M Haji, A Kelly, L Hou, A Bryce… - … on Lasers and …, 2011 - opticsinfobase.org Mode-locked laser diodes (MLLDs) are excellent candidates for generating ultrashort high frequency pulses for a number of applications, including optical clocking, sampling, and clock recovery. Although more prone to noise than active MLLDs, passive MLLDs do not require any ... Related articles
D Arnold, K Amano, T Takeda… - The 33rd Australasian …, 2011 - espace.library.uq.edu.au Moving borders defined by small luminance changes (or colour) can appear to jitter at a characteristic frequency when they are placed in close proximity to moving borders defined by large luminance changes (Arnold & Johnston, 2003). Using psychophysical techniques, we have now ... Cached - All 4 versions
MJ Payne… - The Astrophysical Journal, 2011 - iopscience.iop.org If the two planets in the HAT-P-13 system are coplanar, the orbital states provide a probe of the internal planetary structure. Previous analyses of radial velocity and transit timing data for the system suggested that the observational constraints on the orbital states were rather ... Cited by 3 - Related articles - All 6 versions
VJ Wittwer, CA Zaugg, WP Pallmann… - … on Lasers and …, 2011 - opticsinfobase.org Semiconductor disk lasers (also called VECSELs, vertical external cavity surface emitting lasers) combine the benefits of diode-pumped solid-state lasers (DPSSLs) and semiconductor technologies, resulting in wavelength flexibility and high power operation with excellent ... Related articles
[PDF] from arxiv.orgJD Hartman, GÁ Bakos, G Torres… - Arxiv preprint arXiv: …, 2011 - arxiv.org ABSTRACT We report the discovery of two exoplanets transiting high-jitter stars. HAT-P-32b orbits the bright V=11.289 late-F–early-G dwarf star GSC 3281-00800, with a period P = 2.150008 ± 0.000001d. The stellar and planetary masses and radii depend on the eccentricity of the ... Related articles - All 2 versions
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