Galaxy Cluster MACS J1149.6+2223 and Supernova Refsdal
SN Refsdal, SN HFF14Ref (supernova), MACS J1149.6+2223 (cluster)
9.3 billion light-years or 2.9 billion parsecs (supernova); 5 billion light-years or 1.5 billion parsecs (cluster)
This image is created from data from the following HST proposals: 13459 T. Treu (UCLA) et al. and the GLASS team, 13504 J. Lotz (STScI) et al. and the Frontier Fields team, 13790 S. Rodney (JHU) et al. and the FrontierSN team, and 14041 P. Kelly (UCLA) et al. and the Refsdal team.
The science team includes: P. Kelly (UC Berkeley), S. Rodney (JHU), T. Treu (UCLA), R. Foley (University of Illinois at Urbana-Champaign), G. Brammer (STScI), K. Schmidt (UC Santa Barbara), A. Zitrin (Caltech), A. Sonnenfeld (UCLA), L.-G. Strolger (Western Kentucky University/STScI), O. Graur (New York University/American Museum of Natural History), A. Filippenko (UC Berkeley), S. Jha (Rutgers University), A. Riess (JHU/STScI), M. Bradac (UC Davis), B. Weiner (Steward Observatory/UA), D. Scolnic (University of Chicago), M. Malkan (UCLA), A. von der Linden (Dark Cosmology Centre, Copenhagen/KIPAC, Stanford), M. Trenti (University of Melbourne), J. Hjorth (Dark Cosmology Centre, Copenhagen), R. Gavazzi (Institut d'Astrophysique de Paris), A. Fontana (INAF-OAR), J. Merten (Caltech), C. McCully and T. Jones (UC Santa Barbara), M. Postman (STScI), A. Dressler (Carnegie Observatories), B. Patel (Rutgers University), S. B. Cenko (NASA/GSFC), M. Graham (UC Berkeley), and B. Tucker (UC Berkeley/Australia National University).
ACS/WFC: F606W and F814W
WFC3/IR: F105W, F125W, F140W, and F160W
These images are composites of separate exposures acquired by the ACS and WFC3 instruments on the Hubble Space Telescope. Several filters were used to sample broad wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are:
Blue: F606W+F814W
Green: F105W+F125W
Red: F140W+F160W
NASA, ESA, and S. Rodney (JHU) and the FrontierSN team; T. Treu (UCLA), P. Kelly (UC Berkeley), and the GLASS team; J. Lotz (STScI) and the Frontier Fields team; M. Postman (STScI) and the CLASH team; and Z. Levay (STScI)
