activity
20022026
most citedThe Young Stellar Population of IC1613. I. A New Catalogue of OB Associations

39 citations · 120 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.IM2026

Analysis of Binary O-type Star Systems Using Recurrent Neural Networks

Miguel Flores R., Luis J. Corral, Celia R. Fierro-Santillán +1

This work presents an initial analysis of the estimation of effective temperature and surface gravity for simulated O-type binary systems using a recurrent neural network. The prop…

astro-ph.IM2025★ 4 cited

Disentangling stellar atmospheric parameters in astronomical spectra using Generative Adversarial Neural Networks

Minia Manteiga, Raúl Santoveña, Marco A. Álvarez +4

A method based on Generative Adversaria! Networks (GANs) is developed for disentangling the physical (effective temperature and gravity) and chemical (metallicity, overabundance of…

astro-ph.SR2024

Identification of planetary and proto-planetary nebulae candidates through akari infrared photometry

R. A. Marquez-Lugo, S. N. Kemp, G. Ramos-Larios +3

We utilized photometric data from the space telescope AKARI to identify potential planetary nebulae (PNe) and proto-planetary nebulae (PPNe) candidates. Using the colour-colour dia…

astro-ph.IM2022★ 1 cited

O-type Stars Stellar Parameter Estimation Using Recurrent Neural Networks

Miguel Flores R., Luis J. Corral, Celia R. Fierro-Santillán +1

In this paper, we present a deep learning system approach to estimating luminosity, effective temperature, and surface gravity of O-type stars using the optical region of the stell…

astro-ph.IM2021★ 6 cited

Stellar Spectra Models Classification and Parameter Estimation Using Machine Learning Algorithms

Miguel Flores R., Luis J. Corral, Celia R. Fierro-Santillán

The growth of sky surveys and the large amount of stellar spectra in the current databases, has generated the necessity of developing new methods to estimate atmospheric parameters…

astro-ph.GA2016★ 10 cited

Dark matter inside early-type galaxies as function of mass and redshift

A. Nigoche-Netro, G. Ramos-Larios, P. Lagos +6

We study the behaviour of the dynamical and stellar mass inside the effective radius (re) of early-type galaxies (ETGs). We use several samples of ETGs -ranging from 19 000 to 98 0…

astro-ph.GA2016★ 4 cited

The tidal filament of NGC 4660

S. N. Kemp, C. Martinez-Robles, R. A. Marquez-Lugo +6

NGC 4660, in the Virgo cluster, is a well-studied elliptical galaxy which has a strong disk component (D/T about 0.2-0.3). The central regions including the disk component have ste…

astro-ph.SR2016★ 21 cited

Spitzer mid-infrared spectroscopic observations of planetary nebulae

Héctor Mata, Gerardo Ramos-Larios, Martin A. Guerrero +7

We present Spitzer Space Telescope archival mid-infrared (mid-IR) spectroscopy of a sample of eleven planetary nebulae (PNe). The observations, acquired with the Spitzer Infrared S…

astro-ph.SR2011★ 8 cited

Blue luminous stars in nearby galaxies - UIT005: a possible link to the luminous blue variable stage

M. A. Urbaneja, A. Herrero, D. J. Lennon +2

(abridged) A detailed study of the blue supergiant UIT005 (B2-2.5Ia+) in M33 is presented. The results of our quantitative spectral analysis indicate that the star is a very lumino…

astro-ph.SR2010

In savvy pursuit of Local Group blue massive stars

Miriam Garcia, Artemio Herrero, Norberto Castro +1

The important role of metallicity on massive star evolution and the combination of multi-object spectrographs and 10m class telescopes, have lead to numerous systematic studies of…

astro-ph.SR2009★ 39 cited

The Young Stellar Population of IC1613. I. A New Catalogue of OB Associations

M. Garcia, A. Herrero, B. Vicente +5

Context: Determining the parameters of massive stars is crucial to understand many processes in galaxies and the Universe, since these objects are important sources of ionization,…

astro-ph2002★ 27 cited

An Analysis of STIS HST UV Spectra of M33 early B Supergiants

M. A. Urbaneja, A. Herrero, R. P. Kudritzki +3

We present terminal velocities of M33 B-supergiants, obtained from STIS HST spectra as part of our programme to investigate the Wind Momentum -- Luminosity Relationship (WLR) in th…