Refereed Publications
1)T.G. Slanger, E. O'Neill, B.D. Sharpee, P.C. Cosby,
``Ground-based Measurements of the I(777.4 nm)/I(844.6 nm) Intensity
Ratio in the Nightglow; Evidence for Bowen Fluorescence of the 844.6
nm transition'', in preparation (2006).
2)T.G. Slanger, P.C. Cosby, B.D. Sharpee, K.R. Minschwaner,
D.E. Siskind, ``The
O(1S→1D,3P)
Branching Ratio'', J. Geophys. Res., in press (2006).
3) P.C. Cosby, B.D. Sharpee, T.G. Slanger, D.L. Huestis,
R. Hanuschik, ``High-Resolution Terrestrial Nightglow Emission Line
Atlas from UVES/VLT: Positions, Intensities, and Assignments for 2808
Lines at 314-1043 nm'', J. Geophys. Res., in press (2006).
4) B. Sharpee, Y. Zhang, R. Williams, E. Pellegrini, K. Cavagnolo,
J.A. Baldwin, M. Phillips, and X.-W. Liu, ``s-Process
Abundances in Planetary Nebulae", Astrophys. J. Supp., submitted
(2006).
5) T.G. Slanger, P.C. Cosby, D.L. Huestis, B.D. Sharpee, ``Review of
Tropical Nightglow Studies with Astronomical Instruments'',
J. Atmos. Solar Terr. Phys., 68, 1426 (2006).
6) B.D. Sharpee, T.G. Slanger, ``The
O(1D2 -3P2,1,0)
630.0, 636.4, and 639.2 nm Forbidden Emission Line Intensity Ratios
Measured in the Terrestrial Nightglow'', J. Phys. Chem. A,
110, 6707, doi:10.1021/jp056163x (2006).
7) B.D. Sharpee, T.G. Slanger, P.C. Cosby, D.L. Huestis, ``The
N(2Do-4So)
Forbidden Doublet in the Nightglow: An Experimental Test of the
Theoretical Intensity Ratio'', Geophys. Res. Lett., 32,
L12106, doi:10.1029/2005GL023044 (2005).
8) B. Sharpee, J. Baldwin, R. Williams, ``Identification and
Characterization of Faint Emission Lines in the Spectrum of the
Planetary Nebula IC 418'', Astrophys. J., 615, 323
(2004). preprint
9) B.D. Sharpee, T.G. Slanger, D.L. Huestis, P.C. Cosby,
``Measurements of the Singly Ionized Oxygen Auroral Doublet Lines
λλ 7320,7330 Using High Resolution Sky Spectra'',
Astrophys. J., 606, 605 (2004). preprint
10) A. LaCluyze, H.A. Smith, E.-M. Gill, A. Hedden, K. Kinemuchi,
A.M. Rosas, B.J. Pritzl, B. Sharpee, C. Wilkinson, K.W. Robinson,
M.E. Baldwin, G. Samolyk, ``The Changing Blazhko Effect of XZ Cygni'',
Astron. J., 127, 1653 (2004). preprint
11) B. Sharpee, R. Williams, J. Baldwin, P.A.M. van Hoof, ``Introducing
EMILI: Computer Aided Emission Line Identification'',
Astrophys. J. Supp., 149, 157 (2003). preprint
12) R. Williams, E.B. Jenkins, J.A. Baldwin, B. Sharpee, ``Comparative
Abundances From Absorption and Emission Analyses of IC 418'',
Pub. Astron. Soc. Pacific, 115, 178 (2003). preprint
13) B. Sharpee, M. Stark, B. Pritzl, N. Silberman, R. Wilhelm,
H.A. Smith, A. Walker, ``B,V Photometry of Variable Stars in the
Northeast Arm of the Small Magellanic Cloud'', Astron. J.,
123, 3216 (2002). preprint
Conference Proceedings
1) B.D. Sharpee, T.G. Slanger, D.L. Huestis, P.C. Cosby, "Studying
Atomic Physics Using the Nighttime Atmosphere as a Laboratory",
Proceedings of the NASA Laboratory Astrophysics Workshop, February
14-16, 2006, UNLV, Las Vegas, ed. P.F. Week, V.H.S. Kwong, and F. Salama, 264 (2006).
2) J.R. Walsh, D. Pequignot, B. Sharpee, J. Baldwin, C. Morisset,
P.J. Storey, P. van Hoof, R.E. Williams, ``A Deep Blue-UV Planetary
Nebulae Template Spectrum from NGC 7027'', IAU Symp. 209, Planetary
Nebulae: Their Evolution and Role in the Universe, ed. S. Kwok,
M. Dopita, & R. Sutherland (San Francisco: ASP), 337 (2003).
3) B. Sharpee, R.E. Williams, J. Baldwin, P.A.M. van Hoof, ``EMILI -
An Aid to Emission Line Identification in Emission-Line Regions'',
Proceedings of the NASA Laboratory Astrophysics Workshop,
ed. F. Salama, 85 (2002).
4) H.A. Smith, A. LaCluyze, E.-M. Gill, A. Hedden, K. Kinemuchi,
A.M. Rosas, B.J. Pritzl, B. Sharpee, K. Robinson, M. Baldwin,
G. Samolyk, ``The Changing Blazhko Effect of XZ Cygni'', ASP
Conference Proceedings, Vol. 259, Radial and Nonradial Pulsations as
Probes of Stellar Physics, ed. C. Aerts, T.R. Bedding, &
J. Christensen-Dalsgaard. ISBN: 1-58381-099-4 (2002). Also IAU
Colloquium 185. (San Francisco: ASP), 64 (2002).