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相关论文: The First Weak-lensing Analysis with the James Web…

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We report the discovery of an intriguing, low-mass galaxy-scale strong-lens system in the SMACS J0723.3-7327 galaxy cluster. By modeling James Webb Space Telescope imaging and Very Large Telescope Multi-Unit Spectroscopic Explorer…

星系天体物理 · 物理学 2025-04-28 Limeng Deng , Yiping Shu , Lei Wang , Guoliang Li , Gabriel Bartosch Caminha , Jiang Dong , Zizhao He , Han Qu , Ruibiao Luo

We report the first weak-lensing detection of a large-scale filament funneling matter onto the core of the massive galaxy cluster MACSJ0717.5+3745. Our analysis is based on a mosaic of 18 multi-passband images obtained with ACS aboard the…

We present a weak lensing analysis of the X-ray luminous cluster CL 0152-1357 at z~0.84 using HST/ACS observations. The unparalleled resolution and sensitivity of ACS enable us to measure weakly distorted, faint background galaxies to the…

天体物理学 · 物理学 2014-10-13 M. J. Jee , R. L. White , N. Benitez , H. C. Ford , J. P. Blakeslee , P. Rosati , R. Demarco , G. D. Illingworth

Exploiting the fundamentally achromatic nature of gravitational lensing, we present a lens model for the massive galaxy cluster SMACSJ0723.3-7323 (SMACSJ0723, z=0.388) that significantly improves upon earlier work. Building on…

SMACS~J0723.3-7327 is the first galaxy cluster lens observed by JWST. Based on the ERO data from JWST, several groups have reported the results on strong lensing analysis and mass distribution of this cluster. However, limited by the…

宇宙学与河外天体物理 · 物理学 2023-02-15 A. Liu , E. Bulbul , M. E. Ramos-Ceja , J. S. Sanders , V. Ghirardini , Y. E. Bahar , M. Yeung , E. Gatuzz , M. Freyberg , C. Garrel , X. Zhang , A. Merloni , K. Nandra

We present a combined strong and weak gravitational-lensing analysis of the massive galaxy cluster MACS J1423.8+2404 ($z=0.545$, MACS J1423 hereafter), one of the most dynamically relaxed and massive cool-core clusters discovered in the…

We use the unprecedented resolution and depth of the JWST NIRCam Early Release Observations at 1-5 $\mu$m to study the stellar mass, age, and metallicity of compact star clusters in the neighborhood of the host galaxies in the SMACS…

星系天体物理 · 物理学 2022-12-14 Andreas L. Faisst , Ranga Ram Chary , Gabriel Brammer , Sune Toft

We identify 71 distant stars in JWST/NIRCam ERO images of the field of galaxy cluster SMACS J0723.3-7327 (SMACS 0723). Given the relatively small ($\sim$$10^{\circ}$) angular separation between SMACS 0723 and the Large Magellanic Cloud, it…

Context: In 2.2m MPG-ESO/WFI data we discovered several mass peaks through weak lensing, forming a possible supercluster at redshift 0.45. Through multi-colour wide-field imaging with CFHT/Megaprime and INT/WFC we identify early-type…

宇宙学与河外天体物理 · 物理学 2011-07-25 Mischa Schirmer , Hendrik Hildebrandt , Konrad Kuijken , Thomas Erben

We use weak gravitational lensing to measure the masses of five galaxy clusters selected from the South Pole Telescope (SPT) survey, with the primary goal of comparing these with the SPT Sunyaev--Zel'dovich (SZ) and X-ray based mass…

We present a parametric strong lensing modeling of the galaxy cluster MS\,0440.5+0204 (located at $z$ = 0.19). We have performed a strong lensing mass reconstruction of the cluster using three different models. The first model uses the…

宇宙学与河外天体物理 · 物理学 2020-07-08 Tomás Verdugo , Eleazar R. Carrasco , Gael Foëx , Verónica Motta , Percy L. Gomez , Marceau Limousin , Juan Magaña , José A. de Diego

Galaxy cluster mass distributions are useful probes of Omega_0 and the nature of the dark matter. Large clusters will distort the observed shapes of background galaxies through gravitational lensing allowing the measurement of the cluster…

天体物理学 · 物理学 2009-10-31 Philippe Fischer

We present results of a strong-lensing analysis of MACS J0717.5+3745 (hereafter MACS J0717), an extremely X-ray luminous galaxy cluster at z=0.55. Observations at different wavelengths reveal a complex and dynamically very active cluster,…

宇宙学与河外天体物理 · 物理学 2015-05-30 M. Limousin , H. Ebeling , J. Richard , A. M. Swinbank , G. P. Smith , M. Jauzac , S. Rodionov , C. -J. Ma , I. Smail , A. C. Edge , E. Jullo , J. P. Kneib

This paper highlights initial photometric analyses of JWST NIRCam imaging data in the sightline of SMACS0723, aiming to identify galaxies at redshift $z>7$. By applying a conservative Lyman-break selection followed by photometric redshift…

星系天体物理 · 物理学 2023-04-12 Takahiro Morishita , Massimo Stiavelli

We perform a weak lensing and photometric study of the z=0.42 supercluster MS0302+17 using deep I and V band images taken with the UH8K CCD mosaic camera at the CFHT. We use archival ROSAT HRI data to estimate fluxes, gas masses and, in one…

天体物理学 · 物理学 2007-05-23 N. Kaiser , G. Wilson , G. Luppino , L. Kofman , I. Gioia , M. Metzger , H. Dahle

The first deep field images from the James Webb Space Telescope (JWST) of the galaxy cluster SMACS~J0723.3-7327 reveal a wealth of new lensed images at uncharted infrared wavelengths, with unprecedented depth and resolution. Here we…

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…

星系天体物理 · 物理学 2022-10-14 G. B. Caminha , S. H. Suyu , A. Mercurio , G. Brammer , P. Bergamini , E. Vanzella , A. Acebron

We present a mass estimate of the Planck-discovered cluster PLCK G100.2-30.4, derived from a weak lensing analysis of deep SUBARU griz images. We perform a careful selection of the background galaxies using the multi-band imaging data, and…

The first science image released by the JWST reveals numerous galaxies in the distant background of the galaxy cluster SMACS J0723.3-7327. Some have claimed redshifts of up to $z \simeq 20$, challenging standard cosmological models for…

We present early results regarding the morphological and structural properties of galaxies seen with the James Webb Space Telescope at $z > 3$ in the Early Release Observations of SMACS 0723, a galaxy cluster at $z=0.39$. We investigate,…

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