activity
20092026
most citedStar formation of far-IR AGN and non-AGN galaxies in the green valley: possible implication of AGN positive feedback

54 citations · 378 across the 28 of their papers we have counts for

collaborators

28 papers

astro-ph.GA2026

The OTELO Survey: The main sequence of low-mass galaxies

Bernabé Cedrés, Jordi Cepa, Carmen P. Padilla--Torres +15

This paper describes the relationship between the star formation rate and the stellar mass, the so-called main sequence (MS), of low-mass galaxies at three different redshifts from…

astro-ph.GA2025

Dynamically close galaxy pairs from the unWISE survey: Testing the merger-AGN-star formation connection

Josephine Chishala, Roberto De Propris, Mirjana Pović

Galaxy mergers are expected to have a profound influence on the star formation histories of galaxies. It is generally expected that mergers are the main drivers of galaxy mass grow…

astro-ph.GA2025★ 1 cited

GLACE survey: OSIRIS/GTC multi-object spectroscopy of the rich galaxy cluster ZwCl 0024.0+1652 at z~0.4. III. The mass-SFR relation and the quenching of cluster galaxies

Simon B. De Daniloff, Ángel Bongiovanni, Miguel Sánchez-Portal +21

Galaxy clusters are among the largest and densest structures in the Universe. Their high density generally increases the suppression of star formation, known as quenching, altering…

physics.hist-ph2025

Inspiring stories from women in astronomy in Africa

Priscilla Muheki, Mirjana Pović, Somaya Saad +5

In preparation for the International Astronomical Union (IAU) General Assembly (GA) 2024, the first GA held in Africa, the African Network of Women in Astronomy (AfNWA) embarked on…

astro-ph.GA2025

AGN contribution on the morphological parameters of their host galaxies up to intermediate redshifts of z~2

Tilahun Getachew-Woreta, Mirjana Pović, Jaime Perea +4

The presence of Active Galaxy Nuclei (AGN) can affect the morphological classification of galaxies. This work aims to determine how the contribution of AGN affects the most used mo…

astro-ph.GA2025

The OTELO survey: New evidence of downsizing from the specific star formation rates, stellar mass functions, and star formation histories of a sample of low-mass galaxies at 0.38<z<1.43

Bernabé Cedrés, Ángel Bongiovanni, Jordi Cepa +13

We present an analysis of the emitters (\ha, \hb, and \oii) from the OTELO survey, in order to characterize the star formation properties of low-mass galaxies ( M…

astro-ph.GA2024★ 3 cited

The Quasar 3C 47: Extreme Population B Jetted Source With Double-peaked Profile

Shimeles Terefe Mengistue, Paola Marziani, Ascensión del Olmo +3

Context. An optically thick, geometrically thin accretion disk (AD) around a supermassive black hole might contribute to broad-line emission in type-1 active galactic nuclei (AGN).…

astro-ph.GA2023★ 20 cited

The miniJPAS survey: AGN & host galaxy co-evolution of X-ray selected sources

I. E. López, M. Brusa, S. Bonoli +35

Studies indicate strong evidence of a scaling relation in the local Universe between the supermassive black hole mass ($M_\rm{BH}$) and the stellar mass of their host galaxies ($M_…

astro-ph.GA2022★ 5 cited

Stellar populations of a sample of far-IR AGN and non-AGN green valley galaxies

Antoine Mahoro, Mirjana Pović, Petri Väisänen +2

We present a study on the stellar populations and stellar ages of sub-sample of far-infrared AGN and non-AGN green valley analysed in Mahoro et al. (2017,2019) at 0.6 < z < 1.0 usi…

physics.ed-ph2022

Activity Report of the Second African Conference on Fundamental and Applied Physics, ACP2021

Kétévi A. Assamagan, Obinna Abah, Amare Abebe +38

The African School of Fundamental Physics and Applications, also known as the African School of Physics (ASP), was initiated in 2010, as a three-week biennial event, to offer addit…

astro-ph.IM2021★ 1 cited

Non-Sequential Neural Network for Simultaneous, Consistent Classification and Photometric Redshifts of OTELO Galaxies

José A. de Diego, Jakub Nadolny, Ángel Bongiovanni +17

Context. Computational techniques are essential for mining large databases produced in modern surveys with value-added products. Aims. This paper presents a machine learning proced…

astro-ph.GA2020★ 1 cited

GLACE survey: galaxy activity in ZwCl0024+1652 cluster from strong optical emission lines

Zeleke Beyoro-Amado, Miguel Sánchez-Portal, Angel Bongiovanni +9

Although ZwCl0024+1652 galaxy cluster at has been thoroughly analysed, it lacks a comprehensive study of star formation and nuclear activity of its members. With GaLAxy…

astro-ph.GA2020★ 11 cited

AGN and Star-Formation Properties of Inside-out Assembled Galaxy Candidates at z<0.1

Dejene Zewdie, Mirjana Pović, Manuel Aravena +2

We study a sample of 48127 galaxies selected from the SDSS MPA-JHU catalogue, with and . Local galaxies in this stellar mass range…

astro-ph.GA2020★ 24 cited

Galaxy classification: deep learning on the OTELO and COSMOS databases

José A. de Diego, Jakub Nadolny, Ángel Bongiovanni +19

Context. The accurate classification of hundreds of thousands of galaxies observed in modern deep surveys is imperative if we want to understand the universe and its evolution. Aim…

astro-ph.GA2019★ 11 cited

A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z 0.4

Zeleke Beyoro Amado, Mirjana Pović, Miguel Sánchez-Portal +9

The well-known cluster of galaxies ZwCl0024+1652 at z 0.4, lacks an in-depth morphological classification of its central region. While previous studies provide a visual clas…

astro-ph.GA2018★ 17 cited

The ALHAMBRA survey: tight dependence of the optical mass-to-light ratio on galaxy colour up to z = 1.5

C. López-Sanjuan, L. A. Díaz-García, A. J. Cenarro +18

Our goal is to characterise the dependence of the optical mass-to-light ratio on galaxy colour up to z = 1.5, expanding the redshift range explored in previous work. From the ALHAM…

astro-ph.GA2017

High redshift galaxies in the ALHAMBRA survey: II. strengthening the evidence of bright-end excess in UV luminosity functions at 2.5 <= z <= 4.5 by PDF analysis

K. Viironen, C. López-Sanjuan, C. Hernández-Monteagudo +30

Context. Knowing the exact shape of the UV luminosity function of high-redshift galaxies is important in order to understand the star formation history of the early universe. Howev…

astro-ph.GA2017★ 18 cited

ELDAR, a new method to identify AGN in multi-filter surveys: the ALHAMBRA test-case

Jonás Chaves-Montero, Silvia Bonoli, Mara Salvato +15

We present ELDAR, a new method that exploits the potential of medium- and narrow-band filter surveys to securely identify active galactic nuclei (AGN) and determine their redshifts…

astro-ph.GA2017★ 54 cited

Star formation of far-IR AGN and non-AGN galaxies in the green valley: possible implication of AGN positive feedback

Antoine Mahoro, Mirjana Pović, Pheneas Nkundabakura

In this paper we present the star formation properties of 23 X-ray detected AGN and non-AGN galaxies in the green valley with far-IR (FIR) emission, using dat…

astro-ph.GA2016★ 20 cited

The ALHAMBRA survey : band luminosity function of quiescent and star-forming galaxies at by PDF analysis

C. López-Sanjuan, E. Tempel, N. Benítez +34

Our goal is to study the evolution of the band luminosity function (LF) since using ALHAMBRA data. We used the photometric redshift and the band selection magnitude p…

astro-ph.GA2016★ 20 cited

Star formation and AGN activity in the most luminous LINERs in the local universe

Mirjana Pović, Isabel Márquez, Hagai Netzer +4

This work presents the properties of 42 objects in the group of the most luminous, highest star formation rate LINERs at z = 0.04 - 0.11. We obtained long-slit spectroscopy of the…

astro-ph.GA2015★ 13 cited

High redshift galaxies in the ALHAMBRA survey: I. selection method and number counts based on redshift PDFs

K. Viironen, A. Marín-Franch, C. López-Sanjuan +31

Context. Most observational results on the high redshift restframe UV-bright galaxies are based on samples pinpointed using the so called dropout technique or Ly-alpha selection. H…

astro-ph.GA2014★ 47 cited

The ALHAMBRA survey: Accurate merger fractions by PDF analysis of photometric close pairs

C. López-Sanjuan, A. J. Cenarro, J. Varela +29

Our goal is to develop and test a novel methodology to compute accurate close pair fractions with photometric redshifts. We improve the current methodologies to estimate the merger…

astro-ph.CO2014★ 23 cited

The ALHAMBRA survey: an empirical estimation of the cosmic variance for merger fraction studies based on close pairs

C. López-Sanjuan, A. J. Cenarro, C. Hernández-Monteagudo +27

Our goal is to estimate empirically, for the first time, the cosmic variance that affects merger fraction studies based on close pairs. We compute the merger fraction from photomet…