_version_ 1866917107705315328
author Fernández-Ontiveros, J. A.
López-Sanjuan, C.
Hernán-Caballero, A.
Lumbreras-Calle, A.
Iglesias-Páramo, J.
Torralba, A.
Delgado, R. M. González
del Pino, A.
Rahna, P. T.
López, I. E.
Amorín, R.
Vílchez, J. M.
Kehrig, C.
Breda, I.
Gil, D. Fernández
Arizo-Borillo, F. D.
Giménez-Alcázar, A.
Pérez-Montero, E.
Ruiz, F. J. Sáez
Acharya, N.
Abramo, R.
Alcaniz, J.
Benítez, N.
Bonoli, S.
Carneiro, S.
Cenarro, J.
Cristóbal-Hornillos, D.
Daflon, S.
Dupke, R.
Ederoclite, A.
Hernández-Monteagudo, C.
Liu, J.
Marín-Franch, A.
de Oliveira, C. Mendes
Moles, M.
Roig, F.
Sodré Jr., L.
Taylor, K.
Varela, J.
Ramió, H. Vázquez
Zaragoza-Cardiel, J.
author_facet Fernández-Ontiveros, J. A.
López-Sanjuan, C.
Hernán-Caballero, A.
Lumbreras-Calle, A.
Iglesias-Páramo, J.
Torralba, A.
Delgado, R. M. González
del Pino, A.
Rahna, P. T.
López, I. E.
Amorín, R.
Vílchez, J. M.
Kehrig, C.
Breda, I.
Gil, D. Fernández
Arizo-Borillo, F. D.
Giménez-Alcázar, A.
Pérez-Montero, E.
Ruiz, F. J. Sáez
Acharya, N.
Abramo, R.
Alcaniz, J.
Benítez, N.
Bonoli, S.
Carneiro, S.
Cenarro, J.
Cristóbal-Hornillos, D.
Daflon, S.
Dupke, R.
Ederoclite, A.
Hernández-Monteagudo, C.
Liu, J.
Marín-Franch, A.
de Oliveira, C. Mendes
Moles, M.
Roig, F.
Sodré Jr., L.
Taylor, K.
Varela, J.
Ramió, H. Vázquez
Zaragoza-Cardiel, J.
contents We present the value-added catalogue JOLINES (J-PAS optical line intensities for nebular emission galaxies), which provides emission-line fluxes in galaxies at from the spectrophotometric catalogues of miniJPAS, J-NEP and the J-PAS early data release (EDR). This catalogue will be updated with future data releases, offering a growing resource for the study of emission-line galaxies. To obtain reliable emission-line fluxes from narrow-band photometry, we employed spectral energy distribution (SED) fitting using CIGALE, a robust tool that reconstructs the continuum emission and ensures accurate flux measurements. This method effectively mitigates uncertainties associated with direct continuum subtraction techniques, and systematics such as absorption components in the emission lines. We validate our approach using simulated observations of galaxy spectra with added noise, testing the method's performance across different equivalent width (EW) regimes and emission-line strengths. Additionally, we compare the recovered emission-line fluxes with spectroscopic measurements from the Sloan Digital Sky Survey (SDSS) and the Dark Energy Spectroscopic Instrument (DESI). Our results show a tight correlation between photometric and spectroscopic fluxes, particularly for bright emission lines, with a typical dispersion of $\sim$0.3 dex. Reliable fluxes are obtained for emission lines with EW $\gtrsim20\, \rm{\mathring{A}}$, in agreement with previous empirical studies. The current catalogue comprises approximately 13,900 sources with reliable flux measurements in the H$α$+[NII] complex and 7,200 in [OIII]$λ5007$, ensuring statistically robust samples for the brightest optical emission lines. This resource will be expanded in future J-PAS releases, facilitating large-scale studies of star formation, AGN activity, and galaxy evolution.
format Preprint
id arxiv_https___arxiv_org_abs_2511_21822
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle J-PAS: A value-added catalogue of optical line intensities for nebular emission galaxies (JOLINES)
Fernández-Ontiveros, J. A.
López-Sanjuan, C.
Hernán-Caballero, A.
Lumbreras-Calle, A.
Iglesias-Páramo, J.
Torralba, A.
Delgado, R. M. González
del Pino, A.
Rahna, P. T.
López, I. E.
Amorín, R.
Vílchez, J. M.
Kehrig, C.
Breda, I.
Gil, D. Fernández
Arizo-Borillo, F. D.
Giménez-Alcázar, A.
Pérez-Montero, E.
Ruiz, F. J. Sáez
Acharya, N.
Abramo, R.
Alcaniz, J.
Benítez, N.
Bonoli, S.
Carneiro, S.
Cenarro, J.
Cristóbal-Hornillos, D.
Daflon, S.
Dupke, R.
Ederoclite, A.
Hernández-Monteagudo, C.
Liu, J.
Marín-Franch, A.
de Oliveira, C. Mendes
Moles, M.
Roig, F.
Sodré Jr., L.
Taylor, K.
Varela, J.
Ramió, H. Vázquez
Zaragoza-Cardiel, J.
Astrophysics of Galaxies
We present the value-added catalogue JOLINES (J-PAS optical line intensities for nebular emission galaxies), which provides emission-line fluxes in galaxies at from the spectrophotometric catalogues of miniJPAS, J-NEP and the J-PAS early data release (EDR). This catalogue will be updated with future data releases, offering a growing resource for the study of emission-line galaxies. To obtain reliable emission-line fluxes from narrow-band photometry, we employed spectral energy distribution (SED) fitting using CIGALE, a robust tool that reconstructs the continuum emission and ensures accurate flux measurements. This method effectively mitigates uncertainties associated with direct continuum subtraction techniques, and systematics such as absorption components in the emission lines. We validate our approach using simulated observations of galaxy spectra with added noise, testing the method's performance across different equivalent width (EW) regimes and emission-line strengths. Additionally, we compare the recovered emission-line fluxes with spectroscopic measurements from the Sloan Digital Sky Survey (SDSS) and the Dark Energy Spectroscopic Instrument (DESI). Our results show a tight correlation between photometric and spectroscopic fluxes, particularly for bright emission lines, with a typical dispersion of $\sim$0.3 dex. Reliable fluxes are obtained for emission lines with EW $\gtrsim20\, \rm{\mathring{A}}$, in agreement with previous empirical studies. The current catalogue comprises approximately 13,900 sources with reliable flux measurements in the H$α$+[NII] complex and 7,200 in [OIII]$λ5007$, ensuring statistically robust samples for the brightest optical emission lines. This resource will be expanded in future J-PAS releases, facilitating large-scale studies of star formation, AGN activity, and galaxy evolution.
title J-PAS: A value-added catalogue of optical line intensities for nebular emission galaxies (JOLINES)
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2511.21822