Jelle Sjerp Kaastra

2014- Leiden University, Leiden, Netherlands 
Hig-energy astrophysics
"Jelle Sjerp Kaastra"


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Joannes Maria Elisabeth Kuijpers grad student 1985 Utrecht
Max Kuperus grad student 1985 Utrecht
 (Solar Flares: An Electrodynamic Model.)
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Behar E, Kaspi S, Paubert G, et al. (2020) Simultaneous Millimetre-wave and X-ray monitoring of the Seyfert galaxy NGC 7469 Monthly Notices of the Royal Astronomical Society. 491: 3523-3534
Marco BD, Adhikari TP, Ponti G, et al. (2020) Incoherent fast variability of X-ray obscurers. The case of NGC 3783 Astronomy and Astrophysics. 634
Ahoranta J, Nevalainen J, Wijers N, et al. (2020) Hot WHIM counterparts of FUV O VI absorbers: Evidence in the line-of-sight towards quasar 3C 273 Astronomy & Astrophysics. 634: A106
Grafton-Waters S, Branduardi-Raymont G, Mehdipour M, et al. (2020) Multi-wavelength campaign on NGC 7469 VI. photoionisation modelling of the emission line regions and the warm absorber Astronomy and Astrophysics. 633
Mernier F, Werner N, Lakhchaura K, et al. (2020) How do atomic code uncertainties affect abundance measurements in the intracluster medium Astronomische Nachrichten. 341: 203-209
Kammoun ES, Nardini E, Zoghbi A, et al. (2019) The Nature of the Broadband X-Ray Variability in the Dwarf Seyfert Galaxy NGC 4395 The Astrophysical Journal. 886: 145
Trueba N, Miller JM, Kaastra J, et al. (2019) A Comprehensive Chandra Study of the Disk Wind in the Black Hole Candidate 4U 1630-472 The Astrophysical Journal. 886: 104
Kriss GA, De Rosa G, Ely J, et al. (2019) Space Telescope and Optical Reverberation Mapping Project. VIII. Time Variability of Emission and Absorption in NGC 5548 Based on Modeling the Ultraviolet Spectrum The Astrophysical Journal. 881: 153
Kammoun ES, Miller JM, Zoghbi A, et al. (2019) A Hard Look at NGC 5347: Revealing a Nearby Compton-thick AGN The Astrophysical Journal. 877: 102
Edelson R, Gelbord J, Cackett E, et al. (2019) The First Swift Intensive AGN Accretion Disk Reverberation Mapping Survey The Astrophysical Journal. 870: 123
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