Draft:CEERS2 588
Submission declined on 27 October 2024 by KylieTastic (talk).
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| Submission declined on 22 October 2024 by Jlwoodwa (talk). This draft's references do not show that the subject qualifies for a Wikipedia article. In summary, the draft needs multiple published sources that are: Declined by Jlwoodwa 14 days ago.
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Comment: I don't think this draft demonstrates that the galaxy meets any of the criteria for astronomical objects. jlwoodwa (talk) 02:09, 22 October 2024 (UTC)
| CEERS2 588 | |
|---|---|
| Observation data (J2000 epoch) | |
| Constellation | Boötes |
| Right ascension | 14h 19m 37.5900s |
| Declination | 52° 56′ 43.80″ |
| Redshift | 11.04 |
| Distance |
|
| Apparent magnitude (V) | 26.9 |
| Characteristics | |
| Type | Lyman-break galaxy |
| Size | 3000 ly |
| Half-light radius (apparent) | 120 mas |
References: [1] | |
CEERS2 588 is a high-redshift Lyman-break galaxy discovered by the James Webb Space Telescope (JWST) during the NIRCam and NIRSpec observations for the Cosmic Evolution Early Release Science Survey (CEERS),[1] and is the 10th farthest galaxy known as of october 2024.
Discovery
[edit]CEERS2 588 was discovered using the James Webb Space Telescope's Near-Infrared Spectrograph (NIRSpec) in 2024, and it measured a redshift of 11.04.[1]
See also
[edit]References
[edit]- ^ a b c Finkelstein, Steven L.; Bagley, Micaela B.; Ferguson, Henry C.; Wilkins, Stephen M.; Kartaltepe, Jeyhan S.; Papovich, Casey; Yung, L. Y. Aaron; Haro, Pablo Arrabal; Behroozi, Peter; Dickinson, Mark; Kocevski, Dale D.; Koekemoer, Anton M.; Larson, Rebecca L.; Bail, Aurélien Le; Morales, Alexa M. (March 2023). "CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST". The Astrophysical Journal Letters. 946 (1): L13. arXiv:2211.05792. Bibcode:2023ApJ...946L..13F. doi:10.3847/2041-8213/acade4. ISSN 2041-8205.
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