activity
20202026
most citedJWST's PEARLS: Mothra, a new kaiju star at z=2.091 extremely magnified by MACS0416, and implications for dark matter models

44 citations · 56 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2026

The Roman eXtreme Deep Field (RXDF)

Haojing Yan, Anton M. Koekemoer, Yue Shen +127

The Roman eXtreme Deep Field (RXDF) program is one of the five General Astrophysics Survey (GAS) programs approved for observing time with the Nancy Grace Roman Space Telescope in…

astro-ph.GA2026

JWST's PEARLS: A clumpy ring galaxy at

David Vizgan, Ming-Yang Zhuang, Ian Smail +22

Ring galaxies are an uncommon class of galaxies whose morphology is closely related to dynamical processes that govern galaxy evolution. Some ring galaxies, known as "collisional r…

astro-ph.GA2025

Point-like and Narrow-lined: A Potentially New Population of Objects Discovered by JWST

Haojing Yan, Bangzheng Sun, Riley Shive

We report a potentially new population of objects revealed by the data from the James Webb Space Telescope, which are characterized by their point-like morphology and narrow permit…

astro-ph.GA2025

New Insight from the James Webb Space Telescope on Variable Active Galactic Nuclei

Bangzheng Sun, Haojing Yan, Wei Leong Tee +1

Variability detected in galaxies is usually attributed to their active galactic nuclei (AGNs). While all AGNs are intrinsically variable, the AGN unification model predicts that ty…

astro-ph.GA2025

JWST's PEARLS: A Candidate Massive Binary Star System in a Lensed Galaxy at Redshift 0.94

Hayley Williams, Patrick L. Kelly, Emmanouil Zapartas +18

Massive stars at cosmological distances can be individually detected during transient microlensing events, when gravitational lensing magnifications may exceed ~1000. Nine such sou…

astro-ph.GA2025★ 1 cited

JWST's PEARLS: Temperatures of Nine Highly Magnified Stars in a Galaxy at Redshift 0.94 and Simulated Stellar Population Dependence on Stellar Metallicity and the Initial Mass Function

Hayley Williams, Patrick L. Kelly, Rogier A. Windhorst +17

We present stellar atmosphere modeling of JWST NIRCam photometry of nine highly magnified individual stars in a single galaxy at redshift z=0.94 known as the Warhol arc, which is s…

astro-ph.GA2025

PEARLS: 21 Transients Found in the Three-Epoch NIRCam Observations in the Continuous Viewing Zone of the James Webb Space Telescope

Haojing Yan, Bangzheng Sun, Zhiyuan Ma +39

We present 21 transients from our three-epoch, four-band NIRCam observations covering 14.16 arcmin^2 in the Spitzer IRAC Dark Field (IDF), taken by the JWST Prime Extragalactic Are…

astro-ph.CO2025

Constraining the z 1 Initial Mass Function with {\it HST} and {\it JWST} Lensed Stars in MACS J0416.1-2403

Sung Kei Li, Jose M. Diego, Ashish K. Meena +19

Our understanding of galaxy properties and evolution is contingent on knowing the initial mass function (IMF), and yet to date, the IMF is constrained only to local galaxies. Indiv…

astro-ph.GA2025

A Mysteriously Tight H-[O III] Correlation and Non-Case B Balmer Decrements Revealed by the Spectra from the James Webb Space Telescope NIRSpec Instrument

Bangzheng Sun, Haojing Yan

We report an extremely tight, linear relation between and [O~III] line fluxes in logarithm, discovered using a large sample of low and mid-resolution spectra (totaling 5…

astro-ph.GA2025

On The Very Bright Dropouts Selected Using the James Webb Space Telescope NIRCam Instrument

Bangzheng Sun, Haojing Yan

The selection of candidate high-redshift galaxies using the dropout technique targeting the Lyman-break signature sometimes yields very bright objects that are too luminous to be e…

astro-ph.GA2024

An Edge-on Regular Disk Galaxy at z=5.289

Haojing Yan, Bangzheng Sun, Chenxiaoji Ling

While rotation-supported gas disks are known to exist as early as at z ~ 7, it is still a general belief that stellar disks form late in the Universe. This picture is now being cha…

astro-ph.GA2024

JWST view of four infant galaxies at z=8.31-8.49 in the MACS0416 field and implications for reionization

Zhiyuan Ma, Bangzheng Sun, Cheng Cheng +34

New JWST/NIRCam wide-field slitless spectroscopy provides redshifts for four z>8 galaxies located behind the lensing cluster MACS J0416.1-2403. Two of them, "Y1" and "JD", have pre…

astro-ph.GA2024

A Strongly Lensed Dusty Starburst of an Intrinsic Disk Morphology at Photometric Redshift of

Chenxiaoji Ling, Bangzheng Sun, Cheng Cheng +3

We present COSBO-7, a strong millimeter (mm) source known for more than sixteen years but was just revealed its near-to-mid-IR counterpart by the James Webb Space Telescope (JWST).…

astro-ph.GA2023

Candidate Galaxies at z ~ 11.3--21.8 and beyond: results from JWST's public data taken in its first year

Haojing Yan, Bangzheng Sun, Zhiyuan Ma +1

We present a systematic search of candidate galaxies at z > 11.3 using the public Near Infrared Camera data taken by the James Webb Space Telescope (JWST) in its Cycle 1, which inc…

astro-ph.IM2023

JWST's PEARLS: Improved Flux Calibration for NIRCam

Zhiyuan Ma, Haojing Yan, Bangzheng Sun +23

The Prime Extragalactic Areas for Reionization and Lensing Science (PEARLS), a JWST GTO program, obtained a set of unique NIRCam observations that have enabled us to significantly…

astro-ph.CO2023★ 44 cited

JWST's PEARLS: Mothra, a new kaiju star at z=2.091 extremely magnified by MACS0416, and implications for dark matter models

J. M. Diego, Bangzheng Sun, Haojing Yan +28

We report the discovery of Mothra, an extremely magnified monster star, likely a binary system of two supergiant stars, in one of the strongly lensed galaxies behind the galaxy clu…

astro-ph.GA2023★ 3 cited

JWST's PEARLS: Transients in the MACS J0416.1-2403 Field

Haojing Yan, Zhiyuan Ma, Bangzheng Sun +27

With its unprecedented sensitivity and spatial resolution, the James Webb Space Telescope (JWST) has opened a new window for time-domain discoveries in the infrared. Here we report…

astro-ph.HE2020★ 8 cited

X-ray Spectra and Light Curves of Cooling Novae and a Nova-Like

Bangzheng Sun, Marina Orio, Andrej Dobrotka +3

We present X-ray observations of novae V2491 Cyg and KT Eri about 9 years post-outburst, of the dwarf nova and post-nova candidate EY Cyg, and of a VY Scl variable. The first three…