A procedure to produce excess, probability and significance maps and to compute point-sources flux upper limits
A short note to propose a procedure to construct excess maps, probability maps and to calculate point source flux upper
953 indexed results
A short note to propose a procedure to construct excess maps, probability maps and to calculate point source flux upper
An increased data sample of identified secondary muons is collected at detection level. Project GRAND identifies secondary cosmic ray muons
Gravitational lensing can be by a faint star, a trillion stars of a galaxy, or a cluster of galaxies, and
It is shown on the ground of a simple 6\times 6 neutrino mixing model that one of three conventional sterile
The geometry of three-dimensional space guides the search for a better model than the blackhole with its unwelcome singularity. An
We conjecture that black holes, whether accreting matter or not, can also lose mass to phantom energy production. Such a
Gamma-ray bursts, discovered over three decades ago, can appear to be a hundred times as luminous as the brightest supernovae.
Quasi Elastic Scattering (QEL) is the dominant source for producing both Fully Contained Events and Partially Contained Events in the
Can the submillimetre counts and background be produced by applying a locally derived extinction correction to the population of Lyman
We consider the 2D SU(N) principal chiral model and discuss a vortex condensation mechanism which could explain the existence of
A method of soldering of melt-textured YBa2Cu3O7-d -based (MT-YBCO) superconductive blocks using a TmBaCu3O7-d (Tm123) powder has been suggested. The
We have shown that inflatons with a mass which is calculated to be of the order of $10^{10}\GeV$ can constitute
We present new techniques to produce IRAS 12 micron samples of galaxies and stars. We show that previous IRAS 12
Observations of Her X-1 by the Extreme Ultraviolet Explorer (EUVE) at the end of the x-ray Short High state are
We use a rigorous method, based on Bayesian inference, for calculating the odds favoring the hypothesis that any particular class
Astronomy at the highest energies observed must be performed by studying neutrinos rather than photons because the universe is opaque
It has been conjectured (astro-ph/0103463) that a gravitational lens consisting of n point masses can not produce more than 5(n-1)
Number of monitoring observations of continuum emission from Active Galactic Nuclei (AGNs) have been made in optical--X-ray bands. The results
The evolution of neutrino physics demands new schemes to produce intense, collimated and pure neutrino beams. The current neutrino factory
There are successful approaches to explain the formation of the tachocline by a poloidal magnetic field in the solar core.
The core-accretion mechanism for gas giant formation may be too slow to create all observed gas giant planets during reasonable
While application software does the real work, domain-specific languages (DSLs) are tools to help produce it efficiently, and language design
We give an assessment of the significance of various known effects which may produce genuine fluctuations of star positions comparable
In this work we describe, design and analyze the security of a tamper-evident, append-only data structure for maintaining secure data