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Dark Energy Measured with Record-Breaking Map of 1.2 Million Galaxies
Dark Energy Measured Record-Breaking Map 1.2 Million Galaxies
2016/8/1
A team of hundreds of physicists and astronomers have announced results from the largest-ever, three-dimensional map of distant galaxies. The team constructed this map to make one of the most precise ...
Spectra of Nearby Galaxies Measured with a New Very Broadband Receiver
spectrographs spectroscopic
2014/12/23
Three-millimeter-wavelength spectra of a number of nearby galaxies have been obtained at the Five College Radio Astronomy Observatory (FCRAO) using a new, very broadband receiver. This instrument, whi...
CMS: Cosmic muons in simulation and measured data
CMS Cosmic muons simulation measured data
2011/10/18
A dedicated cosmic muon Monte-Carlo event generator CMSCGEN has been developed for the CMS experiment. The simulation relies on parameterisations of the muon energy and the incidence angle, based on m...
Study of measured pulsar masses and their possible conclusions
measured pulsar masses possible conclusions
2011/1/11
We study the statistics of 61 measured masses of neutron stars (NSs) in binary pulsar systems, including 18 double NS (DNS) systems, 26 radio pulsars (10 in our Galaxy) with white dwarf (WD) companion...
Have Baryonic Acoustic Oscillations in the galaxy distribution really been measured?
galaxies: statistics cosmology theory large-scale structure
2010/11/15
Recent publications claim that there is no convincing evidence for measurements of the baryonic acoustic (BAO) feature in galaxy samples using either monopole or radial information. Di erent claims se...
Solar Meridional Circulation from Doppler Shifts of the Fe I line at lambda 5250 Angstroms as Measured by the 150-foot Solar Tower Telescope at the Mt. Wilson Observatory
Solar and Stellar Astrophysics (astro-ph.SR)
2010/12/23
Doppler shifts of the Fe I spectral line at lambda5250 Angstroms from the full solar disk obtained over the period 1986 to 2009 are analyzed to determine the circulation velocity of the solar surface ...
Implications of the Cosmic Ray Electron Spectrum and Anisotropy measured with Fermi-LAT
High Energy Astrophysical Phenomena (astro-ph.HE)
2010/12/23
The Fermi Large Area Telescope (LAT) collaboration recently released the updated results of the measurement of the cosmic ray electron (CRE) spectrum and published its first constraints on the CRE ani...
The Galactic Bulge velocity dispersion as measured by stellar proper motions in Plaut`s window
velocity dispersion Plaut`s window stellar proper motions
2009/6/26
The Galactic Bulge velocity dispersion as measured by stellar proper motions in Plaut`s window。
The seeing at San Pedro Mártir observatory as measured using the dimm method
San Pedro Mártir dimm method
2009/6/11
The seeing at San Pedro Mártir observatory as measured using the dimm method。
Wind Power Spectrum Measured at the San Pedro Mártir Sierra
San Pedro Mártir Sierra Wind Power Spectrum
2009/6/9
Wind Power Spectrum Measured at the San Pedro Mártir Sierra。
MEASURED STARK WIDTH AND SHIFT OF 393.367 nm Ca II RESONANCE SPECTRAL LINE
MEASURED STARK WIDTH RESONANCE SPECTRAL LINE Ca II
2009/4/21
MEASURED STARK WIDTH AND SHIFT OF 393.367 nm Ca II RESONANCE SPECTRAL LINE。
MEASURED STARK WIDTH AND SHIFT OF THE P HeII SPECTRAL LINE
P HeII SPECTRAL LINE MEASURED STARK WIDTH
2009/4/20
MEASURED STARK WIDTH AND SHIFT OF THE P HeII SPECTRAL LINE。
MEASURED STARK WIDTHS OF A 425.94 nm ArI SPECTRAL LINE
MEASURED STARK WIDTHS 425.94 nm ArI SPECTRAL LINE
2009/4/16
MEASURED STARK WIDTHS OF A 425.94 nm ArI SPECTRAL LINE。
MEASURED, CALCULATED AND PREDICTED STARK WIDTHS OF THE SINGLY IONIZED C, N, O, F, Ne, Si, P, S, Cl AND Ar SPECTRAL LINES
plasma spectroscopy ionized emitters Ar SPECTRAL LINES
2009/3/18
In order to find reliable Stark width data, needed in plasma spectroscopy,
comparision between the existing measured, calculated and predicted
Stark width values was performed for ten singly ionized...
MEASURED, CALCULATED AND PREDICTED STARK WIDTHS ALONG A BERYLLIUM ISOELECTRONIC SEQUENCEIN THE 3s-3p TRANSITION
Stark width values isoelectronic sequence ionized emitters
2009/3/13
On the basis of the observed satisfactory agreement between recent
experimental and calculated Stark width values with our earlier predicted ones
along the beryllium isoelectronic sequence (BeI, BII...