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First JWST observations of a gravitational lens: Mass model from new multiple images with near-infrared observations of SMACS J0723.3-7327
- Source :
- Caminha, G B, Suyu, S H, Mercurio, A, Brammer, G, Bergamini, P, Acebron, A & Vanzella, E 2022, ' First JWST observations of a gravitational lens Mass model from new multiple images with near-infrared observations of SMACS J0723.3-7327 ', Astronomy & Astrophysics, vol. 666, A9 . https://doi.org/10.1051/0004-6361/202244517
- Publication Year :
- 2022
-
Abstract
- We present our lens mass model of SMACS J0723, the first strong gravitational lens observed by the James Webb Space Telescope (JWST). We use data from the Hubble Space Telescope and Multi Unit Spectroscopic Explorer (MUSE) to build our 'pre-JWST' lens model, and refine it with newly available JWST near-infrared imaging in our JWST model. To reproduce the positions of all multiple lensed images with good accuracy, the adopted mass parameterization consists of one cluster-scale component, accounting mainly for the dark matter distribution, the galaxy cluster members and an external shear component. The pre-JWST model has, as constraints, 19 multiple images from six background sources, of which four have secure spectroscopic redshift measurements from this work. The JWST model has more than twice the number of constraints, 30 additional multiple images from another eleven lensed sources. Both models can reproduce very well the multiple image positions with a $\delta_{rms}$ of $0.39''$ and $0.51''$, for the pre-JWST and JWST models, respectively. The total mass estimates within a radius of 128~kpc (~ the Einstein radius) are $7.9_{-0.2}^{+0.3}\times 10^{13}\rm M_{\odot}$ and $8.7_{-0.2}^{+0.2}\times 10^{13}\rm M_{\odot}$, for the pre-JWST and JWST models, respectively. We predict with our mass models the redshifts of the newly detected JWST sources, which are crucial information for systems without spectroscopic measurements for further studies and follow-up observations. Interestingly, one family detected with JWST is found to be at a very high redshift, $z>7.5$ (68% confidence level) and with one image having lensing magnification of $|\mu|=9.5_{-0.8}^{+0.9}$, making it an interesting case for future studies. The lens models, including magnification maps and redshifts estimated from the model are made publicly available, along with the full spectroscopic redshift catalogue from MUSE.<br />Comment: 5 pages, 2 figures, 1 table, plus appendix. Published in A&A Letters. Lens model and redshift catalogue available at: http://cdsarc.u-strasbg.fr/viz-bin/cat/J/A+A/666/L9
- Subjects :
- COSMOLOGICAL CONSTRAINTS
SAMPLE
Strong Gravitational lensing
WEBB-SPACE-TELESCOPE
FOS: Physical sciences
Galaxy clusters
clusters: individual: SMACS J0723.3-7327 [galaxies]
Astronomy and Astrophysics
MIDINFRARED INSTRUMENT
Astrophysics - Astrophysics of Galaxies
dark matter
PRECISE
Settore FIS/05 - Astronomia e Astrofisica
SMACSJ0723.3−7327
Space and Planetary Science
strong [gravitational lensing]
Astrophysics of Galaxies (astro-ph.GA)
MACS
GALAXY CLUSTERS
HUBBLE CONSTANT
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- Caminha, G B, Suyu, S H, Mercurio, A, Brammer, G, Bergamini, P, Acebron, A & Vanzella, E 2022, ' First JWST observations of a gravitational lens Mass model from new multiple images with near-infrared observations of SMACS J0723.3-7327 ', Astronomy & Astrophysics, vol. 666, A9 . https://doi.org/10.1051/0004-6361/202244517
- Accession number :
- edsair.doi.dedup.....c0623c19535aecf62b4b2c2805a5fdf2
- Full Text :
- https://doi.org/10.1051/0004-6361/202244517