activity
19992017
most citedThe XMM-Newton serendipitous ultraviolet source survey catalogue

123 citations · 368 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2017★ 27 cited

Morphological properties of the Crab Nebula: a detailed multiwavelength study based on new VLA, HST, Chandra and XMM-Newton images

G. Dubner, G. Castelletti, O. Kargaltsev +3

We present a detailed analysis of the morphological properties of the Crab Nebula across the electromagnetic spectrum based on new and previous high-quality data from radio to X-ra…

astro-ph.IM2016★ 6 cited

The calibration of read-out-streak photometry in the XMM-Newton Optical Monitor and the construction of a bright-source catalogue

M. J. Page, N. Chan, A. A. Breeveld +7

The dynamic range of the XMM-Newton Optical Monitor (XMM-OM) is limited at the bright end by coincidence loss, the superposition of multiple photons in the individual frames record…

astro-ph.GA2015★ 5 cited

The peculiar optical-UV X-ray spectra of the X-ray weak quasar PG 0043+039

W. Kollatschny, N. Schartel, M. Zetzl +4

The object PG 0043+039 has been identified as a broad absorption line (BAL) quasar based on its UV spectra. However, this optical luminous quasar has not been detected before in de…

astro-ph.GA2014★ 11 cited

The XMM Deep Survey in the CDF-S VII. UV catalogue of the Optical Monitor observations

M. Antonucci, A. Talavera, F. Vagnetti +5

The XMM-Newton X-ray observatory has repeatedly observed the CDFS in 33 epochs (2001-2010) through the XMM-CDFS Deep Survey. During the X-ray observations, XMM-OM targeted the cent…

astro-ph.SR2013★ 36 cited

Discovery of the magnetic field in the pulsating B star beta Cephei

H. F. Henrichs, J. A. de Jong, E. Verdugo +17

Although the star itself is not He enriched, the periodicity and the variability in the UV wind lines of the pulsating B1 IV star beta Cep are similar to what is observed in magnet…

astro-ph.SR2013★ 26 cited

XMM-Newton monitoring of the close pre-main-sequence binary AK Sco. Evidence of tide driven filling of the inner gap in the circumbinary disk

Ana I. Gomez de Castro, Javier Lopez-Santiago, Antonio Talavera +2

AK~Sco stands out among pre-main sequence binaries because of its prominent ultraviolet excess, the high eccentricity of its orbit and the strong tides driven by it. AK Sco consist…