By T.R. Marsh (auth.), Henri M.J. Boffin, Jan Cuypers, Danny Steeghs (eds.)
This finished and particular reference paintings on astro-tomography is predicated on accelerated and definitely edited contributions to the first foreign Workshop on Astro-tomography. the point of interest is on learning oblique imaging and next reconstruction innovations with functions in all parts of observational astronomy, astrophysics and cosmology. specific topic and item indexes, including an inventory of valuable assets on the net, might help the reader to take advantage of this booklet in a most productive way.
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Additional resources for Astrotomography: Indirect Imaging Methods in Observational Astronomy
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14) The third line above follows from the second after transforming from polar coordinates s and φ to cartesian sx = s cos 2πφ and sy = s sin 2πφ, and using Eqs. 13 so that 1 0 ∞ 0 se−i2πs(VR −VR ) ds dφ = ∞ ∞ −∞ −∞ e−i2π[−(Vx −Vx )sx +(Vy −Vy )sy ] dsx dsy and then the integrals over sx and sy separate to give the two Dirac δ-functions of the penultimate line of Eq. 14 since δ(x) = ∞ −∞ e±i2πsx ds. 2. 24 Tom Marsh Appendix B Table 2. Doppler maps of CVs and X-ray novae published in refereed journals as of September 2000.
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Astrotomography: Indirect Imaging Methods in Observational Astronomy by T.R. Marsh (auth.), Henri M.J. Boffin, Jan Cuypers, Danny Steeghs (eds.)