Ivan Lacerna
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View article: The role of supercluster filaments in shaping galaxy clusters
The role of supercluster filaments in shaping galaxy clusters Open
In a hierarchical ΛCDM Universe, cosmic filaments serve as the primary channels for matter accretion into galaxy clusters, influencing the shape of their dark matter halos. We investigate whether the elongation of galaxy clusters correlate…
View article: Targeting cluster galaxies for the 4MOST CHANCES Low-z sub-survey with photometric redshifts
Targeting cluster galaxies for the 4MOST CHANCES Low-z sub-survey with photometric redshifts Open
The evolution of galaxies is shaped by both internal processes and their external environments. Galaxy clusters and their surroundings provide ideal laboratories to study these effects, particularly mechanisms such as quenching and morphol…
View article: Assessing the connection between galactic conformity and assembly-type bias
Assessing the connection between galactic conformity and assembly-type bias Open
Context. Galaxies across the Universe display a conformity in the fraction of quenched galaxies out to large distances, which is much greater around quenched central galaxies than it is for star-forming ones. On the other hand, simulations…
View article: Visual morphological classification of the full MaNGA DR17 sample: a general characterization
Visual morphological classification of the full MaNGA DR17 sample: a general characterization Open
We present the MaNGA (Mapping Nearby Galaxies at Apache Point Observatory) Visual Morphology (MVM) catalogue, featuring a visual morphological classification of 10 059 galaxies in the final MaNGA sample. By combining SDSS (Sloan Digital Sk…
View article: Visual morphological classification of the full MaNGA DR17 sample: a general characterization
Visual morphological classification of the full MaNGA DR17 sample: a general characterization Open
We present the MaNGA Visual Morphology (MVM) catalogue, featuring a visual morphological classification of 10,059 galaxies in the final MaNGA sample. By combining SDSS and DESI Legacy Survey (DLS) images, we classified galaxies into 13 Hub…
View article: SDSS-V black hole mapper: the index diagram as a tool to disentangle the influence of the host galaxy in quasar spectra
SDSS-V black hole mapper: the index diagram as a tool to disentangle the influence of the host galaxy in quasar spectra Open
We revisit the Quasar Main Sequence (QMS) by investigating the impact of the stellar component from the host galaxy (HG) on the emission line spectra of the active galactic nuclei (AGNs). We first detect spectra with broad emission lines u…
View article: Spatially resolved near-infrared spectroscopic indices for the massive elliptical galaxy IC 4296
Spatially resolved near-infrared spectroscopic indices for the massive elliptical galaxy IC 4296 Open
Context. In the near-infrared (NIR) region, a large number of absorption features may be used to constrain the properties of unresolved stellar populations of galaxies. Aims. We present the results of a pilot project assessing the feasibil…
View article: Assessing the connection between galactic conformity and assembly-type bias
Assessing the connection between galactic conformity and assembly-type bias Open
Context. Galaxies in the Universe show a conformity in the fraction of quenched galaxies out to large distances, being much larger around quenched central galaxies than for star-forming ones. On the other hand, simulations have shown that …
View article: Abell548: A rich cluster of galaxies in the making
Abell548: A rich cluster of galaxies in the making Open
We performed an in-depth study of the complex structure of the galaxy cluster A548, based on 108 spectroscopic galaxy velocities reported in this paper. This analysis includes 80 new redshifts, along with velocity data from the literature …
View article: The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity Open
We investigated the population of low-mass central galaxies with M ⋆ = 10 9.5 − 10 10 h −1 M ⊙ , inhabiting regions near massive groups and clusters of galaxies using the IllustrisTNG300 and MDPL2-SAG simulations. We set out to study their…
View article: An iterative method to deblend AGN-Host contributions for Integral Field spectroscopic observations
An iterative method to deblend AGN-Host contributions for Integral Field spectroscopic observations Open
We present a new iterative deblending method to separate the host galaxy (HG) and their Active Galactic Nuclei (AGNs) emission with the use of Integral Field spectroscopic (IFS) data. The method decomposes the resolved HG emission from the…
View article: An iterative method to deblend AGN-Host contributions for Integral Field spectroscopic observations
An iterative method to deblend AGN-Host contributions for Integral Field spectroscopic observations Open
We present a new iterative deblending method to separate the host galaxy (HG) and their Active Galactic Nuclei (AGN) emission with the use of Integral Field spectroscopic (IFS) data. The method decomposes the resolved HG emission from the …
View article: The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity Open
We investigated the population of low-mass central galaxies with Mstar = $10^{9.5}-10^{10}$ Msun/h, inhabiting regions near massive groups and clusters of galaxies using the TNG300 and MDPL2-SAG simulations. We set out to study their evolu…
View article: The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V
The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V Open
The eighteenth data release (DR18) of the Sloan Digital Sky Survey (SDSS) is the first one for SDSS-V, the fifth generation of the survey. SDSS-V comprises three primary scientific programs or “Mappers”: the Milky Way Mapper (MWM), the Bla…
View article: SDSS-IV MaNGA: The Effect of Stellar Mass and Halo Mass on the Assembly Histories of Satellite Galaxies
SDSS-IV MaNGA: The Effect of Stellar Mass and Halo Mass on the Assembly Histories of Satellite Galaxies Open
We combine an unprecedented MaNGA sample of over 3000 passive galaxies in the stellar mass range 10 9 –10 12 M ⊙ with the Sloan Digital Sky Survey group catalog by Tinker to quantify how central and satellite formation, quantified by radia…
View article: SDSS-IV MaNGA: The effect of stellar mass and halo mass on the assembly histories of satellite galaxies
SDSS-IV MaNGA: The effect of stellar mass and halo mass on the assembly histories of satellite galaxies Open
We combine an unprecedented MaNGA sample of over 3,000 passive galaxies in the stellar mass range 10^{9}-10^{12} Msun with the Sloan Digital Sky Survey group catalog by Tinker to quantify how central and satellite formation, quantified by …
View article: The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V
The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V Open
The eighteenth data release of the Sloan Digital Sky Surveys (SDSS) is the first one for SDSS-V, the fifth generation of the survey. SDSS-V comprises three primary scientific programs, or "Mappers": Milky Way Mapper (MWM), Black Hole Mappe…
View article: A Comparative Analysis of the Chemical Compositions of Gaia-Enceladus/Sausage and Milky Way Satellites using APOGEE
A Comparative Analysis of the Chemical Compositions of Gaia-Enceladus/Sausage and Milky Way Satellites using APOGEE Open
We use data from the 17th data release of the Apache Point Observatory Galactic Evolution Experiment (APOGEE 2) to contrast the chemical composition of the recently discovered Gaia Enceladus/Sausage system (GE/S) to those of ten Milky Way …
View article: The H <scp>i</scp> content of red geyser galaxies
The H <span>i</span> content of red geyser galaxies Open
Red geysers are a specific type of quiescent galaxy, denoted by twin jets emerging from their galactic centres. These bisymmetric jets possibly inject energy and heat into the surrounding material, effectively suppressing star formation by…
View article: The HI Content of Red Geyser Galaxies
The HI Content of Red Geyser Galaxies Open
Red geysers are a specific type of quiescent galaxy, denoted by twin jets emerging from their galactic centers. These bisymmetric jets possibly inject energy and heat into the surrounding material, effectively suppressing star formation by…
View article: A comparative analysis of the chemical compositions of Gaia-Enceladus/Sausage and Milky Way satellites using APOGEE
A comparative analysis of the chemical compositions of Gaia-Enceladus/Sausage and Milky Way satellites using APOGEE Open
We use data from the 17th data release of the Apache Point Observatory Galactic Evolution Experiment (APOGEE 2) to contrast the chemical composition of the recently discovered Gaia Enceladus/Sausage system (GE/S) to those of 10 Milky Way (…
View article: Infrared variability of young solar analogues in the Lagoon Nebula
Infrared variability of young solar analogues in the Lagoon Nebula Open
T Tauri stars are low-mass pre-main sequence stars that are intrinsically variable. Due to the intense magnetic fields they possess, they develop dark spots on their surface that, because of rotation, introduce a periodic variation of brig…
View article: New insights into the Triangulum Australis supercluster of galaxies
New insights into the Triangulum Australis supercluster of galaxies Open
The Triangulum Australis cluster is one of about a dozen nearby massive cluster systems which contribute to the gravitational pull behind the so-called Great Attractor that is dominated by the nearby Shapley Supercluster mass, which confor…
View article: SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass
SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass Open
We analyze spatially resolved and co-added SDSS-IV MaNGA spectra with signal-to-noise ratio ∼100 from 2200 passive central galaxies ( z ∼ 0.05) to understand how central galaxy assembly depends on stellar mass ( M * ) and halo mass ( M h )…
View article: SDSS-IV MaNGA: Identification and multiwavelength properties of Type-1 AGN in the DR15 sample
SDSS-IV MaNGA: Identification and multiwavelength properties of Type-1 AGN in the DR15 sample Open
We present a method to identify type-1 active galactic nuclei (AGNs) in the central 3 arcsec integrated spectra of galaxies in the MaNGA DR15 sample. It is based on flux ratios estimates in spectral bands flanking the expected h α broad co…
View article: SDSS-IV MaNGA: How the stellar populations of passive central galaxies\n depend on stellar and halo mass
SDSS-IV MaNGA: How the stellar populations of passive central galaxies\n depend on stellar and halo mass Open
We analyze spatially resolved and co-added SDSS-IV MaNGA spectra with\nsignal-to-noise ~100 from 2200 passive central galaxies (z~0.05) to understand\nhow central galaxy assembly depends on stellar mass (M*) and halo mass (Mh). We\ncontrol…
View article: On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales Open
The environment within dark matter haloes can quench the star formation of galaxies. However, environmental effects beyond the virial radius of haloes (≳1 Mpc) are less evident. An example is the debated correlation between colour or star …
View article: SDSS IV MaNGA: visual morphological and statistical characterization of the DR15 sample
SDSS IV MaNGA: visual morphological and statistical characterization of the DR15 sample Open
We present a detailed visual morphological classification for the 4614 MaNGA galaxies in SDSS Data Release 15, using image mosaics generated from a combination of r band (SDSS and deeper DESI Legacy Surveys) images and their digital post-p…
View article: The differences between mass- and light-derived structural parameters over time for MaNGA elliptical galaxies
The differences between mass- and light-derived structural parameters over time for MaNGA elliptical galaxies Open
We apply stellar population synthesis analysis to obtain spatially resolved archaeological inferences for a large sample of ‘red and dead’ Elliptical galaxies (Classical Ellipticals, CLEs) from the MaNGA/SDSS-IV DR15 survey. From their 2D …
View article: APOGEE Chemical Abundance Patterns of the Massive Milky Way Satellites
APOGEE Chemical Abundance Patterns of the Massive Milky Way Satellites Open
The SDSS-IV Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey has obtained high-resolution spectra for thousands of red giant stars distributed among the massive satellite galaxies of the Milky Way (MW): the Large and …