PMAS, the Potsdam Multi-Aperture Spectrophotometer. I. Design, Manufacture, and Performance
Abstract
We describe the design, manufacture, commissioning, and performance of PMAS, the Potsdam Multi-Aperture Spectrophotometer. PMAS is a dedicated integral field spectrophotometer, optimized to cover the optical wavelength regime of 0.35--1um. It is based on the lens array -- fiber bundle principle of operation. The instrument employs an all-refractive fiber spectrograph, built with CaF2 optics, to provide good transmission and high image quality over the entire nominal wavelength range. A set of user-selectable reflective gratings provides low to medium spectral resolution in first order of approx. 1.5, 3.2, and 7 A, depending on the groove density (1200, 600, 300 gr/mm). While the standard integral field unit (IFU) uses a 16x16 element lens array, which provides seeing-limited sampling in a relatively small field-of-view (FOV) in one of three magnifications (8x8, 12x12, or 16x16 arcsec^2, respectively), a recently retrofitted bare fiber bundle IFU (PPak) expands the FOV to a hexagonal area with a footprint of 65x74 arcsec^2. Other special features include a cryogenic CCD camera for field acquisition and guiding, a nod-shuffle mode for beam switching and improved sky background subtraction, and a scanning Fabry-Perot etalon in combination with the standard IFU (PYTHEAS mode). PMAS was initially designed and built as an experimental traveling instrument with optical interfaces to various telescopes (Calar Alto 3.5m, ESO-VLT, LBT). It is offered as a common user instrument at Calar Alto under contract with MPIA Heidelberg since 2002.
Cite
@article{arxiv.astro-ph/0502581,
title = {PMAS, the Potsdam Multi-Aperture Spectrophotometer. I. Design, Manufacture, and Performance},
author = {M. M. Roth and A. Kelz and T. Fechner and T. Hahn and S. -M. Bauer and T. Becker and P. Boehm and L. Christensen and F. Dionies and J. Paschke and E. Popow and D. Wolter and J. Schmoll and U. Laux and W. Altmann},
journal= {arXiv preprint arXiv:astro-ph/0502581},
year = {2009}
}
Comments
accepted for publication in PASP, 18 pages, 21 figures