Dictionary of Nomenclature of Celestial Objects

ion Line Object survey) is a deep emission-line survey which takes advantage of Tunable Filter (TF) facility of the intrument OSIRIS on GTC, an unique facility in 8-10m class telescopes.
The OTELO multi-wavelength catalogue contains N=11237 entries and is 50% complete at AB magnitude 26.38.
For more information, visit http://research.iac.es/proyecto/otelo
Ref:=2019A&A...631A...9B
byBONGIOVANNI A. , RAMON-PEREZ M., PEREZ GARCIA A.M., CEPA J., CERVINO M., NADOLNY J., PEREZ MARTINEZ R., ALFARO E., CASTANEDA H.O., DE DIEGO J.A., EDEROCLITE A., FERNANDEZ-LORENZO M., GALLEGO J., GONZALEZ J.J., GONZALEZ-SERRANO J.I., LARA-LOPEZ M.A., OTEO-GOMEZ I., PADILLA TORRES C.P., PINTOS-CASTRO I., POVIC M., SANCHEZ-PORTAL M., JONES H., BLAND-HAWTHORN J., CABRERA-LAVERS A.
 Astron. Astrophys., 631A, 9-9 (2019)
  The OTELO survey. I. Description, data reduction, and multi-wavelength catalogue.
o<OTELO NNNNN> N=9900 among (Nos 1-11237).
=E=Catalogue in electronic form as <J/A+A/631/A9/>

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