P3D: a general data-reduction tool for fiber-fed integral-field spectrographs

The reduction of integral-field spectrograph (IFS) data is demanding work. Many repetitive operations are required to convert raw data into, typically, a large number of spectra. This effort can be markedly simplified through the use of a tool or pipeline, which is designed to complete many of the repetitive operations without human interaction. Here we present our semi-automatic data-reduction tool p3d, which is designed to be used with fiber-fed IFSs. Important components of p3d include a novel algorithm for automatic finding and tracing of spectra on the detector and two methods of optimal spectrum extraction in addition to standard aperture extraction. p3d also provides tools to combine several images, perform wavelength calibration and flat field data. p3d is at the moment configured for four IFSs. To evaluate its performance, we tested the different components of the tool. For these tests we used both simulated and observational data. We demonstrate that a correction for so-called cross-talk due to overlapping spectra on the detector is required for three of the IFSs. Without such a correction, spectra will be inaccurate, in particular if there is a significant intensity gradient across the object. Our tests showed that p3d is able to produce accurate results. p3d is a highly general and freely available tool. It is easily extended to include improved algorithms, new visualization tools, and support for additional instruments. The program code can be downloaded from the p3d-project web site http://p3d.sourceforge.net.

[1]  S. F. Sanchez,et al.  Integral field spectroscopy of the ultraluminous X-ray source Holmberg II X-1 , 2005 .

[2]  C. De Breuck,et al.  VIMOS‐VLT and Spitzer observations of a radio galaxy at z= 2.5★ , 2005, astro-ph/0510733.

[3]  A. Kelz,et al.  Spectrophotometry of Planetary Nebulae in the Bulge of M31 , 2003, astro-ph/0311407.

[4]  Michele Cappellari,et al.  Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellations , 2003, astro-ph/0302262.

[5]  David Thomas,et al.  The Pragmatic Programmer: From Journeyman to Master , 1999 .

[6]  W. Pych A Fast Algorithm for Cosmic‐Ray Removal from Single Images , 2003, astro-ph/0311290.

[7]  Steve B. Howell,et al.  Handbook of CCD Astronomy: Contents , 2006 .

[8]  Evencio Mediavilla,et al.  3D Spectroscopy in Astronomy , 2010 .

[9]  J. Turner A scientific overview of requirements for IFU data reduction and analysis , 2006 .

[10]  Luis Colina,et al.  PMAS optical integral field spectroscopy of luminous infrared galaxies - I. The atlas , 2009, 0907.5105.

[11]  K. Herkenhoff,et al.  Handbook of CCD Astronomy; Cambridge Observing Handbooks for Research Astronomers , 2000 .

[12]  K. Horne,et al.  AN OPTIMAL EXTRACTION ALGORITHM FOR CCD SPECTROSCOPY. , 1986 .

[13]  A. Mazure,et al.  The VVDS Data‐Reduction Pipeline: Introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface , 2004, astro-ph/0409248.

[14]  A. Monreal-Ibero,et al.  INTEGRAL FIELD SPECTROSCOPY OF FAINT HALOS OF PLANETARY NEBULAE , 2005 .

[15]  Arlette Pécontal-Rousset,et al.  The Euro3D data format: A common FITS data format for integral field spectrographs , 2004 .

[16]  M. Birchall,et al.  Optimal Extraction of Fibre Optic Spectroscopy , 2009, Publications of the Astronomical Society of Australia.

[17]  Jeremy R. Allington-Smith,et al.  Sampling and Background Subtraction in Fiber‐Lenslet Integral Field Spectrographs , 1998 .

[18]  T. Becker,et al.  Crowded field 3D spectroscopy of LBV candidates in M 33 , 2005, astro-ph/0503586.

[19]  Scott Burles,et al.  An integral-field spectroscopic strong lens survey , 2007 .

[20]  H Germany,et al.  PMAS: The Potsdam Multi‐Aperture Spectrophotometer. I. Design, Manufacture, and Performance , 2005, astro-ph/0502581.

[21]  Martin M. Roth,et al.  Spatially resolved spectroscopy of planetary nebulae and their halos - I. Five galactic disk objects , 2008, 0802.3813.

[22]  Evencio Mediavilla,et al.  Differential atmospheric refraction in integral-field spectroscopy: Effects and correction - Atmospheric refraction in IFS , 1999 .

[23]  David J. Schlegel,et al.  Spectro-Perfectionism: An Algorithmic Framework for Photon Noise-Limited Extraction of Optical Fiber Spectroscopy , 2009, 0911.2689.

[24]  P. Dokkum Cosmic-Ray Rejection by Laplacian Edge Detection , 2001, astro-ph/0108003.

[25]  I. Hook,et al.  Integral Field Spectroscopy with the Gemini Multiobject Spectrograph.I. Design, Construction, and Testing , 2002 .

[26]  A. Monreal-Ibero,et al.  Spatially resolved study of the physical properties of the ionized gas in NGC 595 , 2009, 0911.3006.

[27]  Andreas Kelz,et al.  PMAS: The Potsdam Multi-Aperture Spectrophotometer. II. The Wide Integral Field Unit PPak , 2006 .

[28]  A. V. Filippenko,et al.  THE IMPORTANCE OF ATMOSPHERIC DIFFERENTIAL REFRACTION IN SPECTROPHOTOMETRY. , 1982 .

[29]  S. F. Sánchez,et al.  Techniques for Reducing Fiber-fed and Integral-field Spectroscopy Data , 2006 .