Recent developments of the ACS spectral extraction software aXe
Abstract
The software package aXe provides comprehensive spectral extraction facilities for all the slitless modes of the ACS, covering the Wide Field Channel (WFC) grism, the High Resolution Channel (HRC) grism and prism and the Solar Blind Channel (SBC) prisms. The latest developments to the package apply to all ACS slitless modes leading to improved spectral extraction. Many thousands of spectra may be present on a single deep ACS WFC G800L image such that overlap of spectra is a significant nuisance. Two methods of estimating the contamination of any given spectrum by its near neighbours have been developed: one is based on the catalogue of objects on the direct image; another uses the flux information on multi-filter direct images. An improvement to the extracted spectra can also result from weighted extraction and the Horne optimal extraction algorithm has been implemented in aXe. A demonstrated improvement in signal-to-noise can be achieved. These new features are available in aXe-1.5 with the STSDAS 3.4 release.
Cite
@article{arxiv.astro-ph/0512100,
title = {Recent developments of the ACS spectral extraction software aXe},
author = {J. R. Walsh and M. Kuemmel and S. S. Larsen},
journal= {arXiv preprint arXiv:astro-ph/0512100},
year = {2007}
}
Comments
6 pages, incl. 4 figures. To appear in the proceedings of the 2005 HST Calibration Workshop, STScI, 2005 (eds. A. Koekemoer, P. Goudfrooij and L. Dressel)