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Cited article:

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Novae in M51: a new, much higher rate from multi-epoch HST data

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When does an old nova become a dwarf nova? Kinematics and age of the nova shell of the dwarf nova AT Cancri

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OGLE ATLAS OF CLASSICAL NOVAE. II. MAGELLANIC CLOUDS

P. Mróz, A. Udalski, R. Poleski, I. Soszyński, M. K. Szymański, G. Pietrzyński, Ł. Wyrzykowski, K. Ulaczyk, S. Kozłowski, P. Pietrukowicz and J. Skowron
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A HUBBLE SPACE TELESCOPE SURVEY FOR NOVAE IN M87. I. LIGHT AND COLOR CURVES, SPATIAL DISTRIBUTIONS, AND THE NOVA RATE*

Michael M. Shara, Trisha F. Doyle, Tod R. Lauer, David Zurek, J. D. Neill, Juan P. Madrid, Joanna Mikołajewska, D. L. Welch and Edward A. Baltz
The Astrophysical Journal Supplement Series 227 (1) 1 (2016)
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A tidal flare candidate in Abell 1795★†‡

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Discovery of 13 Nova Candidates in M87

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On the evolution of the Fe abundance and of the Type Ia supernova rate in clusters of galaxies

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Monthly Notices of the Royal Astronomical Society: Letters 378 (1) L11 (2007)
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Cosmic Supernova Rates and the Hubble Sequence

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Astrophysics in 2003

Virginia Trimble and Markus J. Aschwanden
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Hubble Space TelescopeObservations of Novae in M49

Laura Ferrarese, Patrick Cote and Andres Jordan
The Astrophysical Journal 599 (2) 1302 (2003)
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