Identifications and SEDs of the detected sources from the AKARI Deep Field South
K. Malek, A. Pollo, M. Shirahata, S. Matsuura, M. Kawada, T.T., Takeuchi

TL;DR
This paper identifies counterparts of sources in the AKARI Deep Field South across multiple wavelengths and constructs spectral energy distributions for key sources, enhancing understanding of their properties.
Contribution
It provides the first spectral energy distributions for selected sources in the AKARI Deep Field South, integrating multi-wavelength data with AKARI measurements.
Findings
114 sources with possible counterparts identified
78 known galaxies among the counterparts
Constructed SEDs for the most secure sources
Abstract
In order to find counterparts of the detected objects in the AKARI Deep Field South (ADFS) in all available wavelengths, we searched public databases (NED, SIMBAD and others). Checking 500 sources brighter than 0.0482 Jy in the AKARI Wide-S band, we found 114 sources with possible counterparts, among which 78 were known galaxies. We present these sources as well as our first attempt to construct spectral energy distributions (SEDs) for the most secure and most interesting sources among them, taking into account all the known data together with the AKARI measurements in four bands.
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Taxonomy
TopicsAstronomy and Astrophysical Research · Gamma-ray bursts and supernovae · Astronomical Observations and Instrumentation
