activity
20092015
most citedAn improved model of Charge Transfer Inefficiency and correction algorithm for the Hubble Space Telescope

85 citations · 296 across the 5 of their papers we have counts for

collaborators

13 papers

astro-ph.CO2015★ 28 cited

Euclid space mission: a cosmological challenge for the next 15 years

R. Scaramella, Y. Mellier, J. Amiaux +33

Euclid is the next ESA mission devoted to cosmology. It aims at observing most of the extragalactic sky, studying both gravitational lensing and clustering over 15,000 square…

astro-ph.IM2015★ 27 cited

Measuring a Charge-Coupled Device Point Spread Function: Euclid Visible Instrument CCD273-84 PSF Performance

Sami-Matias Niemi, Mark Cropper, Magdalena Szafraniec +1

In this paper we present the testing of a back-illuminated development Euclid Visible Instrument (VIS) Charge-Coupled Device (CCD) to measure the intrinsic CCD Point Spread Functio…

astro-ph.GA2014★ 72 cited

Stellar Kinematics and Structural Properties of Virgo Cluster Dwarf Early-Type Galaxies from the SMAKCED Project II. The Survey and a Systematic Analysis of Kinematic Anomalies and Asymmetries

E. Toloba, P. Guhathakurta, R. Peletier +15

We present spatially resolved kinematics and global stellar populations and mass-to-light ratios for a sample of 39 dwarf early-type (dE) galaxies in the Virgo cluster studied as p…

astro-ph.IM2014★ 85 cited

An improved model of Charge Transfer Inefficiency and correction algorithm for the Hubble Space Telescope

Richard Massey, Tim Schrabback, Oliver Cordes +7

Charge-Coupled Device (CCD) detectors, widely used to obtain digital imaging, can be damaged by high energy radiation. Degraded images appear blurred, because of an effect known as…

astro-ph.CO2013★ 84 cited

A near-infrared census of the multi-component stellar structure of early-type dwarf galaxies in the Virgo cluster

J. Janz, E. Laurikainen, T. Lisker +12

The fraction of star-forming to quiescent dwarf galaxies varies from almost infinity in the field to zero in the centers of rich galaxy clusters. What is causing this pronounced mo…

astro-ph.CO2012

Physical properties of Herschel selected galaxies in a semi-analytic galaxy formation model

Sami-Matias Niemi, Rachel S. Somerville, Henry C. Ferguson +3

[Abridged] We make use of a semi-analytic cosmological model that includes simple prescriptions for dust attenuation and emission to make predictions for the observable and physica…