The Backyard Observatory Supernova Search (BOSS) is conducted by astronomers from Australia and New Zealand since mid 2008 to search for new supernovae in the southern hemisphere. [2] In 2022 the group won the Astronomical Society of Australia's Page Medal [3] for having found around 200 confirmed supernovas. [4] [5] [6]
SN Name [2] | Host Galaxy | Date | Magnitude |
---|---|---|---|
AT2021xtf | PGC64029 | 2021-09-03 | 16.8 |
AT2021skl | ESO297-G16 | 2021-06-25 | 16.7 |
SN2021Itk | IC4367 | 2021-05-21 | 17.6 |
AT2021gfp | ESO42-G14 | 2021-03-18 | 18.8 |
AT2020kbv | ESO184-G64 | 2020-05-16 | 18.5 |
AT2020jvs | NGC642 | 2020-05-13 | 15.9 |
SN2020cdr | ESO119-13 | 2020-02-09 | 17.3 |
SN2019mhm | NGC6753 | 2019-08-02 | 16.6 |
SN2019icv | IC5186 | 2019-06-24 | 16 |
SN2019has | PGC133907 | 2019-06-07 | 15.9 |
SN2019hsa | NGC7038 | 2018-11-01 | 16.0 |
AT2018hmy | ESO-124-G-18 | 2018-10-21 | 16.8 |
SN2018ecf | PGC50325 | 2018-07-23 | 16.5 |
SN2018dfg | NGC5468 | 2018-07-10 | 17.8 |
SN2018ctw | ESO-297-G-36 | 2018-06-21 | 17.4 |
SN2018bta | ESO-101-G-20 | 2018-05-17 | 16.4 |
SN2018bbv | ESO-68-G-13 | 2018-04-25 | 17.1 |
AT2018bbI | NGC7421 | 2018-04-24 | 17.4 |
AT2018vv | ESO-158-G-7 | 2018-02-08 | 18 |
SN2017ixh | NGC2297 | 2017-12-15 | 17 |
SN2017hxt | PGC128734 | 2017-11-08 | 17.1 |
SN2017hbj | ESO-084-G-020 | 2017-10-03 | 16 |
SN2017ggw | ESO-246-G-21 | 2017-08-22 | 17.9 |
AT2017fus | ESO-464-G12 | 2017-07-29 | 18 |
AT2017fqz | ESO-267-IG-041 | 2017-07-25 | 16.5 |
SN2017ezd | ESO-339-G-009 | 2017-06-17 | 16.9 |
AT2017ewu | ESO-104-G-003 | 2017-06-19 | 17.7 |
AT2017ewt | IC2103 | 2017-06-20 | 16.8 |
AT2017eoc | ESO-215-G-037 | 2017-06-08 | 17.1 |
AT2017dgg | NGC1500 | 2017-04-21 | 17.9 |
SN2016adj | NGC5128 | 2016-02-08 [7] | 14 |
AT2015cr | ESO-596-G-10 | 2015-07-19 | 18 |
AT2017cet | NGC922 | 2017-03-15 | 16.2 |
SN2017caw | PGC22822 | 2017-03-08 | 18.0 |
SN2017bzc | NGC7552 | 2017-03-07 | 12.8 |
SN2017bzb | NGC7424 | 2017-03-07 | 13.0 |
SN2017acd | PGC612475 | 2017-02-02 | 17.3 |
SN2017iye | NGC2466 | 2016-12-19 | 17.4 |
AT2017iro | ESO 200-G-054 | 2016-12-03 | 18.5 |
Centaurus A is a galaxy in the constellation of Centaurus. It was discovered in 1826 by Scottish astronomer James Dunlop from his home in Parramatta, in New South Wales, Australia. There is considerable debate in the literature regarding the galaxy's fundamental properties such as its Hubble type and distance. It is the closest radio galaxy to Earth, as well as the closest BL Lac object, so its active galactic nucleus has been extensively studied by professional astronomers. The galaxy is also the fifth-brightest in the sky, making it an ideal amateur astronomy target. It is only visible from the southern hemisphere and low northern latitudes.
The Perth Observatory is the name of two astronomical observatories located in Western Australia (WA). In 1896, the original observatory was founded in West Perth on Mount Eliza overlooking the city of Perth. Due to the city's expansion, the observatory moved to Bickley in 1965. The new Perth Observatory is sometimes referred to as Bickley Observatory.
Leuschner Observatory, originally called the Students' Observatory, is an observatory jointly operated by the University of California, Berkeley and San Francisco State University. The observatory was built in 1886 on the Berkeley campus. For many years, it was directed by Armin Otto Leuschner, for whom the observatory was renamed in 1951. In 1965, it was relocated to its present home in Lafayette, California, approximately 10 miles (16 km) east of the Berkeley campus. In 2012, the physics and astronomy department of San Francisco State University became a partner.
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SN 2018cow was a very powerful astronomical explosion, 10–100 times brighter than a normal supernova, spatially coincident with galaxy CGCG 137-068, approximately 200 million ly (60 million pc) distant in the Hercules constellation. It was discovered on 16 June 2018 by the ATLAS-HKO telescope, and had generated significant interest among astronomers throughout the world. Later, on 10 July 2018, and after AT 2018cow had significantly faded, astronomers, based on follow-up studies with the Nordic Optical Telescope (NOT), formally described AT 2018cow as SN 2018cow, a type Ib supernova, showing an "unprecedented spectrum for a supernova of this class"; although others, mostly at first but also more recently, have referred to it as a type Ic-BL supernova. An explanation to help better understand the unique features of AT 2018cow has been presented. AT2018cow is one of the few reported Fast Blue Optical Transients (FBOTs) observed in the Universe. In May 2020, however, a much more powerful FBOT than AT 2018cow was reportedly observed.
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