Multi-wavelength study of 14 000 star-forming galaxies from the Sloan Digital Sky Survey

Y. I. Izotov; N. G. Guseva; K. J. Fricke; C. Henkel

doi:10.1051/0004-6361/201322338

Free Access

Issue		A&A Volume 561, January 2014


Article Number		A33
Number of page(s)		30
Section		Extragalactic astronomy
DOI		https://doi.org/10.1051/0004-6361/201322338
Published online		20 December 2013

Online material

Table 2

Observed parameters of the galaxies.

Table 3

Derived parameters of the galaxies.

	Fig. 10 20′′ × 20′′ SDSS composite g,r,i images of galaxies with m(3.4 μm)−m(4.6 μm) ≥ 2 mag.
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	Fig. 11 20′′ × 20′′ SDSS composite g,r,i images of galaxies with 2 mag >m(3.4 μm)−m(4.6 μm) ≥ 1.5 mag.
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	Fig. 12 20′′ × 20′′ SDSS composite g,r,i images of ten representative galaxies with m(3.4 μm)−m(4.6 μm) < 0.5 mag.
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Fig. 13

Spectral energy distributions galaxies with m(3.4 μm)−m(4.6 μm) ≥ 2 mag. Observed SDSS optical spectra are shown by black solid lines; observed GALEX, SDSS and WISE monochromatic fluxes are shown by filled red circles. The WISE data are connected by a red solid line. The modelled SED shown by the blue line is a sum of stellar emission (green line) and ionised gas emission (magenta line).

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	Fig. 14 Same as in Fig. 13 but for galaxies with 2 mag >m(3.4 μm)−m(4.6 μm) ≥ 1.5 mag.
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	Fig. 15 Same as in Fig. 13 but for galaxies with m(3.4 μm)−m(4.6 μm) < 0.5 mag.
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© ESO, 2013

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