Figure 5 from THE SPITZER SURVEY OF STELLAR STRUCTURE IN GALAXIES (S4G): MULTI-COMPONENT DECOMPOSITION STRATEGIES AND DATA RELEASE

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THE SPITZER SURVEY OF STELLAR STRUCTURE IN GALAXIES (S⁴G): MULTI-COMPONENT DECOMPOSITION STRATEGIES AND DATA RELEASE

Authors: Heikki Salo, Eija Laurikainen, Jarkko Laine, Sebastien Comerón, Dimitri A. Gadotti, Ron Buta, Kartik Sheth, Dennis Zaritsky, Luis Ho, Johan Knapen , E. Athannassoula, Albert Bosma, Seppo Laine, Mauricio Cisternas, Taehyun Kim, Juan Carlos Muñoz-Mateos, Michael Regan, Joannah L. Hinz, Armando Gil de Paz, Karin Menendez-Delmestre, Trisha Mizusawa, Santiago Erroz-Ferrer, Sharon E. Meidt, and Miguel Querejeta

2015 The Astrophysical Journal Supplement Series 219 4.

Provider: AAS Journals

Caption: Figure 5.

Distribution of axial ratios, calculated with P4 (a), HyperLeda (b), and P3 orientation parameters. Hubble types ﹩T\leqslant -4﹩ and ﹩T\gt 10﹩ are excluded (using Buta et al. 2014 mid-IR classification). Dashed line indicates the whole S⁴G sample, with the magnitude selection ﹩{\mathrm{BT}}_{\mathrm{corr}}\lt 15.5﹩, where BT_corr is the inclination-corrected blue magnitude from HyperLeda. Solid line corresponds to a similar limit, but using non-corrected blue magnitude BT. To ease the comparison the P4 histogram for ﹩\mathrm{BT}\lt 15﹩ is shown as the shaded region in each frame.

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