activity
20112022
most citedStellar mass map and dark matter distribution in M31

212 citations · 720 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.IM2022★ 16 cited

TOPz: Photometric redshifts for J-PAS

J. Laur, E. Tempel, A. Tamm +30

The importance of photometric galaxy redshift estimation is rapidly increasing with the development of specialised powerful observational facilities. We develop a new photometric r…

astro-ph.GA2016★ 80 cited

The Herschel Exploitation of Local Galaxy Andromeda (HELGA) VII: A SKIRT radiative transfer model and insights on dust heating

S. Viaene, M. Baes, A. Tamm +17

The radiation of stars heats dust grains in the diffuse interstellar medium and in star-forming regions in galaxies. Modelling this interaction provides information on dust in gala…

astro-ph.CO2015★ 91 cited

Galaxy Cluster Mass Reconstruction Project: II. Quantifying scatter and bias using contrasting mock catalogues

L. Old, R. Wojtak, G. A. Mamon +21

This article is the second in a series in which we perform an extensive comparison of various galaxy-based cluster mass estimation techniques that utilise the positions, velocities…

astro-ph.CO2014★ 51 cited

Galaxy filaments as pearl necklaces

E. Tempel, R. Kipper, E. Saar +3

Context. Galaxies in the Universe form chains (filaments) that connect groups and clusters of galaxies. The filamentary network includes nearly half of the galaxies and is visually…

astro-ph.CO2013★ 42 cited

Orientation of cosmic web filaments with respect to the underlying velocity field

E. Tempel, N. I. Libeskind, Y. Hoffman +2

The large-scale structure of the Universe is characterised by a web-like structure made of voids, sheets, filaments, and knots. The structure of this so-called cosmic web is dictat…

astro-ph.CO2012★ 212 cited

Stellar mass map and dark matter distribution in M31

A. Tamm, E. Tempel, P. Tenjes +2

Stellar mass distribution in M31 is estimated using optical and infrared imaging data. Combining the derived stellar mass model with various kinematical data, properties of the DM…