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26 April 2024
 
  » arxiv » 0803.1176

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Continuum subtracting Lyman-alpha images: Low redshift studies using the Solar Blind Channel of HST/ACS
Matthew Hayes ; Goran Ostlin ; J. Miguel Mas-Hesse ; Daniel Kunth ;
Date 7 Mar 2008
Abstract(Abridged) We are undertaking an imaging study of local star-forming galaxies in the Lyman-alpha (Lya) emission line using the Solar Blind Channel (SBC) of the ACS onboard HST. Observations have been obtained in Lya and H-alpha and six line-free continuum filters between ~1500 AA and the I-band. In a previous article Hayes et al. (2005) we demonstrated that the production of Lya line-only images (i.e. continuum subtraction) in the SBC-only data-set is non-trivial and that supporting data is a requirement. We here develop various methods of continuum subtraction and assess their relative performance for given input spectral energy distributions (SED). We show that simple assumptions about the behavior of the UV continuum consistently lead to results that are significantly in error, and determine that a spectral fitting approach is essential. Furthermore, fitting of a single component stellar or stellar+nebular spectrum is not always sufficient for realistic template SEDs and, in order to successfully recover the input observables, care must be taken to control the contribution of nebular gas and any underlying stellar population. Independent measurements of the metallicity must first be obtained, while details of the initial mass function play only a small role. We identify the need to bin together pixels to obtain signal--to--noise (S/N) ratios of around 10 in each band before processing. At S/N=10 we are able to recover Lya fluxes accurate to within ~30% for Lya lines with intrinsic equivalent width W(Lya) of 10AA. This accuracy improves to <~10% for W(Lya)=100 AA. We describe the image processing applied to the observations presented in "Ostlin et al. (2008) and the associated data-release. We also present simulations for an observing strategy for a future low-z Lya imaging campaign using ACS/SBC.
Source arXiv, 0803.1176
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