J-HERTz: J-PLUS Heritage Exploration of Radio Targets at z $<$ 5

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Hauptverfasser: Gil, D. Fernández, Fernández-Ontiveros, J. A., López-Sanjuan, C., Arizo-Borillo, F., del Pino, A., Hernán-Caballero, A., Lumbreras-Calle, A., Rahna, P. T., Sobral, David, Ramió, H. Vázquez, Cenarro, A. J., Marín-Franch, A., Angulo, R. E., Ederoclite, A., Cristóbal-Hornillos, D., Dupke, R. A., Hernández-Monteagudo, C., Moles, M., Sodré Jr, L., Varela, J.
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Veröffentlicht: 2025
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author Gil, D. Fernández
Fernández-Ontiveros, J. A.
López-Sanjuan, C.
Arizo-Borillo, F.
del Pino, A.
Hernán-Caballero, A.
Lumbreras-Calle, A.
Rahna, P. T.
Sobral, David
Ramió, H. Vázquez
Cenarro, A. J.
Marín-Franch, A.
Angulo, R. E.
Ederoclite, A.
Cristóbal-Hornillos, D.
Dupke, R. A.
Hernández-Monteagudo, C.
Moles, M.
Sodré Jr, L.
Varela, J.
author_facet Gil, D. Fernández
Fernández-Ontiveros, J. A.
López-Sanjuan, C.
Arizo-Borillo, F.
del Pino, A.
Hernán-Caballero, A.
Lumbreras-Calle, A.
Rahna, P. T.
Sobral, David
Ramió, H. Vázquez
Cenarro, A. J.
Marín-Franch, A.
Angulo, R. E.
Ederoclite, A.
Cristóbal-Hornillos, D.
Dupke, R. A.
Hernández-Monteagudo, C.
Moles, M.
Sodré Jr, L.
Varela, J.
contents We introduce J-HERTz (J-PLUS Heritage Exploration of Radio Targets at $z < 5$), a new multi-wavelength catalog that combines optical narrow-band photometry from J-PLUS, infrared observations from WISE, and deep low-frequency radio data from LoTSS for nearly half a million sources across 2,100 deg$^2$ of the northern sky. Key innovations of J-HERTz include Bayesian neural network classifications for 390,000 galaxies, 31,000 quasars, and 20,000 stars, along with significantly improved photometric redshifts for 235,000 galaxies compared to previous J-PLUS DR3 and LoTSS DR2 estimates. We identify 831 candidate Galactic radio stars, which, if confirmed, would constitute a significant addition to the number of radio-emitting stars identified to date. Among radio-loud galaxies with spectroscopic observations, $\gtrsim$20% lack Seyfert or LINER signatures, indicating a substantial population of optically quiescent radio galaxies, in agreement with previous works. Spectral energy distribution fitting of their host galaxies using J-PLUS photospectra reveals systematically low specific star formation rates, consistent with quenched stellar populations. J-HERTz thus provides a powerful dataset to exploit radio-optical synergies, enabling studies that span from the origin of stellar radio emission to the AGN life cycle and the role of jet activity in shaping host galaxy evolution.
format Preprint
id arxiv_https___arxiv_org_abs_2511_14844
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle J-HERTz: J-PLUS Heritage Exploration of Radio Targets at z $<$ 5
Gil, D. Fernández
Fernández-Ontiveros, J. A.
López-Sanjuan, C.
Arizo-Borillo, F.
del Pino, A.
Hernán-Caballero, A.
Lumbreras-Calle, A.
Rahna, P. T.
Sobral, David
Ramió, H. Vázquez
Cenarro, A. J.
Marín-Franch, A.
Angulo, R. E.
Ederoclite, A.
Cristóbal-Hornillos, D.
Dupke, R. A.
Hernández-Monteagudo, C.
Moles, M.
Sodré Jr, L.
Varela, J.
Astrophysics of Galaxies
We introduce J-HERTz (J-PLUS Heritage Exploration of Radio Targets at $z < 5$), a new multi-wavelength catalog that combines optical narrow-band photometry from J-PLUS, infrared observations from WISE, and deep low-frequency radio data from LoTSS for nearly half a million sources across 2,100 deg$^2$ of the northern sky. Key innovations of J-HERTz include Bayesian neural network classifications for 390,000 galaxies, 31,000 quasars, and 20,000 stars, along with significantly improved photometric redshifts for 235,000 galaxies compared to previous J-PLUS DR3 and LoTSS DR2 estimates. We identify 831 candidate Galactic radio stars, which, if confirmed, would constitute a significant addition to the number of radio-emitting stars identified to date. Among radio-loud galaxies with spectroscopic observations, $\gtrsim$20% lack Seyfert or LINER signatures, indicating a substantial population of optically quiescent radio galaxies, in agreement with previous works. Spectral energy distribution fitting of their host galaxies using J-PLUS photospectra reveals systematically low specific star formation rates, consistent with quenched stellar populations. J-HERTz thus provides a powerful dataset to exploit radio-optical synergies, enabling studies that span from the origin of stellar radio emission to the AGN life cycle and the role of jet activity in shaping host galaxy evolution.
title J-HERTz: J-PLUS Heritage Exploration of Radio Targets at z $<$ 5
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2511.14844