Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- AlbaNovaSE3.4k papers
- KTH Royal Institute of TechnologySE3.1k papers
- Centre National de la Recherche ScientifiqueFR2.9k papers
- Uppsala UniversitySE2k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR1.9k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR1.8k papers
- University of CopenhagenDK1.8k papers
- Lawrence Berkeley National LaboratoryUS1.8k papers
- University of GenevaCH1.7k papers
- University of OxfordGB1.7k papers
- Aix-Marseille UniversitéFR1.7k papers
- University of California, BerkeleyUS1.7k papers
29 papers · 2 filters
The Hubble Diagram of Type Ia Supernovae as a Function of Host Galaxy Morphology
M. Sullivan, R. S. Ellis, G. Aldering +41
(Abridged) We present new results on the Hubble diagram of distant type Ia supernovae (SNe Ia) segregated according to the type of host galaxy. This makes it possible to check earl…
Indirect searches for neutralino dark matter
Joakim Edsjo
There is mounting evidence for dark matter in the Universe and one of the favourite dark matter candidates is the neutralino, which naturally appears as the lightest supersymmetric…
Physics and Operation of the AMANDA-II High Energy Neutrino Telescope
Steven W. Barwick
This paper briefly describes the principle of operation and science goals of the AMANDA high energy neutrino telescope located at the South Pole, Antarctica. Results from an earlie…
The positron excess and supersymmetric dark matter
Edward A. Baltz, Joakim Edsjo, Katherine Freese +1
Using a new instrument, the HEAT collaboration has confirmed the excess of cosmic ray positrons that they first detected in 1994. We explore the possibility that this excess is due…
DarkSUSY - A numerical package for supersymmetric dark matter calculations
Paolo Gondolo, Joakim Edsjo, Piero Ullio +3
The question of the nature of dark matter in the Universe remains one of the most outstanding unsolved problems in basic science. One of the best motivated particle physics candida…
Massive galaxy clusters as gravitational telescopes for distant supernovae
Christofer Gunnarsson, Ariel Goobar
We investigate the potential of using massive clusters as gravitational telescopes for searches and studies of supernovae of Type Ia and Type II in optical and near-infrared bands…
Wide-Field Surveys from the SNAP Mission
A. Kim
The Supernova/Acceleration Probe (SNAP) is a proposed space-borne observatory that will survey the sky with a wide-field optical/near-infrared (NIR) imager. The images produced by…
SNAP Focal Plane
M. Lampton, C. J. Bebek
The proposed SuperNova/Acceleration Probe (SNAP) mission will have a two-meter class telescope delivering diffraction-limited images to an instrumented 0.7 square-degree field sens…
Determining Bolometric Corrections for BATSE Burst Observations
Luis Borgonovo, Felix Ryde, Miguel de Val Borro +1
We compare the energy and count fluxes obtained by integrating over the finite bandwidth of BATSE with a measure proportional to the bolometric energy flux, the phi-measure, introd…
Effects of halo triaxiality, anisotropy and small scale clumping on WIMP direct detection exclusion limits
Anne M Green
Weakly Interacting Massive Particle (WIMP) direct detection experiments are closing in on the region of parameter space where neutralinos may constitute the Galactic halo dark matt…
IceCube - the next generation neutrino telescope at the South Pole
A. Karle
IceCube is a large neutrino telescope of the next generation to be constructed in the Antarctic Ice Sheet near the South Pole. We present the conceptual design and the sensitivity…
Overview of the SuperNova/Acceleration Probe (SNAP)
G. Aldering, SNAP collaboration
The SuperNova / Acceleration Probe (SNAP) is a space-based experiment to measure the expansion history of the Universe and study both its dark energy and the dark matter. The exper…
Effect of halo modelling on WIMP exclusion limits
Anne M Green
WIMP direct detection experiments are just reaching the sensitivity required to detect galactic dark matter in the form of neutralinos. Data from these experiments are usually anal…
Search for Point Sources of High Energy Neutrinos with AMANDA
J. Ahrens, X. Bai, G. Barouch +1
This paper describes the search for astronomical sources of high-energy neutrinos using the AMANDA-B10 detector, an array of 302 photomultiplier tubes, used for the detection of Ch…
The Type Ia Supernova 1999aw: a Probable 1999aa-like Event In a Low-Luminosity Host Galaxy
L. -G. Strolger, R. C. Smith, N. B. Suntzeff +39
SN 1999aw was discovered during the first campaign of the Nearby Galaxies Supernova Search (NGSS) project. This luminous, slow-declining (Delta m_{15} (B) = 0.81 \pm 0.03) Type Ia…
Cosmological parameters from lensed supernovae
A. Goobar, E. Mortsell, R. Amanullah +1
We investigate the possibility of measuring the Hubble constant, the fractional energy density components and the equation of state parameter of the ``dark energy'' using lensed mu…
Cosmological dark matter annihilations into gamma-rays - a closer look
Piero Ullio, Lars Bergstrom, Joakim Edsjo +1
We investigate the prospects of detecting weakly interacting massive particle (WIMP) dark matter by measuring the contribution to the extragalactic gamma-ray radiation induced, in…
Search for Neutrino-Induced Cascades with the AMANDA Detector
J. Ahrens
We report on a search for electromagnetic and/or hadronic showers (cascades) induced by a diffuse flux of neutrinos with energies between 5 TeV and 300 TeV from extraterrestrial so…
SNOC: a Monte-Carlo simulation package for high-z supernova observations
A. Goobar, E. Mortsell, R. Amanullah +3
We present a Monte-Carlo package for simulation of high-redshift supernova data, SNOC. Optical and near-infrared photons from supernovae are ray-traced over cosmological distances…
The distant Type Ia supernova rate
R. Pain, S. Fabbro, M. Sullivan +26
We present a measurement of the rate of distant Type Ia supernovae derived using 4 large subsets of data from the Supernova Cosmology Project. Within this fiducial sample, which su…
Observation of High Energy Atmospheric Neutrinos with the Antarctic Muon and Neutrino Detector Array
AMANDA Collaboration, J. Ahrens
The Antarctic Muon and Neutrino Detector Array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming thr…
Probing the dark side: Constraints on the dark energy equation of state from CMB, large scale structure and Type Ia supernovae
Steen Hannestad, Edvard Mortsell
We have reanalysed constraints on the equation of state parameter, w_Q = P/rho, of the dark energy, using several cosmological data sets and relaxing the usual constraint w_Q > -1.…
Correcting for lensing bias in the Hubble diagram
R. Amanullah, E. Mortsell, A. Goobar
Gravitational lensing will cause a dispersion in the Hubble diagram for high redshift sources. This effect will introduce a bias in the cosmological parameter determination using t…
Are there MACHOs in the Milky Way halo?
Anne M Green, Karsten Jedamzik
Microlensing searches aim to detect compact halo dark matter via its gravitational lensing effect on stars within the Large Magellanic Cloud. The most recent results have led to th…