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[1109.4769] GYOTO: a new general relativistic ray-tracing …
https://arxiv.org/abs/1109.4769
GYOTO, a general relativistic ray-tracing code, is presented. It aims at computing images of astronomical bodies in the vicinity of compact objects, as well as trajectories of massive bodies in relativistic environments. This code is capable of integrating the null and timelike geodesic equations not only in the Kerr metric, but also in any metric computed …
GYOTO: a new general relativistic ray-tracing code
https://iopscience.iop.org/article/10.1088/0264-9381/28/22/225011
GYOTO, a general relativistic ray-tracing code, is presented. It aims at computing images of astronomical bodies in the vicinity of compact objects, as well as trajectories of massive bodies in relativistic environments. This code is capable of integrating the null and timelike geodesic equations not only in the Kerr metric, but also in any metric computed …
GYOTO: A new general relativistic ray-tracing code
https://www.researchgate.net/publication/230937843_GYOTO_A_new_general_relativistic_ray-tracing_code
Abstract. GYOTO, a general relativistic ray-tracing code, is presented. It aims at computing images of astronomical bodies in the vicinity of compact objects, as …
GYOTO: a new general relativistic ray-tracing code
https://www.semanticscholar.org/paper/GYOTO%3A-a-new-general-relativistic-ray-tracing-code-Vincent-Paumard/68fcaa0a562a90f1a8743c69e1d0700500154b20
GYOTO: a new general relativistic ray-tracing code. GYOTO, a general relativistic ray-tracing code, is presented. It aims at computing images of astronomical bodies in the vicinity of compact objects, as well as trajectories of massive bodies in relativistic environments. This code is capable of integrating the null and timelike geodesic equations not only in the Kerr …
GYOTO: a new general relativistic ray-tracing code - obspm.fr
https://luth.obspm.fr/~luthier/gourgoulhon/pdf/VincePGP11.pdf
GYOTO, a general relativistic ray-tracing code, is presented. It aims at computing images of astronomical bodies in the vicinity of compact objects, as well as trajectories of massive bodies in relativistic environments. This code is capable of …
GYOTO: a new general relativistic ray-tracing code
https://www.arxiv-vanity.com/papers/1109.4769/
GYOTO, a general relativistic ray-tracing code, is presented. It aims at computing images of astronomical bodies in the vicinity of compact objects, as well as trajectories of massive bodies in relativistic environments. This code is capable of integrating the null and timelike geodesic equations not only in the Kerr metric, but also in any metric computed numerically within the …
GYOTO: a new general relativistic ray-tracing code - IOPscience
https://iopscience.iop.org/article/10.1088/0264-9381/28/22/225011/meta
GYOTO: a new general relativistic ray-tracing code. F H Vincent 1,2, T Paumard 1, E Gourgoulhon 2 and G Perrin 1. Published 18 October 2011 • 2011 IOP Publishing Ltd Classical and Quantum Gravity, Volume 28, Number 22
GYOTO: a new general relativistic ray-tracing code - NASA/ADS
https://ui.adsabs.harvard.edu/abs/2011CQGra..28v5011V/abstract
GYOTO, a general relativistic ray-tracing code, is presented. It aims at computing images of astronomical bodies in the vicinity of compact objects, as well as trajectories of massive bodies in relativistic environments.
public code for general relativistic, polarised radiative …
https://academic.oup.com/mnras/article/462/1/115/2589406
We present a publicly available, fully general relativistic code, grtrans, 1 for polarised radiative transfer via ray tracing in the Kerr metric. We describe the methods used for the parallel transport of the polarisation basis into the local frame of the fluid (Section 2.2) and the integration of the polarised radiative transfer equations (Section 2.5) using emission, absorption, and rotation …
General Relativistic Ray Tracing - Washington University in St. Louis
https://sites.wustl.edu/xastro/general-relativistic-ray-tracing/
We uses detailed ray tracing simulations (Krawczynski et al. 2012, Hoorman et al. 2016) to study if the combined information from X-ray spectroscopy, timing, and polarization observations of stellar mass and supermassive black holes can be used to test GR’s no-hair theorem. The latter states that stationary astrophysical black holes are ...
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