activity
19952009
most citedThe multiple quasar Q2237+0305 under a microlensing caustic

107 citations · 446 across the 18 of their papers we have counts for

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Showing 2004Show all

8 papers · 1 filter

astro-ph2004

Limits on the Transverse Velocity of the Lensing Galaxy in Q2237+0305 from the Lack of Strong Microlensing Variability

Rodrigo Gil-Merino, Joachim Wambsganss, Luis J. Goicoechea +1

We present a method for the determination of upper limits on the transverse velocity of the lensing galaxy in the quadruple quasar system Q2237+0305, based on the lack of strong mi…

astro-ph2004

Size is Everything: Universal Features of Quasar Microlensing with Extended Sources

Michael J. Mortonson, Paul L. Schechter, Joachim Wambsganss

We examine the effect that the shape of the source brightness profile has on the magnitude fluctuations of images in quasar lens systems due to microlensing. We do this by convolvi…

astro-ph2004

Lensing Survey of the Most X-Ray Luminous Galaxy Clusters

W. Kausch, S. Schindler, T. Kronberger +4

We present the first three galaxy clusters of a larger sample of the most X-ray luminous galaxy clusters selected from the ROSAT Bright Survey. This project, which is a systematic…

astro-ph2004

Potential Direct Single-Star Mass Measurement

H. Ghosh

We analyze the lightcurve of the microlensing event OGLE-2003-BLG-175/MOA-2003-BLG-45 and show that it has two properties that, when combined with future high resolution astrometry…

astro-ph2004

Gravitational lensing in a concordance LCDM universe: The importance of secondary matter along the line of sight

Joachim Wambsganss, Paul Bode, Jeremiah P. Ostriker

To date, in almost all strong gravitational lensing analyses for modeling giant arc systems and multiple quasar images, it has been assumed that all the deflecting matter is concen…

astro-ph2004

OGLE-2003-BLG-238: Microlensing Mass Estimate of an Isolated Star

Guangfei Jiang, D. L. DePoy, A. Gal-Yam +38

Microlensing is the only known direct method to measure the masses of stars that lack visible companions. In terms of microlensing observables, the mass is given by M=(c^2/4G)\tild…