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- Q211320 subject Q10595.
- Q211320 subject Q7144261.
- Q211320 subject Q8273466.
- Q211320 abstract "SCP 06F6 is (or was) an astronomical object of unknown type, discovered on 21 February 2006 in the constellation Boötesduring a survey of galaxy cluster CL 1432.5+3332.8 with the Hubble Space Telescope's Advanced Camera for Surveys Wide Field Channel.According to research authored by Kyle Barbary of the Supernova Cosmology Project, the object brightened over a period of roughly 100 days, reaching a peak intensity of magnitude 21; it then faded over a similar period.Barbary and colleagues report that the spectrum of light emitted from the object does not match known supernova types, and is dissimilar to any known phenomenon in the Sloan Digital Sky Survey database. The light in the blue region shows broad line features, while the red region shows continuous emission. The spectrum shows a handful of spectral lines, but when astronomers try to trace any one of them to an element the other lines fail to match up with any other known elements.Because of its uncommon spectrum, the team was not able to determine the distance to the object using standard redshift techniques; it is not even known whether the object is within or outside the Milky Way. Furthermore, no Milky Way star or external galaxy has been detected at this location, meaning any source is very faint.The European X-ray satellite XMM Newton made an observation in early August 2006 which appears to show an X-ray glow around SCP 06F6, two orders of magnitude more luminous than that of supernovae.Observations from the Palomar Transient Factory, reported in 2009, indicate a redshift z = 1.189 and a peak magnitude of −23.5 absolute (comparable to SN2005ap), making SCP 06F6 one of the most luminous transient phenomena known as of that date.".
- Q211320 thumbnail SCP_06F6.jpg?width=300.
- Q211320 wikiPageExternalLink dn14738-space-firefly-resembles-no-known-object.html.
- Q211320 wikiPageExternalLink dn9360-enigmatic-object-baffles-supernova-team.html.
- Q211320 wikiPageExternalLink CBET000546.txt.
- Q211320 wikiPageExternalLink L129.
- Q211320 wikiPageExternalLink dn17262.
- Q211320 wikiPageWikiLink Q1049029.
- Q211320 wikiPageWikiLink Q1050633.
- Q211320 wikiPageWikiLink Q10595.
- Q211320 wikiPageWikiLink Q1148221.
- Q211320 wikiPageWikiLink Q124313.
- Q211320 wikiPageWikiLink Q130019.
- Q211320 wikiPageWikiLink Q204107.
- Q211320 wikiPageWikiLink Q2273477.
- Q211320 wikiPageWikiLink Q245701.
- Q211320 wikiPageWikiLink Q2513.
- Q211320 wikiPageWikiLink Q321.
- Q211320 wikiPageWikiLink Q333705.
- Q211320 wikiPageWikiLink Q3863.
- Q211320 wikiPageWikiLink Q3937.
- Q211320 wikiPageWikiLink Q483247.
- Q211320 wikiPageWikiLink Q506269.
- Q211320 wikiPageWikiLink Q582000.
- Q211320 wikiPageWikiLink Q5871.
- Q211320 wikiPageWikiLink Q589.
- Q211320 wikiPageWikiLink Q623.
- Q211320 wikiPageWikiLink Q654182.
- Q211320 wikiPageWikiLink Q693861.
- Q211320 wikiPageWikiLink Q6999.
- Q211320 wikiPageWikiLink Q7128610.
- Q211320 wikiPageWikiLink Q7144261.
- Q211320 wikiPageWikiLink Q76250.
- Q211320 wikiPageWikiLink Q8273466.
- Q211320 wikiPageWikiLink Q840332.
- Q211320 wikiPageWikiLink Q865528.
- Q211320 wikiPageWikiLink Q8667.
- Q211320 comment "SCP 06F6 is (or was) an astronomical object of unknown type, discovered on 21 February 2006 in the constellation Boötesduring a survey of galaxy cluster CL 1432.5+3332.8 with the Hubble Space Telescope's Advanced Camera for Surveys Wide Field Channel.According to research authored by Kyle Barbary of the Supernova Cosmology Project, the object brightened over a period of roughly 100 days, reaching a peak intensity of magnitude 21; it then faded over a similar period.Barbary and colleagues report that the spectrum of light emitted from the object does not match known supernova types, and is dissimilar to any known phenomenon in the Sloan Digital Sky Survey database. ".
- Q211320 label "SCP 06F6".
- Q211320 depiction SCP_06F6.jpg.