JWST's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results

Abstract

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 several prime extragalactic survey areas: two fields at the North Ecliptic Pole (NEP); seven gravitationally lensing clusters; two high redshift proto-clusters; and the iconic backlit VV 191 galaxy system to map its dust attenuation. PEARLS also includes NIRISS spectra for one of the NEP fields and NIRSpec spectra of two high-redshift quasars. The main goal of PEARLS is to study the epoch of galaxy assembly, AGN growth, and First Light. Five fields, the JWST NEP Time-Domain Field (TDF), IRAC Dark Field (IDF), and three lensing clusters, will be observed in up to four epochs over a year. The cadence and sensitivity of the imaging data are ideally suited to find faint variable objects such as weak AGN, high-redshift supernovae, and cluster caustic transits. Both NEP fields have sightlines through our Galaxy, providing significant numbers of very faint brown dwarfs whose proper motions can be studied. Observations from the first spoke in the NEP TDF are public. This paper presents our first PEARLS observations, their NIRCam data reduction and analysis, our first object catalogs, the 0.9-4.5 $\mu$m galaxy counts and Integrated Galaxy Light. We assess the JWST sky brightness in 13 NIRCam filters, yielding our first constraints to diffuse light at 0.9-4.5 μm. PEARLS is designed to be of lasting benefit to the community.

Accepted to AJ, comments welcome. We ask anyone who uses our public PEARLS (NEP TDF) data to refer to this overview paper

References in corpus (51)

• Cosmic Star Formation History
• The James Webb Space Telescope
• 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts and Stellar Masses
• The Hubble Ultra Deep Field
• The GLASS James Webb Space Telescope Early Release Science Program. I. Survey Design and Release Plans
• Discovery and properties of ultra-high redshift galaxies ($9<z<12$) in the JWST ERO SMACS 0723 Field
• Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions
• The JWST Early Release Observations
• The Spitzer Deep, Wide-Field Survey
• The Evolution of Galaxy Number Density at z < 8 and its Implications
• UVUDF: Ultraviolet Through Near-infrared Catalog and Photometric Redshifts of Galaxies in the Hubble Ultra Deep Field
• The MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies
• Thermal Emission from Warm Dust in the Most Distant Quasars
• Panic! At the Disks: First Rest-frame Optical Observations of Galaxy Structure at $z>3$ with JWST in the SMACS 0723 Field
• A Highly Magnified Star at Redshift 6.2
• The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deep K-band number counts
• ProFit: Bayesian Profile Fitting of Galaxy Images
• Dust-free quasars in the early Universe
• Galaxy and Mass Assembly (GAMA): Exploring the WISE Cosmic Web in G12
• Galaxy And Mass Assembly (GAMA): Assimilation of KiDS into the GAMA database
• Anomalous Flux in the Cosmic Optical Background Detected With New Horizons Observations
• New Horizons Observations of the Cosmic Optical Background
• JWST Imaging of Earendel, the Extremely Magnified Star at Redshift $z=6.2$
• Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
• Near-Infrared Imaging of a z=6.42 Quasar Host Galaxy With the Hubble Space Telescope Wide Field Camera 3
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Identification of AGN through SED Fitting and the Evolution of the Bolometric AGN Luminosity Function
• The early phases of galaxy clusters formation in IR: coupling hydrodynamical simulations with GRASIL3D
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Consistent multi-wavelength photometry for the DEVILS regions (COSMOS, XMMLSS & ECDFS)
• GAMA/DEVILS: Constraining the cosmic star-formation history from improved measurements of the 0.3-2.2 micron Extragalactic Background Light
• G10/COSMOS: 38 band (far-UV to far-IR) panchromatic photometry using LAMBDAR
• Modelling the cosmic spectral energy distribution and extragalactic background light over all time
• Is there enough star formation in simulated protoclusters?
• Limits to Rest-Frame Ultraviolet Emission From Far-Infrared-Luminous z~6 Quasar Hosts
• Large-scale structure of Lyman break galaxies around a radio galaxy protocluster at z~4
• New Photometric Calibration of the Wide Field Camera 3 Detectors
• SKYSURF: Constraints on Zodiacal Light and Extragalactic Background Light through Panchromatic HST All-Sky Surface-Brightness Measurements: I. Survey Overview and Methods
• Early results from GLASS-JWST VIII: An Extremely Magnified Blue Supergiant Star at Redshift 2.65 in the Abell 2744 Cluster Field
• An Efficient Method for Simulating Light Curves of Cosmological Microlensing and Caustic Crossing Events
• Galaxy And Mass Assembly: Estimating galaxy group masses via caustic analysis
• SKYSURF: Constraints on Zodiacal Light and Extragalactic Background Light through Panchromatic HST All-Sky Surface-Brightness Measurements: II. First Limits on Diffuse Light at 1.25, 1.4, and 1.6 microns
• The isotropic interplanetary dust cloud and near-infrared extragalactic background light observed with COBE/DIRBE
• The NuSTAR Extragalactic Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field
• Molecular gas properties of Planck-selected protocluster candidates at z~1.3-3
• The environments of Ly$\alpha$ blobs I: Wide-field Ly$\alpha$ imaging of TN J1338-1942, a powerful radio galaxy at $z\simeq 4.1$ associated with a giant Ly$\alpha$ nebula
• High resolution science with high redshift galaxies
• The Effect of Atmospheric Cooling on the Vertical Velocity Dispersion and Density Distribution of Brown Dwarfs
• Galactic Latitude Dependence of Near-Infrared Diffuse Galactic Light : Thermal Emission or Scattered Light?
• Questioning Planck-selected star-forming high-redshift galaxy protoclusters and their fate
• Towards a data-driven model of the sky from low Earth orbit as observed by the Hubble Space Telescope
• SKYSURF-3: Testing Crowded Object Catalogs in the Hubble eXtreme Deep Field Mosaics to Study Sample Incompleteness from an Extragalactic Background Light Perspective
• On-orbit Performance of the Spitzer Space Telescope: Science Meets Engineering

Cited by in corpus (67)

• JWST UNCOVER: Extremely red and compact object at$z_{\mathrm{phot}}\simeq 7.6$ triply imaged by Abell 2744
• The GLASS-JWST Early Release Science Program. III. Strong lensing model of Abell 2744 and its infalling regions
• Inferring More from Less: Prospector as a Photometric Redshift Engine in the Era of JWST
• EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations
• JWST's PEARLS: a new lens model for ACT-CL J0102$-$4915, "EL Gordo'', and the first red supergiant star at cosmological distances discovered by JWST
• EPOCHS VII: Discovery of high redshift ($6.5<z<12$) AGN candidates in JWST ERO and PEARLS data
• Lensed Type Ia Supernova "Encore" at z=2: The First Instance of Two Multiply-Imaged Supernovae in the Same Host Galaxy
• Galaxy Mergers in the Epoch of Reionization I: A JWST Study of Pair Fractions, Merger Rates, and Stellar Mass Accretion Rates at $z=4.5-11.5$
• How dark the sky: the JWST backgrounds
• JWST's PEARLS: Mothra, a new kaiju star at z=2.091 extremely magnified by MACS0416, and implications for dark matter models
• JWST Photometric Time-Delay and Magnification Measurements for the Triply-Imaged Type Ia "Supernova H0pe" at z = 1.78
• JWST's PEARLS: A JWST/NIRCam view of ALMA sources
• A state-of-the-art strong lensing model of MACS J0416.1-2403 with the largest sample of spectroscopic multiple images
• Observability of Low-Luminosity AGN in the Early Universe with JWST
• Anatomy of a z=6 Lyman-α emitter down to parsec scales: extreme UV slopes, metal-poor regions and possibly leaking star clusters
• Paper 1: The JWST PEARLS View of the El Gordo Galaxy Cluster and of the Structure It Magnifies
• JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at $z=0.4$
• Statistics of magnification for extremely lensed high redshift stars
• Webb's PEARLS: Bright 1.5--2.0 micron Dropouts in the Spitzer/IRAC Dark Field
• Anatomy of an ionized bubble: NIRCam grism spectroscopy of the $z=6.6$ double-peaked Lyman-$\alpha$ emitter COLA1 and its environment
• Extreme Ionizing Properties of Metal-Poor, Muv ~ -12 Star Complex in the first Gyr
• Dust-free starburst galaxies at redshifts $z>10$
• JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noon
• Strong limits on keV-scale galactic sterile neutrino dark matter with stray light from NuSTAR after 11 years of operation
• JWST's PEARLS: dust attenuation and gravitational lensing in the backlit-galaxy system VV 191
• On the detectability of strong lensing in near-infrared surveys
• Lonely Little Red Dots: Challenges to the AGN-nature of little red dots through their clustering and spectral energy distributions
• CANUCS: Constraining the MACS J0416.1-2403 Strong Lensing Model with JWST NIRISS, NIRSpec and NIRCam
• HEROES: The Hawaii eROSITA Ecliptic Pole Survey Catalog
• Novel bounds on decaying axionlike particle dark matter from the cosmic background
• Spectroscopy of the Supernova H0pe Host Galaxy at Redshift 1.78
• ΛCDM is still not broken: empirical constraints on the star formation efficiency at z ~ 12-30
• PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field II
• J-NEP: 60-band photometry and photometric redshifts for the James Webb Space Telescope North Ecliptic Pole Time-Domain Field
• A model for galaxy-galaxy strong lensing statistics in surveys
• SKYSURF-4: Panchromatic HST All-Sky Surface-Brightness Measurement Methods and Results
• The impact of medium-width bands on the selection, and subsequent luminosity function measurements, of high-z galaxies
• Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim 9-17$
• The BoRG-$JWST$ Survey: Abundance and Mass-to-light Ratio of Luminous $z=7-9$ Galaxies from Independent Sight Lines with NIRSpec
• NOEMA reveals the true nature of luminous red JWST z>10 galaxy candidates
• Galaxy Mergers in the Epoch of Reionization II: Major Merger-Triggered Star Formation and AGN Activities at $z=$ 4.5-8.5
• El Gordo needs El Anzuelo: Probing the structure of cluster members with multi-band extended arcs in JWST data
• PEARLS: Low Stellar Density Galaxies in the El Gordo Cluster Observed with JWST
• Microlensing at Cosmological Distances: Event Rate Predictions in the Warhol Arc of MACS 0416
• BUFFALO Wild Wings: A High Precision Free-Form Lens Model of MACSJ0416 with Constraints on Dark Matter from Substructure and Highly Magnified Arcs
• Heliocentric Distance Dependence of Zodiacal Light Observed by Hayabusa2#
• Cosmic Stillness: High Quiescent Galaxy Fractions Across Upper Mass Scales in the Early Universe to z = 7 with JWST
• Deep Large Binocular Camera r-band Observations of the GOODS-N Field
• JWST's PEARLS: A z=6 quasar in a train-wreck galaxy merger system
• JWSTs PEARLS: NIRCam imaging and NIRISS spectroscopy of a $z=3.6$ star-forming galaxy lensed into a near-Einstein Ring by a $z=1.258$ massive elliptical galaxy
• Galaxy-scale lens search in the PEARLS NEP TDF and CEERS JWST fields
• PEARLS: Discovery of Point-Source Features Within Galaxies in the North Ecliptic Pole Time Domain Field
• Magellanic System Stars Identified in SMACS J0723.3-7327 James Webb Space Telescope Early Release Observations Images
• Searching for Intragroup Light in Deep U-band Imaging of the COSMOS Field
• Testing Lens Models of PLCK G165.7+67.0 Using Lensed SN H0pe
• NEXUS: A Search for Nuclear Variability with the First Two JWST NIRCam Epochs
• MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components
• Nature of High Equivalent Width Emitters in the Epoch of Reionization Revealed by JWST Medium-band Imaging
• The Herschel-SPIRE Dark Field I: The deepest Herschel image of the submillimetre Universe
• Galaxies at the edges: a complete census of MACS J0416.1-2403 cluster
• Transient star B/R ratio and star formation in $z\gtrsim 1$ lensed galaxies
• SKYSURF-11: A New Zodiacal Light Model Optimized for Optical Wavelengths
• Strong Lensing Model and Dust Extinction Maps of the Host Galaxy of Type Ia Supernova H0pe
• Intermediate-mass black holes and contribution to extragalactic background light from Population III stars in Milky Way-like galaxies
• The $N_H$ Distribution of Hard X-ray Selected AGN in the NEP Field
• Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference
• Magnification bias reveals severe contamination in Hubble Frontier Field photo-z catalogs