Roland Hendrik den Hartog
European Space Research and Technology Centre
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Featured researches published by Roland Hendrik den Hartog.
Proceedings of SPIE | 2008
Olivier Absil; Denis Defrere; Vincent Coudé du Foresto; Emmanuel di Folco; Roland Hendrik den Hartog; J.-C. Augereau
The possible presence of large amounts of exozodiacal dust around nearby main sequence stars represents a threat to the detection and characterisation of Earth-like extrasolar planets with future infrared space interferometers such as DARWIN or TPF. In this paper, we first review the current detection capabilities of ground-based infrared interferometers such as CHARA/FLUOR and the detections of hot dust that have been obtained so far around a few main sequence stars. With the help of realistic instrumental simulations, we then discuss the relative merits of various ground-based sites (temperate and Antarctic) versus space-based observatories for the detection of exozodiacal discs down to a few zodi by interferometric nulling as a preparation to future life-finding missions. In particular, we discuss the performance of four proposed nulling interferometers: GENIE, ALADDIN, PEGASE and FKSI. An optimised strategy for the characterisation of candidate DARWIN/TPF targets is finally proposed.
Archive | 2007
Olivier Absil; Jean-Charles Augereau; Roland Hendrik den Hartog; Emilie Herwats; P. Gondoin; M. Fridlund
Lep, using a variety of physical parameters. Both the thermal emission andthe scattered light are included in the model. Two types of grains have beenconsidered: smoothed astronomical silicates (Weingartner & Draine 2000)and cold-coagulation type grains (Li & Lunine 2003) with a porosity up to90% when the H
LOW TEMPERATURE DETECTORS: Ninth International Workshop on Low Temperature Detectors | 2002
Roland Hendrik den Hartog; A. G. Kozorezov; J. K. Wigmore; Piet Verhoeve; D. Martin; A. Peacock
One of the factors that limits the energy resolution of superconducting tunnel junctions (STJs) as photon detectors is the spatial dependence of the response on the photoabsorption site. To assess the role of spatial inhomogeneities, we have analyzed quasiparticle (qp) diffusion processes in detail and developed a general analytical theory to describe the evolution of the qp density in an STJ. This theory accounts for (mild) non-linearity due to qp self-recombination, and includes the effects due to multiple qp tunneling, phonon coupling between the electrodes, diffusive losses into electrical connections and localized traps and losses at the edges. The theory does not require any assumptions about symmetry between base and counter electrode. We have derived an analytical model of the STJ response surface and the corresponding spectral lineshape, which allows the influence of the above features to be treated independently. We discuss two examples of the application of this model in practice and demonstrat...
Monthly Notices of the Royal Astronomical Society | 1996
Roland Hendrik den Hartog; P. Katgert
Astrophysical Letters & Communications | 1997
G. Giuricin; A. Biviano; A. Mazure; P. Katgert; J. Perea; M. Moles; P. Focardi; Roland Hendrik den Hartog; Olivier Le Fevre; P. Dubath; Daniel Gerbal; E. Escalera; George Rhee; William D. Jones
Monthly Notices of the Royal Astronomical Society | 1997
Roland Hendrik den Hartog
Archive | 1998
P. Katgert; A. Mazure; Roland Hendrik den Hartog; C. Adami; A. Biviano; J. Perea
Archive | 1996
P. Katgert; A. Mazure; J. Perea; Roland Hendrik den Hartog; Michael Moles; Olivier Le Fevre; P. Dubath; P. Focardi; George Rhee; Bernard J. T. Jones; E. Escalera; A. Biviano; Daniel Gerbal; G. Giuricin
Archive | 1996
A. Mazure; P. Katgert; Roland Hendrik den Hartog; A. Biviano; P. Dubath; E. Escalera; P. Focardi; Daniel Gerbal; G. Giuricin; Bernard J. T. Jones; Olivier Le Fevre; Michael Moles; J. Perea; George Rhee
Astrophysical Letters & Communications | 1996
A. Biviano; G. Giuricin; P. Katgert; A. Mazure; Roland Hendrik den Hartog; P. Dubath; E. Escalera; P. Focardi; Daniel Gerbal; William D. Jones; George Rhee