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In order to understand the appropriate field of view (FOV) size of celestial automatic navigation systems for surface ships, we investigate the variations of measurement accuracy of star position and probability of successful star…

We propose an efficient way to test rotational invariance in the cosmological perturbations by use of galaxy correlation functions. In symmetry-breaking cases, the galaxy power spectrum can have extra angular dependence in addition to the…

Cosmology and Nongalactic Astrophysics · Physics 2017-03-10 Maresuke Shiraishi , Naonori S. Sugiyama , Teppei Okumura

A rapid algorithm is derived for the Helmholtz--Hodge decomposition on the surface of the sphere in spherical coordinates. The algorithm uncouples modes of spherical harmonics with different absolute order, writes the conversion as…

Numerical Analysis · Mathematics 2018-09-13 Julien Molina , Richard Mikael Slevinsky

Topological physics desires stable methods to measure the polarization singularities in optical vector fields. Here a periodic plasmonic metasurface is proposed to perform divergence computation of vectorial paraxial beams. We design such…

Optics · Physics 2020-09-09 Yijie Lou , Yisheng Fang , Zhichao Ruan

Observations of circumstellar environments to look for the direct signal of exoplanets and the scattered light from disks has significant instrumental implications. In the past 15 years, major developments in adaptive optics, coronagraphy,…

Instrumentation and Methods for Astrophysics · Physics 2019-11-13 J. -L. Beuzit , A. Vigan , D. Mouillet , K. Dohlen , R. Gratton , A. Boccaletti , J. -F. Sauvage , H. M. Schmid , M. Langlois , C. Petit , A. Baruffolo , M. Feldt , J. Milli , Z. Wahhaj , L. Abe , U. Anselmi , J. Antichi , R. Barette , J. Baudrand , P. Baudoz , A. Bazzon , P. Bernardi , P. Blanchard , R. Brast , P. Bruno , T. Buey , M. Carbillet , M. Carle , E. Cascone , F. Chapron , G. Chauvin , J. Charton , R. Claudi , A. Costille , V. De Caprio , A. Delboulbé , S. Desidera , C. Dominik , M. Downing , O. Dupuis , C. Fabron , D. Fantinel , G. Farisato , P. Feautrier , E. Fedrigo , T. Fusco , P. Gigan , C. Ginski , J. Girard , E. Giro , D. Gisler , L. Gluck , C. Gry , T. Henning , N. Hubin , E. Hugot , S. Incorvaia , M. Jaquet , M. Kasper , E. Lagadec , A. -M. Lagrange , H. Le Coroller , D. Le Mignant , B. Le Ruyet , G. Lessio , J. -L. Lizon , M. Llored , L. Lundin , F. Madec , Y. Magnard , M. Marteaud , P. Martinez , D. Maurel , F. Ménard , D. Mesa , O. Möller-Nilsson , T. Moulin , C. Moutou , A. Origné , J. Parisot , A. Pavlov , D. Perret , J. Pragt , P. Puget , P. Rabou , J. Ramos , J. -M. Reess , F. Rigal , S. Rochat , R. Roelfsema , G. Rousset , A. Roux , M. Saisse , B. Salasnich , E. Santambrogio , S. Scuderi , D. Segransan , A. Sevin , R. Siebenmorgen , C. Soenke , E. Stadler , M. Suarez , D. Tiphène , M. Turatto , S. Udry , F. Vakili , L. B. F. M. Waters , L. Weber , F. Wildi , G. Zins , A. Zurlo

X-ray observatories contribute fundamental advances in Solar System studies by probing Sun-object interactions, developing planet and satellite surface composition maps, probing global magnetospheric dynamics, and tracking astrochemical…

The stellar haloes of galaxies can currently be studied either through observations of resolved halo stars or through surface photometry. Curiously, the two methods appear to give conflicting results, as a number of surface photometry…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 E. Zackrisson , R. S. de Jong , G. Micheva

Studies of large-scale structures in the Universe, such as superstructures or cosmic voids, have been widely used to characterize the properties of the cosmic web through statistical analyses. On the other hand, the 2-point correlation…

Cosmology and Nongalactic Astrophysics · Physics 2020-05-04 M. V. Santucho , H. E. Luparello , M. Lares , D. G. Lambas , A. N. Ruiz , M. A. Sgró

Structured light harnessing multiple degrees of freedom has become a powerful approach to use complex states of light in fundamental studies and applications. Here, we investigate the light field of an ultrafast laser beam with a…

Astronomical data are typically irregular in time, e.g. the space (HIPPARCOS/TYCHO, KEPLER, GAIA, WISE etc.) and ground-based CCD (NSVS, ASAS, CRTS, SuperWASP etc.) and photographic (Harvard, Sonneberg, Odessa etc.) photometrical surveys.…

Solar and Stellar Astrophysics · Physics 2019-02-05 Ivan L. Andronov

Recently, the theory concerning piecewise smooth vector fields (PSVFs for short) have been undergoing important improvements. In fact, many results obtained do not have an analogous for smooth vector fields. For example, the chaoticity of…

Dynamical Systems · Mathematics 2021-12-07 Andre Amaral Antunes , Tiago Carvalho

In many applications, the ability to measure the vector information of a magnetic field with high spatial resolution and low cost is essential, but it is still a challenge for existing magnetometers composed of multiple sensors. Here, we…

Mesoscale and Nanoscale Physics · Physics 2022-08-05 Xin Chen , Hang Xie , Haoxuan Shen , Yihong Wu

Modern coronagraphic systems require very precise alignment between optical components and can benefit greatly from automated image processing. We discuss three techniques commonly employed in the fields of computer vision and image…

Instrumentation and Methods for Astrophysics · Physics 2013-05-09 Dmitry Savransky , Sandrine J. Thomas , Lisa A. Poyneer , Bruce A. Macintosh

A symplectic integrator algorithm suitable for hierarchical triple systems is formulated and tested. The positions of the stars are followed in hierarchical Jacobi coordinates, whilst the planets are referenced purely to their primary. The…

Astrophysics · Physics 2009-11-13 P. E. Verrier , N. W. Evans

The shapelets method for image analysis is based upon the decomposition of localised objects into a series of orthogonal components with convenient mathematical properties. We extend the "Cartesian shapelet" formalism from earlier work, and…

Astrophysics · Physics 2009-11-10 Richard Massey , Alexandre Refregier

We summarize some of the compelling new scientific opportunities for understanding stars and stellar systems that can be enabled by sub-milliarcsec (sub-mas) angular resolution, UV-Optical spectral imaging observations, which can reveal the…

We present a novel method to search for structures of coherently aligned patterns in ultra-high energy cosmic-ray arrival directions simultaneously across the entire sky. This method can be used to obtain information on the Galactic…

Instrumentation and Methods for Astrophysics · Physics 2022-01-31 Marcus Wirtz , Teresa Bister , Martin Erdmann

Vector beams are inhomogeneously polarized optical fields with nonseparable, quantum-like correlations between their polarisation and spatial components, and hold tremendous promise for classical and quantum communication across various…

In this paper we study the decoherence processes of the semiclassical branches of an accelerated universe due to their interaction with a scalar field with given mass. We use a third quantization formalism to analyze the decoherence between…

General Relativity and Quantum Cosmology · Physics 2015-06-03 S. Robles-Perez , A. Alonso-Serrano , P. F. Gonzalez-Diaz

We propose a new systematic method of studying correlations between parameters that describe an astronomical (or any) physical system. We recall that behind Dimensionless scaling laws in complex, self-interacting physical objects lies a…

Astrophysics of Galaxies · Physics 2019-02-26 R. N. Henriksen , J. A. Irwin