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most citedMolecfit: A general tool for telluric absorption correction. I. Method and application to ESO instruments

762 citations · 3.1k across the 33 of their papers we have counts for

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11 papers · 1 filter

astro-ph2008★ 154 cited

The environments of starburst and post-starburst galaxies at z=0.4-0.8

Bianca M. Poggianti, Alfonso Aragon-Salamanca, Dennis Zaritsky +16

Post-starburst (E+A or k+a) spectra, characterized by their exceptionally strong Balmer lines in absorption and the lack of emission lines, belong to galaxies in which the star for…

astro-ph2008★ 155 cited

The relation between star formation, morphology and local density in high redshift clusters and groups

Bianca M. Poggianti, Vandana Desai, Rose Finn +17

We investigate how the [OII] properties and the morphologies of galaxies in clusters and groups at z=0.4-0.8 depend on projected local galaxy density, and compare with the field at…

astro-ph2008★ 125 cited

The evolution of the brightest cluster galaxies since z~1 from the ESO Distant Cluster Survey (EDisCS)

I. M. Whiley, A. Aragon-Salamanca, G. De Lucia +13

[Abridged] We present K-band data for the brightest cluster galaxies (BCGs) from the ESO Distant Cluster Survey. These data are combined with photometry from Aragon-Salamanca et al…

astro-ph2008★ 84 cited

Spectroscopy of clusters in the ESO distant cluster survey (EDisCS).II. Redshifts, velocity dispersions, and substructure for clusters in the last 15 fields

Bo Milvang-Jensen, Stefan Noll, Claire Halliday +17

AIMS. We present spectroscopic observations of galaxies in 15 survey fields as part of the ESO Distant Cluster Survey (EDisCS). We determine the redshifts and velocity dispersions…

astro-ph2007★ 23 cited

A deep i-selected multi-waveband galaxy catalogue in the COSMOS field

A. Gabasch, Y. Goranova, U. Hopp +2

In this paper we present a deep and homogeneous i-band selected multi-waveband catalogue in the COSMOS field covering an area of about 0.7 square-degree. Our catalogue with a forma…

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…