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M. R. Goad

5 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author3
  • last author1

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph5
ORCID 0000-0002-2908-7360

identity via Semantic Scholar / OpenAlex

most citedThe Intrinsic Fraction of Broad Absorption Line Quasars

195 citations · 406 across the 5 of their papers we have counts for

collaborators

4 papers

astro-ph2008★ 28 cited

An anti-correlation between X-ray luminosity and H-alpha equivalent width in X-ray binaries

R. P. Fender, D. M. Russell, C. Knigge +3

We report an anticorrelation between continuum luminosity and the equivalent width (EW) of the H-alpha emission line in X-ray binary systems. The effect is evident both in a univer…

astro-ph2008★ 195 cited

The Intrinsic Fraction of Broad Absorption Line Quasars

Christian Knigge, Simone Scaringi, Michael R. Goad +1

We carefully reconsider the problem of classifying broad absorption line quasars (BALQSOs) and derive a new, unbiased estimate of the intrinsic BALQSO fraction from the SDSS DR3 QS…

astro-ph2008★ 2 cited

The Swift X-Ray Telescope: Status and Performance

David N. Burrows, J. A. Kennea, A. F. Abbey +23

We present science highlights and performance from the Swift X-ray Telescope (XRT), which was launched on November 20, 2004. The XRT covers the 0.2-10 keV band, and spends most of…

astro-ph2007★ 75 cited

The SSS phase of RS Ophiuchi observed with Chandra and XMM-Newton I.: Data and preliminary Modeling

J. -U. Ness, S. Starrfield, A. P. Beardmore +13

The phase of Super-Soft-Source (SSS) emission of the sixth recorded outburst of the recurrent nova RS Oph was observed twice with Chandra and once with XMM-Newton. The observations…

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