Now showing items 1-4 of 4

    • ARRAKIS: atlas of resonance rings as known in the S⁴G 

      Comerón, Sébastien; Salo, Heikki J.; Laurikainen, Eija; Knapen, Johan H.; Buta, Ronald J.; Herrera-Endoqui, M.; Laine, Jarkko; Holwerda, Benne Willem; Sheth, Kartik; Mizusawa, Trisha (2014-02)
      Context. Resonance rings and pseudorings (here collectively called rings) are thought to be related to the gathering of material near dynamical resonances caused by non-axisymmetries in galaxy discs. This means that they ...
    • Morphology and environment of galaxies with disc breaks in the S4G and NIRS0S 

      Mizusawa, Trisha F.; Laine, Jarkko; Laurikainen, Eija; Salo, Heikki J.; Comerón, Sébastien; Buta, Ronald J.; Zaritsky, Dennis; Athanassoula, E.; Bosma, Albert; Muñoz-Mateos, Juan Carlos (2014-05-15)
      We study the surface brightness profiles of disc galaxies in the 3.6 μm images from the Spitzer Survey of Stellar Structure in Galaxies (S4G) and Ks-band images from the Near-Infrared S0-Sa galaxy Survey (NIRS0S).We ...
    • THE SPITZER SURVEY of STELLAR STRUCTURE in GALAXIES (S4G): MULTI-COMPONENT DECOMPOSITION STRATEGIES and DATA RELEASE 

      Salo, Heikki J.; Laurikainen, Eija; Laine, Jarkko; Comerón, Sébastien; Gadotti, Dimitri Alexei; Buta, Ronald J.; Sheth, Kartik; Zaritsky, Dennis; Ho, Luis; Mizusawa, Trisha (2015-07-20)
      The Spitzer Survey of Stellar Structure in Galaxies (S4G) is a deep 3.6 and 4.5 μm imaging survey of 2352 nearby (<40 Mpc) galaxies. We describe the S4G data analysis pipeline 4, which is dedicated to two-dimensional ...
    • THE SPITZER SURVEY of STELLAR STRUCTURE in GALAXIES (S4G): STELLAR MASSES, SIZES, and RADIAL PROFILES for 2352 NEARBY GALAXIES 

      Muñoz-Mateos, Juan Carlos; Sheth, Kartik; Regan, Michael W.; Kim, Taehyun; Laine, Jarkko; Ferrer, Santiago Erroz; Paz, Armando Gil De; Comerón, Sébastien; Hinz, Joannah L.; Mizusawa, Trisha (2015-07-20)
      The Spitzer Survey of Stellar Structure in Galaxies is a volume, magnitude, and size-limited survey of 2352 nearby galaxies with deep imaging at 3.6 and 4.5 μm. In this paper, we describe our surface photometry pipeline ...