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Ultra-Deep Optical Spectroscopy with PMAS. Using the Nod-and-Shuffle Technique

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Abstract

PMAS, the Potsdam Multi-Aperture Spectrophotometer, is a new integral field spectrograph in the optical, which is optimized for good transmission and high image quality from 350 nm to 1 μm. We present our plan to implement a CCD charge-shuffle mode to allow for beam switching with a very high degree of sky subtraction accuracy for faint object 3-D spectroscopy.

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References

  • Cuillandre, J. C., Fort, B., Picat, J. P., Soucail, G., Altieri, B., Beigbeder, F., Dupin, J. P., Pourthie, T. and Ratier, G.: 1994, ‘’Va-et-Vient’ Spectroscopy: A New Mode for Faint Object CCD Spectroscopy with Very Large Telescopes’, A&A 281, pp. 603.

    ADS  Google Scholar 

  • Fechner, T., Wolter, D. and Roth, M. M.: 2000, ‘CCD Systems for PMAS – A New Optical Integral Field Spectrophotometer for the Calar Alto Observatory 3.5 m telescope’, in Proc., Optical Detectors For Astronomy II, Kluwer Dordrecht, p. 153.

  • Glazebrook, K. and Bland-Hawthorn, J.: 2001, ‘Microslit Nod-Shuffle Spectroscopy: A Technique for Achieving Very High Densities of Spectra’, PASP 113, p. 197.

    Article  ADS  Google Scholar 

  • Hu, E. M., Cowie, L. L., McMahon, R. G., Capak, P., Iwamuro, F., Kneib, J.-P., Maihara, T. and Motohara, K.: 2002, ‘A Redshift z=6.56 Galaxy behind the Cluster Abell 370’, ApJ 568, L75.

    Article  ADS  Google Scholar 

  • Massey, P. and Foltz, C. B.: 2000, ‘The Spectrum of the Night Sky over Mount Hopkins and Kitt Peak: Changes after a Decade’, PASP 112, p. 566.

    Article  ADS  Google Scholar 

  • Roth, M. M., Becker, T., Böhm, P. and Kelz, A.: 2002, ‘Galaxies – The Third Dimension’, in Margarita Rosado, Luc Binette, Lorena Arias (eds), Proc., ASP Conf. Ser.

  • Roth, M. M., Becker, T. and Schmoll, J.: 2000, ‘Faint Object 2-D Spectroscopy: Promise and Limitations’, in Proc., 3D – Imaging the Universe in Three Dimensions, ASP Conf. Ser. 195, p. 122.

    ADS  Google Scholar 

  • Roth, M. M., Bauer, S. M., Dionies, F., Fechner, T., Hahn, T., Laux, U., Nickel, U., Popow, E., Schmoll, J. and Wolter, D.: 1998, ‘PMAS – the Potsdam Multiaperture Spectrophotometer: A Progress Report’, in Proc. SPIE 3355, p. 798.

    Article  ADS  Google Scholar 

  • Roth, M. M. and Laux, U.: 1998, ‘The PMAS Fiber Spectrograph’, in Proc., Fiber Optics in Astronomy III, ASP Conf. Ser. 152.

  • Roth, M. M., Seydack, M., Bauer, S. M. and Laux, U.: 1997, Design study for the Potsdam Multiaperture Spectrophotometer (PMAS), in Proc. SPIE 2871, p. 1235.

    Google Scholar 

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Roth, M.M., Fechner, T., Wolter, D. et al. Ultra-Deep Optical Spectroscopy with PMAS. Using the Nod-and-Shuffle Technique. Experimental Astronomy 14, 99–105 (2002). https://doi.org/10.1023/B:EXPA.0000004352.56068.a8

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  • DOI: https://doi.org/10.1023/B:EXPA.0000004352.56068.a8

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