output
20072024
most citedA calibration of the stellar mass fundamental plane at z ~ 0.5 using the micro-lensing induced flux ratio anomalies of macro-lensed quasars

93 citations

Showing 2014Show all

9 papers · 1 filter

hep-ph20142 cited

Third Generation in Cascade Decays

Bhaskar Dutta, Tianjun Li, James A. Maxin +3

In supersymmetric models with gluinos around 1000-2000 GeV, new physics searches based on cascade decay products of the gluino are viable at the next run of the LHC. We investigate…

astro-ph.CO201436 cited

New Constraints on Quantum Gravity from X-ray and Gamma-Ray Observations

Eric S. Perlman, Saul A. Rappaport, Wayne A. Christensen +3

One aspect of the quantum nature of spacetime is its "foaminess" at very small scales. Many models for spacetime foam are defined by the accumulation power , which parameterizes…

astro-ph.GA201415 cited

A comprehensive X-ray and multiwavelength study of the Colliding Galaxy Pair NGC2207/IC2163

S. Mineo, S. Rappaport, A. Levine +3

We present a comprehensive study of the total X-ray emission from the colliding galaxy pair NGC2207/IC2163, based on Chandra, Spitzer, and GALEX data. We detect 28 ultra-luminous X…

astro-ph.GA20141 cited

Stellar masses calibrated with micro-lensed quasars

Paul L. Schechter, Jeffrey A. Blackburne, David Pooley +1

We measure the stellar mass surface densities of early type galaxies by observing the micro-lensing of macro-lensed quasars caused by individual stars, including stellar remnants,…

hep-ph201429 cited

Confronting Electroweak Fine-tuning with No-Scale Supergravity

Tristan Leggett, Tianjun Li, James A. Maxin +2

Applying No-Scale Supergravity boundary conditions at a heavy unification scale to the Flipped grand unified theory with extra TeV-scale vector-like multiplets, No-S…

astro-ph.SR201422 cited

M4 Core Project with HST - III. Search for variable stars in the primary field

V. Nascimbeni, L. R. Bedin, D. C. Heggie +14

We present the results of a photometric search for variable stars in the core of the Galactic globular cluster M4. The input data are a large and unprecedented set of deep Hubble S…