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A simple non-parametric method for resolving merged doublet lines
Doublet line emission and absorption are common in astronomical sources (e.g. [OIII], [O II], NaD, MgII). In many cases, complex kinematics in the emitting source can cause the doublet lines to merge, making characterization...
A simple non-parametric method for resolving merged doublet lines
Doublet line emission and absorption are common in astronomical sources (e.g. [OIII], [O II], NaD, MgII). In many cases, complex kinematics in the emitting source can cause the doublet lines to merge, making characterization...
The VIMOS Ultra Deep Survey
L Guaita, M Talia, L Pentericci, A Verhamme, P Cassata, BC Lemaux, I Orlitova, B Ribeiro, D Schaerer, G Zamorani, B Garilli, V Le Brun, O Le Fèvre, D Maccagni, LAM Tasca, R Thomas, E Vanzella, E Zucca, R Amorin, S Bardelli, M Castellano, A Grazian, NP Hathi, A Koekemoer, F Marchi
Dec 01, 2017