HerS-3: An Exceptional Einstein Cross Reveals a Massive Dark Matter Halo

Fuente: arXiv
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Autori principali: Cox, P., Butler, K. M., Keeton, C. R., Eid, L., Borsato, E., Bakx, T. J. L. C., Neri, R., Jones, B. M., Prajapati, P., Baker, A. J., Berta, S., Cooray, A., Corsini, E. M., Marchetti, L., Omont, A., Beelen, A., Gavazzi, R., Ismail, D., Ivison, R. J., Krips, M., Lehnert, M. D., Messias, H., Riechers, D., Vlahakis, C., Weiß, A., van der Werf, P., Yang, C.
Natura: Preprint
Pubblicazione: 2025
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author Cox, P.
Butler, K. M.
Keeton, C. R.
Eid, L.
Borsato, E.
Bakx, T. J. L. C.
Neri, R.
Jones, B. M.
Prajapati, P.
Baker, A. J.
Berta, S.
Cooray, A.
Corsini, E. M.
Marchetti, L.
Omont, A.
Beelen, A.
Gavazzi, R.
Ismail, D.
Ivison, R. J.
Krips, M.
Lehnert, M. D.
Messias, H.
Riechers, D.
Vlahakis, C.
Weiß, A.
van der Werf, P.
Yang, C.
author_facet Cox, P.
Butler, K. M.
Keeton, C. R.
Eid, L.
Borsato, E.
Bakx, T. J. L. C.
Neri, R.
Jones, B. M.
Prajapati, P.
Baker, A. J.
Berta, S.
Cooray, A.
Corsini, E. M.
Marchetti, L.
Omont, A.
Beelen, A.
Gavazzi, R.
Ismail, D.
Ivison, R. J.
Krips, M.
Lehnert, M. D.
Messias, H.
Riechers, D.
Vlahakis, C.
Weiß, A.
van der Werf, P.
Yang, C.
contents We present a study of HerS-3, a dusty star-forming galaxy at zspec = 3.0607, which is gravitationally amplified into an Einstein cross with a fifth image of the background galaxy seen at the center of the cross. Detailed 1-mm spectroscopy and imaging with NOEMA and ALMA resolve the individual images and show that each of the five images display a series of molecular lines that have similar central velocities, unambiguously confirming that they have identical redshifts. The HST F110W image reveals a foreground lensing group of four galaxies with a photometric redshift zphot~1.0. Lens models that only include the four visible galaxies are unable to reproduce the properties of HerS-3. By adding a fifth massive component, lying south-east of the brightest galaxy of the group, the source reconstruction is able to match the peak emission, shape and orientation for each of the five images. The fact that no galaxy is detected near that position indicates the presence of a massive dark matter halo in the lensing galaxy group. In the source plane, HerS-3 appears as an infrared luminous starburst galaxy seen nearly edge-on. The serendipitous discovery of this exceptional Einstein cross offers a potential laboratory for exploring at small spatial scales a nuclear starburst at the peak of cosmic evolution and studying the properties of a massive dark matter halo associated with the lensing galaxy group.
format Preprint
id arxiv_https___arxiv_org_abs_2509_14983
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle HerS-3: An Exceptional Einstein Cross Reveals a Massive Dark Matter Halo
Cox, P.
Butler, K. M.
Keeton, C. R.
Eid, L.
Borsato, E.
Bakx, T. J. L. C.
Neri, R.
Jones, B. M.
Prajapati, P.
Baker, A. J.
Berta, S.
Cooray, A.
Corsini, E. M.
Marchetti, L.
Omont, A.
Beelen, A.
Gavazzi, R.
Ismail, D.
Ivison, R. J.
Krips, M.
Lehnert, M. D.
Messias, H.
Riechers, D.
Vlahakis, C.
Weiß, A.
van der Werf, P.
Yang, C.
Astrophysics of Galaxies
We present a study of HerS-3, a dusty star-forming galaxy at zspec = 3.0607, which is gravitationally amplified into an Einstein cross with a fifth image of the background galaxy seen at the center of the cross. Detailed 1-mm spectroscopy and imaging with NOEMA and ALMA resolve the individual images and show that each of the five images display a series of molecular lines that have similar central velocities, unambiguously confirming that they have identical redshifts. The HST F110W image reveals a foreground lensing group of four galaxies with a photometric redshift zphot~1.0. Lens models that only include the four visible galaxies are unable to reproduce the properties of HerS-3. By adding a fifth massive component, lying south-east of the brightest galaxy of the group, the source reconstruction is able to match the peak emission, shape and orientation for each of the five images. The fact that no galaxy is detected near that position indicates the presence of a massive dark matter halo in the lensing galaxy group. In the source plane, HerS-3 appears as an infrared luminous starburst galaxy seen nearly edge-on. The serendipitous discovery of this exceptional Einstein cross offers a potential laboratory for exploring at small spatial scales a nuclear starburst at the peak of cosmic evolution and studying the properties of a massive dark matter halo associated with the lensing galaxy group.
title HerS-3: An Exceptional Einstein Cross Reveals a Massive Dark Matter Halo
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2509.14983