Context. The upcoming new generation of optical spectrographs on four-meter-class telescopes will provide valuable opportunities for forthcoming galaxy surveys...
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PublicationWEAVE-StePS: A stellar population survey using WEAVE at WHT
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PublicationWeCAPP - Wendelstein Calar Alto pixellensing project I. Tracing dark and bright matter in M 31
We present WeCAPP, a long term monitoring project searching for microlensing events towards M 31. Since 1997 the bulge of M 31 was monitored in two different...
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PublicationWeCAPP Survey. M31 variables (Fliri+, 2006)
Observations of M31 were obtained using the 0.8-m telescope at Wendelstein, Germany and the 1.2-m telescope at Calar Alto, Spain, over three observing seasons...
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PublicationWelcome to the Twilight Zone: The Mid-infrared Properties of Post-starburst Galaxies
We investigate the optical and Wide-field Survey Explorer (WISE) colors of “E+A” identified post-starburst galaxies, including a deep analysis of 190 post...
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PublicationWHaD diagram: Classifying the ionizing source with one single emission line
Context. The usual approach to classify the ionizing source using optical spectroscopy is based on the use of diagnostic diagrams that compare the relative...
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PublicationWhat boost galaxy mergers in two massive galaxy protoclusters at z = 2.24?
Characterizing the structural properties of galaxies in high-redshift protoclusters is key to our understanding of the environmental effects on galaxy evolution...
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PublicationWhat do galaxies look like beyond 31 mag/arcsec2?
Detection of optical surface brightness structures with magnitudes fainter than 30 mag/arcsec2 has remained elusive in current photometric deep surveys. We are...
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PublicationWhat do Simulations Predict for the Galaxy Stellar Mass Function and its Evolution in Different Environments?
We present a comparison between the observed galaxy stellar mass function and the one predicted from the De Lucia & Blaizot semi-analytic model applied to the...
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PublicationWhat drives the variance of galaxy spectra?
We present a study aimed at understanding the physical phenomena underlying the formation and evolution of galaxies following a data-driven analysis of...