Determining the spatial origin of X-ray and optical emission in the $z = 3.1$ strongly lensed radio-quiet quasar GraL J065904.1+162909 to hundreds of parsecs
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arXiv
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| Autori principali: | , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| _version_ | 1866913012557807616 |
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| author | Sisk-Reynes, Julia Schwartz, Daniel Barnacka, Anna Spingola, Cristiana Migliori, Giulia |
| author_facet | Sisk-Reynes, Julia Schwartz, Daniel Barnacka, Anna Spingola, Cristiana Migliori, Giulia |
| contents | We perform milliarcsecond X-ray astrometry of the quadruply lensed radio-quiet quasar GraL J065904.1+162909 (J0659). This $z = 3.083$ quasar is lensed into four images and was discovered with the second Data Release of the $Gaia$ Space Observatory ($Gaia$ DR2). Our J0659 study exploits strong gravitational lenses as high resolution telescopes. This technique shows promise to elucidate the origin of optical and X-ray emission in distant lensed quasars at spatial scales beyond the reach of current instruments. In our study, we use $Gaia$ DR3 and $HST$ observations of J0659 to infer a mass model for the deflector. Our model reproduces the $Gaia$ DR3 quasar lensed image positions to one milliarcsecond and determines the position of the optical source in J0659 to within this precision. Next, we analyze $Chandra$ observations of J0659 and conduct a Bayesian test evaluating whether the X-ray emission region coincides with the optical source. We then constrain the origin of the X-ray emission to within a $0.''020 \times 0.''010$ ellipse centered $0.''014$ away from the optical source at the $1σ$ level. We demonstrate that our approach can be extended to pinpoint the distinct origins of the soft and hard X-ray emission regions in lensed quasars. We discuss the potential of upcoming broadband and spectrally resolved X-ray astrometric studies to probe complex quasar morphology and AGN multiplicity at sub-kiloparsec scales otherwise inaccessible at high redshifts. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2509_22797 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Determining the spatial origin of X-ray and optical emission in the $z = 3.1$ strongly lensed radio-quiet quasar GraL J065904.1+162909 to hundreds of parsecs Sisk-Reynes, Julia Schwartz, Daniel Barnacka, Anna Spingola, Cristiana Migliori, Giulia High Energy Astrophysical Phenomena We perform milliarcsecond X-ray astrometry of the quadruply lensed radio-quiet quasar GraL J065904.1+162909 (J0659). This $z = 3.083$ quasar is lensed into four images and was discovered with the second Data Release of the $Gaia$ Space Observatory ($Gaia$ DR2). Our J0659 study exploits strong gravitational lenses as high resolution telescopes. This technique shows promise to elucidate the origin of optical and X-ray emission in distant lensed quasars at spatial scales beyond the reach of current instruments. In our study, we use $Gaia$ DR3 and $HST$ observations of J0659 to infer a mass model for the deflector. Our model reproduces the $Gaia$ DR3 quasar lensed image positions to one milliarcsecond and determines the position of the optical source in J0659 to within this precision. Next, we analyze $Chandra$ observations of J0659 and conduct a Bayesian test evaluating whether the X-ray emission region coincides with the optical source. We then constrain the origin of the X-ray emission to within a $0.''020 \times 0.''010$ ellipse centered $0.''014$ away from the optical source at the $1σ$ level. We demonstrate that our approach can be extended to pinpoint the distinct origins of the soft and hard X-ray emission regions in lensed quasars. We discuss the potential of upcoming broadband and spectrally resolved X-ray astrometric studies to probe complex quasar morphology and AGN multiplicity at sub-kiloparsec scales otherwise inaccessible at high redshifts. |
| title | Determining the spatial origin of X-ray and optical emission in the $z = 3.1$ strongly lensed radio-quiet quasar GraL J065904.1+162909 to hundreds of parsecs |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2509.22797 |