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Status of GDL - GNU Data Language

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arxiv 1101.0679 v1 pith:ZP3FWXYD submitted 2011-01-04 astro-ph.IM cs.CE

A. Coulais (1) , M. Schellens , J. Gales (2) , S. Arabas (3) , M. Boquien (4) , P. Chanial (5) , P. Messmer (6) , D. Fillmore (5)
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O. Poplawski (6) S. Maret (7) G. Marchal (1) N. Galmiche (1) T. Mermet (1) ((1) LERMA Obs. de Paris ENS UPMC UCP CNRS Paris France (2) Goddard Space Flight Center Greenbelt MD USA (3) Institute of Geophysics Faculty of Physics University of Warsaw Poland (4) University of Massachusetts Dep. of Astronomy Amherst MA (5) Tech-X GmbH Zurich Switzerland Tech-X Corp Boulder CO (6) Colorado Div. (CoRA) of NorthWest Res. Ass. Inc. (7) LAOG Obs. de Grenoble UJF Grenoble France)
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GNU Data Language (GDL) is an open-source interpreted language aimed at numerical data analysis and visualisation. It is a free implementation of the Interactive Data Language (IDL) widely used in Astronomy. GDL has a full syntax compatibility with IDL, and includes a large set of library routines targeting advanced matrix manipulation, plotting, time-series and image analysis, mapping, and data input/output including numerous scientific data formats. We will present the current status of the project, the key accomplishments, and the weaknesses - areas where contributions are welcome !

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Excess Ultraviolet Emission at High Galactic Latitudes: A New Horizons View

    astro-ph.GA 2025-01 conditional novelty 6.0 of 10

    Measurements from 57 AU show a cosmic UV background of about 221 photon units at 1000 Å and 264 at 1500 Å after accounting for dust, about half of which is unexplained.

  2. Modeling the Cosmic Ultraviolet Background at the North Galactic Pole

    astro-ph.IM 2025-07 conditional novelty 4.0 of 10

    A quadratic parametrization of dust-scattered UV light, fitted to GALEX data at the North Galactic Pole, yields an isotropic background of 267 ± 7 photon units and is consistent with the Astrodust dust model.

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