Specialized Resource (Document): Compute Redshifts of Quasars Using SPLAT-VO
Description
This tutorial uses SPLAT-VO to search the VO registry for spectra of galaxies and quasars. From the obtained spectra, the Hydrogen Lyman Alpha line will be used to compute redshift and velocity
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Publisher: The GAVO DC team
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This resource was registered on: 2016 Jan 24 00:00:00ZThis resource description was last updated on: 2025 Apr 03 09:45:51Z
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To the extent possible under law, the publisher has waived all copyright and related or neighboring rights to The GAVO SPLAT tutorial. For details, see the `Creative Commons CC0 1.0 Public Domain dedication <http://creativecommons.org/publicdomain/zero/1.0/>`_. Of course, you should still give proper credit when using this data as required by good scientific practice. .. image:: /static/img/cc0.png :alt: [CC0]
This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
Developed with the support of the National Science Foundation under Cooperative Agreement AST0122449 with the Johns Hopkins University The NAVO project is a member of the International Virtual Observatory Alliance
This NAVO Application is hosted by the Space Telescope Science Institute