activity
19982023
most citedOptical Continuum and Emission-Line Variability of Seyfert 1 Galaxies

282 citations · 942 across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.SR2023★ 8 cited

V445 Puppis -- Dustier than a Thousand Novae

D. P. K. Banerjee, A. Evans, C. E. Woodward +4

V445 Puppis, the only known Galactic helium nova, is a unique test-bed to verify supernova (SN) theories in the single degenerate channel that involve a white dwarf (WD) accreting…

astro-ph.SR2022★ 3 cited

The recurrent nova V3890~Sgr: a near-infrared and optical study of the red giant component and its environment

B. Kaminsky, A. Evans, Ya. V. Pavlenko +8

We present an analysis of the red giant component of the recurrent nova V3890 Sgr, using data obtained before and after its 2019 eruption. Its effective temperature is $T_{\rm eff}…

astro-ph.HE2022

V392 Persei: a γ-ray bright nova eruption from a known dwarf nova

F. J. Murphy-Glaysher, M. J. Darnley, É. J. Harvey +57

V392 Persei is a known dwarf nova (DN) that underwent a classical nova eruption in 2018. Here we report ground-based optical, Swift UV and X-ray, and Fermi-LAT γ-ray observations f…

astro-ph.SR2021★ 2 cited

SOFIA/FORCAST Monitoring of the Dust Emission from R Aqr: Start of the Eclipse

Ravi Sankrit, Eric Omelian, Uma Gorti +3

We present mid-infrared spectra from our continued monitoring of R Aquarii, the nearest symbiotic Mira, using the Stratospheric Observatory for Infrared Astronomy (SOFIA). New phot…

astro-ph.SR2021★ 22 cited

Near-infrared studies of nova V1674 Herculis: A shocking record-breaker

C. E. Woodward, D. P. K. Banerjee, T. R. Geballe +3

We present near infrared spectroscopy of Nova Herculis 2021 (V1674 Her), obtained over the first 70 days of its evolution. This fastest nova on record displays a rich emission line…

astro-ph.SR2021

Spectroscopy of the Proposed White Dwarf Pulsar ASASSN-V J205543.90+240033.5

R. Mark Wagner, Peter Garnavich, John R. Thorstensen +2

We obtained spectra of ASASSN-V J205543.90+240033.5 (J2055), a system that shows photometric variations similar to the white dwarf (WD) pulsar AR Scorpii (Kato et al. arXiv:2109.03…