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The ATLAS^(3D) project – XXIX. The new look of early-type galaxies and surrounding fields disclosed by extremely deep optical images
- Source :
- Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, 2015, 446, pp.120-143. ⟨10.1093/mnras/stu2019⟩, Monthly Notices of the Royal Astronomical Society, 446(1), 120-143. Oxford University Press
- Publication Year :
- 2015
- Publisher :
- Royal Astronomical Society, 2015.
-
Abstract
- Galactic archeology based on star counts is instrumental to reconstruct the past mass assembly of Local Group galaxies. The development of new observing techniques and data-reduction, coupled with the use of sensitive large field of view cameras, now allows us to pursue this technique in more distant galaxies exploiting their diffuse low surface brightness (LSB) light. As part of the Atlas3D project, we have obtained with the MegaCam camera at the Canada-France Hawaii Telescope extremely deep, multi--band, images of nearby early-type galaxies. We present here a catalog of 92 galaxies from the Atlas3D sample, that are located in low to medium density environments. The observing strategy and data reduction pipeline, that achieve a gain of several magnitudes in the limiting surface brightness with respect to classical imaging surveys, are presented. The size and depth of the survey is compared to other recent deep imaging projects. The paper highlights the capability of LSB--optimized surveys at detecting new prominent structures that change the apparent morphology of galaxies. The intrinsic limitations of deep imaging observations are also discussed, among those, the contamination of the stellar halos of galaxies by extended ghost reflections, and the cirrus emission from Galactic dust. The detection and systematic census of fine structures that trace the present and past mass assembly of ETGs is one of the prime goals of the project. We provide specific examples of each type of observed structures -- tidal tails, stellar streams and shells --, and explain how they were identified and classified. We give an overview of the initial results. The detailed statistical analysis will be presented in future papers.<br />Comment: MNRAS in press, On-line version of the catalog of galaxies with available deep images and figures (including navigation tools) are available from http://irfu.cea.fr/Projets/matlas/public/Atlas3D/atlas3d-pXXIX.html
- Subjects :
- FOS: Physical sciences
interactions [Galaxies]
Astrophysics
Star count
Astrophysics::Cosmology and Extragalactic Astrophysics
elliptical and lenticular, cD [Galaxies]
01 natural sciences
law.invention
cD
Telescope
techniques: photometric
law
0103 physical sciences
galaxies: interactions
QB Astronomy
Surface brightness
galaxies: elliptical and lenticular
010303 astronomy & astrophysics
QC
Astrophysics::Galaxy Astrophysics
QB
Dwarf galaxy
Luminous infrared galaxy
Physics
010308 nuclear & particles physics
Star formation
photometry [Galaxies]
photometric [Techniques]
Astronomy
Local Group
Astronomy and Astrophysics
3rd-DAS
Astrophysics - Astrophysics of Galaxies
Galaxy
galaxies: photometry
QC Physics
Space and Planetary Science
Astrophysics of Galaxies (astro-ph.GA)
galaxies: stellar content
stellar content [Galaxies]
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Subjects
Details
- Language :
- English
- ISSN :
- 00358711 and 13652966
- Database :
- OpenAIRE
- Journal :
- Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, 2015, 446, pp.120-143. ⟨10.1093/mnras/stu2019⟩, Monthly Notices of the Royal Astronomical Society, 446(1), 120-143. Oxford University Press
- Accession number :
- edsair.doi.dedup.....729616cb4a8102b40d7c0bc5d1748d7a