SPHEREx mapping of diffuse PAH and H II emission in the Galactic plane
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2026
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| author | Murgia, Giulia Cukierman, Ari J. Hensley, Brandon S. Ashby, Matthew L. N. Bock, James J. Chang, Tzu-Ching Chen, Shuang-Shuang Cheng, Yun-Ting Chiang, Yi-Kuan Cooray, Asantha Crill, Brendan P. Doré, Olivier Dowell, C. Darren Faisst, Andreas L. Hora, Joseph L. Hui, Howard Kang, Miju Kang, Jae Hwan Korngut, Phil M. Lee, Dennis Lee, Jeong-Eun Lee, Bomee Lisse, Carey M. Masters, Daniel C. Melnick, Gary J. Minasyan, Mary H. Nguyen, Chi H. Paladini, Roberta Tolls, Volker Wen, Robin Y. Werner, Michael W. Zemcov, Michael |
| author_facet | Murgia, Giulia Cukierman, Ari J. Hensley, Brandon S. Ashby, Matthew L. N. Bock, James J. Chang, Tzu-Ching Chen, Shuang-Shuang Cheng, Yun-Ting Chiang, Yi-Kuan Cooray, Asantha Crill, Brendan P. Doré, Olivier Dowell, C. Darren Faisst, Andreas L. Hora, Joseph L. Hui, Howard Kang, Miju Kang, Jae Hwan Korngut, Phil M. Lee, Dennis Lee, Jeong-Eun Lee, Bomee Lisse, Carey M. Masters, Daniel C. Melnick, Gary J. Minasyan, Mary H. Nguyen, Chi H. Paladini, Roberta Tolls, Volker Wen, Robin Y. Werner, Michael W. Zemcov, Michael |
| contents | We present preliminary SPHEREx maps of diffuse Galactic emission tracing polycyclic aromatic hydrocarbons (PAHs) and ionized hydrogen gas, and we study their relationship across the Galactic plane. Since its launch in early 2025, the SPHEREx space telescope has been conducting an all-sky near-infrared spectral survey from 0.75 to 5.0 microns. We produce a large-scale map of the 3.3-micron PAH emission feature, which is bright and detectable throughout the Galactic plane, and find a strong correlation with the thermal dust radiance measured by Planck. We also trace ionized hydrogen gas by producing a map of Brackett-alpha emission at 4.05 microns. By combining the two maps, we identify extended shells of PAH emission associated with photodissociation regions surrounding ionized gas. We construct a PAH abundance map and find a significant anticorrelation between PAH abundance and ionized hydrogen, indicating systematic PAH depletion within ionized gas regions across the Galactic plane and demonstrating that ionizing radiation is a dominant driver of PAH abundance variations. These early SPHEREx results provide a large-scale view of PAHs and ionized hydrogen and preview the capability of the mission to map diffuse emission in the interstellar medium. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2603_23620 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | SPHEREx mapping of diffuse PAH and H II emission in the Galactic plane Murgia, Giulia Cukierman, Ari J. Hensley, Brandon S. Ashby, Matthew L. N. Bock, James J. Chang, Tzu-Ching Chen, Shuang-Shuang Cheng, Yun-Ting Chiang, Yi-Kuan Cooray, Asantha Crill, Brendan P. Doré, Olivier Dowell, C. Darren Faisst, Andreas L. Hora, Joseph L. Hui, Howard Kang, Miju Kang, Jae Hwan Korngut, Phil M. Lee, Dennis Lee, Jeong-Eun Lee, Bomee Lisse, Carey M. Masters, Daniel C. Melnick, Gary J. Minasyan, Mary H. Nguyen, Chi H. Paladini, Roberta Tolls, Volker Wen, Robin Y. Werner, Michael W. Zemcov, Michael Astrophysics of Galaxies We present preliminary SPHEREx maps of diffuse Galactic emission tracing polycyclic aromatic hydrocarbons (PAHs) and ionized hydrogen gas, and we study their relationship across the Galactic plane. Since its launch in early 2025, the SPHEREx space telescope has been conducting an all-sky near-infrared spectral survey from 0.75 to 5.0 microns. We produce a large-scale map of the 3.3-micron PAH emission feature, which is bright and detectable throughout the Galactic plane, and find a strong correlation with the thermal dust radiance measured by Planck. We also trace ionized hydrogen gas by producing a map of Brackett-alpha emission at 4.05 microns. By combining the two maps, we identify extended shells of PAH emission associated with photodissociation regions surrounding ionized gas. We construct a PAH abundance map and find a significant anticorrelation between PAH abundance and ionized hydrogen, indicating systematic PAH depletion within ionized gas regions across the Galactic plane and demonstrating that ionizing radiation is a dominant driver of PAH abundance variations. These early SPHEREx results provide a large-scale view of PAHs and ionized hydrogen and preview the capability of the mission to map diffuse emission in the interstellar medium. |
| title | SPHEREx mapping of diffuse PAH and H II emission in the Galactic plane |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2603.23620 |