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Massive foreground galaxy clusters magnify and distort the light of objects behind them, permitting a view into both the extremely distant and intrinsically faint galaxy populations. We present here the z ~ 6 - 8 candidate high-redshift…

Surveys with James Webb Space Telescope (JWST) have discovered candidate galaxies in the first 400 Myr of cosmic time. Preliminary indications have suggested these candidate galaxies may be more massive and abundant than previously thought.…

We present accurate photometric redshifts for galaxies observed by the Cluster Lensing and Supernova survey with Hubble (CLASH). CLASH observed 25 massive galaxy cluster cores with the Hubble Space Telescope in 16 filters spanning 0.2 - 1.7…

The discovery both through spectroscopy and photometry of multiple stellar populations in Galactic globular clusters, and in Magellanic Clouds' massive intermediate-age and old clusters, has led to a major change in our views about the…

Solar and Stellar Astrophysics · Physics 2019-09-11 M. Salaris , S. Cassisi , A. Mucciarelli , D. Nardiello

The inner hundred parsecs of the Milky Way hosts the nearest supermassive black hole, largest reservoir of dense gas, greatest stellar density, hundreds of massive main and post main sequence stars, and the highest volume density of…

Astrophysics of Galaxies · Physics 2025-10-15 Rainer Schoedel , Steve Longmore , Jonny Henshaw , Adam Ginsburg , John Bally , Anja Feldmeier , Matt Hosek , Francisco Nogueras Lara , Anna Ciurlo , Mélanie Chevance , J. M. Diederik Kruijssen , Ralf Klessen , Gabriele Ponti , Pau Amaro-Seoane , Konstantina Anastasopoulou , Jay Anderson , Maria Arias , Ashley T. Barnes , Cara Battersby , Giuseppe Bono , Lucía Bravo Ferres , Aaron Bryant , Miguel Cano Gonzáalez , Santi Cassisi , Leonardo Chaves-Velasquez , Francesco Conte , Rodrigo Contreras Ramos , Angela Cotera , Samuel Crowe , Enrico di Teodoro , Tuan Do , Frank Eisenhauer , Rei Enokiya , Rubén Fedriani , Jennifer K. S. Friske , Dimitri Gadotti , Carme Gallart , Teresa Gallego Calvente , Eulalia Gallego Cano , Pablo García Fuentes , Macarena García Marín , Angela Gardini , Abhimat K. Gautam , Andrea Ghez , Stefan Gillessen , Naoteru Gouda , Alessia Gualandris , Mario Giuseppe Guarcello , Robert Gutermuth , Daryl Haggard , Matthew Hankins , Yue Hu , Rebecca Houghton , Ryohei Kano , Jens Kauffmann , Ryan Lau , Alexandre Lazarian , Rebecca Levy , Mattia Libralato , Anan Lu , Xing Lu , Jessica R. Lu , Nora Luetzgendorf , John Magorrian , Shifra Mandel , Sera Markoff , Álvaro Martínez Arranz , Alessandra Mastrobuono-Battisti , Maria Melamed , Elisabeth Mills , Kaya Mori , Mark Morris , Elena Murchikova , Tetsuya Nagata , Francisco Najarro , Govind Nandakumar , David Nataf , Nadine Neumayer , Shogo Nishiyama , Masayoshi Nobukawa , Dylan M Paré , Florian Peissker , Maya Petkova , Thushara G. S. Pillai , Mike Rich Carlos Román , Michael Rugel , Nils Ryde , Nadeen Sabha , Joel Sánchez Bermúdez , Álvaro Sánchez-Monge , Mathias Schultheis , Lijing Shao , Hiroko Shinnaga , Janet Simpson , Mattia C. Sormani , Shunya Takekawa , Jonathan C. Tan , Sabine Thater , Brian Thorsbro , Pablo Torne , Robin Goppala Tress , Hideki Uchiyam , Elena Valenti , Roeland van der Marel , Sill Verberne , Pierre Vermot , Sebastiano von Fellenberg , Daniel Walker , Gunther Witzel , Siyao Xu , Taihei Yano , Farhad Yusef-Zadeh , Michal Zajaček , Manuela Zoccali

The NIRCam instrument on the upcoming James Webb Space Telescope (JWST) will offer an unprecedented view of the most distant galaxies. In preparation for future deep NIRCam extragalactic surveys, it is crucial to understand the color…

We present here an efficient method for selecting high luminosity and massive high redshift clusters of galaxies, crucially important tools in cosmology. By selecting bright and extremely X-ray loud (high F(X)/F(V)) sources, we were able to…

Astrophysics · Physics 2007-05-23 I. Cagnoni , M. Elvis , D. -W. Kim , P. Mazzotta , J. -S. Huang , A. Celotti

Gravitationally lensed galaxies with magnification ~10-100 are routinely detected at high redshifts, but magnifications significantly higher than this are hampered by a combination of low probability and large source sizes. Magnifications…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-23 Erik Zackrisson , Juan Gonzalez , Simon Eriksson , Saghar Asadi , Chalence Safranek-Shrader , Michele Trenti , Akio K. Inoue

We investigate the gravitational lensing properties of lines of sight containing multiple cluster-scale halos, motivated by their ability to lens very high-redshift (z ~ 10) sources into detectability. We control for the total mass along…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Kenneth C. Wong , S. Mark Ammons , Charles R. Keeton , Ann I. Zabludoff

We present the clump populations detected in 18 lensed galaxies at redshifts 1 to 8.5 within the lensing cluster field SMACS0723. The recent JWST Early Release Observations of this poorly known region of the sky have revealed numerous…

The James Webb Space Telescop (JWST) promises to revolutionise our understanding of the early Universe, and contrasting its upcoming observations with predictions of the $\Lambda$CDM model requires detailed theoretical forecasts. Here, we…

Recent data from the James Webb Space Telescope allow a first glimpse of galaxies at $z \gtrsim 11$. The most successful tool for identifying ultra-high-redshift candidates and inferring their properties is photometric template fitting.…

Astrophysics of Galaxies · Physics 2023-07-19 Charles L. Steinhardt , Vasily Kokorev , Vadim Rusakov , Ethan Garcia , Albert Sneppen

As the densest galaxy environments in the universe, clusters are vital to our understanding of the role that environment plays in galaxy formation and evolution. Unfortunately, the evolution of high-redshift cluster galaxies is poorly…

Wide-field optical imaging surveys are efficient at identifying galaxy clusters, but optically identified clusters suffer from projection effects--physically unassociated galaxies along the line of sight can be misidentified as cluster…

Cosmology and Nongalactic Astrophysics · Physics 2026-04-02 Lei Yang , Hao-Yi Wu , Tesla Jeltema , Chun-Hao To , Ross Cawthon , Shulei Cao

We present a first strong-lensing model for the galaxy cluster RM J121218.5+273255.1 ($z=0.35$; hereafter RMJ1212; also known as Abell 1489). This cluster is amongst the top 0.1\% richest clusters in the redMaPPer catalog; it is…

We forecast constraints on the amplitude of matter clustering sigma_8(z) achievable with the combination of cluster weak lensing and number counts, in current and next-generation weak lensing surveys. We advocate an approach, analogous to…

Cosmology and Nongalactic Astrophysics · Physics 2021-03-29 Hao-Yi Wu , David H. Weinberg , Andrés N. Salcedo , Benjamin D. Wibking

Small galaxies consisting entirely of population III (pop III) stars may form at high redshifts, and could constitute one of the best probes of such stars. Here, we explore the prospects of detecting gravitationally lensed pop III galaxies…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 E. Zackrisson , A. Zitrin , M. Trenti , C. -E. Rydberg , L. Guaita , D. Schaerer , T. Broadhurst , G. Ostlin , T. Strom

We present the first three galaxy clusters of a larger sample of the most X-ray luminous galaxy clusters selected from the ROSAT Bright Survey. This project, which is a systematic search for strong lensing, aims at arc statistics, mass…

Astrophysics · Physics 2009-11-10 W. Kausch , S. Schindler , T. Kronberger , J. Wambsganss , A. Schwope , T. Erben , ;

As the James Webb Space Telescope (JWST) has become fully operational, early-release data are now available to begin building the tools and calibrations for precision point-source photometry and astrometry in crowded cluster environments.…

Solar and Stellar Astrophysics · Physics 2022-09-28 D. Nardiello , L. R. Bedin , A. Burgasser , M. Salaris , S. Cassisi , M. Griggio , M. Scalco