Showing 1997 · astro-phShow all

18 papers · 2 filters

astro-ph1997★ 12 cited

Preliminary Limits on the WIMP-Nucleon Cross Section from the Cryogenic Dark Matter Search (CDMS)

DS Akerib, PD Barnes, DA Bauer +28

We are conducting an experiment to search for WIMPs, or weakly-interacting massive particles, in the galactic halo using terrestrial detectors. This generic class of hypothetical p…

astro-ph1997★ 237 cited

Multiwavelength Observations of a Dramatic High Energy Flare in the Blazar 3C 279

A. E. Wehrle, E. Pian, C. M. Urry +3

The blazar 3C 279, one of the brightest identified extragalactic objects in the gamma-ray sky, underwent a flare of a factor 10 amplitude in gamma-rays towards the end of a 3-week…

astro-ph1997

Distribution of Fluences versus Peak Fluxes and the Cosmological Density Evolution of the Rate of GRBs

Vahe' Petrosian, Nicole M. Lloyd-Ronning

We argue that recent observations of afterglows and some theoretical considerations indicate that the gamma-ray fluence may be a better measure of strength of a burst than its peak…

astro-ph1997★ 1 cited

The Extent of the Spectral Bias in BATSE: The True Distribution of the nu F_nu Peak Energy

Nicole M. Lloyd-Ronning, Vahe' Petrosian

The distributions of spectral characteristics and their correlations with fluence, peak flux, or duration, are essential in understanding the nature of GRBs. However, the selection…

astro-ph1997★ 10 cited

The art of fitting p-mode spectra: Part II. Leakage and noise covariance matrices

T. Appourchaux, M. C. Rabello-Soares, L. Gizon

In Part I we have developed a theory for fitting p-mode Fourier spectra assuming that these spectra have a multi-normal distribution. We showed, using Monte-Carlo simulations, how…

astro-ph1997★ 87 cited

The art of fitting p-mode spectra: Part I. Maximum Likelihood Estimation

T. Appourchaux, L. Gizon, M. C. Rabello-Soares

In this article we present our state of the art of fitting helioseismic p-mode spectra. We give a step by step recipe for fitting the spectra: statistics of the spectra both for sp…