The Complete Spitzer Survey of Stellar Structure in Galaxies (CS${}^4$G)

Abstract

The Spitzer Survey of Stellar Structure in Galaxies (S${}^4$G), together with its Early Type Galaxy (ETG) extension, stand as the most extensive dataset of deep, uniform mid-infrared (mid-IR; 3.6 and 4.5$\mu$m) imaging for a sample of $2817$ nearby ($d<40$Mpc) galaxies. However, the velocity criterion used to select the original sample results in an additional 422 galaxies without HI detection that ought to have been included in the S${}^4$G on the basis of their optical recession velocities. In order to create a complete magnitude-, size- and volume-limited sample of nearby galaxies, we collect $3.6\mu$m and $i$-band images using archival data from different surveys and complement it with new observations for the missing galaxies. We denote the sample of these additional galaxies as Disc Galaxy (DG) extension. We present the Complete Spitzer Survey of Stellar Structure in Galaxies (CS${}^4$G), encompassing a sample of $3239$ galaxies with consistent imaging, surface brightness profiles, photometric parameters, and revised morphological classification. Following the original strategy of the S${}^4$G survey, we produce masks, surface brightness profiles, and curves of growth using masked $3.6\mu$m and $i$-band images. From these profiles, we derive the integrated quantities: total magnitude, stellar mass, concentration parameter, and galaxy size, converting to $3.6\mu$m. We re-measure these parameters also for the S${}^4$G and ETG to create a homogenous sample. We present new morphological revised $T$-types, and we showcase mid-IR scaling relations for the photometric parameters. We complete the S${}^4$G sample by incorporating 422 galaxies. The CS${}^4$G includes at least 99.94\% of the complete sample of nearby galaxies, meeting the original selection criteria, and it will enable a wide set of investigations into galaxy structure and evolution.

arXiv comment22 pages, 11 figures, 3 tables, 3 appendices. Accepted for publication in A&A

References in corpus (49)

• SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
• Array Programming with NumPy
• Astropy: A Community Python Package for Astronomy
• The Sloan Digital Sky Survey: Technical Summary
• Galactic Stellar and Substellar Initial Mass Function
• The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
• Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
• LSST: from Science Drivers to Reference Design and Anticipated Data Products
• The Infrared Array Camera (IRAC) for the Spitzer Space Telescope
• The Spitzer Space Telescope Mission
• The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
• Overview of the DESI Legacy Imaging Surveys
• The Photometric Performance and Calibration of the HST Advanced Camera For Surveys
• The Hyper Suprime-Cam SSP Survey: Overview and Survey Design
• The Dark Energy Camera
• The First Data Release of the Sloan Digital Sky Survey
• HyperLEDA. III. The catalogue of extragalactic distances
• Drizzle: A Method for the Linear Reconstruction of Undersampled Images
• The Spitzer Survey of Stellar Structure in Galaxies (S^4G)
• A Classical Morphological Analysis of Galaxies in the Spitzer Survey of Stellar Structure in Galaxies (S4G)
• The Dark Energy Survey Data Release 2
• Cosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density field
• Reconstructing the stellar mass distributions of galaxies using S4G IRAC 3.6 and 4.5 micron images: II. The conversion from light to mass
• The Spitzer Survey of Stellar Structure in Galaxies (S${}^4$G): Precise Stellar Mass Distributions from Automated Dust Correction at 3.6 microns
• The HI Mass Function of Galaxies from a Deep Survey in the 21cm Line
• Near-IR Atlas of S0-Sa galaxies (NIRS0S)
• Thick disks of edge-on galaxies seen through the Spitzer Survey of Stellar Structure in Galaxies (S4G): Lair of missing baryons?
• ARRAKIS: Atlas of Resonance Rings As Known In the S4G
• The DECam Local Volume Exploration Survey: Overview and First Data Release
• Galactic cirri in deep optical imaging
• The WISE Extended Source Catalogue (WXSC) I: The 100 Largest Galaxies
• Breaks in thin and thick discs of edge-on galaxies imaged in the Spitzer Survey of Stellar Structure in Galaxies (S4G)
• Old and young bulges in late-type disk galaxies
• Morphology and environment of galaxies with disc breaks in the S4G and NIRS0S
• The reports of thick discs' deaths are greatly exaggerated: thick discs are NOT artefacts caused by diffuse scattered light
• The shapes of spiral arms in the S${}^4$G survey and their connection with stellar bars
• Barlenses and X-shape features compared: different manifestations of Boxy/Peanut bulges
• Optical imaging for the Spitzer Survey of Stellar Structure in Galaxies. Data release and notes on interacting galaxies
• A Comprehensive Examination of the Optical Morphologies of 719 Isolated Galaxies in the AMIGA Sample
• Stellar masses, sizes, and radial profiles for 465 nearby early-type galaxies: an extension to the Spitzer Survey of Stellar Structure in Galaxies (S${}^4$G)
• Influence of galaxy stellar mass and observed wavelength on disc breaks in S${}^4$G, NIRS0S, and SDSS data
• On the varied origins of up-bending breaks in galaxy disks
• IRAC Near-Infrared Features in the Outer Parts of S4G Galaxies
• Best Practices for Data Publication in the Astronomical Literature
• The AMIGA sample of isolated galaxies. XIV. Disc breaks and interactions through ultra-deep optical imaging
• A Recipe for Unbiased Background Modeling in Deep Wide-Field Astronomical Images
• Testing for relics of past strong buckling events in edge-on galaxies: Simulation predictions and data from S${}^4$G
• MIGHTEE-\HI: Possible interactions with the galaxy NGC~895
• Fully Adaptive Bayesian Algorithm for Data Analysis, FABADA

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