Zobrazeno 1 - 10
of 112
pro vyhledávání: '"Lane, Benjamin F."'
Autor:
Brown, Julian A., Spector, Steven J., Moebius, Michael, Benney, Lucas, Vresilovic, Daniel, Dolle, Brian, Greenbaum, Alexandra Z., Huang, Alex, Poulton, Christopher V., Watts, Michael R., Dawson, Robin, Lane, Benjamin F., Laine, J. P., Cahoy, Kerri, Clevenson, Hannah A.
Compressive sensing has been used to demonstrate scene reconstruction and source localization in a wide variety of devices. To date, optical compressive sensors have not been able to achieve significant volume reduction relative to conventional optic
Externí odkaz:
http://arxiv.org/abs/2107.09456
Autor:
Muterspaugh, Matthew W., Wijngaarden, M. J. P., Henrichs, H. F., Lane, Benjamin F., Hartkopf, William I., Henry, Gregory W.
The dwarf stars in the 26 year period binary alpha Com were predicted to eclipse each other in early 2015. That prediction was based on an orbit model made with over 600 astrometric observations using micrometers, speckle interferometry, and long bas
Externí odkaz:
http://arxiv.org/abs/1501.05639
Publikováno v:
High-precision infra-red stellar interferometry [electronic thesis]
Thesis (Ph. D.). PQ #3081246.
Includes bibliographical references.
Includes bibliographical references.
Externí odkaz:
http://resolver.caltech.edu/CaltechETD:etd-03122003-112232
Autor:
Lane, Benjamin F.
Thesis (Ph.D.)-- California Institute of Technology.
1.6 megabytes, 167 pages in Adobe pdf format. Also privately published by the author in paperback format. Includes bibliographical references (leaves 141-151).
1.6 megabytes, 167 pages in Adobe pdf format. Also privately published by the author in paperback format. Includes bibliographical references (leaves 141-151).
Autor:
Rajabi, Samira, Muterspaugh, Matthew W., Lane, Benjamin F., Sirk, Martin M., Browne, Stanley, Ghasempour, Askari, Halverson, Samuel P., Kelly, John G., Williamson, Michael
We used the Palomar Testbed Interferometer (PTI) to resolve 2.2 $\mu$m emission from the classical nova V458 Vul 2007 over the course of several days following its discovery on 2007 August 8.54 UT. We also obtained K-band photometric data and spectra
Externí odkaz:
http://arxiv.org/abs/1206.5172
The non-orthogonality of algebraic polynomials of field coordinates traditionally used to model field-dependent corrections to astrometric measurements, gives rise to subtle adverse effects. In particular, certain field dependent perturbations in the
Externí odkaz:
http://arxiv.org/abs/1110.2967
Autor:
Muterspaugh, Matthew W., Fekel, Francis C., Lane, Benjamin F., Hartkopf, William I., Kulkarni, S. R., Konacki, Maciej, Burke, Bernard F., Colavita, M. M., Shao, M., Williamson, M.
(Abridged) Differential astrometry measurements from the Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) are used to constrain the astrometric orbit of the previously known lesssim 2 day subsystem in the triple system 63 Gem
Externí odkaz:
http://arxiv.org/abs/1010.4045
Autor:
Muterspaugh, Matthew W., Lane, Benjamin F., Kulkarni, S. R., Konacki, Maciej, Burke, Bernard F., Colavita, M. M., Shao, M., Hartkopf, William I., Boss, Alan P., Williamson, M.
The Palomar High-precision Astrometric Search for Exoplanet Systems monitored 51 subarcsecond binary systems to evaluate whether tertiary companions as small as Jovian planets orbited either the primary or secondary stars, perturbing their otherwise
Externí odkaz:
http://arxiv.org/abs/1010.4048
Autor:
Muterspaugh, Matthew W., Lane, Benjamin F., Kulkarni, S. R., Konacki, Maciej, Burke, Bernard F., Colavita, M. M., Shao, M.
The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) monitored 51 subarcsecond binary systems to evaluate whether tertiary companions as small as Jovian planets orbited either the primary or secondary stars, perturbing their o
Externí odkaz:
http://arxiv.org/abs/1010.4044
Autor:
Muterspaugh, Matthew W., Hartkopf, William I., Lane, Benjamin F., O'Connell, J., Williamson, M., Kulkarni, S. R., Konacki, Maciej, Burke, Bernard F., Colavita, M. M., Shao, M., Wiktorowicz, Sloane J.
Differential astrometry measurements from the Palomar High-precision Astrometric Search for Exoplanet Systems have been combined with lower precision single-aperture measurements covering a much longer timespan (from eyepiece measurements, speckle in
Externí odkaz:
http://arxiv.org/abs/1010.4043