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| Main Authors: | , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
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2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2504.07622 |
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| _version_ | 1866918036068368384 |
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| author | Bazzanini, L. Angora, G. Scialpi, M. Di Rosa, G. Bergamini, P. Rosati, P. Lombardi, M. Abriola, D. Acebron, A. D'Addona, M. Granata, G. Grillo, C. Mannucci, F. Maturi, M. Meneghetti, M. Mercurio, A. Radovich, M. |
| author_facet | Bazzanini, L. Angora, G. Scialpi, M. Di Rosa, G. Bergamini, P. Rosati, P. Lombardi, M. Abriola, D. Acebron, A. D'Addona, M. Granata, G. Grillo, C. Mannucci, F. Maturi, M. Meneghetti, M. Mercurio, A. Radovich, M. |
| contents | Time-delay cosmography (TDC) using multiply-lensed quasars (QSOs) by galaxies has recently emerged as an independent and competitive tool to measure the value of the Hubble constant. Lens galaxy clusters hosting multiply-imaged QSOs, when coupled with an accurate and precise knowledge of their total mass distribution, are equally powerful cosmological probes. However, less than ten such systems have been identified to date. Our study aims to expand the limited sample of cluster-lensed QSO systems by identifying new candidates within rich galaxy clusters. Starting from a sample of ~$10^5$ galaxy cluster candidates (Wen & Han, 2022), built from Dark Energy Survey and Wide-field Infrared Survey Explorer imaging data, and a highly-pure catalogue of over one million QSOs, based on Gaia DR3 data, we cross-correlate them to identify candidate lensed QSOs near the core of massive galaxy clusters. Our search yielded 3 lensed double candidates over an area of ~$5000$ sq. degree. In this work, we focus on the best candidate consisting of a double QSO with Gaia-based redshift of 1.35, projected behind a moderately rich cluster (WHJ0400-27) at $z_{phot}=0.65$. Based on a first spectroscopic follow-up study, we confirm the two QSOs at $z=1.345$, with indistinguishable spectra, and a brightest cluster galaxy at $z=0.626$. These observations seem to support the strong lensing nature of this system, although some tension emerges when the cluster mass from a preliminary lens model is compared with that from other mass proxies. We also discuss the possibility that such system is a rare physical association of two distinct QSOs with a projected physical distance of ~$150$ kpc. If further spectroscopic observations confirm its lensing nature, such a rare lens system would exhibit one of the largest image separations observed to date ($Δ\vartheta=17.8''$), opening interesting TDC applications. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2504_07622 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | A new quasar strongly-lensed candidate by the galaxy cluster WHJ0400-27 with a $18''$ image-separation Bazzanini, L. Angora, G. Scialpi, M. Di Rosa, G. Bergamini, P. Rosati, P. Lombardi, M. Abriola, D. Acebron, A. D'Addona, M. Granata, G. Grillo, C. Mannucci, F. Maturi, M. Meneghetti, M. Mercurio, A. Radovich, M. Astrophysics of Galaxies Time-delay cosmography (TDC) using multiply-lensed quasars (QSOs) by galaxies has recently emerged as an independent and competitive tool to measure the value of the Hubble constant. Lens galaxy clusters hosting multiply-imaged QSOs, when coupled with an accurate and precise knowledge of their total mass distribution, are equally powerful cosmological probes. However, less than ten such systems have been identified to date. Our study aims to expand the limited sample of cluster-lensed QSO systems by identifying new candidates within rich galaxy clusters. Starting from a sample of ~$10^5$ galaxy cluster candidates (Wen & Han, 2022), built from Dark Energy Survey and Wide-field Infrared Survey Explorer imaging data, and a highly-pure catalogue of over one million QSOs, based on Gaia DR3 data, we cross-correlate them to identify candidate lensed QSOs near the core of massive galaxy clusters. Our search yielded 3 lensed double candidates over an area of ~$5000$ sq. degree. In this work, we focus on the best candidate consisting of a double QSO with Gaia-based redshift of 1.35, projected behind a moderately rich cluster (WHJ0400-27) at $z_{phot}=0.65$. Based on a first spectroscopic follow-up study, we confirm the two QSOs at $z=1.345$, with indistinguishable spectra, and a brightest cluster galaxy at $z=0.626$. These observations seem to support the strong lensing nature of this system, although some tension emerges when the cluster mass from a preliminary lens model is compared with that from other mass proxies. We also discuss the possibility that such system is a rare physical association of two distinct QSOs with a projected physical distance of ~$150$ kpc. If further spectroscopic observations confirm its lensing nature, such a rare lens system would exhibit one of the largest image separations observed to date ($Δ\vartheta=17.8''$), opening interesting TDC applications. |
| title | A new quasar strongly-lensed candidate by the galaxy cluster WHJ0400-27 with a $18''$ image-separation |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2504.07622 |