_version_ 1866910174313185280
author Razza, Alessandro
Blanc, Guillermo A.
Groves, Brent
Congiu, Enrico
Neumann, Justus
Pan, Hsi-An
Ho, I-Ting
Barnes, Ashley T.
Belfiore, Francesco
Boquien, Médéric
Burton, Charlie
Chevance, Mélanie
Egorov, Oleg
Emsellem, Eric
Faesi, Chris
Glover, Simon C. O.
Grasha, Kathryn
Klessen, Ralf S.
Kreckel, Kathryn
Leroy, Adam K.
McElroy, Rebecca
Pessa, Ismael
Schinnerer, Eva
Tomičić, Neven
Amiri, Amirnezam
Anand, Gagandeep S.
Cao, Yixian
Dale, Daniel A.
Dlamini, Simthembile
Li, Jing
Méndez-Delgado, J. Eduardo
Murphy, Eric J.
Pathak, Debosmita
Querejeta, Miguel
Ramambason, Lise
Rosolowsky, Erik
Scheuermann, Fabian
Úbeda, Leonardo
Williams, Thomas G.
author_facet Razza, Alessandro
Blanc, Guillermo A.
Groves, Brent
Congiu, Enrico
Neumann, Justus
Pan, Hsi-An
Ho, I-Ting
Barnes, Ashley T.
Belfiore, Francesco
Boquien, Médéric
Burton, Charlie
Chevance, Mélanie
Egorov, Oleg
Emsellem, Eric
Faesi, Chris
Glover, Simon C. O.
Grasha, Kathryn
Klessen, Ralf S.
Kreckel, Kathryn
Leroy, Adam K.
McElroy, Rebecca
Pessa, Ismael
Schinnerer, Eva
Tomičić, Neven
Amiri, Amirnezam
Anand, Gagandeep S.
Cao, Yixian
Dale, Daniel A.
Dlamini, Simthembile
Li, Jing
Méndez-Delgado, J. Eduardo
Murphy, Eric J.
Pathak, Debosmita
Querejeta, Miguel
Ramambason, Lise
Rosolowsky, Erik
Scheuermann, Fabian
Úbeda, Leonardo
Williams, Thomas G.
contents We present PHANGS-Hα, a narrow-band imaging survey that maps Hα emission over a sample of 65 nearby massive star-forming galaxies. The data were obtained using the MPG-ESO 2.2-meter telescope at La Silla and the du Pont 2.5-meter telescope at Las Campanas Observatory, in the framework of the multi-wavelength cloud-scale (50-100 pc) resolution mapping of molecular gas and star formation conducted by the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) collaboration. PHANGS-Hα complements the already published PHANGS-ALMA, PHANGS-MUSE, PHANGS-HST, and PHANGS-JWST surveys, providing an anchor point for the photometric and astrometric calibration of these datasets, as well as samples of H ii regions, and star formation rate maps for the bulk of the PHANGS sample. We present observations, data processing, and calibration of the PHANGS-Hα dataset, as well as the procedures used to derive emission-line fluxes from narrow-band imaging. A subset of galaxies with available spectroscopic Ha mapping from the PHANGS-MUSE survey allows for a detailed comparison with the narrow-band photometry presented here. This informs a series of best practices for the processing of narrow-band Hα imaging that we apply to the full dataset.
format Preprint
id arxiv_https___arxiv_org_abs_2604_25627
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle The PHANGS-Hα survey. Ground-based narrow-band imaging of nearby star-forming galaxies
Razza, Alessandro
Blanc, Guillermo A.
Groves, Brent
Congiu, Enrico
Neumann, Justus
Pan, Hsi-An
Ho, I-Ting
Barnes, Ashley T.
Belfiore, Francesco
Boquien, Médéric
Burton, Charlie
Chevance, Mélanie
Egorov, Oleg
Emsellem, Eric
Faesi, Chris
Glover, Simon C. O.
Grasha, Kathryn
Klessen, Ralf S.
Kreckel, Kathryn
Leroy, Adam K.
McElroy, Rebecca
Pessa, Ismael
Schinnerer, Eva
Tomičić, Neven
Amiri, Amirnezam
Anand, Gagandeep S.
Cao, Yixian
Dale, Daniel A.
Dlamini, Simthembile
Li, Jing
Méndez-Delgado, J. Eduardo
Murphy, Eric J.
Pathak, Debosmita
Querejeta, Miguel
Ramambason, Lise
Rosolowsky, Erik
Scheuermann, Fabian
Úbeda, Leonardo
Williams, Thomas G.
Astrophysics of Galaxies
We present PHANGS-Hα, a narrow-band imaging survey that maps Hα emission over a sample of 65 nearby massive star-forming galaxies. The data were obtained using the MPG-ESO 2.2-meter telescope at La Silla and the du Pont 2.5-meter telescope at Las Campanas Observatory, in the framework of the multi-wavelength cloud-scale (50-100 pc) resolution mapping of molecular gas and star formation conducted by the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) collaboration. PHANGS-Hα complements the already published PHANGS-ALMA, PHANGS-MUSE, PHANGS-HST, and PHANGS-JWST surveys, providing an anchor point for the photometric and astrometric calibration of these datasets, as well as samples of H ii regions, and star formation rate maps for the bulk of the PHANGS sample. We present observations, data processing, and calibration of the PHANGS-Hα dataset, as well as the procedures used to derive emission-line fluxes from narrow-band imaging. A subset of galaxies with available spectroscopic Ha mapping from the PHANGS-MUSE survey allows for a detailed comparison with the narrow-band photometry presented here. This informs a series of best practices for the processing of narrow-band Hα imaging that we apply to the full dataset.
title The PHANGS-Hα survey. Ground-based narrow-band imaging of nearby star-forming galaxies
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2604.25627