The Spitzer Survey of Stellar Structure in Galaxies (S(4)G) is a deep 3.6 and 4.5 mu m imaging survey of 2352 nearby (<40 Mpc) galaxies. We describe the S(4)G data analysis pipeline 4, which is dedicated to two-dimensional structural surface brightness decompositions of 3.6 mu m images, using GALFIT3.0. Besides automatic 1-component Sersic fits, and 2-component Sersic bulge + exponential disk fits, we present human-supervised multi-component decompositions, which include, when judged appropriate, a central point source, bulge, disk, and bar components. Comparison of the fitted parameters indicates that multi-component models are needed to obtain reliable estimates for the bulge Sersic index and bulge-to-total light ratio (B/T), confirming e...
With the availability of large integral field unit (IFU) spectral surveys of nearby galaxies, there ...
With the availability of large integral field unit (IFU) spectral surveys of nearby galaxies, there ...
Bulge–disc decomposition is a valuable tool for understanding galaxies. However, achieving robust me...
The Spitzer Survey of Stellar Structure in Galaxies (S(4)G) is a deep 3.6 and 4.5 mu m imaging surve...
The Spitzer Survey of Stellar Structure in Galaxies (S^4G) is a deep 3.6 and 4.5 μm imaging survey o...
The Spitzer Survey of Stellar Structure in Galaxies (S^4G) is a deep 3.6 and 4.5 μm imaging survey o...
The Spitzer Survey of Stellar Structure in Galaxies (S(4)G) is a deep 3.6 and 4.5 mu m imaging surve...
International audienceThe Spitzer Survey of Stellar Structure in Galaxies (S(4)G) is a deep 3.6 and ...
The Spitzer Survey of Stellar Structure in Galaxies is a volume, magnitude, and size-limited survey ...
The Spitzer Survey of Stellar Structure in Galaxies is a volume, magnitude, and size-limited survey ...
To ascertain whether photometric decompositions of galaxies into bulges and discs are astrophysicall...
The Spitzer Survey of Stellar Structure in Galaxies ( 4 G ) is an Exploration Science Legacy Program...
The Spitzer Survey of Stellar Structure in Galaxies (S^4G) is an Exploration Science Legacy Program ...
The Spitzer Survey of Stellar Structure in Galaxies (S(4)G) is an Exploration Science Legacy Program...
The Spitzer Survey of Stellar Structure in Galaxies is a volume, magnitude, and size-limited survey ...
With the availability of large integral field unit (IFU) spectral surveys of nearby galaxies, there ...
With the availability of large integral field unit (IFU) spectral surveys of nearby galaxies, there ...
Bulge–disc decomposition is a valuable tool for understanding galaxies. However, achieving robust me...
The Spitzer Survey of Stellar Structure in Galaxies (S(4)G) is a deep 3.6 and 4.5 mu m imaging surve...
The Spitzer Survey of Stellar Structure in Galaxies (S^4G) is a deep 3.6 and 4.5 μm imaging survey o...
The Spitzer Survey of Stellar Structure in Galaxies (S^4G) is a deep 3.6 and 4.5 μm imaging survey o...
The Spitzer Survey of Stellar Structure in Galaxies (S(4)G) is a deep 3.6 and 4.5 mu m imaging surve...
International audienceThe Spitzer Survey of Stellar Structure in Galaxies (S(4)G) is a deep 3.6 and ...
The Spitzer Survey of Stellar Structure in Galaxies is a volume, magnitude, and size-limited survey ...
The Spitzer Survey of Stellar Structure in Galaxies is a volume, magnitude, and size-limited survey ...
To ascertain whether photometric decompositions of galaxies into bulges and discs are astrophysicall...
The Spitzer Survey of Stellar Structure in Galaxies ( 4 G ) is an Exploration Science Legacy Program...
The Spitzer Survey of Stellar Structure in Galaxies (S^4G) is an Exploration Science Legacy Program ...
The Spitzer Survey of Stellar Structure in Galaxies (S(4)G) is an Exploration Science Legacy Program...
The Spitzer Survey of Stellar Structure in Galaxies is a volume, magnitude, and size-limited survey ...
With the availability of large integral field unit (IFU) spectral surveys of nearby galaxies, there ...
With the availability of large integral field unit (IFU) spectral surveys of nearby galaxies, there ...
Bulge–disc decomposition is a valuable tool for understanding galaxies. However, achieving robust me...