Imagen de Portada

The First Photometric Evidence of a Transient/Variable Source at z>5 with JWST

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	DeCoursey, Christa, Egami, Eiichi, Sun, Fengwu, Akhtarkavan, Arshia, Bhatawdekar, Rachana, Bunker, Andrew J., Coulter, David A., Engesser, Michael, Fox, Ori D., Gomez, Sebastian, Inayoshi, Kohei, Johnson, Benjamin D., Karmen, Mitchell, Larison, Conor, Lin, Xiaojing, Lyu, Jianwei, Mattila, Seppo, Moriya, Takashi J., Pierel, Justin D. R., Puskás, Dávid, Rest, Armin, Rieke, George H., Robertson, Brant, Salamat, Sepehr, Strolger, Louis-Gregory, Tacchella, Sandro, Vassallo, Christian, Williams, Christina C., Zenati, Yossef, Zhang, Junyu
Formato:	Preprint
Publicado:	2025
Materias:	High Energy Astrophysical Phenomena Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Properties of high-redshift Type II supernovae discovered by the JADES transient survey
por: Moriya, Takashi J., et al.
Publicado: (2025)

The Reliability of Type Ia Supernovae Delay Time Distributions Recovered from Galaxy Star Formation Histories
por: Joshi, Bhavin A., et al.
Publicado: (2024)

Discovery of a likely Type II SN at $z$=3.6 with JWST
por: Coulter, D. A., et al.
Publicado: (2025)

The JADES Transient Survey: Discovery and Classification of Supernovae in the JADES Deep Field
por: DeCoursey, Christa, et al.
Publicado: (2024)

SN 2025ogs: A Spectroscopically-Normal Type Ia Supernova at z = 2 as a Benchmark for Redshift Evolution
por: Siebert, M. R., et al.
Publicado: (2025)

Discovery of a Relativistic Stripped Envelope Type Ic-BL Supernova at z = 2.83 with JWST
por: Siebert, M. R., et al.
Publicado: (2024)

Discovery of An Apparent Red, High-Velocity Type Ia Supernova at z = 2.9 with JWST
por: Pierel, J. D. R., et al.
Publicado: (2024)

The Structure of Poloidal Fields Embedded in Thin Disks
por: Zenati, Yossef, et al.
Publicado: (2026)

Distinct First-to-Second Peak Yield Ratios and Timescales Reveal a Sub-dominant Prompt Channel
por: Zenati, Yossef, et al.
Publicado: (2026)

Revisiting the Mass Step: Environmental Dependence of Type Ia Supernovae in Low-Metallicity Host Galaxies
por: Gonzalez, Estefania Padilla, et al.
Publicado: (2025)

Thermal Evolution of the Central Star in Pa 30
por: Piro, Anthony L., et al.
Publicado: (2026)

Identification of High-Redshift Galaxy Overdensities in GOODS-N and GOODS-S
por: Helton, Jakob M., et al.
Publicado: (2023)

ATClean: A Novel Method for Detecting Low-Luminosity Transients and Application to Pre-explosion Counterparts from SN 2023ixf
por: Rest, S., et al.
Publicado: (2024)

Evidence‐Based Practices to Enliven Integrated Reading‐to‐Writing Instruction
por: Kathleen A. J. Mohr, et al.
Publicado: (2024)

Neutrino signals from Neutron Star implosions to Black Holes
por: Zenati, Yossef, et al.
Publicado: (2023)

Mass transfer in eccentric black hole - neutron star mergers
por: Zenati, Yossef, et al.
Publicado: (2024)

Expanding the High-z Supernova Frontier: "Wide-Area" JWST Discoveries from the First Two Years of COSMOS-Web
por: Fox, Ori D., et al.
Publicado: (2026)

Testing for Intrinsic Type Ia Supernova Luminosity Evolution at z>2 with JWST
por: Pierel, J. D. R., et al.
Publicado: (2024)

Neutrino diagnostics of hadron-quark phase transition in Neutron Stars
por: Zenati, Yossef, et al.
Publicado: (2025)

Slitless Areal Pure-Parallel HIgh-Redshift Emission Survey (SAPPHIRES): Early Data Release of Deep JWST/NIRCam Images and Spectra in MACS J0416 Parallel Field
por: Sun, Fengwu, et al.
Publicado: (2025)

Transients from ONe White-Dwarf - Neutron-Star/Black-Hole Mergers
por: Bobrick, Alexey, et al.
Publicado: (2021)

Spectroscopic analysis of the strongly lensed SN~Encore: Constraints on cosmic evolution of Type Ia supernovae
por: Dhawan, S., et al.
Publicado: (2024)

Abundant Population of Broad H$α$ Emitters in the GOODS-N Field Revealed by CONGRESS, FRESCO, and JADES
por: Zhang, Junyu, et al.
Publicado: (2025)

On the Origins of "Hostless'' Supernovae: Testing the Faint-end Galaxy Luminosity Function and Supernova Progenitors with Events in Dwarf Galaxies
por: Strolger, Louis-Gregory, et al.
Publicado: (2025)

Aprendizaje informal a través de Facebook entre alumnos eslovenos
por: Karmen Erjavec
Publicado: (2013)

JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
por: Ji, Zhiyuan, et al.
Publicado: (2024)

BUL TEZIS ÚY-JAY QATNASÍQLARÍN PUQARALÍQ-HUQÍQÍY TÁRTIPKE SALÍW MÁSELELERINE BAǴÍShLANADÍ
por: Rzambetov, Salamat
Publicado: (2026)

What is the nature of Little Red Dots and what is not, MIRI SMILES edition
por: Pérez-González, Pablo G., et al.
Publicado: (2024)

BayeSN-TD: Time Delay and $H_0$ Estimation for Lensed SN H0pe
por: Grayling, M., et al.
Publicado: (2025)

Presaging Doppler beaming discoveries of double white dwarfs during the Rubin LSST era
por: Pallathadka, Gautham Adamane, et al.
Publicado: (2026)

Teatro universitario y teatro sin universidad
por: Karmen Saavedra Garfias
Publicado: (2015)

El teatro boliviano y su particular manera de existir
por: Karmen Saavedra Garfias
Publicado: (2008)

Historical Research. A Guide to Selected Library Information at the University of Tennessee, Knoxville.
por: Crowther, Karmen N. T.
Publicado: (1979)

Building the First Galaxies -- Chapter 2. Starbursts Dominate The Star Formation Histories of 6 < z <12 Galaxies
por: Dressler, Alan, et al.
Publicado: (2023)

Chapter Final Phases of Medieval Hebraism
por: Schwartz, Yossef
Publicado: (2019)

Relay Channels with Unreliable Helpers
por: Steinberg, Yossef
Publicado: (2024)

Degradedness Under Cooperation
por: Steinberg, Yossef
Publicado: (2025)

Discovery of young, oxygen-rich supernova remnants in PHANGS-MUSE galaxies
por: Kravtsov, Timo, et al.
Publicado: (2024)

JWST Discovery of a High-Redshift Tidal Disruption Event Candidate in COSMOS-Web
por: Karmen, Mitchell, et al.
Publicado: (2025)

The Ultraviolet Spectra of 2003fg-like Type Ia Supernovae
por: Bhattacharjee, Snehasish, et al.
Publicado: (2025)