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Sherpa: a Mission-Independent Data Analysis Application

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arxiv astro-ph/0108426 v1 pith:4UCW3BOY submitted 2001-08-27 astro-ph

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keywords analysisdatamodelsherpaincludinglanguagemulti-dimensionalneed
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The ever-increasing quality and complexity of astronomical data underscores the need for new and powerful data analysis applications. This need has led to the development of Sherpa, a modeling and fitting program in the CIAO software package that enables the analysis of multi-dimensional, multi-wavelength data. In this paper, we present an overview of Sherpa's features, which include: support for a wide variety of input and output data formats, including the new Model Descriptor List (MDL) format; a model language which permits the construction of arbitrarily complex model expressions, including ones representing instrument characteristics; a wide variety of fit statistics and methods of optimization, model comparison, and parameter estimation; multi-dimensional visualization, provided by ChIPS; and new interactive analysis capabilities provided by embedding the S-Lang interpreted scripting language. We conclude by showing example Sherpa analysis sessions.

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Cited by 4 Pith papers

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    astro-ph.HE 2026-07 conditional novelty 7.0 of 10

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  2. Exploring Constraints on Axion-like Particles with the Observations for blazar Mrk 501

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

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  3. Origin of the Sloshing Spiral in the Abell 2107 Galaxy Cluster

    astro-ph.CO 2026-07 conditional novelty 5.0 of 10

    A previously unknown sloshing spiral with three cold fronts is discovered in the ICM of the apparently relaxed cluster Abell 2107, pointing to a past off-axis merger with a possibly dark perturber.

  4. IXPE Observations of the Blazar Mrk 501 in 2022: A Multiwavelength View

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

    IXPE's third 2022 observation of Mrk 501 yields X-ray polarization degree 6±2% at angle 143±11°, consistent with earlier epochs and with shock-based jet models.

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