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The IAC Stripe82 Legacy Survey: improved sky-rectified images

Astrophysics of Galaxies 2018-08-09 v1

Abstract

The IAC Stripe 82 Legacy Survey is a new co-addition of the SDSS Stripe 82 data (Abazajian et al. 2009), especially reduced to preserve the faintest surface brightness features of this data set. The survey maps a 2.5 degree wide stripe along the Celestial Equator in the Southern Galactic Cap (-50^{\circ} << R.A. << 60^{\circ}, -1.25^{\circ} << Dec.<< 1.25^{\circ}) with a total of 275 square degrees in all the five SDSS filters (u,g,r,i,z). The new reduction includes an additional and deeper band (rdeep), which is a combination of g, r and i bands. The average seeing of the Stripe82 dataset is around 1 arcsec. The mean surface brightness limits are μlim\mu_{lim}[3σ\sigma,10×\times10 arcsec2^{2}] = 27.9, 29.1, 28.6, 28.1 and 26.7 mag arcsec2^{-2} for the u, g, r, i and z bands respectively. The significant depth of the data and the emphasis on preserving the characteristics of the background (sky + diffuse light) through a non-aggressive sky subtraction strategy make this dataset suitable for the study of the low surface brightness Universe. In this research note we present a new data release with improved sky-rectified images. This new data-set is published on the survey webpage and is publicly available for the community.

Keywords

Cite

@article{arxiv.1808.02499,
  title  = {The IAC Stripe82 Legacy Survey: improved sky-rectified images},
  author = {Javier Román and Ignacio Trujillo},
  journal= {arXiv preprint arXiv:1808.02499},
  year   = {2018}
}

Comments

Accepted for publication in the Research Notes of the AAS (RNAAS)