Fig. 5: MUSE Spectrum of W0410-0913. | Nature Communications

Fig. 5: MUSE Spectrum of W0410-0913.

From: Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913

Fig. 5

a We show a spectrum of W0410-0913, covering the full MUSE wavelength domain, extracted from a circular aperture with a 1-radius. Vertical red lines are located at the expected position of several rest-frame UV lines, according to its redshift (as traced by the rest-frame FIR lines). A sigma-clipping procedure was performed to remove the residuals of sky-lines and make the visualization easier. Nvλ 1240 and Civλλ 1548,1550 show very broad line-profiles (FWHM~2800 km s−1) and large blueshifts (−2000 km s−1) with respect to W0410-0913, indicative of fast nuclear outflows. A narrow Lyman-α line (FWHM~400 km s−1) is detected with an offset of ~−1460 km s−1 from the systemic redshift. b We show a zoom of the spectrum at wavelengths closer to the expected Lyman-α line.

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