Peter Gustaaf Jonker

Affiliations: 
2001 University of Amsterdam, Amsterdam, Netherlands 
 2009- Radboud University Nijmegen, Nijmegen, Gelderland, Netherlands 
Website:
https://personal.sron.nl/~peterj/home.html
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"Peter Gustaaf Jonker"
Bio:

https://www.astro.ru.nl/wiki/nl/general/people/peter_jonker
P.G. Jonker at the Album Academicum of the University of Amsterdam

Parents

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Michiel B.M. van der Klis grad student 2001 Amsterdam
 (Probing low-mass X-ray binaries with X-ray timing.)
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Publications

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Poutanen J, Veledina A, Berdyugin AV, et al. (2022) Black hole spin-orbit misalignment in the x-ray binary MAXI J1820+070. Science (New York, N.Y.). 375: 874-876
Miller-Jones JCA, Tetarenko AJ, Sivakoff GR, et al. (2019) A rapidly changing jet orientation in the stellar-mass black-hole system V404 Cygni. Nature
Clementini G, Eyer L, Ripepi V, et al. (2017) Gaia Data Release 1. Testing parallaxes with local Cepheids and RR Lyrae stars Astronomy and Astrophysics. 605: 1-29
Marsh TR, Gänsicke BT, Hümmerich S, et al. (2016) A radio-pulsing white dwarf binary star. Nature
Broderick JW, Fender RP, Breton RP, et al. (2016) Low-radio-frequency eclipses of the redback pulsar J2215+5135 observed in the image plane with LOFAR. Monthly Notices of the Royal Astronomical Society. 459: 2681-2689
Feroci M, Bozzo E, Brandt S, et al. (2016) The LOFT mission concept: a status update Proceedings of Spie. 9905: 1-20
Pilia M, Hessels JWT, Stappers BW, et al. (2016) Wide-band, low-frequency pulse profiles of 100 radio pulsars with LOFAR Astronomy and Astrophysics. 586
van Velzen S, Anderson GE, Stone NC, et al. (2015) A radio jet from the optical and X-ray bright stellar tidal disruption flare ASASSN-14li. Science (New York, N.Y.)
Feroci M, Stella L, van der Klis M, et al. (2012) The Large Observatory for X-ray Timing (LOFT) Experimental Astronomy. 34: 415-444
Jonker PG, Torres MAP, Fabian AC, et al. (2010) A bright off-nuclear X-ray source: A type IIn supernova, a bright ULX or a recoiling supermassive black hole in CXO J122518.6+144545 Monthly Notices of the Royal Astronomical Society. 407: 645-650
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