| 释义 |
- See also
- Further reading
- References
{{Infobox supernova
| name=SN UDS10Wil
| image =
| caption=Record-breaking supernova SN UDS10Wil in the CANDELS Ultra Deep Survey[1]
| type = Ia
| epoch =
| SNRtype =
| host =
| constellation =
| ra =
| dec =
| gal =
| discovery =
| iauc =
| mag_v =
| redshift = 1.914
| distance = {{convert|10500000000|ly|kpc|lk=on}}
| progenitor =
| progenitor_type =
| b-v =
| notes =
| names = SN UDS10Wil, SN Wilson
}}SN UDS10Wil (SN Wilson)[2] is a type Ia supernova, and as of April 2013, the farthest known.[3]It has a redshift of 1.914, which strongly implies that it exploded when the universe was about a third of its current size. It was discovered with the Hubble Space Telescope's Wide Field Camera 3.[1] See also- List of most distant supernovae
- List of the most distant astronomical objects
Further reading - {{Cite journal |title= The Discovery of the Most Distant Known Type Ia Supernova at Redshift 1.914 |author1=David O. Jones |author2=Steven A. Rodney |author3=Adam G. Riess |author4=Bahram Mobasher |author5=Tomas Dahlen |author6=Curtis McCully |author7=Teddy F. Frederiksen |author8=Stefano Casertano |author9=Jens Hjorth |author10=Charles R. Keeton |author11=Anton Koekemoer |author12=Louis-Gregory Strolger |author13=Tommy G. Wiklind |author14=Peter Challis |author15=Or Graur |author16=Brian Hayden |author17=Brandon Patel |author18=Benjamin J. Weiner |author19=Alexei V. Filippenko |author20=Peter Garnavich |author21=Saurabh W. Jha |author22=Robert P. Kirshner |author23=Henry C. Ferguson |author24=Norman A. Grogin |author25=Dale Kocevski |arxiv= 1304.0768 |bibcode= 2013ApJ...768..166J |doi= 10.1088/0004-637X/768/2/166 |journal= The Astrophysical Journal |volume= 768 |issue= 2 |id= 166 |publicationdate= May 2013 |date= 2 April 2013 }}
References[1][2][3] 2 : Supernovae|Astronomical objects discovered in 2013 |