activity
19982026
most citedCALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation

1.3k citations · 4.1k across the 75 of their papers we have counts for

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Showing 2012Show all

8 papers · 1 filter

astro-ph.CO2012★ 29 cited

The Herschel Fornax Cluster Survey I: The Bright Galaxy Sample

J. I. Davies, S. Bianchi, M. Baes +18

We present Herschel observations of the Fornax cluster at 100, 160, 250, 350 and 500u with a spatial resolution of 7 - 36 arc sec (10" = 1 kpc at d_Fornax=17.9 Mpc). We define a sa…

astro-ph.CO2012★ 251 cited

CALIFA, the Calar Alto Legacy Integral Field Area survey. II. First public data release

CALIFA collaboration, B. Husemann, K. Jahnke +74

We present the first public data release of the CALIFA survey. It consists of science-grade optical datacubes for the first 100 of eventually 600 nearby (0.005<z<0.03) galaxies, ob…

astro-ph.CO2012★ 90 cited

The Herschel Virgo Cluster Survey XII: FIR properties of optically-selected Virgo Cluster galaxies

R. Auld, S. Bianchi, M. W. L. Smith +24

The Herschel Virgo Cluster Survey (HeViCS) is the deepest, confusion-limited survey of the Virgo Cluster at far-infrared (FIR) wavelengths. The entire survey at full depth covers $…

astro-ph.GA2012★ 84 cited

M82 - A radio continuum and polarisation study I. Data reduction and cosmic ray propagation

B. Adebahr, M. Krause, U. Klein +3

The potential role of magnetic fields and cosmic ray propagation for feedback processes in the early Universe can be probed by studies of local starburst counterparts with an equiv…

astro-ph.HE2012★ 69 cited

The XMM-Newton survey of the Small Magellanic Cloud

F. Haberl, R. Sturm, J. Ballet +13

Although numerous archival XMM-Newton observations existed towards the Small Magellanic Cloud (SMC) before 2009, only a fraction of the whole galaxy was covered. Between May 2009 a…

astro-ph.CO2012★ 14 cited

Tidal interaction vs. ram pressure stripping effects as seen in X-rays. Hot gas in group and cluster galaxies

M. Wezgowiec, D. J. Bomans, M. Ehle +4

The hot intracluster/intragroup medium (ICM/IGM) and a high galaxy density can lead to perturbations of the galactic interstellar medium (ISM) due to ram pressure and/or tidal inte…