activity
19972010
most citedStar formation and UV colors of the brightest Cluster Galaxies in the representative XMM-Newton Cluster Structure Survey

70 citations · 260 across the 9 of their papers we have counts for

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7 papers · 1 filter

astro-ph2008★ 1 cited

The Central Component of Gravitational Lens Q0957+561

Deborah B. Haarsma, Joshua N. Winn, Irwin Shapiro +1

In 1981, a faint radio source (G') was detected near the center of the lensing galaxy of the famous "twin quasar" Q0957+561. It is still unknown whether this central radio source i…

astro-ph2005★ 11 cited

The FIRST-Optical-VLA Survey for Lensed Radio Lobes

D. B. Haarsma, J. N. Winn, E. E. Falco +7

We present results from a survey for gravitationally lensed radio lobes. Lensed lobes are a potentially richer source of information about galaxy mass distributions than lensed poi…

astro-ph2000★ 48 cited

Further Investigation of the Time Delay, Magnification Ratios, and Variability in the Gravitational Lens 0218+357

A. S. Cohen, J. N. Hewitt, C. B. Moore +1

High precision VLA flux density measurements for the lensed images of 0218+357 yield a time delay of 10.1(+1.5-1.6)days (95% confidence). This is consistent with independent measur…

astro-ph2000

New VLBI Constraints for 0957+561 Lens Models

Deborah Haarsma, Joseph Leh'ar, Rennan Barkana

Time-delay measurements of 0957+561 based on radio monitoring now agree with optical monitoring. Recent models incorporate many recent observations, but the systematic uncertaintie…

astro-ph1998★ 46 cited

The Radio Wavelength Time Delay of Gravitational Lens 0957+561

Deborah B. Haarsma, Jacqueline N. Hewitt, Joseph Lehár +1

The gravitational lens 0957+561 was monitored with the Very Large Array from 1979 to 1997. The 6 cm light curve data from 1995-1997 and the 4 cm data from 1990-1997 are reported he…

astro-ph1998★ 27 cited

Radio Wavelength Constraints on the Sources of the Far Infrared Background

D. B. Haarsma, R. B. Partridge

The cosmic far infrared background detected recently by the COBE-DIRBE team is presumably due, in large part, to the far infrared (FIR) emission from all galaxies. We take the well…