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We describe a framework that allows a scientist-user to easily query for information across all Virtual Observatory (VO) repositories and pull it back for analysis. This framework hides the gory details of meta-data remediation and data…

天体物理仪器与方法 · 物理学 2015-02-24 Brian Thomas , Edward Shaya , Zenping Huang , Peter Teuben

I have carried out a search for Planet 9 in the IRAS data. At the distance range proposed for Planet 9, the signature would be a 60 micron unidentified IRAS point source with an associated nearby source from the IRAS Reject File of sources…

地球与行星天体物理 · 物理学 2021-11-24 Michael Rowan-Robinson

Sky coverage is one of the most important pieces of information about astronomical observations. We discuss possible representations, and present algorithms to create and manipulate shapes consisting of generalized spherical polygons with…

天体物理仪器与方法 · 物理学 2015-05-19 Tamas Budavari , Alex Szalay , Gyorgy Fekete

A selection of astrometric catalogues are presented in three tables for respectively positions, proper motions and trigonometric parallaxes. The tables contain characteristics of each catalogue showing the evolution in optical astrometry,…

天体物理仪器与方法 · 物理学 2017-07-11 Erik Høg

The IVOA works towards standardising interoperability and curation of data and service holdings of the global astrophysical community. Within the IVOA, the Data Access Layer (DAL) Working Group's goal is to provide technical standards for…

天体物理仪器与方法 · 物理学 2020-12-03 Marco Molinaro , James Dempsey

The exploration of interstellar space will require autonomous navigation systems that do not rely on tracking from the Earth. Here I develop a method to determine the 3D position and 3D velocity of a spacecraft in deep space using a star…

天体物理仪器与方法 · 物理学 2021-07-22 Coryn A. L. Bailer-Jones

VOEvent defines the content and meaning of a standard information packet for representing, transmitting, publishing and archiving information about a transient celestial event, with the implication that timely follow-up is of interest. The…

In the current data-driven science era, it is needed that data analysis techniques has to quickly evolve to face with data whose dimensions has increased up to the Petabyte scale. In particular, being modern astrophysics based on…

天体物理仪器与方法 · 物理学 2017-06-14 Giuseppe Riccio , Massimo Brescia , Stefano Cavuoti , Amata Mercurio , Anna Maria Di Giorgio , Sergio Molinari

It is shown here how prior estimates on the local shape of the universe can be used to reduce, to a small region, the full parameter space for the search of circles in the sky. This is the first step towards the development of efficient…

天体物理学 · 物理学 2007-05-23 G. I. Gomero

Although the Gaia catalogue on its own will be a very powerful tool, it is the combination of this highly accurate archive with other archives that will truly open up amazing possibilities for astronomical research. The advanced…

太阳与恒星天体物理 · 物理学 2017-11-22 P. M. Marrese , S. Marinoni , M. Fabrizio , G. Giuffrida

In this paper, we describe a very simple method to calculate the positions of the planets in the sky. The technique used enables us to calculate planetary positions to an accuracy of $\stackrel{<}{_{\sim}} 1^{\circ}$ for $\pm 50$ years from…

天体物理仪器与方法 · 物理学 2020-09-14 Tanmay Singal , Ashok k. Singal

The first step in a science project is the acquisition and understanding of the relevant data. This paper outlines the results of a project to design and test network tools specifically oriented at retrieving astronomical data. The tools…

天体物理仪器与方法 · 物理学 2009-10-07 James Schombert

With the success and widespread of the IVOA Table Access Protocol (1) for discovering and querying tabular data in astronomy, more than one hundred of TAP services exposing altogether 22 thousands of tables are accessible from the IVOA…

天体物理仪器与方法 · 物理学 2022-01-06 Mireille Louys , Laurent Michel , François Bonnarel , Joann Vetter

The ESA Gaia mission, to be launched during 2013, will observe billions of objects, among which many galaxies, during its scanning of the sky. This will provide a large space-based dataset with unprecedented spatial resolution. Because of…

We present the preliminary result of our project, consisting in studying the properties of a large sample of galaxy clusters. The M\"{u}nster Red Sky Survey, which is a large galaxy catalogue covering an area of about 5000 square degrees on…

天体物理学 · 物理学 2009-11-10 E. Panko , P. Flin

Source confusion has been a long-standing problem in the astronomical history. In the previous formulation, sources are assumed to be distributed homogeneously on the sky. This fundamental assumption is not realistic in many applications.…

天体物理学 · 物理学 2009-11-10 Tsutomu T. Takeuchi , Takako T. Ishii

We present a system for performing visual search over billions of aerial and satellite images. The purpose of visual search is to find images that are visually similar to a query image. We define visual similarity using 512 abstract visual…

计算机视觉与模式识别 · 计算机科学 2020-02-10 Ryan Keisler , Samuel W. Skillman , Sunny Gonnabathula , Justin Poehnelt , Xander Rudelis , Michael S. Warren

A new realization of the International Celestial Reference Frame (ICRF) is presented based on the work achieved by a working group of the International Astronomical Union (IAU) mandated for this purpose. This new realization, referred to as…

Quasars are very important in materializing the reference frame. The excess emission of AGNs (active galactic nuclei) in the mid infrared band can be used to identify quasar candidates. As extremely distant and point like objects, quasars…

星系天体物理 · 物理学 2022-12-12 Qiqi Wu , Shilong Liao , Zhaoxiang Qi , Hao Luo , Zhenghong Tang , Zihuang Cao

Polarimetry of stars at optical and near-infrared wavelengths is an invaluable tool for tracing interstellar dust and magnetic fields. Recent studies have demonstrated the power of combining stellar polarimetry with distances from the Gaia…