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Processing Data from Large Infrared Surveys

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Star Clusters in the Era of Large Surveys

Abstract

At the Cambridge Astronomical Survey Unit (CASU) we are responsible for the development and implementation of a number of pipelines for the routine processing of large area near-infrared surveys. In this paper, we discuss some of the challenges we face when tackling the large volumes of data generated nightly from WFCAM on UKIRT and VIRCAM on VISTA.

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Notes

  1. 1.

    http://casu.ast.cam.ac.uk/

  2. 2.

    http://casu.ast.cam.ac.uk/surveys-projects/software-release/software-release/view.

  3. 3.

    email:casuhelp@ast.cam.ac.uk.

References

  1. Bertin, E., Arnouts, S.: Astron. Astrophys. Suppl. 117, 393 (1996)

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  2. Hodgkin, S.T., Irwin, M.J., Hewett, P.C., Warren, S.J.: Mon. Not. R. Astron. Soc. 394, 675 (2009)

    Article  ADS  Google Scholar 

  3. Irwin, M.J.: Mon. Not. R. Astron. Soc. 214, 575 (1985)

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  4. Irwin, M.J.: UKIRT Newsl. 26, 14 (2010)

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Correspondence to Simon Hodgkin .

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© 2012 Springer-Verlag Berlin Heidelberg

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Hodgkin, S., Irwin, M., Lewis, J., Gonzalez-Solares, E., Yoldaş, A.K. (2012). Processing Data from Large Infrared Surveys. In: Moitinho, A., Alves, J. (eds) Star Clusters in the Era of Large Surveys. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-22113-2_5

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  • DOI: https://doi.org/10.1007/978-3-642-22113-2_5

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-22112-5

  • Online ISBN: 978-3-642-22113-2

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