activity
19962005
most citedIdentification of 13 DB + dM and 2 DC + dM binaries from the Sloan Digital Sky Survey

9 citations · 17 across the 15 of their papers we have counts for

collaborators

37 papers

astro-ph20051 cited

Are WC9 Wolf-Rayet stars in colliding-wind binaries?

P. M. Williams, K. A. van der Hucht, G. Rauw

We present results from a spectroscopic search for massive companions to dust-making Galactic WC9 stars as a step to testing the paradigm that dust formation in these systems requi…

astro-ph20059 cited

Identification of 13 DB + dM and 2 DC + dM binaries from the Sloan Digital Sky Survey

E. J. M. van den Besselaar, G. H. A. Roelofs, G. A. Nelemans +2

We present the identification of 13 DB + dM binaries and 2 DC + dM binaries from the Sloan Digital Sky Survey (SDSS). Before the SDSS only 2 DB + dM binaries and 1 DC + dM binary w…

astro-ph20051 cited

Discovering the microJy Radio VLBI Sky via "Full-beam" Self-calibration

M. A. Garrett, J. M. Wrobel, R. Morganti

We demonstrate that at 1.4 GHz the combined response of sources detected serendipitously in deep, wide-field VLBI images is sufficient to permit self-calibration techniques to be e…

astro-ph2004

Probing the polarization characteristics of SS433 on mas scales

Z. Paragi, R. C. Vermeulen, D. C. Homan +5

We present a status report of dedicated circular polarization (CP) global VLBI observations of SS433. The total intensity image of the source is presented. We do not detect linear…

astro-ph2004

A VLBI Study of the Gravitational Lens JVAS B0218+357

R. Mittal, R. Porcas, O. Wucknitz +1

We present the results of phase-referenced VLBA+Effelsberg observations at five frequencies of the gravitational lens B0218+357 to establish the precise registration of the A and B…

astro-ph2004

Spitzer 24 micron imaging of Faint Radio Sources in the FLSv: a new radio-loud, Mid-IR/optically obscured population?

M. Orienti, M. A. Garrett, C. Reynolds +1

Data from the Spitzer Space Telescope (the First Look Survey - FLS) have recently been made public. We have compared the 24 micron images with very deep WSRT 1.4 GHz observations (…