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Astrophysics > Astrophysics of Galaxies

arXiv:2507.06696 (astro-ph)
[Submitted on 9 Jul 2025 (v1), last revised 8 Sep 2025 (this version, v5)]

Title:Blowing Star Formation Away in AGN Hosts (BAH) -- III. Serendipitous discovery of a $z\sim2.9$ star-forming galaxy lensed by the galactic bulge of CGCG 012-070 using JWST NIRSpec

Authors:Rogemar A. Riffel, Carlos R. Melo-Carneiro, Gabriel Luan Souza-Oliveira, Rogério Riffel, Cristina Furlanetto, Nadia L. Zakamska, Santiago Arribas, Marina Bianchin, Ana L. Chies-Santos, José Henrique Costa-Souza, Maitê S. Z. de Mellos, Michele Perna, Thaisa Storchi-Bergmann
View a PDF of the paper titled Blowing Star Formation Away in AGN Hosts (BAH) -- III. Serendipitous discovery of a $z\sim2.9$ star-forming galaxy lensed by the galactic bulge of CGCG 012-070 using JWST NIRSpec, by Rogemar A. Riffel and 12 other authors
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Abstract:We report the detection of a gravitationally lensed galaxy by the nearby spiral galaxy CGCG 012-070 ($z = 0.048$) using Integral Field Unit (IFU) observations with the Near-Infrared Spectrograph (NIRSpec) instrument on board the James Webb Space Telescope (JWST). The lensed galaxy is identified through the flux distributions of emission lines in the rest-frame optical, consistent with a source located at a redshift of $z\sim2.89$. The system is detected in [O III]$\lambda\lambda4959,5007$, H$\beta$, and H$\alpha$ emission lines, exhibiting line ratios typical of a star-forming galaxy. The emission-line flux distributions reveal three distinct components, which are modeled using an elliptical power-law (EPL) mass profile for the lens galaxy. This model provides a good characterization of the source and reveals a disturbed star-forming morphology consistent with those of galaxies at cosmic noon. This serendipitous discovery of a rare low-redshift strong lens highlights the critical role of IFU observations in expanding the lens census and advancing our understanding of galaxy mass profiles and evolution.
Comments: Accepted by A&A Letters, 6 pages
Subjects: Astrophysics of Galaxies (astro-ph.GA)
Cite as: arXiv:2507.06696 [astro-ph.GA]
  (or arXiv:2507.06696v5 [astro-ph.GA] for this version)
  https://doi.org/10.48550/arXiv.2507.06696
arXiv-issued DOI via DataCite
Journal reference: A&A 701, L11 (2025)
Related DOI: https://doi.org/10.1051/0004-6361/202556329
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Submission history

From: Rogemar Andre Riffel [view email]
[v1] Wed, 9 Jul 2025 09:40:08 UTC (5,506 KB)
[v2] Thu, 10 Jul 2025 07:42:34 UTC (5,506 KB)
[v3] Thu, 28 Aug 2025 16:11:38 UTC (1,420 KB)
[v4] Fri, 29 Aug 2025 11:54:50 UTC (1,420 KB)
[v5] Mon, 8 Sep 2025 09:54:49 UTC (1,421 KB)
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