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Longer titles found: Supercluster: The Big Dipper Anthology (view), Supercluster (band) (view), Supercluster (disambiguation) (view), Supercluster (genetic) (view), Virgo Supercluster (view), Laniakea Supercluster (view), Shapley Supercluster (view), Hercules Superclusters (view), Pisces–Cetus Supercluster Complex (view), Hyperion proto-supercluster (view), Draco Supercluster (view), Vela Supercluster (view), Horologium-Reticulum Supercluster (view), Hydra–Centaurus Supercluster (view), Perseus–Pisces Supercluster (view), Lynx Supercluster (view), Saraswati Supercluster (view), Corona Borealis Supercluster (view), Coma Supercluster (view), Ophiuchus Supercluster (view), Pavo–Indus Supercluster (view), Microscopium Supercluster (view), Leo Supercluster (view), Lynx–Ursa Major Supercluster (view), Southern Supercluster Strand (view), Southern Supercluster (view)

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NGC 4305 (413 words) [view diff] no match in snippet view article find links to article

NGC 4305 is a dwarf spiral galaxy located about 100 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer John Herschel

NGC 4306 is a dwarf barred lenticular galaxy located about 100 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer

NGC 4318 is a small lenticular galaxy located about 72 million light-years away in the constellation Virgo. It was discovered by astronomer John Herschel

NGC 404 is a field galaxy located about 10 million light years away in the constellation Andromeda. It was discovered by William Herschel in 1784, and

NGC 404 is a field galaxy located about 10 million light years away in the constellation Andromeda. It was discovered by William Herschel in 1784, and

NGC 3632 (also known as Caldwell 40) and NGC 3626 is an unbarred lenticular galaxy and Caldwell object in the constellation Leo. It was discovered by William

The BOSS Great Wall is a supercluster complex that was identified, using the Baryon Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky Survey

NGC 55, also known as the String of Pearls Galaxy, is a Magellanic type barred spiral galaxy located about 6.5 million light-years away in the constellation

The Eridanus Group, sometimes called the Eridanus Cloud, is a nearby loose grouping of galaxies at a mean distance of approximately 75 Mly (23 ± 2 Mpc)

million light-years away from Earth. The group resides in the Local Supercluster. The largest galaxy within the cluster is M106 (NGC 4258), which is a

from Earth containing NGC 2997 as a member. It is a group in the Local Supercluster along with the Local Group. "NAME NGC 2997 Group". SIMBAD. Centre de

Galaxy (redshift of approximately z=0.03), also known as the Sculptor superclusters. The superstructure is also called the Southern Great Wall, the Great

The Eridanus Cluster is a galaxy cluster roughly 23 Mpc (75 Mly) from Earth, containing about 73 main galaxies and about 200 total galaxies. About 30%

NGC 3593 is a lenticular galaxy located in the constellation Leo. It has a morphological classification of SA(s)0/a, which indicates it is a lenticular

The Black Eye Galaxy (also called Sleeping Beauty Galaxy or Evil Eye Galaxy and designated Messier 64, M64, or NGC 4826) is a relatively isolated spiral

NGC 3593 is a lenticular galaxy located in the constellation Leo. It has a morphological classification of SA(s)0/a, which indicates it is a lenticular

initially more massive cluster which had partly evaporated, the Hyades Supercluster). Boss published a chart that traced the scattered stars' movements back

The Fornax Cluster is a cluster of galaxies lying at a distance of 19 megaparsecs (62 million light-years). It has an estimated mass of (7±2)×1013 solar

lenticular galaxy, a member of the NGC 1023 group of galaxies in the Local Supercluster. Distance measurements vary from 9.3 to 19.7 million parsecs (30 to 64

NGC 300 (also known as Caldwell 70 or the Sculptor Pinwheel Galaxy) is a spiral galaxy in the constellation Sculptor. It was discovered on 5 August 1826

the northern constellation of Andromeda, and a member of the Sirius supercluster. It lies near the lower limit of visibility to the naked eye at an apparent

134 km/s. Eggen (1985) suggested it is a probable member of the Hyades Supercluster. Samuel Molyneux named this star Telescopica in Auriga. Flamsteed catalogued

treated as being related and both are considered members of the IC 2391 supercluster. Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation"

heliocentric radial velocity of −9 km/s, and is a member of the Sirius supercluster: a stream of stars that share a common motion through space. This is

velocity of −13 km/s, and is catalogued as a member of the Pleiades supercluster. This is an ordinary A-type main-sequence star with a stellar classification

heliocentric radial velocity of −7.6 km/s. It is a member of the Sirius supercluster. This is an aging giant star with a stellar classification of K1 III

The Dorado Group is a loose concentration of galaxies containing both spirals and ellipticals. It is generally considered a 'galaxy group' but may approach

to the group. Sirius may instead be a member of the proposed Sirius Supercluster, along with other scattered stars such as Beta Aurigae, Alpha Coronae

light-years in around 5.3 million years. It is a member of the Sirius supercluster. This object is an ordinary A-type main-sequence star with a stellar

The Sculptor Group is a loose group of galaxies visible near the south galactic pole. The group is one of the closest groups of galaxies to the Local Group;

has this star flagged as a blue straggler and a member of the HR1614 supercluster. Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data

heliocentric radial velocity of 31 km/s. It is a probable member of the Hyades Supercluster. As of 2012, the pair had an angular separation of 7.39″ along a position

from its motion through space, it is a candidate member of the Sirius supercluster. This object is a superficially normal A-type star. However, there is

radial velocity of +12 km/s. It was considered a member of the Hyades Supercluster, but in 1990 this was brought into question. This object is an aging

The pristinamycin biosynthetic gene cluster is the largest antibiotic supercluster known so far, with a size of ~210 kb, wherein the PI and PII biosynthetic

years ago. Olin J. Eggen listed it as a probable member of the Hyades supercluster. This is an aging red giant star currently on the asymptotic giant branch

velocity of +10 km/s. Eggen (1991) listed it as a member of the IC 2391 supercluster. It has also been catalogued as a member of the Hyades group. However

velocity of +10 km/s. Eggen (1991) listed it as a member of the IC 2391 supercluster. It has also been catalogued as a member of the Hyades group. However

motion through space, this system appears to be a member of the Sirius supercluster. The brighter component is a white hued A-type main-sequence star with

209 light years from the Sun. The star is considered a member of the Sirius supercluster. This is an ordinary A-type main sequence star with a stellar classification

0.181″/yr. According to Eggen (1998), this is a member of the Hyades Supercluster. This is an A-type main-sequence star with a stellar classification of

another similar but much more energetic AGN outburst - the Ophiuchus Supercluster eruption in the NeVe 1 galaxy, was five times the energy of MS 0735.6+7421

listed it as a proper motion candidate for membership in the IC 2391 supercluster. This star has a stellar classification of A3 IV–Vn, showing a spectrum

heliocentric radial velocity of +8 km/s. It is a candidate member of the Hyades Supercluster. This is an aging K-type star with a stellar classification of K2 II-III

2019-02-03. Gregory, S. A.; Thompson, L. A. (1978-06-01). "The Coma/A1367 supercluster and its environs". The Astrophysical Journal. 222: 784–799. Bibcode:1978ApJ

heliocentric radial velocity of +36 km/s, and are members of the Hyades Supercluster. The visible component of this system is an ordinary A-type main-sequence

listed it as a proper motion candidate for membership in the IC 2391 supercluster. It may be a runaway star, having a peculiar velocity of 25.9+3.9 −6

2019-02-03. Gregory, S. A.; Thompson, L. A. (1978-06-01). "The Coma/A1367 supercluster and its environs". The Astrophysical Journal. 222: 784–799. Bibcode:1978ApJ

2019-02-03. Gregory, S. A.; Thompson, L. A. (1978-06-01). "The Coma/A1367 supercluster and its environs". The Astrophysical Journal. 222: 784–799. Bibcode:1978ApJ

radial velocity of +2.6 km/s. It is a candidate member of the Hyades supercluster and has a peculiar velocity of 9.2 km/s. The visible component of this

2019-02-03. Gregory, S. A.; Thompson, L. A. (1978-06-01). "The Coma/A1367 supercluster and its environs". The Astrophysical Journal. 222: 784–799. Bibcode:1978ApJ

The M109 Group (also known as the NGC 3992 Group or Ursa Major cloud) is a group of galaxies about 55 million light-years away in the constellation Ursa

star's proper motion makes it a candidate for membership in the IC 2391 supercluster. This is an evolved, G-type giant star with a stellar classification

years away from the Sun based on parallax. It is a member of the Hyades Supercluster. The brighter component is an A-type main-sequence star with a stellar

radial velocity of −16 km/s. It is a candidate member of the Hyades Supercluster. The two components are designated Gamma Aquarii Aa, formally called

The galaxy is a member of the NGC 1023 group of galaxies in the Local Supercluster. It has an H II nucleus. The object is visible in small to moderate size

large, nearly empty region of space (a void). It lies next to the Local Supercluster, which contains our galaxy the Milky Way. Its center is 96 megaparsecs

parsecs) away from the Earth. It is considered a member of the Sirius supercluster. 21 Leonis Minoris rotates fairly fast for a star; its projected rotational

The NGC 5866 Group is a small group of galaxies located in the constellation Draco. The group is named after NGC 5866, the galaxy with the highest apparent

system's proper motion makes it a candidate for membership in the IC 2391 supercluster. They are moving away from the Earth with a heliocentric radial velocity

2019-02-02. Gregory, S. A.; Thompson, L. A. (1978-06-01). "The Coma/A1367 supercluster and its environs". The Astrophysical Journal. 222: 784–799. Bibcode:1978ApJ

between the two components is 0.1. It is considered a member of the Sirius supercluster. The primary component is an Am star with a stellar classification of

motion through space, this star appears to be a member of the Hyades Supercluster. This is an evolved K-type giant star with a stellar classification of

velocity of −13.5 km/s. It has been catalogued as a member of the Hyades Supercluster, although its membership status remains doubtful. The innermost system

visual magnitude of 5.88. It is catalogued as a member of the IC 2391 supercluster by Olin J. Eggen. In the past the inner pair, designated component A

2019-02-03. Gregory, S. A.; Thompson, L. A. (1978-06-01). "The Coma/A1367 supercluster and its environs". The Astrophysical Journal. 222: 784–799. Bibcode:1978ApJ

combination of these movements indicate this star is a member of the Hyades supercluster. Li et al. (2000) categorized this as an F-type main-sequence star with

listed it as a proper motion candidate for membership in the IC 2391 supercluster. The stellar classification of A5 III suggests this is an A-type giant

Olin J. Eggen (1991) included this system as a member of the IC 2391 supercluster, but it was later excluded. The variable nature of RS Canum Venaticorum

on its motion through space, it appears to be a member of the IC 2391 supercluster. This is an F-type main-sequence star with a stellar classification of

2019-01-15. Gregory, S. A.; Thompson, L. A. (1978-06-01). "The Coma/A1367 supercluster and its environs". The Astrophysical Journal. 222: 784–799. Bibcode:1978ApJ

The Fornax Wall is a superstructure known as a galaxy filament or galaxy wall. It is a long filament of galaxies with a major axis longer than its minor

10.7 km/s. Eggen (1995) lists it as a probable member of the Hyades Supercluster. HD 75171 has a stellar classification of A4 V, indicating that it is

years from the Sun. The system is deemed to be a member of the Sirius supercluster of stars that share a common motion through space. The primary, component

magnitude 7.84 star. Zeta Crateris is a confirmed member of the Sirius supercluster and is a candidate member of the Ursa Major Moving Group, a collection

the Galaxy, placing it within a thin disk. It belongs to the Hyades supercluster of stars, and is one of 155 K-type stars within 50 light years. It is

2019-01-15. Gregory, S. A.; Thompson, L. A. (1978-06-01). "The Coma/A1367 supercluster and its environs". The Astrophysical Journal. 222: 784–799. Bibcode:1978ApJ

2019-02-03. Gregory, S. A.; Thompson, L. A. (1978-06-01). "The Coma/A1367 supercluster and its environs". The Astrophysical Journal. 222: 784–799. Bibcode:1978ApJ

multiple galaxy NGC 4933. The group lies between the Local Supercluster and Hydra-Centaurus Supercluster. "Results for object NGC 4939". NASA/IPAC Extragalactic

of an outlying group belonging to the Ursa Major flow of the Sirius supercluster. This is an evolved giant star with a stellar classification of K1 III

plug-in boards MultiCluster (T800) – Up to 64 processors in a single rack SuperCluster (T800) – 16 to 1,024 processors in a single frame GigaCluster (planned:

the term Gur was used, Mabia has been used to refer to the linguistic supercluster. The Mabia ethnic group include the following peoples: Dagomba Mossi

upon its space velocity components, this star is a member of the Hyades supercluster of stars that share a common motion through space. Houk and Cowley (1978)

universe, with a mean size of about 5.6 billion light years. Such a supercluster can explain the significant distribution of GRBs because of its tie to

Browser. Retrieved 2017-09-12. Tully, R. B. (June 1982). "The Local Supercluster". The Astrophysical Journal. 257: 389–422. Bibcode:1982ApJ...257..389T

velocity of 19.2 km/s. The star is a possible member of the IC 2391 supercluster. Flare activity was first reported for this star by N. I. Shakhovskaya

(September 1995), "Neutral hydrogen observations of galaxies in the Hercules supercluster. III. CGCG fields at the edge of the void", Astronomy and Astrophysics

distance light travels in one second Local Supercluster (LS) or Virgo Superclaster, our galaxy supercluster Lung surfactant, a lipoprotein complex Legius

Gregory, S. A. (1979-07-01). "Band theory applied to the Coma/A1367 supercluster". The Astrophysical Journal. 231: 23–27. Bibcode:1979ApJ...231...23T

Gregory, S. A. (1979-07-01). "Band theory applied to the Coma/A1367 supercluster". The Astrophysical Journal. 231: 23–27. Bibcode:1979ApJ...231...23T

Gregory, S. A. (1979-07-01). "Band theory applied to the Coma/A1367 supercluster". The Astrophysical Journal. 231: 23–27. Bibcode:1979ApJ...231...23T

doi:10.1086/113874. ISSN 0004-6256. Tully, R. B. (June 1982). "The Local Supercluster". The Astrophysical Journal. 257: 389–422. Bibcode:1982ApJ...257..389T

Gregory, S. A. (1979-07-01). "Band theory applied to the Coma/A1367 supercluster". The Astrophysical Journal. 231: 23–27. Bibcode:1979ApJ...231...23T

Gregory, S. A. (1979-07-01). "Band theory applied to the Coma/A1367 supercluster". The Astrophysical Journal. 231: 23–27. Bibcode:1979ApJ...231...23T

of NGC 4329 places it in the within the bounds of the Hydra-Centaurus supercluster. List of NGC objects (4001–5000) "NASA/IPAC Extragalactic Database".

Antlia cluster of galaxies and its environment : the Hydra I-Centaurus supercluster". Astronomy and Astrophysics Supplement Series. 61: 93–106. ISSN 0365-0138

largest known stars in galaxies outside the Local Group inside the Virgo supercluster Star name Solar radii (Sun = 1) Galaxy Group Method Notes NGC 300-125

Gregory, S. A. (1979-07-01). "Band theory applied to the Coma/A1367 supercluster". The Astrophysical Journal. 231: 23–27. Bibcode:1979ApJ...231...23T

shown that Denebola is part of a stellar association dubbed the IC 2391 supercluster. All the stars of this group share a roughly common motion through space

of small, dwarf galaxies with emission-lines on the edges of galaxy supercluster voids. Moody is best known for work in astronomical publishing. He served

"Galaxy Evolution in the Mid-Infrared Green Valley: A Case of the A2199 Supercluster". The Astrophysical Journal. 800 (2): 80. arXiv:1412.3996. Bibcode:2015ApJ

doi:10.1086/113874. ISSN 0004-6256. Tully, R. B. (June 1982). "The Local Supercluster". The Astrophysical Journal. 257: 389–422. Bibcode:1982ApJ...257..389T

include: Local Association (Pleiades moving group) Hyades Stream IC 2391 supercluster Beta Pictoris moving group Castor moving group AB Doradus moving group

(2011-09-26). "The complete census of optically selected AGNs in the Coma supercluster: the dependence of AGN activity on the local environment". Astronomy

Cornell University in 2005, entitled "Galaxy flows in and around the Local Supercluster", under the supervision of Martha Haynes and Riccardo Giovanelli. In

Markham's tech-innovation hub, VentureLabs, in the Southern Ontario Supercluster. Ng has also helped deliver infrastructure improvements to Markham and

Markham's tech-innovation hub, VentureLabs, in the Southern Ontario Supercluster. Ng has also helped deliver infrastructure improvements to Markham and

1051/0004-6361/201526413. S2CID 73623700. Eggen, O. J. (1985). "Hyades and Sirius supercluster members brighter than magnitude(V) 7.1. I - the first six hours of right

record for this source at VizieR. Eggen, O. J. (1986). "Hyades and Sirius supercluster members brighter than magnitude (V) 7.1. II - Right ascension six to

(October 2011). "The complete census of optically selected AGNs in the Coma supercluster: the dependence of AGN activity on the local environment". Astronomy

Champion Race Car Driver Will Pilot Axiom's Second Crewed Mission". Supercluster. Retrieved 2021-06-03. Margetta, Robert (13 December 2021). "NASA Selects

dimming FRB 180916 location and periodicity Radcliffe wave Ophiuchus Supercluster explosion PSO J03094+27 (distant blazar) 2MASS J1047+21 wind speed measurements

dimming FRB 180916 location and periodicity Radcliffe wave Ophiuchus Supercluster explosion PSO J03094+27 (distant blazar) 2MASS J1047+21 wind speed measurements

Galaxy clusters Horologium Supercluster

Diffuse-type galaxy DGSAT I – Ultra diffuse galaxy in the Perseus–Pisces Supercluster Van Dokkum, Pieter; et al. (7 January 2015). "Forty-Seven Milky Way-sized

Bibcode:2020AAS...23545301P. "Astronomers map massive structure beyond Laniakea Supercluster". University of Hawaii. 10 July 2020. Retrieved 10 July 2020. Overbye

(October 2011). "The complete census of optically selected AGNs in the Coma Supercluster: the dependence of AGN activity on the local environment". Astronomy

Bibcode:1990A&AS...85.1015M Eggen, Olin J. (August 1998), "The Sirius Supercluster and Missing Mass near the Sun", The Astronomical Journal, 116 (2): 782–788

Antlia cluster of galaxies and its environment : the Hydra I-Centaurus supercluster". Astronomy and Astrophysics Supplement Series. 61: 93–106. Bibcode:1985A&AS

Bibcode:1999VeARI..35....1W Eggen, Olin J. (August 1998), "The Sirius Supercluster and Missing Mass near the Sun", The Astronomical Journal, 116 (2): 782–788

Brown, David. "EUROPA CLIPPER INCHES FORWARD, SHACKLED TO THE EARTH". SuperCluster. Retrieved 26 November 2022. "Star-48". space.skyrocket.de. Retrieved

Jr. (1988). "Starbursts, binary stars, and blue stragglers in local superclusters and groups. I - The very young disk and young disk populations". Astronomical

United Women's Orchestra, Blue One (1999) United Women's Orchestra, Virgo Supercluster (2002) Roelofs had gone to the Melkweg club to meet a friend, unaware

As part of the federal government's "next generation manufacturing supercluster" program, Providence and Northern mRNA had also been "cleared to access

Galaxy clusters Horologium Supercluster

No. Title Producer(s) Length 1. "Absolutions in the Hottentot Supercluster" (featuring Zeroh and Kaveh Rastegar) Fumitake Tamura 4:33 2. "Black Labor (as

JAAW (featuring Cairns on vocals) announced their debut album called Supercluster to be released on 26 May 2023 on Svart Records. Much has been made over

Bibcode:1986EgUBV........0M. Eggen, Olin J. (August 1998), "The Sirius Supercluster and Missing Mass near the Sun", The Astronomical Journal, 116 (2): 782–788

the Taurus Stream (now generally known as the Hyades Stream or Hyades Supercluster). Boss published a chart that traced the scattered stars' movements back

jewel of the Soviet space program, the Buran became a graffitied wreck". Supercluster. Retrieved 23 May 2022. Berger, Eric (10 April 2021). "Let's make a deal:

Big Bang, dark matter clumped into blobs along narrow filaments with superclusters of galaxies forming a cosmic web at scales on which entire galaxies

Bibcode:1967IAUS...30...57E. Eggen, Olin J. (August 1998), "The Sirius Supercluster and Missing Mass near the Sun", The Astronomical Journal, 116 (2): 782–788

Galaxy clusters Horologium Supercluster

Bibcode:1993A&AS..100...47G. ISSN 0365-0138. Tully, R. B. (1982-06-01). "The Local Supercluster". The Astrophysical Journal. 257: 389–422. Bibcode:1982ApJ...257..389T

Retrieved 2006-11-30. Eggen, O. J. (1992). "HR 1614 and the dissolution of a supercluster". Astronomical Journal. 104 (5): 1906–1915. Bibcode:1992AJ....104.1906E

community and key industries. A part of this approach was Colorado State's Supercluster research model, designed to utilize interdisciplinary, issue-based research

the Milky Way, not part of the Sculptor Group. The Sculptor Wall, a supercluster of more distant galaxies. The Sculptor Squirrel, a species of Malaysian

Great Attractor – Region of overdensity of galaxies within the local supercluster Timeline of the early universe Timeline of the far future – Scientific

Eggen, O. J. (June 1985), "A systematic search for members of the Hyades Supercluster. IV - The metallic-line stars and ultrashort-period Cepheids", Astronomical

portal Gaofen Fengyun Chinese State Oceanic Administration "Haiyang-1D". Supercluster. Retrieved 12 October 2024. "HY 1A, 1B". Gunter's Space Page. 31 March

The galaxy is a member of the Coma I Group, which is part of the Local Supercluster. NGC 4747 is interacting with neighboring spiral galaxy NGC 4725, with

dimming FRB 180916 location and periodicity Radcliffe wave Ophiuchus Supercluster explosion PSO J03094+27 (distant blazar) 2MASS J1047+21 wind speed measurements

Its observed kinematics suggest that it is a member of the Pleiades supercluster. HD 29678 has a stellar classification of A9/F0 IV, indicating that it

Galaxy clusters Horologium Supercluster

Scalable Server and Engineered System -- the SPARC M6-32 and Oracle SuperCluster M6-32". Retrieved 2013-09-23. Oracle's Big Memory Machines are Ideal

Galaxy clusters Horologium Supercluster

Galaxy clusters Horologium Supercluster

Appliance Big Data Appliance – integrated map-reduce/big data solution SPARC SuperCluster T4-4 – a general purpose engineered system Oracle Cloud is a cloud computing

speciation of a large and diverse clade within the Agrobacterium/Rhizobium supercluster characterized by the presence of a linear chromid". Mol Phylogenet Evol

global energy needs. He is the founding director of CSU's Clean Energy Supercluster, founder and director of CSU's Engines and Energy Conversion Laboratory;

4242, NGC 4248, NGC 4288 and NGC 4460. The group is part of the Local Supercluster. "NASA/IPAC Extragalactic Database". Results for NGC 4096. Retrieved

Galaxy clusters Horologium Supercluster

Retrieved 2007-05-18. Michael J. West (December 1997). "THE GALAXY-CLUSTER-SUPERCLUSTER CONNECTION". Canadian Astronomical Society/Société Canadienne D'Astronomie

doi:10.1093/mnras/148.1.1. Eggen, Olin J. (August 1998), "The Sirius Supercluster and Missing Mass near the Sun", The Astronomical Journal, 116 (2): 782–788

search for the extended Sunyaev-Zel'dovich effect in the Corona Borealis supercluster". MNRAS. 363 (1): 79–92. arXiv:astro-ph/0507285. Bibcode:2005MNRAS.363

Redshift of spectral lines in the optical spectrum of a supercluster of distant galaxies (right), as compared to that of the Sun (left)

Giovanelli. "Large-Scale Structure in the Local Universe: The Pisces-Perseus Supercluster." In Large-Scale Motions in the Universe, V. C. Rubin and G. F. Coyne

showed Virginia Tech's Mac OS X computer cluster supercomputer (a.k.a. supercluster) known as System X, consisting of 1,100 Power Mac G5 towers operating

dimming FRB 180916 location and periodicity Radcliffe wave Ophiuchus Supercluster explosion PSO J03094+27 (distant blazar) 2MASS J1047+21 wind speed measurements

largest known explosion in the history of the universe, the Ophiuchus Supercluster explosion. In January 2023, the telescope picked up a radio signal (21 cm

dimming FRB 180916 location and periodicity Radcliffe wave Ophiuchus Supercluster explosion PSO J03094+27 (distant blazar) 2MASS J1047+21 wind speed measurements

determine just what the Xeelee are constructing at the center of the local supercluster. Bolder is provided with a Xeelee nightfighter that can travel faster