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Related papers: CANUCS/Technicolor Data Release 1: Imaging, Photom…

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In the third paper of this series aimed at developing the tools for analysing resolved stellar populations using the cameras on board of the James Webb Space Telescope (JWST), we present a detailed multi-band study of the 2 Gyr Galactic…

Solar and Stellar Astrophysics · Physics 2023-08-22 D. Nardiello , L. R. Bedin , M. Griggio , M. Salaris , M. Scalco , S. Cassisi

The Grism Lens-Amplified Survey from Space (GLASS) is a Hubble Space Telescope (HST) Large Program, which will obtain 140 orbits of grism spectroscopy of the core and infall regions of 10 galaxy clusters, selected to be among the very best…

The 3D-HST and CANDELS programs have provided WFC3 and ACS spectroscopy and photometry over ~900 square arcminutes in five fields: AEGIS, COSMOS, GOODS-North, GOODS-South, and the UKIDSS UDS field. All these fields have a wealth of publicly…

We present the Snapshot Hubble U-band Cluster Survey (SHUCS), a project aimed at characterizing the star cluster populations of ten nearby galaxies (d<23 Mpc, half within 12 Mpc) through new F336W (U band equivalent) imaging from WFC3, and…

One way to constrain the evolutionary histories of galaxies is to analyse their stellar populations. In the local Universe, our understanding of the stellar population properties of galaxies has traditionally relied on the study of optical…

We use CFHTLS deep optical data, WIRCam Deep Survey (WIRDS) NIR data and XMM data to identify z>1.1 clusters in the CFHTLS D1 and D4 fields. Counterparts to such clusters can not be identified without deep NIR data and as such the total of…

We give an overview and describe the rationale, methods, and first results from NIRCam images of the JWST "Prime Extragalactic Areas for Reionization and Lensing Science" ("PEARLS") project. PEARLS uses up to eight NIRCam filters to survey…

Cosmology and Nongalactic Astrophysics · Physics 2022-12-21 Rogier A. Windhorst , Seth H. Cohen , Rolf A. Jansen , Jake Summers , Scott Tompkins , Christopher J. Conselice , Simon P. Driver , Haojing Yan , Dan Coe , Brenda Frye , Norman Grogin , Anton Koekemoer , Madeline A. Marshall , Rosalia O'Brien , Nor Pirzkal , Aaron Robotham , Russell E. Ryan, , Christopher N. A. Willmer , Timothy Carleton , Jose M. Diego , William C. Keel , Paolo Porto , Caleb Redshaw , Sydney Scheller , Stephen M. Wilkins , S. P. Willner , Adi Zitrin , Nathan J. Adams , Duncan Austin , Richard G. Arendt , John F. Beacom , Rachana A. Bhatawdekar , Larry D. Bradley , Thomas J. Broadhurst , Cheng Cheng , Francesca Civano , Liang Dai , Herve Dole , Jordan C. J. D'Silva , Kenneth J. Duncan , Giovanni G. Fazio , Giovanni Ferrami , Leonardo Ferreira , Steven L. Finkelstein , Lukas J. Furtak , Hansung B. Gim , Alex Griffiths , Heidi B. Hammel , Kevin C. Harrington , Nimish P. Hathi , Benne W. Holwerda , Rachel Honor , Jia-Sheng Huang , Minhee Hyun , Myungshin Im , Bhavin A. Joshi , Patrick S. Kamieneski , Patrick Kelly , Rebecca L. Larson , Juno Li , Jeremy Lim , Zhiyuan Ma , Peter Maksym , Giorgio Manzoni , Ashish Kumar Meena , Stefanie N. Milam , Mario Nonino , Massimo Pascale , Justin D. R. Pierel , Andreea Petric , Maria del Carmen Polletta , Huub J. A. Rottgering , Michael J. Rutkowski , Ian Smail , Amber N. Straughn , Louis-Gregory Strolger , Andi Swirbul , James A. A. Trussler , Lifan Wang , Brian Welch , J. Stuart B. Wyithe , Min Yun , Erik Zackrisson , Jiashuo Zhang , Xiurui Zhao

The next generation of data-intensive surveys are bound to produce a vast amount of data, which can be dealt with using machine-learning methods to explore possible correlations within the multi-dimensional parameter space. We explore the…

We present a first-look analysis of the JWST ERO data in the SMACS J0723.3-7327 cluster field. We begin by reporting 10 new spectroscopic redshifts from $\lambda_\mathrm{obs}=1.8-5.2\mu$m NIRSpec medium-resolution ($R=\lambda/\Delta\lambda…

The Munich Near-IR Cluster Survey (MUNICS) is a wide-area, medium-deep, photometric survey selected in the K' band. It covers an area of roughly one square degree in the K' and J near-IR pass-bands. The survey area consists of 16 6' x 6'…

We present the construction of a deep multi-wavelength PSF-matched photometric catalog in the UDS field following the final UKIDSS UDS DR11 release. The catalog includes photometry in 24 filters, from the MegaCam-uS (0.38 microns) band to…

NEXUS is a JWST Multi-Cycle (Cycles 3-5; 368 primary hrs) GO Treasury imaging and spectroscopic survey around the North Ecliptic Pole. It contains two overlapping tiers. The Wide tier ($\sim 400~{\rm arcmin}^2$) performs NIRCam/WFSS 2.4-5…

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 use images collected with the near-infrared camera (NIRCam) on board the James Webb Space Telescope and with the Hubble Space Telescope (HST) to investigate multiple populations at the bottom of the main sequence (MS) of 47 Tucanae. The…

On 2022 July 8, NASA shared$^{a}$ the list of five public showcase targets which have been observed with the new \textit{James Webb Space Telescope} (JWST), and whose data are expected to be released to the public around Tuesday, July 12.…

Cosmology and Nongalactic Astrophysics · Physics 2022-10-26 Miriam Golubchik , Lukas J. Furtak , Ashish K. Meena , Adi Zitrin

The Galactic Centre is of fundamental astrophysical interest, but existing near-infrared surveys fall short to cover it adequately. We introduce the GALACTICNUCLEUS survey, a $JHK_s$ imaging survey of the centre of the Milky Way with a…

We present the fourth data release of JADES, the JWST Advanced Deep Extragalactic Survey, providing deep spectroscopic observations in the two GOODS fields. A companion paper presents the target selection, spectroscopic redshifts and…