GRB 130427A was a record-setting gamma-ray burst, discovered starting on April 27, 2013. This GRB was associated to SN 2013cq, of which the appearance of optical signal was predicted on May 2, 2013 and detected on May 13, 2013. The Fermi space observatory detected a gamma-ray with an energy of at least 94 billion electron volts. It was simultaneously detected by the Burst Alert Telescope aboard the Swift telescope and was the brightest burst Swift had ever detected. It was one of the five closest GRBs, at about 3.6 billion light-years away, and was comparatively long-lasting. — NASA
| Attributes | Values |
|---|
| rdf:type
| |
| rdfs:label
| - GRB 130427A (ca)
- GRB 130427A (en)
- GRB 130427A (pl)
- GRB 130427A (sv)
- GRB 130427A (zh)
|
| rdfs:comment
| - GRB 130427A – rekordowy rozbłysk gamma odkryty 27 kwietnia 2013. Energia promieniowania rozbłysku osiągnęła 94 miliardy elektronowoltów, a w momencie jego odkrycia był to jeden z pięciu najbliższych rozbłysków. Wywołany został wybuchem supernowej typu Ic, oznaczonej SN 2013cq. (pl)
- GRB 130427A var en extremt kraftig gammablixt som upptäcktes samtidigt av rymdteleskopet Fermi och Swift med början den 27 april 2013. (sv)
- GRB 130427A是由费米伽玛射线空间望远镜和雨燕卫星在2013年4月27日探测到的迄今最强的伽玛射线暴（未归算红移）。 这次伽玛射线暴位于狮子座方向，其中单个光子的最高能量至少为940亿电子伏（94 GeV），距离地球约36亿光年，是已知最近的五个伽玛射线暴之一，同时也是持续时间相对较长的一次伽玛射线暴。 (zh)
- GRB 130427A va ser un esclat de raigs gamma rècord, descobert iniciant-se el 27 d'abril de 2013. L'observatori espacial Fermi va detectar un raig gamma amb una energia d'almenys 94000 milions d'electró-volts. Va ser detectat simultàniament pel Burst Alert Telescope a bord del telescopi Swift i va ser un dels esclats més brillants detectats pel Swift. Va ser un dels cinc GRBs més propers, a una distància de 3600 milions d'anys llum, i va ser comparativament de llarga durada. L'observatori espacial Swift també va observar l'esclat, determinant ràpidament la seva ubicació. (ca)
- GRB 130427A was a record-setting gamma-ray burst, discovered starting on April 27, 2013. This GRB was associated to SN 2013cq, of which the appearance of optical signal was predicted on May 2, 2013 and detected on May 13, 2013. The Fermi space observatory detected a gamma-ray with an energy of at least 94 billion electron volts. It was simultaneously detected by the Burst Alert Telescope aboard the Swift telescope and was the brightest burst Swift had ever detected. It was one of the five closest GRBs, at about 3.6 billion light-years away, and was comparatively long-lasting. — NASA (en)
|
| dcterms:subject
| |
| Wikipage page ID
| |
| Wikipage revision ID
| |
| Link from a Wikipage to another Wikipage
| |
| sameAs
| |
| dbp:wikiPageUsesTemplate
| |
| has abstract
| - GRB 130427A va ser un esclat de raigs gamma rècord, descobert iniciant-se el 27 d'abril de 2013. L'observatori espacial Fermi va detectar un raig gamma amb una energia d'almenys 94000 milions d'electró-volts. Va ser detectat simultàniament pel Burst Alert Telescope a bord del telescopi Swift i va ser un dels esclats més brillants detectats pel Swift. Va ser un dels cinc GRBs més propers, a una distància de 3600 milions d'anys llum, i va ser comparativament de llarga durada. L'observatori espacial Swift també va observar l'esclat, determinant ràpidament la seva ubicació. L'emissió també va ser detectada utilitzant la radiació de ràdio, infraroig i visible des dels telescopis terrestres utilitzant la ubicació en el cel proporcionada pel Swift. L'esclat va ser observat amb un telescopi òptic de 350mm i es va mesurar la seva brillantor. La magnitud aparent visible va disminuir de 13 a 15,5 en un període de tres hores començant a les 08:05:12 UTC el 27 d'abril de 2013. El també va detectar l'esclat òpticament, independentment de l'alerta. Va rebre la designació CSS130502:113233+274156. Es va trobar en ascensió recta 11:32:32.90, i declinació +27:41:56.5 (J2000).El catàleg SDSS mostra una galàxia (SDSS J113232.84+274155.4) gairebé coincident amb aquesta posició a una magnitud r=21,26 però sense obtindre espectre SDSS. (ca)
- GRB 130427A was a record-setting gamma-ray burst, discovered starting on April 27, 2013. This GRB was associated to SN 2013cq, of which the appearance of optical signal was predicted on May 2, 2013 and detected on May 13, 2013. The Fermi space observatory detected a gamma-ray with an energy of at least 94 billion electron volts. It was simultaneously detected by the Burst Alert Telescope aboard the Swift telescope and was the brightest burst Swift had ever detected. It was one of the five closest GRBs, at about 3.6 billion light-years away, and was comparatively long-lasting. Fermi's Large Area Telescope (LAT) recorded one gamma ray with an energy of at least 94 billion electron volts (GeV), or some 35 billion times the energy of visible light, and about three times greater than the LAT's previous record. The GeV emission from the burst lasted for hours, and it remained detectable by the LAT for the better part of a day, setting a new record for the longest gamma-ray emission from a GRB. — NASA Swift space observatory also observed the burst, quickly determining its location. The X-ray afterglow of the burst was so bright that Swift was able to observe it for the next six months. The emission was also detected using radio, infrared and visible radiation from ground-based telescopes using the sky location from Swift. The burst was observed with a 350mm optical telescope and its brightness measured. The visible apparent magnitude decreased from 13 to 15.5 over a three-hour period starting at 08:05:12 UTC 27 April 2013. The Catalina Real-time Transient Survey also detected the burst optically, independent of the alert. It received designation CSS130502:113233+274156. It was found at right ascension 11:32:32.90, and declination +27:41:56.5 (J2000).The SDSS catalogue shows a galaxy (SDSS J113232.84+274155.4) almost coincident with this position at magnitude r=21.26 but with no SDSS spectrum obtained. (en)
- GRB 130427A – rekordowy rozbłysk gamma odkryty 27 kwietnia 2013. Energia promieniowania rozbłysku osiągnęła 94 miliardy elektronowoltów, a w momencie jego odkrycia był to jeden z pięciu najbliższych rozbłysków. Wywołany został wybuchem supernowej typu Ic, oznaczonej SN 2013cq. (pl)
- GRB 130427A var en extremt kraftig gammablixt som upptäcktes samtidigt av rymdteleskopet Fermi och Swift med början den 27 april 2013. (sv)
- GRB 130427A是由费米伽玛射线空间望远镜和雨燕卫星在2013年4月27日探测到的迄今最强的伽玛射线暴（未归算红移）。 这次伽玛射线暴位于狮子座方向，其中单个光子的最高能量至少为940亿电子伏（94 GeV），距离地球约36亿光年，是已知最近的五个伽玛射线暴之一，同时也是持续时间相对较长的一次伽玛射线暴。 (zh)
|
| gold:hypernym
| |
| prov:wasDerivedFrom
| |
| page length (characters) of wiki page
| |
| foaf:isPrimaryTopicOf
| |
| is Link from a Wikipage to another Wikipage
of | |
| is Wikipage redirect
of | |
| is foaf:primaryTopic
of | |
![[RDF Data]](/fct/images/sw-rdf-blue.png)
![[cxml]](/fct/images/cxml_doc.png)
![[csv]](/fct/images/csv_doc.png)
![[text]](/fct/images/ntriples_doc.png)
![[turtle]](/fct/images/n3turtle_doc.png)
![[ld+json]](/fct/images/jsonld_doc.png)
![[rdf+json]](/fct/images/json_doc.png)
![[rdf+xml]](/fct/images/xml_doc.png)
![[atom+xml]](/fct/images/atom_doc.png)
![[html]](/fct/images/html_doc.png)