KMTNet Nearby Galaxy Survey I. : Optimal strategy for low surface brightness imaging with KMTNet
arXiv:1810.02075 · doi:10.3847/1538-3881/aae647
Abstract
In hierarchical galaxy formation models, galaxies evolve through mergers and accretions. Tidally-disrupted debris from these processes can remain as diffuse, faint structures, which can provide useful insight into the assembly history of galaxies. To investigate the properties of the faint structures in outskirts of nearby galaxies, we conduct deep and wide-field imaging survey with KMTNet. We present our observing strategy and optimal data reduction process to recover the faint extended features in the imaging data of NGC 1291 taken with KMTNet. Through the dark sky flat-fielding and optimal sky subtraction, we can effectively remove inhomogeneous patterns. In the combined images, the peak-to-peak global sky gradients were reduced to less than % and % of the original - and -band sky levels, respectively. However, we find local spatial fluctuations in the background sky which can affect the precise measurement of the sky value. Consequently, we can reach the surface brightness of 29.5 and 28.5 mag arcsec in azimuthally averaged one-dimensional surface brightness profiles, that is mainly limited by the uncertainty in the sky determination. These results suggest that the deep imaging data produced by KMTNet are suitable to study the faint features of nearby galaxies such as outer disks and dwarf companions, but unideal (not impossible) to detect stellar halos. The one-dimensional profile revealed that NGC 1291 appeared to have Type I disk out to 30 kpc with no obvious color gradient and excess light due to a stellar halo was undetected.
8 pages, 10 figures, accepted to AJ
References in corpus (35)
- Tracing Galaxy Formation with Stellar Halos I: Methods
- Galactic stellar haloes in the CDM model
- Structure and Kinematics of the Stellar Halos and Thick Disks of the Milky Way Based on Calibration Stars from SDSS DR7
- A direct dynamical measurement of the Milky Way's disk surface density profile, disk scale length, and dark matter profile at 4 kpc < R < 9 kpc
- Tracing Galaxy Formation with Stellar Halos II: Relating Substructure in Phase- and Abundance-Space to Accretion Histories
- The Recent and Continuing Assembly of Field Ellipticals by Red Mergers
- Stellar Tidal Streams in Spiral Galaxies of the Local Volume: A Pilot Survey with Modest Aperture Telescopes
- A Search for Extended Ultraviolet Disk (XUV-disk) Galaxies in the Local Universe
- The Atlas3D project -- XXIX. The new look of early-type galaxies and surrounding fields disclosed by extremely deep optical images
- The structure of galactic disks: Studying late-type spiral galaxies using SDSS
- Hierarchical galaxy formation and substructure in the Galaxy's stellar halo
- The Frequency of Tidal Features Associated with Nearby Luminous Elliptical Galaxies from a Statistically Complete Sample
- The Galaxy and its stellar halo: insights on their formation from a hybrid cosmological approach
- The Luminosity Profile and Structural Parameters of the Andromeda Galaxy
- Color Profiles of Spiral Galaxies: Clues on Outer-Disk Formation Scenarios
- The Burrell Schmidt Deep Virgo Survey: Tidal Debris, Galaxy Halos, and Diffuse Intracluster Light in the Virgo Cluster
- Beyond 31 mag/arcsec^2: the low surface brightness frontier with the largest optical telescopes
- The Carnegie-Irvine Galaxy Survey. I. Overview and Atlas of Optical Images
- Halo Mass and Assembly History Exposed in the Faint Outskirts: the Stellar and Dark Matter Haloes of Illustris Galaxies
- The Dragonfly Nearby Galaxies Survey. I. Substantial variation in the diffuse stellar halos around spiral galaxies
- Diverse Stellar Haloes in Nearby Milky Way-Mass Disc Galaxies
- First results from the Dragonfly Telephoto Array: the apparent lack of a stellar halo in the massive spiral galaxy M101
- Faint Tidal Features in Galaxies within the Canada-France-Hawaii Telescope Legacy Survey Wide Fields
- Intracluster Planetary Nebulae in the Virgo Cluster III: Luminosity of the Intracluster Light and Tests of the Spatial Distribution
- The Extended Optical Disk of M101
- Post-merger Signatures of Red-sequence Galaxies in Rich Abell Clusters at
- Dwarf Galaxy Discoveries from the KMTNet Supernova Program I. The NGC 2784 Galaxy Group
- The Red and Featureless Outer Disks of Nearby Spiral Galaxies
- Dynamic S0 Galaxies II: the Role of Diffuse Hot Gas
- Deep Imaging of M51: a New View of the Whirlpool's Extended Tidal Debris
- Light-Element Abundances of Giant Stars in the Globular Cluster M71 (NGC 6838)
- Deep Surface Brightness Profiles of Spiral Galaxies from SDSS Stripe82: Touching Stellar Halos
- The Size and Shape of the Milky Way Disk and Halo from M-type Brown Dwarfs in the BoRG Survey
- A Comparison Between the Half-Light Radii, Luminosities, and UBV Colors of Globular Clusters in M31 and the Galaxy
- Cool Dust in the Outer Ring of NGC 1291
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- Census and classification of low-surface-brightness structures in nearby early-type galaxies from the MATLAS survey
- KMTNet Nearby Galaxy Survey II. Searching for Dwarf Galaxies in Deep and Wide-field Images of the NGC 1291 system
- Performance Assessment of the KASI-Deep Rolling Imaging Fast-optics Telescope pathfinder
- KMTNet Nearby Galaxy Survey III. Deficient H flux in the Extended Disks of Spiral Galaxies
- Age-Divided Mean Stellar Populations from Full Spectrum Fitting as the Simplified Star Formation and Chemical Evolution History of a Galaxy: Methodology and Reliability
- KMTNet Nearby Galaxy Survey: Overview and a Survey Description