activity
20142022
most citedSDSS-IV MaNGA: pyPipe3D analysis release for 10,000 galaxies

141 citations · 389 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2022★ 4 cited

Examining the Properties of Low-Luminosity Hosts of Type Ia Supernovae from ASAS-SN

Thomas W. -S. Holoien, Vera L. Berger, Jason T. Hinkle +14

We present a spectroscopic analysis of 44 low-luminosity host galaxies of Type Ia supernovae (SNe Ia) detected by the All-Sky Automated Survey for Supernovae (ASAS-SN), using the e…

astro-ph.GA2022★ 10 cited

Investigating the link between inner gravitational potential and star-formation quenching in CALIFA galaxies

V. Kalinova, D. Colombo, S. F. Sánchez +9

It has been suggested that the gravitational potential can have a significant role in suppressing the star formation in the nearby galaxies. To establish observational constrains o…

astro-ph.GA2022★ 22 cited

Spatial metallicity distribution statistics at pc scales in the AMUSING++ nearby galaxy sample

Zefeng Li, Emily Wisnioski, J. Trevor Mendel +6

We analyse the spatial statistics of the 2D gas-phase oxygen abundance distributions in a sample of 219 local galaxies. We introduce a new adaptive binning technique to enhance the…

astro-ph.GA2022★ 141 cited

SDSS-IV MaNGA: pyPipe3D analysis release for 10,000 galaxies

S. F. Sánchez, J. K. Barrera-Ballesteros, E. Lacerda +12

We present here the analysis performed using the pyPipe3D pipeline for the final MaNGA dataset included in the SDSS seventeenth data-release. This dataset comprises more than 10,00…

astro-ph.GA2022★ 2 cited

SDSS-IV MaNGA: The radial distribution of physical properties within galaxies in the nearby universe

J. K. Barrera-Ballesteros, S. F. Sánchez, C. Espinosa-Ponce +10

Using the largest sample of galaxies observed with an optical integral field unit (IFU, the SDSS-IV MaNGA survey, 10000 targets), we derive the radial distribution of the phy…

astro-ph.GA2022★ 3 cited

Spectral Evidence of Solar Neighborhood Analogs in CALIFA Galaxies

Alfredo Mejía-Narváez, Sebastian F. Sánchez, Leticia Carigi +3

We introduce a novel non-parametric method to find solar neighborhood analogs (SNAs) in extragalactic IFS surveys. The main ansatz is that the physical properties of the solar neig…

astro-ph.GA2022

pyHIIextractor: A tool to detect and extract physical properties of HII regions from Integral Field Spectroscopic data

A. Z. Lugo-Aranda, S. F. Sánchez, C. Espinosa-Ponce +5

We present a new code named pyHIIextractor, which detects and extracts the main features (positions and radii) of clumpy ionized regions, i.e. candidate HII regions, using Hα emiss…

astro-ph.GA2022

Chemical evolution history of MaNGA galaxies

Artemi Camps-Fariña, Sebastián F. Sánchez, Alfredo Mejía-Narváez +8

We show the results of a study using the spectral synthesis technique study for the full MaNGA sample showing their Chemical Enrichment History (ChEH) as well as the evolution of t…

astro-ph.GA2017★ 51 cited

SSDSS IV MaNGA - Properties of AGN host galaxies

S. F. Sanchez, V. Avila-Reese, H. Hernandez-Toledo +22

We present here the characterization of the main properties of a sample of 98 AGN host galaxies, both type-II and type-I, in comparison with those of about 2700 non-active galaxies…

astro-ph.GA2016★ 40 cited

SDSS IV MaNGA: Deep observations of extra-planar, diffuse ionized gas around late-type galaxies from stacked IFU spectra

A. Jones, G. Kauffmann, R. D'Souza +16

We have conducted a study of extra-planar diffuse ionized gas using the first year data from the MaNGA IFU survey. We have stacked spectra from 49 edge-on, late-type galaxies as a…

astro-ph.GA2016★ 14 cited

The Califa and Hipass velocity function for all morphological galaxy types

S. Bekeraitė, C. J. Walcher, L. Wisotzki +17

The velocity function is a fundamental observable statistic of the galaxy population, similarly impor- tant as the luminosity function, but much more difficult to measure. In this…

astro-ph.GA2014★ 102 cited

P-MaNGA: Emission Lines Properties - Gas Ionisation and Chemical Abundances from Prototype Observations

F. Belfiore, R. Maiolino, K. Bundy +27

MaNGA (Mapping Nearby Galaxies at Apache Point Observatory) is a SDSS-IV survey that will obtain spatially resolved spectroscopy from 3600 Å to 10300 Å for a representative sample…