English

J-PLUS: Discovery and characterisation of ultracool dwarfs using Virtual Observatory tools II. Second data release and machine learning methodology

Solar and Stellar Astrophysics 2022-10-19 v1 Astrophysics of Galaxies Instrumentation and Methods for Astrophysics

Abstract

Ultracool dwarfs (UCDs) comprise the lowest mass members of the stellar population and brown dwarfs, from M7 V to cooler objects with L, T, and Y spectral types. Most of them have been discovered using wide-field imaging surveys, for which the Virtual Observatory (VO) has proven to be of great utility. We aim to perform a search for UCDs in the entire Javalambre Photometric Local Universe Survey (J-PLUS) second data release (2176 deg2^2) following a VO methodology. We also explore the ability to reproduce this search with a purely machine learning (ML)-based methodology that relies solely on J-PLUS photometry. We followed three different approaches based on parallaxes, proper motions, and colours, respectively, using the VOSA tool to estimate the effective temperatures. For the ML methodology, we built a two-step method based on principal component analysis and support vector machine algorithms. We identified a total of 7827 new candidate UCDs, which represents an increase of about 135% in the number of UCDs reported in the sky coverage of the J-PLUS second data release. Among the candidate UCDs, we found 122 possible unresolved binary systems, 78 wide multiple systems, and 48 objects with a high Bayesian probability of belonging to a young association. We also identified four objects with strong excess in the filter corresponding to the Ca II H and K emission lines and four other objects with excess emission in the Hα\alpha filter. With the ML approach, we obtained a recall score of 92% and 91% in the test and blind test, respectively. We consolidated the proposed search methodology for UCDs, which will be used in deeper and larger upcoming surveys such as J-PAS and Euclid. We concluded that the ML methodology is more efficient in the sense that it allows for a larger number of true negatives to be discarded prior to analysis with VOSA, although it is more photometrically restrictive.

Keywords

Cite

@article{arxiv.2208.09377,
  title  = {J-PLUS: Discovery and characterisation of ultracool dwarfs using Virtual Observatory tools II. Second data release and machine learning methodology},
  author = {P. Mas-Buitrago and E. Solano and A. González-Marcos and C. Rodrigo and E. L. Martín and J. A. Caballero and F. Jiménez-Esteban and P. Cruz and A. Ederoclite and J. Ordieres-Meré and A. Bello-García and R. A. Dupke and A. J. Cenarro and D. Cristóbal-Hornillos and C. Hernández-Monteagudo and C. López-Sanjuan and A. Marín-Franch and M. Moles and J. Varela and H. Vázquez Ramió and J. Alcaniz and L. Sodré and R. E. Angulo},
  journal= {arXiv preprint arXiv:2208.09377},
  year   = {2022}
}

Comments

Accepted in A&A

R2 v1 2026-06-25T01:49:26.768Z