scholarly journals Spectral classification of emission-line galaxies

1987 ◽  
Vol 63 ◽  
pp. 295 ◽  
Author(s):  
Sylvain Veilleux ◽  
Donald E. Osterbrock
2017 ◽  
Vol 843 (2) ◽  
pp. 130 ◽  
Author(s):  
Andrew S. Leung ◽  
Viviana Acquaviva ◽  
Eric Gawiser ◽  
Robin Ciardullo ◽  
Eiichiro Komatsu ◽  
...  

1979 ◽  
Vol 47 ◽  
pp. 151-153
Author(s):  
T. D. Kinman

Four methods for finding emission-line galaxies have been compared. Method (a) uses the ultraviolet excess, as found either by filter photography (Haro 1956) or by objective prism spectra (Markarian 1967). glanco (1974) introduced a thin prism with the CTIO Schmidt (1740 Å mm-1 at Hβ) which with IIIa-J plates [Method (b)] gave enough resolution for Smith (1975) and MacAlpine et al. (1977a, 1977b) to detect and classify galaxies by strong emission lines. Following a suggestion by McCarthy that even higher dispersion might be useful, I have used the CTIO Schmidt with [Method (c)] the 4° prism, a GGl+55 filter and IIIa-J emulsion and with [Method (d)] the 10° prism, an RG630 filter and IIIa-F emulsion. These latter give about 400 Å mm-1 at Hβ and Hα respectively which improves the visibility of emission lines against the galaxy continuum so that [0111] 5007 and 4959 and Hβ can be seen on the green plates and Hα and [SII] 6725 can be seen on the red plates.


2013 ◽  
Vol 437 (1) ◽  
pp. 968-975 ◽  
Author(s):  
Stefano Cavuoti ◽  
Massimo Brescia ◽  
Raffaele D'Abrusco ◽  
Giuseppe Longo ◽  
Maurizio Paolillo

2019 ◽  
Vol 485 (1) ◽  
pp. 1085-1102 ◽  
Author(s):  
Vasileios Stampoulis ◽  
David A van Dyk ◽  
Vinay L Kashyap ◽  
Andreas Zezas

2015 ◽  
Vol 451 (1) ◽  
pp. 629-633 ◽  
Author(s):  
Fei Shi ◽  
Yu-Yan Liu ◽  
Pei-Yu Li ◽  
Ming Yu ◽  
Yu-Ming Lei ◽  
...  

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