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- W3106270854 abstract "We report the $4 , sigma$ detection of a faint object with a flux of ~ 0.3 mJy, in the vicinity of the quadruply lensed QSO MG0414+0534 using the Atacama Large Millimeter/submillimeter array (ALMA) Band 7. The object is most probably a dusty dark dwarf galaxy, which has not been detected in either the optical, near-infrared (NIR) or radio (cm) bands. An anomaly in the flux ratio of the lensed images observed in Band 7 and the mid-infrared (MIR) band and the reddening of the QSO light color can be simultaneously explained if we consider the object as a lensing substructure with an ellipticity ~ 0.7 at a redshift of $0.5 lesssim z lesssim 1$. Using the best-fit lens models with three lenses, we find that the dark matter plus baryon mass associated with the object is $sim 10^9, M_{odot}$, the dust mass is $sim 10^7,M_{odot}$ and the linear size is $gtrsim 5,$kpc. Thus our findings suggest that the object is a dusty dark dwarf galaxy. A substantial portion of faint submillimeter galaxies (SMGs) in the universe may be attributed to such dark objects." @default.
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- W3106270854 date "2017-01-30" @default.
- W3106270854 modified "2023-10-16" @default.
- W3106270854 title "Evidence for a Dusty Dark Dwarf Galaxy in the Quadruple Lens MG 0414+0534" @default.
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- W3106270854 doi "https://doi.org/10.3847/2041-8213/835/2/l23" @default.
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