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The SIMPLE survey: observations, reduction, and catalog
catalogs – galaxies evolution – galaxies observations – galaxies photometry –infrared galaxies
2010/11/15
We present the Spitzer IRAC/MUSYC Public Legacy Survey in the Extended CDF-South (SIM-
PLE), which consists of deep IRAC observations covering the 1,600 arcmin2 area surrounding
GOODS-S. The limiti...
Tidal stirring of Milky Way satellites: a simple picture with the integrated tidal force
stirring of Milky Way satellites simple picture integrated tidal force
2010/11/16
Most of dwarf spheroidal galaxies in the Local Group were probably formed via environmental processes like the tidal interaction with the Milky Way.We study this process via N-body simulations of dwar...
Mode width fitting with a simple bayesian approach. Application to CoRoT targets HD 181420 and HD 49933
statistics detection data analysis asteroseismology
2010/11/15
Aims. We investigate the asteroseismology of two solar-like targets as observed with the CoRoT satellite, with particular attention paid to the mode fitting. HD 181420 and HD 49933 are typical CoRoT s...
A simple connection between the near- and mid-infrared emission of galaxies and their star-formation rates
the near- and mid-infrared emission galaxies
2011/1/10
We have measured the near-infrared colors and the fluxes of individual pixels in 68 galaxies common to the Spitzer Infrared Nearby Galaxies Survey and the Large Galaxy Atlas Survey. Each galaxy was se...
A simple analytic model for astrophysical S-factors
High Energy Astrophysical Phenomena (astro-ph.HE)
2010/12/29
We propose a physically transparent analytic model of astrophysical S-factors as a function of a center-of-mass energy E of colliding nuclei (below and above the Coulomb barrier) for non-resonant fusi...
A simple accretion model of a rotating gas sphere onto a Schwarzschild black hole
gas sphere Schwarzschild black hole
2009/7/9
A simple accretion model of a rotating gas sphere onto a Schwarzschild black hole。
A simple model to determine chaotic motions around asteroids
determine chaotic motions asteroids
2009/6/26
A simple model to determine chaotic motions around asteroids。
A Simple Model for Hydromagnetic Instabilities in the Presence of a Constant Magnetic Field
Hydromagnetic Instabilities Constant Magnetic Field
2009/6/25
A Simple Model for Hydromagnetic Instabilities in the Presence of a Constant Magnetic Field。
A simple, unifying model of the extreme Ultraviolet spectra of dwarf novae in outburst
extreme Ultraviolet spectra dwarf novae outburst
2009/6/17
A simple, unifying model of the extreme Ultraviolet spectra of dwarf novae in outburst。
Global Evolution of Solids in Protoplanetary Disks：a Simple Model
Protoplanetary Disks Global Evolution
2009/6/16
Global Evolution of Solids in Protoplanetary Disks：a Simple Model。
A SIMPLE, APPROXIMATE METHOD FOR ANALYSIS OF KERR-NEWMAN BLACK HOLE DYNAMICS AND THERMODYNAMICS
Black hole physics Kerr-Newman black hole
2010/10/29
In this work we present a simple approximate method for analysis of the basic dynamical and thermodynamical characteristics of Kerr-Newman black hole. Instead of the complete dynamics of the black hol...
A Simple Model for Reflection-Driven Spectral Evolution of Turbulence in the Corona and Inner Heliosphere
Inner Heliosphere Corona Reflection-Driven Spectral Evolution
2009/5/27
Dissipation of turbulence is generally considered as a prime candidate for the heating and acceleration of solar wind from the corona throughout the heliosphere, due to radially evolving dissipation p...
Making the Search Simple（图）
optical electronics
2006/12/20
December 14, 2006,Could SETI efforts be simpler? While today’s radio searches rely on highly sophisticated antennas and receivers, our fledgling optical search systems are far less intricate. Experi...