2026-06-27T15:26:55Zhttps://docta.ucm.es/rest/oai/requestoai:docta.ucm.es:20.500.14352/598092023-08-28T09:30:15Zcom_20.500.14352_14col_20.500.14352_15
Docta Complutense
author
Alonso, O.
author
García Dabó, C. E.
author
Zamorano Calvo, Jaime
author
Gallego Maestro, Jesús
author
Rego Fernández, Manuel
2023-06-20T20:11:52Z
2023-06-20T20:11:52Z
1999-06
0067-0049
10.1086/313219
https://hdl.handle.net/20.500.14352/59809
http://dx.doi.org/10.1086/313219
http://iopscience.iop.org/
A new low-dispersion objective-prism search for low-redshift (z<0.045) emission-line galaxies (ELGs) has been carried out by the Universidad Complutense de Madrid using the Schmidt Telescope at the Calar-Alto Observatory. This is a continuation of the UCM Survey, which was performed by visual selection of candidates in photographic plates via the presence of the Hα+[N II] λ6584 blend in emission. In making this new list we have applied an automatic procedure, fully developed by us, for selecting and analyzing ELG candidates on the digitized images obtained with the Machine Automatique à Mesurer pour l'Astronomie (MAMA). The analyzed region of the sky covers 189 deg^2 in nine fields near α=14^h and 17^h, δ=25 ºC. The final sample contains 113 candidates. Special effort has been made to obtain a large amount of information directly from our uncalibrated plates by using several external calibrations. The parameters obtained for the ELG candidates allow us to study the statistical properties of the sample.
eng
Survey for emission-line galaxies: Universidad Complutense de Madrid list 3
journal article
URL
https://docta.ucm.es/bitstreams/ca646bb7-e025-458e-9c2b-4ccb6be6a3c9/download
File
MD5
c32a2220b21681c7ab935d52c24e7f06
13161724
application/pdf
jesusgallego101libre.pdf