Evolución de galaxias
Evolucion
Niels Bohr Institute
Copenaguen, DinamarcaNiels Bohr Institute-ko ikertzaileekin lankidetzan egindako argitalpenak (11)
2021
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The OTELO survey: Faint end of the luminosity function of [O II]3727 emitters at ⟨ z »= 1.43
Astronomy and Astrophysics, Vol. 649
2020
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Erratum: The OTELO survey: A case study of [O III] λ 4959,5007 emitters at z »= 0.83 (Astronomy and Astrophysics (2020) 635 (A35) DOI: 10.1051/0004-6361/201833656)
Astronomy and Astrophysics
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Galaxy classification: Deep learning on the OTELO and COSMOS databases
Astronomy and Astrophysics, Vol. 638
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The OTELO survey: A case study of [O III] λ 4959,5007 emitters at λ z »= 0.83
Astronomy and Astrophysics, Vol. 635
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The OTELO survey: Nature and mass-metallicity relation for H α emitters at z ∼0.4
Astronomy and Astrophysics, Vol. 636
2019
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The OTELO survey: I. Description, data reduction, and multi-wavelength catalogue
Astronomy and Astrophysics, Vol. 631
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The OTELO survey: II. The faint-end of the Hα luminosity function at z ∼ 0.40
Astronomy and Astrophysics, Vol. 631
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The OTELO survey: III. Demography, morphology, IR luminosity and environment of AGN hosts
Astronomy and Astrophysics, Vol. 631
2013
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OSIRIS Ha imaging of the NGC 2770 supernova factory and its satellite NGC 2770B
Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
2012
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SDSS galaxies with double-peaked emission lines: Double starbursts or active galactic nuclei?
Monthly Notices of the Royal Astronomical Society, Vol. 419, Núm. 1, pp. 490-502
2011
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Study of the NGC 2770 interstellar medium through H α , millimetric and optical polarimetric data of SN 2008D and SN 2007uy
Advances in Space Research, Vol. 47, Núm. 8, pp. 1421-1426