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We describe a software package used at the Special Astrophysical Observatory of the Russian Academy of Sciences to reduce and analyze the data obtained with the Fabry-Perot scanning interferometer. We already described most of the…

Astrophysics · Physics 2011-08-31 A. V. Moiseev , O. V. Egorov

The upcoming space missions that will characterize exoplanets, such as PLATO and Ariel, will collect huge amounts of data that will need to be complemented with ground-based observations. The aim of the PLATOSpec project is to perform…

This article presents a high-throughput computer program, called EasyDD, for batch processing, analyzing and visualizing of spectral data; particularly those related to the new generation of synchrotron detectors and X-ray powder…

Data Analysis, Statistics and Probability · Physics 2013-07-16 Taha Sochi

The Planet Hunting and Asteroseismology Explorer Spectrophotometer, PHASES, is a concept for a space-borne instrument to obtain flux calibrated spectra and measure micro-magnitude photometric variations of nearby stars. The science drivers…

Instrumentation and Methods for Astrophysics · Physics 2010-01-13 Carlos del Burgo , Carlos Allende Prieto , Tully Peacocke

ImageJ is a graphical user interface (GUI) driven, public domain, Java-based, software package for general image processing traditionally used mainly in life sciences fields. The image processing capabilities of ImageJ are useful and…

Instrumentation and Methods for Astrophysics · Physics 2017-09-27 Karen A. Collins , John F. Kielkopf , Keivan G. Stassun , Frederic V. Hessman

We briefly overview the new features of PlanetPack2, the forthcoming update of PlanetPack, which is a software tool for exoplanets detection and characterization from Doppler radial velocity data. Among other things, this major update…

Instrumentation and Methods for Astrophysics · Physics 2015-07-15 Roman V. Baluev

We present TA-DA, a new software aimed at greatly simplify and improve the analysis of stellar photometric data in comparison with theoretical models, and allow the derivation of stellar parameters from multi-band photometry. Its…

Solar and Stellar Astrophysics · Physics 2015-06-11 Nicola Da Rio , Massimo Robberto

The Gaia-ESO Survey is a large public spectroscopic survey that aims to derive radial velocities and fundamental parameters of about 10^5 Milky Way stars in the field and in clusters. Observations are carried out with the multi-object…

The general context of this study is the inversion of stellar fundamental parameters from high-resolution Echelle spectra. We aim at developing a fast and reliable tool for the post-processing of spectra produced, in particular, by the…

Instrumentation and Methods for Astrophysics · Physics 2014-08-05 F. Paletou , J. -F. Trouilhet , T. Boehm

SMART is a software package written in IDL to reduce and analyze Spitzer data from all four modules of the Infrared Spectrograph, including the peak-up arrays. The software is designed to make full use of the ancillary files generated in…

Hyperspectral imaging is a powerful tool for Earth exploration, allowing for detailed analysis of spectral features. India has launched a dedicated hyperspectral Earth observation satellite capable of capturing data across a wide…

Image and Video Processing · Electrical Eng. & Systems 2024-11-15 Ankur Garg , Abhishek Patil , Meenakshi Sarkar , S. Manthira Moorthi , Debajyoti Dhar

Digital Access to a Sky Century @ Harvard (DASCH) is a project to digitize the collection of approximately 525,000 astronomical plates held at the Harvard College Observatory. This paper presents an overview of the DASCH data processing…

Instrumentation and Methods for Astrophysics · Physics 2011-02-25 Edward Los , Jonathan Grindlay , Sumin Tang , Mathieu Servillat , Silas Laycock

A dedicated mission to investigate exoplanetary atmospheres represents a major milestone in our quest to understand our place in the universe by placing our Solar System in context and by addressing the suitability of planets for the…

Earth and Planetary Astrophysics · Physics 2015-06-03 G. Tinetti , J. P. Beaulieu , T. Henning , M. Meyer , G. Micela , I. Ribas , D. Stam , M. Swain , O. Krause , M. Ollivier , E. Pace , B. Swinyard , A. Aylward , R. van Boekel , A. Coradini , T. Encrenaz , I. Snellen , M. R. Zapatero-Osorio , J. Bouwman , J. Y-K. Cho , V. Coudé du Foresto , T. Guillot , M. Lopez-Morales , I. Mueller-Wodarg , E. Palle , F. Selsis , A. Sozzetti , P. A. R. Ade , N. Achilleos , A. Adriani , C. B. Agnor , C. Afonso , C. Allende Prieto , G. Bakos , R. J. Barber , M. Barlow , P. Bernath , B. Bezard , P. Bordé , L. R. Brown , A. Cassan , C. Cavarroc , A. Ciaravella , C. O. U. Cockell , A. Coustenis , C. Danielski , L. Decin , R. De Kok , O. Demangeon , P. Deroo , P. Doel , P. Drossart , L. N. Fletcher , M. Focardi , F. Forget , S. Fossey , P. Fouqué , J. Frith , M. Galand , P. Gaulme , J. I. González Hernández , O. Grasset , D. Grassi , J. L. Grenfell , M. J. Griffin , C. A. Griffith , U. Grözinger , M. Guedel , P. Guio , O. Hainaut , R. Hargreaves , P. H. Hauschildt , K. Heng , D. Heyrovsky , R. Hueso , P. Irwin , L. Kaltenegger , P. Kervella , D. Kipping , T. T. Koskinen , G. Kovács , A. La Barbera , H. Lammer , E. Lellouch , G. Leto , M. Lopez Morales , M. A. Lopez Valverde , M. Lopez-Puertas , C. Lovis , A. Maggio , J. P. Maillard , J. Maldonado Prado , J. B. Marquette , F. J. Martin-Torres , P. Maxted , S. Miller , S. Molinari , D. Montes , A. Moro-Martin , J. I. Moses , O. Mousis , N. Nguyen Tuong , R. Nelson , G. S. Orton , E. Pantin , E. Pascale , S. Pezzuto , D. Pinfield , E. Poretti , R. Prinja , L. Prisinzano , J. M. Rees , A. Reiners , B. Samuel , A. Sanchez-Lavega , J. Sanz Forcada , D. Sasselov , G. Savini , B. Sicardy , A. Smith , L. Stixrude , G. Strazzulla , J. Tennyson , M. Tessenyi , G. Vasisht , S. Vinatier , S. Viti , I. Waldmann , G. J. White , T. Widemann , R. Wordsworth , R. Yelle , Y. Yung , S. N. Yurchenko

Complex field measurements are increasingly becoming the standard for state-of-the-art astronomical instrumentation. Complex field measurements have been used to characterize a suite of ground, airborne, and space-based heterodyne receiver…

Instrumentation and Methods for Astrophysics · Physics 2018-09-25 Kristina K. Davis , Willem Jellema , Stephen J. C. Yates , Christopher E. Groppi , Jochem J. A. Baselmans , Andrey M. Baryshev

Instrument simulators are becoming ever more useful for planning and analysing large astronomy survey data. In this paper we present a simulator for the Herschel-SPIRE photometer. We describe the models it uses and the form of the input and…

Instrumentation and Methods for Astrophysics · Physics 2015-05-13 B. Sibthorpe , P. Chanial , M. Griffin

We present a light and fast, public available, ray-tracer {\tt Splotch} software tool which supports the effective visualization of cosmological simulations data. We describe the algorithm it relies on, which is designed in order to deal…

Astrophysics · Physics 2008-12-18 K. Dolag , M. Reinecke , C. Gheller , S. Imboden

We describe an automatic procedure for determining abundances from high resolution spectra. Such procedures are becoming increasingly important as large amounts of data are delivered from 8m telescopes and their high-multiplexing fiber…

Astrophysics · Physics 2009-11-07 Piercarlo Bonifacio , Elisabetta Caffau

ImageJ is a graphical user interface (GUI) driven, public domain, Java-based, software package for general image processing traditionally used mainly in life sciences fields. The image processing capabilities of ImageJ are useful and…

Instrumentation and Methods for Astrophysics · Physics 2017-02-01 Karen A. Collins , John F. Kielkopf , Keivan G. Stassun , Frederic V. Hessman

We present here the first release of the open-source python package ExoTETHyS, which aims to provide a stand-alone set of tools for modeling spectro-photometric observations of the transiting exoplanets. In particular, we describe: (1) a…

Earth and Planetary Astrophysics · Physics 2020-02-05 Giuseppe Morello , Antonio Claret , Marine Martin-Lagarde , Christophe Cossou , Angelos Tsiaras , Pierre-Olivier Lagage

In this article, a software package code named OPSIAL (Optical Plasma Spectral Calculation And Parameters Retrieval) for rigorously calculating optical plasma spectra and for automatically retrieving plasma parameters is presented. OPSIAL…

Computational Physics · Physics 2018-02-06 Xiaofeng Tan
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