WebNov 16, 2016 · [Submitted on 16 Nov 2016 , last revised 2 Aug 2024 (this version, v2)] Title: Galaxy clustering dependence on the $\left[\mathrm{O\scriptsize{II}}\right]$ emission line luminosity in the local Universe. Authors: Ginevra Favole, Sergio A. Rodríguez-Torres, Johan Comparat, ... WebWe found an unprecedented linear correlation between the pc-scale core luminosity (∼10 21.3 –10 23.6 W Hz − 1) and [O III] line luminosity, generally considered as proxy of the accretion power, for a large sample of LINER-type radio-loud low-luminosity active nuclei, all hosted in massive ETGs, which include FR 0s and FR Is. This result ...
The [O iii] emission line luminosity function of optically selected ...
WebThis line can also be used to measure the systemic redshift of the galaxies (e.g. Pentericci et al. 2016). In addition, the [CII]-line ALMA surveys will derive the line luminosity functions, thus measuring the abundance and intensity distributions of [CII] emitters (Aravena et al. 2016). WebSep 26, 2024 · to modeling line luminosity functions, several techniques to separate the desired signal from foregrounds, ... Starting in early 2016, the line-intensity mapping … brackley body shop
[1611.05457] Galaxy clustering dependence on the …
WebSep 26, 2024 · Finally, we describe recent theoretical advances: different approaches to modeling line luminosity functions, several techniques to separate the desired signal … WebNov 9, 2016 · We calculated the completeness as a function of [CII] line luminosity and distance, based on the far-IR color and flux densities. The [CII] luminosity function is … WebApr 3, 2024 · We detect a prominent H α emission line (L H ... {-1}}$ H α emission line with comparable line luminosity as ASASSN-18tb, emphasizing the rarity of such emission in the nebular phase. Based on preliminary results from our survey, ... (Inserra et al. 2016), and infrared observations should be sought to construct a late-time light curve ... h2 inheritor\u0027s