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Ata uhi

I tiakina i:
Ngā taipitopito rārangi puna kōrero
Ngā kaituhi matua: 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
Hōputu: Preprint
I whakaputaina: 2025
Ngā marau:
High Energy Astrophysical Phenomena
Astrophysics of Galaxies
Urunga tuihono:https://arxiv.org/abs/2504.17007
Ngā Tūtohu: Tāpirihia he Tūtohu
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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Ngā tūemi rite

  • Properties of high-redshift Type II supernovae discovered by the JADES transient survey
    mā: Moriya, Takashi J., me ētahi atu.
    I whakaputaina: (2025)
  • The Reliability of Type Ia Supernovae Delay Time Distributions Recovered from Galaxy Star Formation Histories
    mā: Joshi, Bhavin A., me ētahi atu.
    I whakaputaina: (2024)
  • Discovery of a likely Type II SN at $z$=3.6 with JWST
    mā: Coulter, D. A., me ētahi atu.
    I whakaputaina: (2025)
  • The JADES Transient Survey: Discovery and Classification of Supernovae in the JADES Deep Field
    mā: DeCoursey, Christa, me ētahi atu.
    I whakaputaina: (2024)
  • SN 2025ogs: A Spectroscopically-Normal Type Ia Supernova at z = 2 as a Benchmark for Redshift Evolution
    mā: Siebert, M. R., me ētahi atu.
    I whakaputaina: (2025)

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