It is now clear that supermassive black holes (M>1e6 Msun) live in the center of most (all) galaxies, including our own Milky Way. Furthermore, the energy...
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CharlaThe Cosmic History of Black Hole Growth
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CharlaThe dark and bright sides of massive early-type galaxies
Massive early-type galaxies constitute an ideal test bed to probe our understanding of galaxy formation and evolution. Their high mass, spheroidal morphology...
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CharlaThe Dark Energy Spectroscopic Instrument (DESI)
DESI is a massively multiplexed fiber-fed spectrograph that will make the nextmajor advance in dark energy in the timeframe 2018-2022. On the Mayalltelescope...
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PublicaciónThe EDGE-CALIFA Survey: An Extragalactic Database for Galaxy Evolution Studies
The EDGE-CALIFA survey provides spatially resolved optical integral-field unit and CO spectroscopy for 125 galaxies selected from the Calar Alto Legacy Integral...
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CharlaThe epoch of formation of galaxy disks using extragalactic rings
The Time Inference with MUSE in Extragalactic Rings, TIMER, is a project dedicated to study the central regionsof 24 nearby galaxies with the integral field...
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PublicaciónThe Evolution of AGN Activity in Brightest Cluster Galaxies
We present the results of an analysis of Wide-field Infrared Survey Explorer (WISE) observations of the full 2500 deg 2 South Pole Telescope (SPT)-Sunyaev-Zel...
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CharlaThe evolution of galaxies during the first billion years.
Evolution of galaxies is relatively well known up to z ~ 5, but beyond this limit and regarding the few number of galaxies confirmed by spectroscopy, their...
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CharlaThe Evolution of quiescent galaxies at high-z: towards the high-mass end of the GSMF
In this talk we will show the evolution of high-redshift (z≥ 1.4) quiescent galaxies in the COSMOS field. We have studied an IRAC (mag 3.6 μm < 22.0) selected...
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CharlaThe Extragalactic Background Light: Connecting Classical and High Energy Astronomy
The extragalactic background light (EBL) is the second most energetic diffuse background that fills our Universe. It is produced by star formation processes and...