Outputs (5)

The complex case of MACS J0717.5+3745 and its extended filament: intra-cluster light, galaxy luminosity function, and galaxy orientations (2019)
Journal Article
Ellien, A., Durret, F., Adami, C., Martinet, N., Lobo, C., & Jauzac, M. (2019). The complex case of MACS J0717.5+3745 and its extended filament: intra-cluster light, galaxy luminosity function, and galaxy orientations. Astronomy & Astrophysics, 628, Article A34. https://doi.org/10.1051/0004-6361/201935673

Context. The properties of galaxies are known to be aected by their environment, but although galaxies in clusters and groups have been quite thoroughly investigated, little is known about galaxies belonging to filaments of the cosmic web, or about t... Read More about The complex case of MACS J0717.5+3745 and its extended filament: intra-cluster light, galaxy luminosity function, and galaxy orientations.

Observable tests of self-interacting dark matter in galaxy clusters: cosmological simulations with SIDM and baryons (2019)
Journal Article
Robertson, A., Harvey, D., Massey, R., Eke, V., McCarthy, I. G., Jauzac, M., …Schaye, J. (2019). Observable tests of self-interacting dark matter in galaxy clusters: cosmological simulations with SIDM and baryons. Monthly Notices of the Royal Astronomical Society, 488(3), 3646-3662. https://doi.org/10.1093/mnras/stz1815

We present BAHAMAS-SIDM, the first large-volume, (400 h−1 Mpc)3, cosmological simulations including both self-interacting dark matter (SIDM) and baryonic physics. These simulations are important for two primary reasons: 1) they include the effects of... Read More about Observable tests of self-interacting dark matter in galaxy clusters: cosmological simulations with SIDM and baryons.

Dark matter stripping in galaxy clusters: a look at the stellar-to-halo mass relation in the Illustris simulation (2019)
Journal Article
Niemiec, A., Jullo, E., Giocoli, C., Limousin, M., & Jauzac, M. (2019). Dark matter stripping in galaxy clusters: a look at the stellar-to-halo mass relation in the Illustris simulation. Monthly Notices of the Royal Astronomical Society, 487(1), 653-666. https://doi.org/10.1093/mnras/stz1318

Satellite galaxies in galaxy clusters represent a significant fraction of the global galaxy population. Because of the unusual dense environment of clusters, their evolution is driven by different mechanisms than the ones affecting field or central g... Read More about Dark matter stripping in galaxy clusters: a look at the stellar-to-halo mass relation in the Illustris simulation.

Deep and rapid observations of strong-lensing galaxy clusters within the sky localization of GW170814 (2019)
Journal Article
Smith, G., Bianconi, M., Jauzac, M., Richard, J., Robertson, A., Berry, C., …Veitch, J. (2019). Deep and rapid observations of strong-lensing galaxy clusters within the sky localization of GW170814. Monthly Notices of the Royal Astronomical Society, 485(4), 5180-5191. https://doi.org/10.1093/mnras/stz675

We present observations of two strong-lensing galaxy clusters located within the 90 per cent credible sky localization maps released following LIGO-Virgo’s discovery of the binary black hole (BH-BH) gravitational wave (GW) source GW170814. Our object... Read More about Deep and rapid observations of strong-lensing galaxy clusters within the sky localization of GW170814.

RELICS: Strong Lensing Analysis of MACS J0417.5–1154 and Predictions for Observing the Magnified High-redshift Universe with JWST (2019)
Journal Article
Mahler, G., Sharon, K., Fox, C., Coe, D., Jauzac, M., Strait, V., …Zitrin, A. (2019). RELICS: Strong Lensing Analysis of MACS J0417.5–1154 and Predictions for Observing the Magnified High-redshift Universe with JWST. Astrophysical Journal, 873(1), Article 96. https://doi.org/10.3847/1538-4357/ab042b

Strong gravitational lensing by clusters of galaxies probes the mass distribution at the core of each cluster and magnifies the universe behind it. MACS J0417.5−1154 at z = 0.443 is one of the most massive clusters known based on weak lensing, X-ray,... Read More about RELICS: Strong Lensing Analysis of MACS J0417.5–1154 and Predictions for Observing the Magnified High-redshift Universe with JWST.