As part of a systematic effort to characterize the properties and progenitors of the most luminous planetary nebulae (PNe), we obtained a sample among the...
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PublicaciónThe origin of the most luminous Planetary Nebulae
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PublicaciónThe Origin of the Relation between Metallicity and Size in Star-forming Galaxies
For the same stellar mass, physically smaller star-forming galaxies are also metal richer. What causes the relation remains unclear. The central star-forming...
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PublicaciónThe Origins of Planetary Nebulae in the Inner and Outer Disks of M 31
The planetary nebulae (PNe) of M 31 are receiving considerable attention as probes of its structure and chemical evolution in a galactic environment that is...
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PublicaciónThe origins of post-starburst galaxies at z < 0.05
Post-starburst galaxies can be identified via the presence of prominent Hydrogen Balmer absorption lines in their spectra. We present a comprehensive study of...
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PublicaciónThe OTELO Project
OTELO, (OSIRIS Tunable Emission Line Object Survey), will survey emission line objects using OSIRIS tunable filters in selected atmospheric windows relatively...
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PublicaciónThe OTELO Project
The OTELO Project is an extragalactic survey under way using the tunable filters of the instrument OSIRIS at the GTC. OTELO is already providing the deepest...
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PublicaciónThe OTELO Project
OSIRIS is the Spanish Day One instrument for the GTC 10.4-m telescope. OSIRIS is a general purpose instrument for imaging, low-resolution long slit and multi...
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PublicaciónThe OTELO survey as a morphological probe. Last ten Gyr of galaxy evolution. The mass-size relation up to z = 2
Context. The morphology of galaxies provide us with a unique tool for relating and understanding other physical properties and their changes over the course of...
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PublicaciónThe OTELO survey. A case study of [O III] λ4959,5007 emitters at ⟨z⟩ = 0.83
Context. The OSIRIS Tunable Filter Emission Line Object (OTELO) survey is a very deep, blind exploration of a selected region of the Extended Groth Strip and is...