Proceedings of SPIE

By Zhen Tan. 2017

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Density profiles of galaxy groups and clusters from SDSS galaxy–galaxy weak lensing (2006, background): “…including the fundamental plane relating luminosity, radius, and central velocity dispersion (Faber 1973; Visvanathan & Sandage 1977; Djorgovski & Davis 1987; Kormendy & Djorgovski 1989; Bower et al. 1992; Roberts & Haynes 1994; Bernardi et al. 2003) of which the Faber-Jackson relation (Faber &…”
Weak Gravitational Lensing with COSMOS: Galaxy Selection and Shape Measurements (2007, neutral): “Given accurate deblending and a high number density of galaxies, one can expect to measure shear statistically on subarcminute scales, where baryonic physics may begin to influence the dark matter distribution.”
The WFCAM Science Archive (2006, background): “For example, the UKIDSS LAS Source prescription is for visits in YJHK with a second epoch in J. Modern imaging surveys, however, increasingly aspire to extensive sampling of the time domain (e.g. Pan–STARRS, Kaiser 2004; GAIA, Perryman 2005; LSST, Claver 2004), and we note that both WFCAM and VISTA ”
The ExoMol database: Molecular line lists for exoplanet and other hot atmospheres (2016, background): “Molecule Broadener Reference Methodology H2O H2 Lavrentieva et al [177] Semi-empirical Lavrentieva et al [178] Semi-empirical Steyert et al [179] Experimental Brown & Plymate [180] Experimental Brown et al [181] Experimental Gamache et al [182] Theoretical Dick et al [183] Experimental Faure et al [”
THE GREATER IMPACT OF MERGERS ON THE GROWTH OF MASSIVE GALAXIES: IMPLICATIONS FOR MASS ASSEMBLY AND EVOLUTION SINCE z ≃ 1 (2009, methodology): “This project combines publicly available data in GOODS-S with new observations obtained in GOODS-N with the recentlycommissioned Multi-Object Infrared Camera and Spectrograph (MOIRCS, Ichikawa et al. 2006) panoramic infrared imager on the Subaru 8.2m telescope.”
Circuit elements at optical frequencies: nanoinductors, nanocapacitors, and nanoresistors. (2004, background): “effective “inductance”, as discussed in [4-6].”