A Study on the Line of Sight to Galaxies Detected at Gamma-Ray Energies
The large-scale universal structure comprises strands of dark matter and galaxies with large underdense volumes known as voids. We measure the fraction of the line of sight that intersects voids for active galactic nuclei (AGN) detected by Fermi Large Area Telescope (LAT) and quasars from the Sloan...
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IOP Publishing
2025-01-01
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| Series: | The Astrophysical Journal Letters |
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| Online Access: | https://doi.org/10.3847/2041-8213/adae9d |
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| author | Amy Furniss Josepf N. Amador Olivier Hervet Ollie Jackson David A. Williams |
| author_facet | Amy Furniss Josepf N. Amador Olivier Hervet Ollie Jackson David A. Williams |
| author_sort | Amy Furniss |
| collection | DOAJ |
| description | The large-scale universal structure comprises strands of dark matter and galaxies with large underdense volumes known as voids. We measure the fraction of the line of sight that intersects voids for active galactic nuclei (AGN) detected by Fermi Large Area Telescope (LAT) and quasars from the Sloan Digital Sky Survey (SDSS). This “voidiness” fraction is a rudimentary proxy for the density along the line of sight to the galaxies. The voidiness of SDSS-observed quasars (QSOs) is distinctly different from randomly distributed source populations, with a median p -value of 4.6 × 10 ^−5 and ≪1 × 10 ^−7 , when compared with 500 simulated populations with randomly simulated locations but matching redshifts in the 0.1 ≤ z < 0.4 and 0.4 ≤ z < 0.7 intervals, respectively. A similar comparison of the voidiness for LAT-detected AGN shows median p -values greater than 0.05 in each redshift interval. When comparing the SDSS QSO population to the LAT-detected AGN, we mitigate potential bias from a relationship between redshift and voidiness by comparing the LAT-detected AGN to a “redshift-matched” set of SDSS QSOs. The LAT-detected AGN between a redshift of 0.4 and 0.7 show higher voidiness compared to the redshift-matched SDSS QSO populations, with a median p -value of 2.3 × 10 ^−5 (a 4.1 σ deviation). No deviation is found when comparing the same populations between redshifts of 0.1 and 0.4 ( p > 0.05). We do not study possible causes of this voidiness difference. It might relate to propagation effects from lower magnetic or radiative background fields within voids or to an environment more favorable for gamma-ray production for AGN near voids. |
| format | Article |
| id | doaj-art-c1027a0d105e4bdb90343157a1428ba8 |
| institution | Kabale University |
| issn | 2041-8205 |
| language | English |
| publishDate | 2025-01-01 |
| publisher | IOP Publishing |
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| series | The Astrophysical Journal Letters |
| spelling | doaj-art-c1027a0d105e4bdb90343157a1428ba82025-02-10T15:59:49ZengIOP PublishingThe Astrophysical Journal Letters2041-82052025-01-019801L1510.3847/2041-8213/adae9dA Study on the Line of Sight to Galaxies Detected at Gamma-Ray EnergiesAmy Furniss0https://orcid.org/0000-0003-1614-1273Josepf N. Amador1https://orcid.org/0009-0009-1807-0078Olivier Hervet2https://orcid.org/0000-0003-3878-1677Ollie Jackson3David A. Williams4https://orcid.org/0000-0003-2740-9714Santa Cruz Institute for Particle Physics and Department of Physics, University of California , Santa Cruz, USADepartment of Physics and Astronomy, San José State University , San José, CA, USA; Department of Physics and Astronomy, California State Polytechnic University , Pomona, USASanta Cruz Institute for Particle Physics and Department of Physics, University of California , Santa Cruz, USASanta Cruz Institute for Particle Physics and Department of Physics, University of California , Santa Cruz, USASanta Cruz Institute for Particle Physics and Department of Physics, University of California , Santa Cruz, USAThe large-scale universal structure comprises strands of dark matter and galaxies with large underdense volumes known as voids. We measure the fraction of the line of sight that intersects voids for active galactic nuclei (AGN) detected by Fermi Large Area Telescope (LAT) and quasars from the Sloan Digital Sky Survey (SDSS). This “voidiness” fraction is a rudimentary proxy for the density along the line of sight to the galaxies. The voidiness of SDSS-observed quasars (QSOs) is distinctly different from randomly distributed source populations, with a median p -value of 4.6 × 10 ^−5 and ≪1 × 10 ^−7 , when compared with 500 simulated populations with randomly simulated locations but matching redshifts in the 0.1 ≤ z < 0.4 and 0.4 ≤ z < 0.7 intervals, respectively. A similar comparison of the voidiness for LAT-detected AGN shows median p -values greater than 0.05 in each redshift interval. When comparing the SDSS QSO population to the LAT-detected AGN, we mitigate potential bias from a relationship between redshift and voidiness by comparing the LAT-detected AGN to a “redshift-matched” set of SDSS QSOs. The LAT-detected AGN between a redshift of 0.4 and 0.7 show higher voidiness compared to the redshift-matched SDSS QSO populations, with a median p -value of 2.3 × 10 ^−5 (a 4.1 σ deviation). No deviation is found when comparing the same populations between redshifts of 0.1 and 0.4 ( p > 0.05). We do not study possible causes of this voidiness difference. It might relate to propagation effects from lower magnetic or radiative background fields within voids or to an environment more favorable for gamma-ray production for AGN near voids.https://doi.org/10.3847/2041-8213/adae9dGamma-raysBlazarsVoidsGamma-ray sourcesGamma-ray astronomy |
| spellingShingle | Amy Furniss Josepf N. Amador Olivier Hervet Ollie Jackson David A. Williams A Study on the Line of Sight to Galaxies Detected at Gamma-Ray Energies The Astrophysical Journal Letters Gamma-rays Blazars Voids Gamma-ray sources Gamma-ray astronomy |
| title | A Study on the Line of Sight to Galaxies Detected at Gamma-Ray Energies |
| title_full | A Study on the Line of Sight to Galaxies Detected at Gamma-Ray Energies |
| title_fullStr | A Study on the Line of Sight to Galaxies Detected at Gamma-Ray Energies |
| title_full_unstemmed | A Study on the Line of Sight to Galaxies Detected at Gamma-Ray Energies |
| title_short | A Study on the Line of Sight to Galaxies Detected at Gamma-Ray Energies |
| title_sort | study on the line of sight to galaxies detected at gamma ray energies |
| topic | Gamma-rays Blazars Voids Gamma-ray sources Gamma-ray astronomy |
| url | https://doi.org/10.3847/2041-8213/adae9d |
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