Figure 6 from THE SPITZER SURVEY OF STELLAR STRUCTURE IN GALAXIES (S4G): MULTI-COMPONENT DECOMPOSITION STRATEGIES AND DATA RELEASE

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 6.

Left panel the used P4 sky background estimates (SKY) in comparison to P3 (Muñoz-Mateos et al. 2015; their variable “SKY1”). The large apparent differences are due to use of different versions of P1 mosaics. Right panel we have corrected the P4 values to correspond to the final P1 mosaics (= those used in P3). Excluding the few deviant cases (discussed in the text) the median difference between P3 and P4 is 0.003 MJy sr⁻¹. Light and dark blue symbols indicate observations during cryogenic and warm Spitzer missions, respectively.

Other Images in This Article

Copyright and Terms & Conditions