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Edwin E. Salpeter grad student 1964 Cornell (Physics Tree)
 (M.S. Thesis: Back-scattering of a plane wave incident upon a medium at an angle greater than critical.)
Philip Morrison grad student 1966 Cornell (Physics Tree)
 (Ph. D. Thesis: Optical emission from a charged particle slowing down in a plasma.)
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Publications

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Wanders I, Peterson BM, Alloin D, et al. (1997) Steps toward determination of the size and structure of the broad-line region in active galactic nuclei. XI. Intensive monitoring of the ultraviolet spectrum of NGC 7469 Astrophysical Journal, Supplement Series. 113: 69-88
Rodríguez-Pascual PM, Alloin D, Clavel J, et al. (1997) Steps toward determination of the size and structure of the broad-line region in active galactic nuclei. IX. Ultraviolet observations of fairall Astrophysical Journal, Supplement Series. 110: 9-20
Reichert GA, Rodriguez-Pascual PM, Alloin D, et al. (1994) Steps toward determination of the size and structure of the broad-line region in active galactic nuclei. 5: Variability of the ultraviolet continuum and emission lines of NGC 3783 The Astrophysical Journal. 425: 582
Clavel J, Reichert GA, Alloin D, et al. (1991) Steps toward determination of the size and structure of the broad-line region in active galactic nuclei. I. An 8 month campaign of monitoring NGC 5548 with IUE Astrophysical Journal. 366: 64-81
Stoner RE, Ptak R, Ellis D. (1974) The interpretation of broad emission lines in high-redshift QSOS The Astrophysical Journal. 191: 291
Ptak RL, Stoner RE. (1973) The Broad Component of Hα in the Seyfert Galaxy NGC 5548 The Astrophysical Journal. 179
Ptak R, Stoner RE. (1973) A Radially Streaming Proton Model for the Broad Component of Hydrogen Emission in Seyfert Galaxies The Astrophysical Journal. 185: 121-136
Ellis D, Ptak R, Stoner R. (1973) Balmer-line emission from auroral protons The Astrophysical Journal. 182: 637-648
Ptak R, Stoner R. (1973) Origin of Broad Emission Lines from Quasistellar Objects Nature. 243: 280-280
Ptak R. (1970) Balmer Emission Lines In Seyfert Galaxies. The Astrophysical Journal. 162: 425
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