Galaxies behind a gravitational magnifier

The James Webb Telescope reveals highly distant objects

Using the first science image released by the James Webb Space Telescope (JWST) this month, an international team of scientists led by the Max Planck Institute for Astrophysics has built an improved model for the mass distribution of the galaxy cluster SMACS J0723.3−7327. They used dozens of multiple images of far-away background galaxies revealed in the JWST image, some of which were too faint to be detected previously. Acting as a so-called gravitational lens, the foreground galaxy cluster produces both multiple images of background galaxies and magnifies these images. One family of such multiple images belongs to a galaxy, which the model predicts to be at a large distance, i.e. whose light travelled some 13 billion years before reaching the telescope. If confirmed, this will emphasise the importance of accurate gravitational lens models for the identification of distant galaxies and their detailed study.

The first science image released by the James Webb Space Telescope (JWST) was of a gravitational lens, in particular the galaxy cluster SMACS J0723.3−7327. Gravitational lenses, especially galaxy clusters, magnify the light from background galaxies and produce multiple images of these. Before JWST, 19 multiple images of six background sources were known in SMACS J0723.3−7327. The JWST data now revealed 27 additional multiple images from another ten lensed sources.

“In this first step towards the road opened by JWST, we used recent data from this brand new telescope, to model the lensing effect of SMACS0723 with great accuracy,” points out Gabriel Bartosch Caminha, postdoc fellow at the Max Planck Institute for Astrophysics (MPA) and the German Centre for Cosmological Lensing (GCCL). The collaboration first used data from the Hubble Space Telescope (HST) and Multi Unit Spectroscopic Explorer (MUSE) to build a “pre-JWST” lens model, and then refined it with newly available JWST near-infrared imaging. “The JWST imaging is absolutely astounding and beautiful, showing many more multiply lensed background sources, which allowed us to substantially refine our lens mass model,” he adds.

Many of these new, lensed sources do not yet have distance estimates, and the scientists used their mass model to predict how far away these lensed galaxies are most likely to be. One of them was found to be probably an amazing distance (redshift > 7.5), i.e. its light was emitted during the Universe's early stages. This galaxy is multiply lensed into three images and its luminosity is magnified by a factor of about 20 in total.

However, to study these primordial objects, it is fundamental to describe accurately the lensing effect of the foreground galaxy cluster. “Our accurate mass model forms the foundation for the exploration of the JWST data,” emphasizes Sherry Suyu, Max Planck Research Group Leader at MPA, an Associate Professor at the Technical University of Munich, and a Visiting Scholar at the Academia Sinica Institute of Astronomy and Astrophysics. “The spectacular JWST images show a great variety of strongly lensed galaxies, which can be studied in detail thanks to our accurate model.”

The new model for the mass distribution of the foreground cluster is capable of reproducing the positions of all multiple images with a high accuracy, making the model one of the most accurate available. For follow-up studies of these sources, the lens models, including magnification maps and redshifts (i.e. distances) estimated from the model are made publicly available. “We are very excited about this,” Suyu adds, “we are eagerly awaiting future JWST observations of other strong lensing galaxy clusters. These will not only allow us to better constrain the mass distributions of galaxy clusters, but also to study high-redshift galaxies.”

HAE / HOR

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