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19982017
most citedThe evolution of the luminosity functions in the FORS Deep Field from low to high redshift: I. The blue bands

159 citations · 574 across the 21 of their papers we have counts for

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19 papers · 1 filter

astro-ph2007★ 93 cited

Lyman alpha emission in high-redshift galaxies

C. Tapken, I. Appenzeller, S. Noll +4

A significant fraction of the high-redshift galaxies show strong Lyman emission lines. For redshifts z>5, most known galaxies belong to this class. However, so far not much is know…

astro-ph2005★ 9 cited

SDSS J1553+0056: A BALQSO mimicking a Lyman-break galaxy

I. Appenzeller, O. Stahl, C. Tapken +2

Using the UVES echelle spectrograph at the ESO VLT we obtained high-resolution (R = 40 000) spectra of the object SDSS J1553+0056, which has been identified in the literature alter…

astro-ph2005★ 53 cited

Edge-on T Tauri stars

Immo Appenzeller, Claude Bertout, Otmar Stahl

Using the UVES echelle spectrograph at the ESO VLT we obtained two-dimensional high-resolution (R = 50 000) spectra of the edge-on disk objects HH30*, HK Tau B, and HV Tau C. For c…

astro-ph2004★ 159 cited

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

A. Gabasch, R. Bender, S. Seitz +13

We use the very deep and homogeneous I-band selected dataset of the FORS Deep Field (FDF) to trace the evolution of the luminosity function over the redshift range 0.5 < z < 5.0. W…

astro-ph2003★ 7 cited

The metal absorption systems of the QSO 0103-260 and the galaxy redshift distribution in the FORS Deep Field

Stephan Frank, Immo Appenzeller, Stefan Noll +1

Using the Uves echelle spectrograph at the ESO VLT, we observed the absorption line spectrum of the QSO 0103-260 in the Fors Deep Field. In addition to the expected Ly-alpha forest…

astro-ph2003★ 27 cited

Spectropolarimetry of the borderline Seyfert 1 galaxy ESO 323-G077

H. M. Schmid, I. Appenzeller, U. Burch

We report the detection of high linear polarization in the bright Seyfert 1 galaxy ESO 323-G077. Based on optical spectropolarimetry with FORS1 at the VLT we find a continuum polar…