![]() ![]() ![]() Please declare your traffic by updating your user agent to include company specific information.įor best practices on efficiently downloading information from SEC.gov, including the latest EDGAR filings, visit sec.gov/developer. Your request has been identified as part of a network of automated tools outside of the acceptable policy and will be managed until action is taken to declare your traffic. To allow for equitable access to all users, SEC reserves the right to limit requests originating from undeclared automated tools. ![]() It informs readers on how to achieve the best angular resolution in the visible and near-infrared regimes from diffraction-limited to micro-arcsecond scales.Your Request Originates from an Undeclared Automated Tool This book is intended to enable a next generation of astronomers to apply high-resolution techniques. Written by experts in their fields, the chapters cover adaptive optics, aperture masking imaging, spectra disentangling, interferometry, lucky imaging, Roche tomography, imaging with interferometry, interferometry of AGN, AGN reverberation mapping, Doppler- and magnetic imaging of stellar surfaces, Doppler tomography, eclipse mapping, Stokes imaging, and stellar tomography. As reflected in the book, these techniques can be divided into direct methods, interferometry, and reconstruction methods, and can be applied to a huge variety of astrophysical systems, ranging from planets, single stars and binaries to active galactic nuclei, providing angular resolution in the micro- to tens of milliarcsecond scales. Recent years have seen considerable developments in such techniques, which are critical to advances in many areas of astronomy. This book offers an essential compendium of astronomical high-resolution techniques. ![]()
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