We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.

Durham Research Online
You are in:

Hubble Frontier Fields : predictions for the return of SN Refsdal with the MUSE and GMOS spectrographs.

Jauzac, M. and Richard, J. and Limousin, M. and Knowles, K. and Mahler, G. and Smith, G. P. and Kneib, J.-P. and Jullo, E. and Natarajan, P. and Ebeling, H. and Atek, H. and Clément, B. and Eckert, D. and Egami, E. and Massey, R. and Rexroth, M. (2016) 'Hubble Frontier Fields : predictions for the return of SN Refsdal with the MUSE and GMOS spectrographs.', Monthly notices of the Royal Astronomical Society., 457 (2). pp. 2029-2042.


We present a high-precision mass model of the galaxy cluster MACS J1149.6+ 2223, based on a strong gravitational lensing analysis of Hubble Space Telescope Frontier Fields (HFF) imaging data and spectroscopic follow-up with Gemini/Gemini Multi-Object Spectrographs (GMOS) and Very Large Telescope (VLT)/Multi Unit Spectroscopic Explorer (MUSE). Our model includes 12 new multiply imaged galaxies, bringing the total to 22, composed of 65 individual lensed images. Unlike the first two HFF clusters, Abell 2744 and MACS J0416.1−2403, MACS J1149 does not reveal as many multiple images in the HFF data. Using the LENSTOOL software package and the new sets of multiple images, we model the cluster with several cluster-scale dark matter haloes and additional galaxy-scale haloes for the cluster members. Consistent with previous analyses, we find the system to be complex, composed of five cluster-scale haloes. Their spatial distribution and lower mass, however, makes MACS J1149 a less powerful lens. Our best-fitting model predicts image positions with an rms of 0.91 arcsec. We measure the total projected mass inside a 200-kpc aperture as (1.840 ± 0.006) × 1014 M⊙, thus reaching again 1 per cent precision, following our previous HFF analyses of MACS J0416.1−2403 and Abell 2744. In light of the discovery of the first resolved quadruply lensed supernova, SN Refsdal, in one of the multiply imaged galaxies identified in MACS J1149, we use our revised mass model to investigate the time delays and predict the rise of the next image between 2015 November and 2016 January.

Item Type:Article
Keywords:Gravitational lensing: strong, Supernovae: individual: SN Refsdal, Galaxies: clusters: individual: MACS J1149.
Full text:(VoR) Version of Record
Download PDF
Publisher Web site:
Publisher statement:This article has been accepted for publication in Monthly notices of the Royal Astronomical Society ©: 2016 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Date accepted:06 January 2016
Date deposited:11 February 2016
Date of first online publication:06 February 2016
Date first made open access:11 February 2016

Save or Share this output

Look up in GoogleScholar