. Saracco, 2005 .