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Small-scale Intensity Mapping: Extended Lyα, Hα, and Continuum Emission as a Probe of Halo Star Formation in High-redshift Galaxies

  • Authors: Lluís Mas-Ribas, Mark Dijkstra, Joseph F. Hennawi, Michele Trenti, Rieko Momose, and Masami Ouchi

2017 The Astrophysical Journal 841 19.

  • Provider: AAS Journals

Caption: Figure 7.

Distribution of luminosities for satellite sources in the range ﹩10\leqslant r\leqslant 160\,\mathrm{pkpc}﹩ from the central LAE, using the parameters in Table 1 and our fiducial clustering model. The left panel represents the distribution of Lyα luminosities and the right panel those of UV magnitudes. Every panel quotes the average number of galaxies obtained from Equation (10). Both panels indicate the presence of a few sources close to the observational thresholds, and a larger number of significantly fainter objects.

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