Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR10.1k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR4.1k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR3.2k papers
- Université Paris-SaclayFR3.1k papers
- National Institute for Subatomic PhysicsNL2k papers
- University of ManchesterGB2k papers
- Sapienza University of RomeIT2k papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT1.9k papers
- CEA Paris-SaclayFR1.9k papers
- Heidelberg UniversityDE1.8k papers
- Rutherford Appleton LaboratoryGB1.8k papers
- Laboratoire de Physique Nucléaire et de Hautes ÉnergiesFR1.8k papers
41 papers · 2 filters
The Nature of the Low-Metallicity ISM in the Dwarf Galaxy NGC 1569
F. Galliano, S. C. Madden, A. P. Jones +3
We are modeling the spectra of dwarf galaxies from infrared to submillimeter wavelengths to understand the nature of the various dust components in low-metallicity environments, wh…
Ho Measurement from VLT Deep I-band Surface Brightness Fluctuations in NGC 564 and NGC 7619
S. Mei, M. Scodeggio, D. R. Silva +1
We have measured the Hubble constant Ho in NGC 564 at cz ~ 5800 km/s and in NGC 7619 at cz ~ 3700 km/s with deep I-band Surface Brightness Fluctuation distance measurements at the…
Cosmological Magnetogenesis driven by Radiation Pressure
Mathieu Langer, Jean-Loup Puget, Nabila Aghanim
The origin of large scale cosmological magnetic fields remains a mystery, despite the continuous efforts devoted to that problem. We present a new model of magnetic field generatio…
A simplified numerical model of coronal energy dissipation based on reduced MHD
E. Buchlin, V. Aletti, S. Galtier +3
A 3D model intermediate between cellular automata (CA) models and the reduced magnetohydrodynamic (RMHD) equations is presented to simulate solar impulsive events generated along a…
Extraction of cluster parameters with future Sunyaev-Zel'dovich observations
Nabila Aghanim, Steen H. Hansen, Sergio Pastor +1
The Sunyaev-Zel'dovich (SZ) effect of galaxy clusters is characterized by three parameters: Compton parameter, electron temperature and cluster peculiar velocity. In the present st…
Simulating Cosmic Microwave Background maps in multi-connected spaces
Alain Riazuelo, Jean-Philippe Uzan, Roland Lehoucq +1
This article describes the computation of cosmic microwave background anisotropies in a universe with multi-connected spatial sections and focuses on the implementation of the topo…
A 1.2mm MAMBO/IRAM-30m Study of Dust Emission from optically luminous z~2 Quasars
A. Omont, A. Beelen, F. Bertoldi +5
We report 250GHz (1.2mm) observations of redshift 1.8 < z < 2.8 optically luminous (M_B < -27.0), radio quiet quasars using the Max-Planck Millimeter Bolometer (MAMBO) array at the…
Results of the ESO-SEST Key Programme on CO in the Magellanic Clouds. IX. The giant LMC HII region complex N11
F. P. Israel, Th. de Graauw, L. E. B. Johansson +7
We present maps and a catalogue containing the J=1-0 12CO parameters of 29 individual molecular clouds in the second-brightest LMC star formation complex, N11. In the southwestern…
Predictions for Cosmological Infrared Surveys from Space with the Multiband Imaging Photometer for SIRTF (MIPS)
H. Dole, G. Lagache, J. -L. Puget +1
We make predictions for the cosmological surveys to be conducted by MIPS/SIRTF at 24, 70 and 160 microns, for the GTO and the legacy programs, using the latest knowledge of the ins…
Bias and the power spectrum beyond the turn-over
Ruth Durrer, Andrea Gabrielli, Michael Joyce +1
Threshold biasing of a Gaussian random field gives a linear amplification of the reduced two point correlation function at large distances. We show that for standard cosmological m…
Study of a Strategy for Parallax Microlensing Detection Towards the Magellanic Clouds
S. Rahvar, M. Moniez, R. Ansari +1
In this article, we have investigated the possibility to distinguish between different galactic models through the microlensing parallax studies. We show that a systematic search f…
Cosmological constraints from Archeops
A. Benoit, P. Ade, A. Amblard +65
We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum ha…
Generation of Primordial Cosmological Perturbations from Statistical Mechanical Models
A. Gabrielli, B. Jancovici, M. Joyce +3
The initial conditions describing seed fluctuations for the formation of structure in standard cosmological models, i.e.the Harrison-Zeldovich distribution, have very characteristi…
Collision-induced galaxy formation: semi-analytical model and multi-wavelength predictions
Christophe Balland, Julien E. G. Devriendt, Joe Silk
A semi-analytic model is proposed that couples the Press-Schechter formalism for the number of galaxies with a prescription for galaxy-galaxy interactions that enables to follow th…
Detection of abundant solid CO in the disk around CRBR 2422.8-3423
W. F. Thi, K. M. Pontoppidan, E. F. van Dishoeck +2
We present direct evidence for CO freeze-out in a circumstellar disk around the edge-on class I object CRBR 2422.8-3423, observed in the M band with VLT-ISAAC at a resolving power…
Detecting Topology in a Nearly Flat Spherical Universe
Jeffrey Weeks, Roland Lehoucq, Jean-Philippe Uzan
When the density parameter is close to unity, the universe has a large curvature radius independently of its being hyperbolic, flat, or spherical. Whatever the curvature, the unive…
Inflationary models inducing non-Gaussian metric fluctuations
Francis Bernardeau, Jean-Philippe Uzan
We construct explicit models of multi-field inflation in which the primordial metric fluctuations do not necessarily obey Gaussian statistics. These models are realizations of mech…
Data analysis methods for XMM-Newton observations of extended sources. Application to bright massive clusters of galaxies at z=0.2
Philippe B. Marty, Jean-Paul Kneib, Rachida Sadat +2
In this paper, a review is given of methods useful for XMM-Newton EPIC data analysis of extended sources, along with some applications to a bright massive cluster of galaxies at z=…
ISO-LWS observations of C+ and O lines in absorption toward SgrB2
Charlotte Vastel, Edward Polehampton, Jean-Paul Baluteau +3
High spectral resolution ISO-LWS observations of the [OI] 63.2 and 145.5 microns and [CII] 157.7 microns fine structure lines are presented for the center of the Sagittarius B2 com…
Power spectrum of the cosmic infrared background at 60 and 100 microns with IRAS
M. -A. Miville-Deschenes, G. Lagache, J. -L. Puget
Based on a power spectrum analysis of the IRAS ISSA maps, we present the first detection of the Cosmic far-Infrared Background (CIB) fluctuations at 60 and 100 microns. The power s…
EROS 2 proper motion survey: Constraints on the halo white dwarfs
B. Goldman, C. Afonso, Ch. Alard +9
We are conducting a 377-square-degree proper motion survey in the ~V and I bands in order to determine the cool white dwarf contribution to the Galactic dark matter. Using the 250…
High Resolution CO and H2 Molecular Line Imaging of a Cometary Globule in the Helix Nebula
P. J. Huggins, T. Forveille, R. Bachiller +3
We report high resolution imaging of a prominent cometary globule in the Helix nebula in the CO J=1-0 (2.6 mm) and H2 v=1-0 S(1) (2.12 micron) lines. The observations confirm that…
H2 formation and excitation in the diffuse interstellar medium
Cecile Gry, Francois Boulanger, Cyrine Nehme +3
We use far-UV absorption spectra obtained with FUSE towards three late B stars to study the formation and excitation of H2 in the diffuse ISM. The data interpretation relies on a m…
Optimization of the Coupling of High-Frequency Horn Antenna Array to the ESA PLANCK Submillimeter-Wave Telescope
Vladimir Yurchenko, John Anthony Murphy, Jean-Michel Lamarre
We study the electromagnetic coupling of the array of Gaussian and multi-moded horn antennas to the dual-reflector submillimeter-wave telescope on the ESA PLANCK Surveyor designed…