M. P. Rupen

Herzberg Institute of Astrophysics — Canada

Physics and Astronomy · Physical Sciences

52h-index8.8kcitations370works2.02yr avg
OpenAlex↗Google Scholar↗Lab page↗

Accepting Students?

No reports yet. Know if this professor is taking students?

Research Topics

Astrophysical Phenomena and Observations(182), Gamma-ray bursts and supernovae(159), Pulsars and Gravitational Waves Research(117), Astrophysics and Cosmic Phenomena(104), Astronomy and Astrophysical Research(44)

Publications370 total

The Symbiotic Recurrent Nova V745 Sco at Radio Wavelengths
arXiv (Cornell University)·2024Open Access
The symbiotic recurrent nova V745 Sco at radio wavelengths
Monthly Notices of the Royal Astronomical Society·2024· 4 citedOpen Access
TESS photometry of the nova eruption in V606 Vul: asymmetric photosphere and multiple ejections?
arXiv (Cornell University)·2023Open Access
First Detection of Radio Emission Associated with a Classical Cepheid
The Astronomical Journal·2023· 3 citedOpen Access
Short time-scale evolution of the polarized radio jet during V404 Cygni’s 2015 outburst
Monthly Notices of the Royal Astronomical Society·2023· 3 citedOpen Access
Short Timescale Evolution of the Polarized Radio Jet during V404 Cygni's 2015 Outburst
arXiv (Cornell University)·2023Open Access
The first nova eruption in a novalike variable: YZ Ret as seen in X-rays and <i>γ</i>-rays
Monthly Notices of the Royal Astronomical Society·2022· 24 citedOpen Access
Classical Novae at Radio Wavelengths
The Astrophysical Journal Supplement Series·2021· 29 citedOpen Access
The first nova eruption in a novalike variable: YZ Ret as seen in X-rays and gamma-rays
arXiv (Cornell University)·2021· 2 citedOpen Access
Classical Novae at Radio Wavelengths
Maryland Shared Open Access Repository (USMAI Consortium)·2021Open Access
An end-to-end model for the correlator and beamformer of the Square Kilometer Array Mid Telescope
2020· 2 cited
Strong J-band variability but no radio or X-ray emission from Nova PGIR20eig
The astronomer's telegram·2020
Erratum: “A Detailed Observational Analysis of V1324 Sco, the Most Gamma-Ray-luminous Classical Nova to Date” (2018, ApJ, 852, 108)
The Astrophysical Journal·2020Open Access
X-ray evolution of the nova V959 Mon suggests a delayed ejection and a non-radiative shock
Monthly Notices of the Royal Astronomical Society·2020· 5 citedOpen Access
Rapid compact jet quenching in the Galactic black hole candidate X-ray binary MAXI J1535−571
Monthly Notices of the Royal Astronomical Society·2020· 45 citedOpen Access
X-ray spectroscopy of the γ-ray brightest nova V906 Car (ASASSN-18fv)
Monthly Notices of the Royal Astronomical Society·2020· 25 citedOpen Access
NuSTAR detection of Nova Reticuli 2020 = MGAB-V207
The astronomer's telegram·2020· 1 cited
Radio Emission from delta Cephei: Evidence of Mass Loss Via an Ionized Wind?
American Astronomical Society Meeting Abstracts·2020
Regulation of accretion by its outflow in a symbiotic star: the 2016 outflow fast state of MWC 560
Monthly Notices of the Royal Astronomical Society·2019· 26 citedOpen Access
A Search for Late-time Radio Emission and Fast Radio Bursts from Superluminous Supernovae
The Astrophysical Journal·2019· 39 citedOpen Access
page 1 of 19Next →

Frequent Co-authors

R. P. Fender(10), J. Homan(7), J. C. A. Miller‐Jones(7), R. Wijnands(5), M. van der Klis(5), A. J. Mioduszewski(5), R. M. Hjellming(4), M. F. Bietenholz(4), J. M. Mïller(4), D. Steeghs(4), P. G. Jonker(4), V. Dhawan(4), Elena Gallo(4), Ronald A. Remillard(4), Elmar Körding(4), J. L. Sokoloski(4), G. R. Knapp(4), N. Bartel(4), Casey Law(3), Sarah Burke-Spolaor(3)