Extreme magnification of an individual star at redshift 1.5 by a galaxy-cluster lens
Article 2018 en
Authors
PK
Patrick L. Kelly
JD
J. M. Diego
SR
S. Rodney
Abstract
1 min read
Galaxy-cluster gravitational lenses can magnify background galaxies by a total factor of up to ~50. Here we report an image of an individual star at redshift z=1.49 (dubbed "MACS J1149 Lensed Star 1 (LS1)") magnified by >2000. A separate image, detected briefly 0.26 arcseconds from LS1, is likely a counterimage of the first star demagnified for multiple years by a >~3 solar-mass object in the cluster. For reasonable assumptions about the lensing system, microlensing fluctuations in the stars' light curves can yield evidence about the mass function of intracluster stars and compact objects, including binary fractions and specific stellar evolution and supernova models. Dark-matter subhalos or massive compact objects may help to account for the two images' long-term brightness ratio.
Patrick L. Kelly, J. M. Diego, S. Rodney, Nick Kaiser, Tom Broadhurst, Adi Zitrin, Tommaso Treu, Pablo G. Pérez‐González, Takahiro Morishita, Mathilde Jauzac, J. Selsing, Masamune Oguri, Laurent Pueyo, Timothy W. Ross, Alexei V Filippenko, Nathan Smith, J. Hjorth, S. B. Cenko, Xin Wang, D. A. Howell, Johan Richard, Brenda Frye, Saurabh W. Jha, R. J. Foley, Colin Norman, Maruša Bradač, WeiKang Zheng, Gabriel Brammer, Alberto Molino Benito, A. Cava, L. Christensen, S. E. de Mink, Or Graur, C. Grillo, Ryota Kawamata, Jean‐Paul Kneib, T. Matheson, C. McCully, M. Nonino, I. Pérez‐Fournon, Adam G. Riess, P. Rosati, Marko Shuntov, Keren Sharon, Benjamin J. Weiner
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