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19992026
most citedStokes imaging, Doppler mapping and Roche tomography of the AM Her system V834 Cen

38 citations · 133 across the 12 of their papers we have counts for

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Showing 2023Show all

6 papers · 1 filter

astro-ph.HE2023

A Multi-wavelength Study of Swift J0503.7-2819: a Chimeric magnetic CV

Kala G. Pradeep, Kulinder Pal Singh, G. C. Dewangan +7

We present multi-wavelength temporal and spectral characteristics of a magnetic cataclysmic variable (MCV) Swift J0503.7-2819, using far ultraviolet (FUV) and X-ray data from Astro…

astro-ph.HE2023

Swift Deep Galactic Plane Survey Classification of Swift J170800402551.8 as a Candidate Intermediate Polar Cataclysmic Variable

B. O'Connor, E. Gogus, J. Hare +24

Here, we present the results of our multi-wavelength campaign aimed at classifying \textit{Swift} J170800402551.8 as part of the \textit{Swift} Deep Galactic Plane Survey (DGPS)…

astro-ph.IM2023★ 12 cited

The RoboPol sample of optical polarimetric standards

D. Blinov, S. Maharana, F. Bouzelou +34

Optical polarimeters are typically calibrated using measurements of stars with known and stable polarization parameters. However, there is a lack of such stars available across the…

astro-ph.HE2023★ 18 cited

X-ray properties of the white dwarf pulsar eRASSU J191213.9-441044

Axel Schwope, T. R. Marsh, Annie Standke +5

We report X-ray observations of the newly discovered pulsating white dwarf eRASSU J191213.9-441044 with Spectrum Roentgen Gamma and eROSITA (SRG/eROSITA) and XMM-Newton. The new so…

astro-ph.HE2023★ 2 cited

Identification of 1RXS J165424.6-433758 as a polar cataclysmic variable

B. O'Connor, J. Brink, D. A. H. Buckley +25

We present the results of our X-ray, ultraviolet, and optical follow-up campaigns of 1RXS J165424.6-433758, an X-ray source detected with the \textit{Swift} Deep Galactic Plane Sur…

astro-ph.IM2023★ 4 cited

Bright-Moon Sky as a Wide-Field Linear Polarimetric Flat Source for Calibration

S. Maharana, S. Kiehlmann, D. Blinov +20

Next-generation wide-field optical polarimeters like the Wide-Area Linear Optical Polarimeters (WALOPs) have a field of view (FoV) of tens of arcminutes. For efficient and accurate…