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16 papers · 1 filter
Quantifying the Impact of Cosmological Parameter Uncertainties on Strong Lensing Models With an Eye Toward the Frontier Fields
Matthew B. Bayliss, Keren Sharon, Traci Johnson
We test the effects of varying the cosmological parameter values used in the strong lens modeling process for the six Hubble Frontier Fields (HFF) galaxy clusters. The standard pro…
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Luminosity and Color Dependence and Redshift Evolution
Hong Guo, Idit Zehavi, Zheng Zheng +40
We measure the luminosity and color dependence and the redshift evolution of galaxy clustering in the Sloan Digital Sky Survey-III Baryon Oscillation Spectroscopic Survey Ninth Dat…
An ultraviolet-optical flare from the tidal disruption of a helium-rich stellar core
S. Gezari, R. Chornock, A. Rest +31
The flare of radiation from the tidal disruption and accretion of a star can be used as a marker for supermassive black holes that otherwise lie dormant and undetected in the centr…
An Improved Forecast of Patchy Reionization Reconstruction with CMB
Meng Su, Amit P. S. Yadav, Matthew McQuinn +2
Inhomogeneous reionization gives rise to angular fluctuations in the Cosmic Microwave Background (CMB) optical depth tau(n) to the last scattering surface, correlating different sp…
Turbulent formation of protogalaxies at the plasma to gas transition
Rudolph E. Schild, Carl H. Gibson
The standard model of gravitational structure formation is based on the Jeans 1902 acoustic theory, neglecting crucial effects of viscosity, turbulence and diffusion. A Jeans lengt…
Formation of Planets by Hydrogravitational Dynamics
Carl H. Gibson, Rudolph E. Schild
From hydro-gravitational cosmology, hydrogen-helium gas planets fragmented at the plasma to gas transition 300,000 years after the big bang in million-star-mass clumps. Stars may f…