%0 Generic %1 kelly2023constraints %A Kelly, Patrick L. %A Rodney, Steven %A Treu, Tommaso %A Oguri, Masamune %A Chen, Wenlei %A Zitrin, Adi %A Birrer, Simon %A Bonvin, Vivien %A Dessart, Luc %A Diego, Jose M. %A Filippenko, Alexei V. %A Foley, Ryan J. %A Gilman, Daniel %A Hjorth, Jens %A Jauzac, Mathilde %A Mandel, Kaisey %A Millon, Martin %A Pierel, Justin %A Sharon, Keren %A Thorp, Stephen %A Williams, Liliya %A Broadhurst, Tom %A Dressler, Alan %A Graur, Or %A Jha, Saurabh %A McCully, Curtis %A Postman, Marc %A Schmidt, Kasper Borello %A Tucker, Brad E. %A von der Linden, Anja %D 2023 %K tifr %R 10.1126/science.abh1322 %T Constraints on the Hubble constant from Supernova Refsdal's reappearance %U http://arxiv.org/abs/2305.06367 %X The gravitationally lensed Supernova Refsdal appeared in multiple images, produced through gravitational lensing by a massive foreground galaxy cluster. After the supernova appeared in 2014, lens models of the galaxy cluster predicted an additional image of the supernova would appear in 2015, which was subsequently observed. We use the time delays between the images to perform a blinded measurement of the expansion rate of the Universe, quantified by the Hubble constant (H0). Using eight cluster lens models, we infer H0 = 64.8 +4.4-4.3 km / s / Mpc, where Mpc is the megaparsec. Using the two models most consistent with the observations, we find H0 = 66.6 +4.1-3.3 km / s / Mpc. The observations are best reproduced by models that assign dark-matter halos to individual galaxies and the overall cluster.

@misc{kelly2023constraints, abstract = {The gravitationally lensed Supernova Refsdal appeared in multiple images, produced through gravitational lensing by a massive foreground galaxy cluster. After the supernova appeared in 2014, lens models of the galaxy cluster predicted an additional image of the supernova would appear in 2015, which was subsequently observed. We use the time delays between the images to perform a blinded measurement of the expansion rate of the Universe, quantified by the Hubble constant (H0). Using eight cluster lens models, we infer H0 = 64.8 +4.4-4.3 km / s / Mpc, where Mpc is the megaparsec. Using the two models most consistent with the observations, we find H0 = 66.6 +4.1-3.3 km / s / Mpc. The observations are best reproduced by models that assign dark-matter halos to individual galaxies and the overall cluster.}, added-at = {2023-05-12T07:46:28.000+0200}, author = {Kelly, Patrick L. and Rodney, Steven and Treu, Tommaso and Oguri, Masamune and Chen, Wenlei and Zitrin, Adi and Birrer, Simon and Bonvin, Vivien and Dessart, Luc and Diego, Jose M. and Filippenko, Alexei V. and Foley, Ryan J. and Gilman, Daniel and Hjorth, Jens and Jauzac, Mathilde and Mandel, Kaisey and Millon, Martin and Pierel, Justin and Sharon, Keren and Thorp, Stephen and Williams, Liliya and Broadhurst, Tom and Dressler, Alan and Graur, Or and Jha, Saurabh and McCully, Curtis and Postman, Marc and Schmidt, Kasper Borello and Tucker, Brad E. and von der Linden, Anja}, biburl = {https://www.bibsonomy.org/bibtex/21fc305f33d99e52230951a564ab38bc4/citekhatri}, description = {Constraints on the Hubble constant from Supernova Refsdal's reappearance}, doi = {10.1126/science.abh1322}, interhash = {35f5b99e2269c52d503f489b54377520}, intrahash = {1fc305f33d99e52230951a564ab38bc4}, keywords = {tifr}, note = {cite arxiv:2305.06367Comment: Published in Science. Companion paper presenting time-delay and relative magnification measurements published in ApJ (DOI: 10.3847/1538-4357/ac4ccb)}, timestamp = {2023-05-12T07:46:28.000+0200}, title = {Constraints on the Hubble constant from Supernova Refsdal's reappearance}, url = {http://arxiv.org/abs/2305.06367}, year = 2023 }