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| Autores principales: | , , , , , , , |
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| Formato: | Preprint |
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2026
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| Acceso en línea: | https://arxiv.org/abs/2604.13211 |
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| _version_ | 1866908964887724032 |
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| author | Baron, Dalya Setton, David J. Ma, Yilun Prochaska, J. X. Canalizo, Gabriela Davies, Ric Greene, Jenny E. Lutz, Dieter |
| author_facet | Baron, Dalya Setton, David J. Ma, Yilun Prochaska, J. X. Canalizo, Gabriela Davies, Ric Greene, Jenny E. Lutz, Dieter |
| contents | Rapid transitions from starburst to quiescence constitute a key evolutionary pathway in galaxy formation. Post-starburst galaxies trace this brief phase, exhibiting optical spectra dominated by intermediate-age stellar populations with strong Balmer absorption features. Although rare locally, such systems are commonly revealed by JWST observations among massive galaxies at $z \gtrsim 3$. In the nearby Universe, their evolutionary stage remains uncertain: Balmer-strong galaxies hosting active galactic nuclei (AGN) show conflicting star formation rates (SFRs), with optical diagnostics implying quenching while far-infrared emission suggests ongoing obscured star formation. We present Sparks, an infrared survey designed to study the transition from starburst to post-starburst. Using the FIRE spectrograph on the Magellan Telescope, Sparks provides near-infrared spectra (0.82-2.51 $μ$m) for 93 local massive galaxies spanning three orders of magnitude in SFR, from starbursts to quenched post-starbursts, including AGN hosts. Here, we describe the survey goals, sample selection, observations, and data reduction, and examine galaxy properties derived from stellar population synthesis fitting of photometric data covering far-ultraviolet to far-infrared. Our new panchromatic-based SFR and star formation history measurements divide the sample into three groups: galaxies undergoing their first major starburst in the past $\sim 1$ Gyr; galaxies undergoing their second major starburst, with optical continua dominated by intermediate-age stellar populations formed during the previous recent burst; and post-burst quenching systems. AGN appear predominantly in the second group, explaining why systems with strong Balmer absorption and AGN show elevated far-infrared emission, and implying a short delay between starburst and black hole accretion. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2604_13211 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Sparks: The Magellan/FIRE survey from starburst to post-starburst Baron, Dalya Setton, David J. Ma, Yilun Prochaska, J. X. Canalizo, Gabriela Davies, Ric Greene, Jenny E. Lutz, Dieter Astrophysics of Galaxies Rapid transitions from starburst to quiescence constitute a key evolutionary pathway in galaxy formation. Post-starburst galaxies trace this brief phase, exhibiting optical spectra dominated by intermediate-age stellar populations with strong Balmer absorption features. Although rare locally, such systems are commonly revealed by JWST observations among massive galaxies at $z \gtrsim 3$. In the nearby Universe, their evolutionary stage remains uncertain: Balmer-strong galaxies hosting active galactic nuclei (AGN) show conflicting star formation rates (SFRs), with optical diagnostics implying quenching while far-infrared emission suggests ongoing obscured star formation. We present Sparks, an infrared survey designed to study the transition from starburst to post-starburst. Using the FIRE spectrograph on the Magellan Telescope, Sparks provides near-infrared spectra (0.82-2.51 $μ$m) for 93 local massive galaxies spanning three orders of magnitude in SFR, from starbursts to quenched post-starbursts, including AGN hosts. Here, we describe the survey goals, sample selection, observations, and data reduction, and examine galaxy properties derived from stellar population synthesis fitting of photometric data covering far-ultraviolet to far-infrared. Our new panchromatic-based SFR and star formation history measurements divide the sample into three groups: galaxies undergoing their first major starburst in the past $\sim 1$ Gyr; galaxies undergoing their second major starburst, with optical continua dominated by intermediate-age stellar populations formed during the previous recent burst; and post-burst quenching systems. AGN appear predominantly in the second group, explaining why systems with strong Balmer absorption and AGN show elevated far-infrared emission, and implying a short delay between starburst and black hole accretion. |
| title | Sparks: The Magellan/FIRE survey from starburst to post-starburst |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2604.13211 |