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{{Short description|Largest known structure in the observable universe}}
The '''Hercules-Corona Borealis Great Wall''' is a huge superstructure of galaxies that measures more than 10 billion [[light year]]s across.<ref name=conundrum/><ref name=original/> It is the largest and the most massive structure known in the observable universe.
{{Infobox galaxy cluster
| name = Hercules–Corona Borealis [[Galaxy filament|Great Wall]]
| image = {{multiple image
| direction = vertical
| width = 300
| image1 = Horváth et al. - New data support the existence of the Hercules-Corona Borealis Great Wall - Distribution of GRBs with measured redshift.svg
| image2 = Horváth et al. - New data support the existence of the Hercules-Corona Borealis Great Wall - Anisotropic distribution of GRBs near redshift z = 2.svg
}}
| caption = ''Top'': The total sample of 283 [[gamma-ray burst]]s (GRBs) recorded between 1997 and 2012 and examined by Horváth ''et al''., shown as blue dots in galactic coordinates. The reduced instances of GRBs through the equator are due to the [[Zone of Avoidance]] of the [[Milky Way]] plane.<br />
''Bottom'': The specific GRBs in group 4 of the sample lying at 1.6 < [[Cosmological redshift|z]] < 2.1. The clustering at the upper-left quarter region is the suspected Hercules–Corona Borealis Great Wall.<br />''Images credit: I. Horváth, Z. Bagoly, J. Hakkila and L. V. Tóth.''
| epoch = J2000
| constellation = [[Hercules (constellation)|Hercules]], [[Corona Borealis]], [[Lyra (constellation)|Lyra]], [[Boötes (constellation)|Boötes]] and [[Draco (constellation)|Draco]]<ref name=HBHT2/>
| ra = {{RA|17|0}}
| dec = {{DEC|+27|45}}
| major_axis_mpc = {{cvt|3|Gpc|Gly|0|lk=on}}<ref name=2014paper/><ref name=original/>
| minor_axis_mpc = {{cvt|2.2|Gpc|Gly|0|lk=on}} {{hub|0.6780}}
| redshift = 1.6 to 2.1<ref name=2014paper/><ref name=original/>
| distance = 9.612 to 10.538 [[Giga-|billion]] [[light-year]]s ([[Distance measures (cosmology)|light travel distance]])<ref name=z>{{cite web|title=Redshift-distance relation|url= http://www.lizard-tail.com/isana/lab/redshift/redshift-distance.php?h=70.5&m=0.272&l=0.728&scale=0.1&start_z=1.6&end_z=2.2}}</ref><br/> 15.049 to 17.675 billion light-years<br/>(present [[comoving distance]])<ref name=z/>
| mass =
| luminosity =
| flux =
| other_names =
}}


The '''Hercules–Corona Borealis Great Wall''' (HCB)<ref name=HBHT2>{{cite journal|last1=Horváth|first1=István|last2=Bagoly|first2=Zsolt|last3=Hakkila|first3=Jon|last4=Tóth|first4=L. Viktor|title=New data support the existence of the Hercules-Corona Borealis Great Wall|journal=Astronomy & Astrophysics|volume = 584|pages = A48|arxiv=1510.01933|year = 2015|doi = 10.1051/0004-6361/201424829|bibcode = 2015A&A...584A..48H |s2cid=56073380}}</ref><ref name=HBHT>{{cite journal|last1=Horváth|first1=István|last2=Bagoly|first2=Zsolt|last3=Hakkila|first3=Jon|last4=Tóth|first4=L. Viktor|title=Anomalies in the GRB spatial distribution|journal=Proceedings of Science|year=2014|page=78|doi=10.22323/1.233.0078 |arxiv=1507.05528|bibcode = 2014styd.confE..78H |doi-access=free }}</ref> or simply the '''Great Wall'''<ref name=cookie>{{Cite journal|arxiv =1507.00675 |last1 = Balazs|first1 = L. G.|title = A giant ring-like structure at 0.78<z<0.86 displayed by GRBs|journal = Monthly Notices of the Royal Astronomical Society|volume = 452|issue = 3|pages = 2236|last2 = Bagoly|first2 = Z.|last3 = Hakkila|first3 = J. E.|last4 = Horváth|first4 = I.|last5 = Kobori|first5 = J.|last6 = Racz|first6 = I.|last7 = Tóth|first7 = L. V.|year = 2015|doi = 10.1093/mnras/stv1421| doi-access=free |bibcode = 2015MNRAS.452.2236B |s2cid = 109936564}}</ref> is a [[galaxy filament]] that is the [[List of largest cosmic structures|largest known structure]] in the [[observable universe]], measuring approximately 10 billion [[Light-year|light-years]] in length (the [[observable universe]] is about 93 billion light-years in diameter). This massive superstructure is a region of the sky seen in the data set mapping of [[gamma-ray burst]]s (GRBs) that has been found to have a concentration of similarly distanced GRBs that is unusually higher than the expected average distribution.<ref name=2014paper/><ref name=original/> It was discovered in early November 2013 by a team of American and Hungarian astronomers led by István Horváth, Jon Hakkila and Zsolt Bagoly while analyzing data from the [[Swift Gamma-Ray Burst Mission]], together with other data from ground-based telescopes.<ref name=2014paper>{{cite journal | arxiv=1401.0533 | bibcode=2014A&A...561L..12H | title=Possible structure in the GRB sky distribution at redshift two | last1=Horváth | first1=István | last2=Hakkila | first2=Jon | last3=Bagoly | first3=Zsolt | journal=Astronomy & Astrophysics | date=2014 | volume=561 | pages=id.L12 | doi=10.1051/0004-6361/201323020 | s2cid=24224684 }}</ref><ref name=original>{{cite journal|author = Horváth I.|author2 = Hakkila J.|author3 = Bagoly Z. |name-list-style = amp|title = The largest structure of the Universe, defined by Gamma-Ray Bursts|journal =7th Huntsville Gamma-Ray Burst Symposium, GRB 2013: Paper 33 in EConf Proceedings C1304143 |volume = 1311|pages = 1104|date = 2013|arxiv=1311.1104|bibcode = 2013arXiv1311.1104H}}</ref> It is the largest known formation in the universe, exceeding the size of the [[Huge-LQG]] by about a factor of two.<ref>{{cite web |url= https://www.youtube.com/watch?v=36ngn5rS3Og |title= The Impossibly Huge Quasar Group |author= SciShow Space |website= [[YouTube]] |date= 21 July 2016 }}</ref>
This huge structure was discovered in November 2013 by a mapping of gamma ray bursts that occurs in the distant universe.<ref name=conundrum>{{cite web | last = | first = Irene Klotz | url = http://news.discovery.com/space/galaxies/universes-largest-structure-is-a-cosmic-conundrum-131119.htm | title = Universe's Largest Structure is a Cosmic Conundrum | date = 2013-11-19 | publisher = discovery |accessdate=2013-11-22}}</ref><ref name=original>{{cite journal|last = Horvath I. |first = Hakkila J.|coauthors = Bagoly Z. |title = The largest structure of the Universe, defined by Gamma-Ray Bursts|journal = |volume = |issue = |pages = |year = 2013|doi = |arxiv=1311.1104|bibcode = }}</ref>


The overdensity lies at the Second, Third and Fourth [[Galactic quadrant|Galactic Quadrants]] (NGQ2, NGQ3 and NGQ4) of the sky. Thus, it lies in the Northern Hemisphere, centered on the border of the [[constellation]]s [[Draco (constellation)|Draco]] and [[Hercules (constellation)|Hercules]]. The entire clustering consists of around 19 GRBs with the redshift ranges between 1.6 and 2.1.<ref name=original/>
==Physical characteristics==


Typically, the distribution of GRBs in the universe appears in the sets of less than the 2σ distribution, or with less than two GRBs in the average data of the point-radius system.{{clarify|date=January 2023}} One possible explanation of this concentration is the Hercules–Corona Borealis Great Wall.<ref name=conundrum>{{cite web | last = Klotz | first = Irene | url = http://news.discovery.com/space/galaxies/universes-largest-structure-is-a-cosmic-conundrum-131119.htm | title = Universe's Largest Structure is a Cosmic Conundrum | date = 2013-11-19 | publisher = discovery | access-date = 2013-11-22 | archive-date = 2016-05-16 | archive-url = https://web.archive.org/web/20160516172545/http://news.discovery.com/space/galaxies/universes-largest-structure-is-a-cosmic-conundrum-131119.htm | url-status = dead }}</ref><ref name=huff>{{cite web
The said structure is a [[galactic filament]],<ref name=original/> or a huge group of galaxies assembled by gravity. It is about 10 billion light-years (3 [[Parsec|Gpc]]) at its longest dimension, and about 7.2 billion light-years (2.2 Gpc) wide.<ref name=original/> The astonishing structure was found with the help of data from the [[Swift Gamma-Ray Burst Mission|Swift Spacecraft]] that tracks down [[gamma-ray burst]]s, large cosmic explosions of [[gamma ray]]s of distant stars heralding the birth of new [[black hole]]s.
| work = The Huffington Post
| title = Biggest Thing In The Universe Is So Gigantic It Shouldn't Exist At All
| date = 27 May 2014
| url = http://www.huffingtonpost.com/2014/05/27/biggest-thing-in-universe-video_n_5365111.html}}</ref> The wall has a mean size in excess of 2 billion to 3 billion parsecs (6 to 10 billion light-years).<ref name=HBHT/> Such a supercluster can explain the significant distribution of GRBs because of its tie to star formation.


Doubt has been placed on the existence of the structure in other studies, positing that the structure was found through biases in certain statistical tests, without considering the full effects of extinction.<ref name=":0">{{Cite journal|last=Christian|first=Sam|date=2020-07-11|title=Re-examining the evidence of the Hercules–Corona Borealis Great Wall|url=https://academic.oup.com/mnras/article/495/4/4291/5843300|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=495|issue=4|pages=4291–4296|doi=10.1093/mnras/staa1448|doi-access=free |issn=0035-8711|arxiv=2006.00141|s2cid=219177572}}</ref><ref name=":1">{{Cite journal|last1=Ukwatta|first1=T. N.|last2=Woźniak|first2=P. R.|date=2016-01-01|title=Investigation of redshift- and duration-dependent clustering of gamma-ray bursts|url=https://academic.oup.com/mnras/article/455/1/703/986230|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=455|issue=1|pages=703–711|doi=10.1093/mnras/stv2350|issn=0035-8711|doi-access=free|arxiv=1507.07117}}</ref> A 2020 paper (by the original group of discoverers and others) says that their analysis of the most reliable current dataset supports the structure's existence, but that the [[THESEUS (satellite)|THESEUS satellite]] will be needed to decide the question conclusively.<ref name="HS">{{Cite journal|last1=Horvath|first1=I.|last2=Szecsi|first2=D.|last3=Hakkila|first3=J.|last4=Szabo|first4=A.|last5=Racz|first5=I.I.|last6=Toth|first6=L.V.|last7=Pinter|first7=S.|last8=Bagoly|first8=Z.|date=2020-08-22|title=The clustering of gamma-ray bursts in the Hercules-Corona Borealis Great Wall: the largest structure in the Universe?|url=https://academic.oup.com/mnras/article/498/2/2544/5895980|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=498|issue=2|pages=2544–2553|doi=10.1093/mnras/staa2460 | arxiv=2008.03679 |issn=0035-8711|doi-access=free|quote=Our statistical analyses confirm the clustering's presence in the most reliable dataset currently available, ... We conclude from all this that the Hercules-Corona Borealis Great Wall may indeed be the largest structure in the Universe - but to be able to decide conclusively whether it actually exists, we need THESEUS.}}</ref>
The structure was named from its location, in the [[constellation]]s [[Hercules (constellation)|Hercules]] and [[Corona Borealis]].<ref name=conundrum/> It is at [[redshift]] 1.6-2.1, corresponding to a distance of approximately 10 billion light-years away.<ref name=original/>


==Discovery==
==Homogeneity problem==
[[File:Artist’s impression of a gamma-ray burst.jpg|thumb|Artist's interpretation of a [[gamma-ray burst]], like the ones used to map the wall]]
The overdensity was discovered using data from different space telescopes operating at [[gamma-ray]] and [[X-ray]] wavelengths, plus some data from ground-based telescopes. By the end of 2012 they successfully recorded 283 GRBs and measured their redshifts spectroscopically. They subdivided them to different group subsamples of different redshifts, initially with five groups, six groups, seven groups and eight groups, but each group division in the tests suggest a weak anisotropy and concentration, but this is not the case when it is subdivided to nine groups, each containing 31 GRBs; they noticed a significant clustering of GRBs of the fourth subsample (z = 1.6 to 2.1) with 19 of the 31 GRBs of the subsample are concentrated within the vicinity of the Second, Third and Fourth Northern [[Galactic quadrant|Galactic Quadrant]]s (NGQ2, NGQ3 and NGQ4) spanning no less than 120 degrees of the sky.<ref name=2014paper/><ref name="epic">{{cite web|date=15 July 2014|title=College of Charleston Professor Makes Discovery of Epic Proportions|url=http://today.cofc.edu/2014/07/15/college-charleston-professor-makes-scientific-discovery-epic-proportions/|access-date=14 November 2014|website=The College Today|publisher=Ron Mehanca}}</ref> Under current stellar evolutionary models GRBs are only caused by neutron star collision and collapse of massive stars, and as such, stars causing these events are only found in regions with more matter in general. Using the two-point [[Kolmogorov–Smirnov test]], a nearest-neighbor test, and a Bootstrap point-radius method, they found the statistical significance of this observation to be less than 0.05 %. The possible binomial probability to find a clustering was p=0.0000055. It is later reported in the paper that the clustering may be associated with a previously unknown supermassive structure.<ref name=2014paper/>


==Nomenclature==
According to the [[cosmological principle]], the random fluctuations in quantities such as the matter density between different regions of the universe are small. Different data approves this and found out that scales exceeding this limit may defy the said principle. Yadav ''et al'' suggested that the tips of the scales might be as well to 260[[Parsec#Megaparsecs and gigaparsecs|/h Mpc]].<ref name="Yadav">{{cite journal|last=Yadav|first=Jaswant|coauthors=J. S. Bagla and Nishikanta Khandai|title=Fractal dimension as a measure of the scale of homogeneity|journal=Monthly notices of the Royal Astronomical Society|date=25 February 2010|volume=405|issue=3|pages=2009–2015|doi=10.1111/j.1365-2966.2010.16612.x|url=http://mnras.oxfordjournals.org/content/405/3/2009.abstract?ijkey=dee165dd1cdd9c394d4f6c3ad6bbd7d468d7997a&keytype2=tf_ipsecsha|accessdate=15 January 2013}}</ref> Some scientists say that the maximum sizes of structures was somewhere around 70-130/h Mpc based on the measure of the homogeneity scale<ref name="Hogg">Hogg, D.W. ''et al''., (May 2005) "Cosmic Homogeneity Demonstrated with Luminous Red Galaxies". ''The Astrophysical Journal '''''624''': 54-58. [http://arxiv.org/abs/astro-ph/0411197 arXiv:astro-ph/0411197]. [http://adsabs.harvard.edu/abs/2005ApJ...624...54H Bibcode:2005ApJ...624...54H]. [http://dx.doi.org/10.1086/429084 doi:10.1086/429084].</ref><ref name="Scrimgeour">Scrimgeour, Morag I. ''et al.'', (May 2012) "The WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneity". ''Monthly Notices of the Royal Astronomical Society'' 425 (1): 116-134. [http://arxiv.org/abs/1205.6812 arXiv:1205.6812]. [http://adsabs.harvard.edu/abs/2012MNRAS.425..116S Bibcode: 2012MNRAS.425...116S]. [http://dx.doi.org/10.1111/j.1365-2966.2012.21402.x doi: 10.1111/j.1365-2966.2012.21402.x].</ref><ref name="Nadathur">Nadathur, Seshadri, (July 2013) "Seeing patterns in noise: gigaparsec-scale 'structures' that do not violate homogeneity". ''Monthly Notices of the Royal Astronomical Society'' in press. [http://arxiv.org/abs/1306.1700 arXiv:1306.1700]. [http://adsabs.harvard.edu/abs/2013MNRAS.tmp.1690N Bibcode: 2013MNRAS.tmp.1690N]. [http://dx.doi.org/10.1093%2Fmnras%2Fstt1028 doi: 10.1093/mnras/stt1028].</ref>. No structures are expected to be larger than the scale since the current evolutionary theories of the formation of the universe do not accept objects larger than the scale.
The authors of the paper concluded that a structure was the possible explanation of the clustering, but they never associated any name with it.<ref name=magazine>{{cite web
| url = https://magazine.cofc.edu/2014/11/03/jon-hakkila/
| title = Starstruck
| date = 3 November 2014
| website = College of Charleston Magazine
| publisher = Mark Berry
| access-date = 14 November 2014
}}</ref> Hakkila stated that "During the process, we were more concerned with whether it was real or not."<ref name=magazine/> The term "Hercules–Corona Borealis Great Wall" was coined by Johndric Valdez, a [[Philippines|Filipino]] teenager from [[Marikina]] on [[Wikipedia]],<ref name=magazine/><ref>{{cite web|title=Hercules-Corona Borealis Great Wall|url=https://en.wikipedia.org/enwiki/w/index.php?title=Hercules-Corona_Borealis_Great_Wall&oldid=582805180|website=Wikipedia|access-date=12 January 2016|date=22 November 2013}}</ref><!--Please do not remove this reference without going to talk. It references an early version of this article, where the structure was named.--> after reading a [[Discovery News]] report<ref name=DN>{{cite news|last1=Klotz|first1=Irene|title=Universe's Largest Structure is a Cosmic Conundrum|url=http://news.discovery.com/space/galaxies/universes-largest-structure-is-a-cosmic-conundrum-131119.htm|access-date=12 January 2016|work=Discovery News|date=19 November 2013|archive-date=16 May 2016|archive-url=https://web.archive.org/web/20160516172545/http://news.discovery.com/space/galaxies/universes-largest-structure-is-a-cosmic-conundrum-131119.htm|url-status=dead}}</ref> three weeks after the structure's discovery in 2013. The nomenclature was used by Jacqueline Howard, on her "Talk Nerdy to Me" video series,<ref>{{cite news|last1=Howard|first1=Jacqueline|title=The Biggest Thing In The Universe Is So Gigantic It Shouldn't Exist At All|url=http://www.huffingtonpost.com/2014/05/27/biggest-thing-in-universe-video_n_5365111.html|work=The Huffington Post|date=27 May 2014}}</ref> and Hakkila would later use the name.<ref name="HBHT2"/>


The term is misleading, since the clustering occupies a region much larger than the constellations [[Hercules (constellation)|Hercules]] and [[Corona Borealis]]. In fact, it covers the region from [[Boötes]] to as far as the [[Zodiac]] constellation [[Gemini (constellation)|Gemini]]. In addition, the clustering is somewhat roundish in shape, which is more likely a [[supercluster]], in contrast to an elongated shape of a galaxy wall. Another name, the Great GRB Wall, was proposed in a later paper.<ref name=cookie/>
The [[Sloan Great Wall]], discovered in 2003, is 1.37 billion light years across,<ref name=apj624_2_463>{{Cite journal | display-authors=1 | last1=Gott | first1=J. Richard, III | last2=Jurić | first2=Mario | last3=Schlegel| first3=David | last4=Hoyle | first4=Fiona | last5=Vogeley | first5=Michael | last6=Tegmark | first6=Max | last7=Bahcall | first7=Neta |last8=Brinkmann | first8=Jon | title=A Map of the Universe | journal=The Astrophysical Journal | volume=624 | issue=2 | pages=463–484 |month=May | year=2005 | doi=10.1086/428890 | bibcode=2005ApJ...624..463G |arxiv = astro-ph/0310571 | postscript=<!-- Bot inserted parameter. Either remove it; or change its value to "." for the cite to end in a ".", as necessary. -->{{inconsistent citations}} }}</ref> and is marginally larger than the scale.


==Characteristics==
The [[Huge-LQG]] (Huge Large Quasar Group), discovered in 2012, is 4 billion light years across.<ref name="RAS2">{{cite journal | arxiv=1211.6256 | bibcode=2012arXiv1211.6256C | url=http://mnras.oxfordjournals.org/content/early/2013/01/07/mnras.sts497.full | title=A structure in the early Universe at z ∼ 1.3 that exceeds the homogeneity scale of the R-W concordance cosmology | date=2012-01-11 | accessdate=14 January 2013 | last=Clowes | first=Roger | last2=Harris | last3=Raghunathan | last4=Campusano | last5=Soechting | last6=Graham | coauthors=Kathryn A. Harris, Srinivasan Raghunathan, Luis E. Campusano, Ilona K. Söchting and Matthew J. Graham | journal=Monthly notices of the royal astronomical society | year=2013 | volume=1211 | pages=6256 | doi=10.1093/mnras/sts497 | issue=4}}</ref> However, long range correlations provide evidences of the impossibility of this structure.<ref>Gaite, Jose, Dominguez, Alvaro and Perez-Mercader, Juan (August 1999) "The fractal distribution of galaxies and the transition to homogeneity". ''The Astrophysical Journal'' '''522''': L5-L8. [http://arxiv.org/abs/astro-ph/9812132 arXiv:astroph/9812132]. [http://adsabs.harvard.edu/abs/1999ApJ...522L...5G Bibcode: 1999ApJ...522L...5G]. [http://dx.doi.org/10.1086/312204 doi: 10.1086/312204].</ref>


The paper states that "14 of the 31 GRBs are concentrated within 45 degrees of the sky",<ref name=original/> which translates to the size of about 10 billion light-years (3 [[gigaparsec]]s) in its longest dimension,{{or|date=January 2022}} which is approximately one ninth (10.7%) of the diameter of the observable universe. However, the clustering contains 19 to 22 GRBs, and spans a length three times longer than the remaining 14 GRBs. Indeed, the clustering crosses over 20 constellations and covers 125 degrees of the sky, or almost 15,000 square degrees in total area, which translates to about 18 to 23 billion light-years (5.5 to 7 gigaparsecs) in length. It lies at [[redshift]] 1.6 to 2.1.
The Hercules-Corona Borealis Great Wall, is more than 8 times larger than the scale,<ref name=conundrum/> and so greatly exceeds the homogeneity scale.

==Methods for discovery==
{{multiple issues|section=yes|
{{technical|section|date=January 2023}}
{{overly detailed|section|date=January 2023}}
}}
The team subdivides the 283 GRBs into nine groups in sets of 31 GRBs. At least three different methods have been used to reveal the significance of the clustering.

===Two-dimensional Kolmogorov–Smirnov test===

The [[Kolmogorov–Smirnov test]] (K–S test) is a nonparametric test of the equality of continuous, one-dimensional probability distributions that can be used to compare a sample with a reference probability distribution (one-sample K–S test), or to compare two samples (two-sample K–S test), thus, it can be used to test the comparisons of the distributions of the nine subsamples. However, the K–S test can only be used for one dimensional data—it cannot be used for sets of data involving two dimensions such as the clustering. However, a 1983 paper by J. A. Peacock suggests that one should use all four possible orderings between ordered pairs to calculate the difference between the two distributions. Since the sky distribution of any object is composed of two orthogonal angular coordinates, the team used this methodology.<ref name=original/>

{| class="wikitable"
|-
! Group no.
! 2
! 3
! 4
! 5
! 6
! 7
! 8
! 9
|-
| '''1'''
| 9
| 9
| style="background:yellow;"|''15''
| 11
| 13
| 9
| 12
| 8
|-
| '''2'''
|
| 10
| style="background:yellow;"|''18''
| 7
| style="background:yellow;"|''15''
| 11
| 9
| 12
|-
| '''3'''
|
|
| style="background:yellow;"|''14''
| 9
| 11
| style="background:yellow;"|''14''
| 9
| 10
|-
| '''4'''
|
|
|
| style="background:yellow;"|''15''
| 10
| style="background:yellow;"|''15''
| style="background:yellow;"|''17''
| 11
|-
| '''5'''
|
|
|
|
| 13
| 13
| 8
| 10
|-
| '''6'''
|
|
|
|
|
| 10
| 13
| 8
|-
| '''7'''
|
|
|
|
|
|
| 10
| 10
|-
| '''8'''
|
|
|
|
|
|
|
| 11
|}

The above table shows the results of the 2D K–S test of the nine GRB subsamples. For example, the difference between group 1 and group 2 is 9 points. Values greater than 2{{mvar|σ}} (significant values equal to or greater than 14) are italicized and colored in yellow background. Note the six significant values in group 4.

The results of the test shows that out of the six largest numbers, five belong to group 4. Six of the eight numerical comparisons of group 4 belong to the eight largest numerical differences, that is, numbers greater than 14. To calculate the approximate probabilities for the different numbers, the team ran 40 thousand simulations where 31 random points are compared with 31 other random points. The result contains the number 18 twenty-eight times and numbers larger than 18 ten times, so the probability of having numbers larger than 17 is 0.095%. The probability of having numbers larger than 16 is {{mvar|p}}=0.0029, of having numbers larger than 15 is {{mvar|p}}=0.0094, and of having numbers larger than 14 is {{mvar|p}}=0.0246. For a random distribution, this means that numbers larger than 14 correspond to 2{{mvar|σ}} deviations and numbers larger than 16 correspond to 3{{mvar|σ}} deviations. The probability of having numbers larger than 13 is {{mvar|p}}=0.057, or 5.7%, which is not statistically significant.<ref name=original/>

===Nearest-neighbor test===

Using nearest neighbor statistics, a similar test to the 2D K–S test; 21 consecutive probabilities in group 4 reach the 2{{mvar|σ}} limit and 9 consecutive comparisons reach the 3{{mvar|σ}} limit. One can calculate binomial probabilities. For example, 14 out of the 31 GRBs in this redshift band are concentrated in approximately one eighth of the sky. The binomial probability of finding this deviation is {{mvar|p}}=0.0000055.

===Bootstrap point-radius===

The team also used a [[Bootstrapping (statistics)|bootstrapping statistic]] to determine the number of GRBs within a preferred angular area of the sky. The test showed that the 15–25% of the sky identified for group 4 contains significantly more GRBs than similar circles at other GRB redshifts. When the area is chosen to be {{math|0.1125 × 4{{mvar|π}}}}, 14 GRBs out of the 31 lie inside the circle. When the area is chosen to be {{math|0.2125 × 4{{var|π}}}}, 19 GRBs out of the 31 lie inside the circle. When the area is chosen to be {{math|0.225 × 4{{var|π}}}}, 20 GRBs out of the 31 lie inside the circle. In this last case only 7 out of the 4,000 bootstrap cases had 20 or more GRBs inside the circle. This result is, therefore, a statistically significant ({{mvar|p}}=0.0018) deviation (the binomial probability for this being random is less than 10<sup>−6</sup>). The team built statistics for this test by repeating the process a large number of times (ten thousand). From the ten thousand Monte Carlo runs they selected the largest number of bursts found within the angular circle. Results show that only 7 out of the 4,000 bootstrap cases have 20 GRBs in a preferred angular circle.

== Controversy ==
Some studies have cast doubt on the existence of the HCB. A study in 2016 found that the observed distribution of GRBs was consistent with what could be derived from Monte Carlo simulations, but was below the 95% probability threshold (p < .05) of significance typically used in [[p-value|''p''-value]] analyses.<ref name=":1"/> A study in 2020 found even higher probability levels when considering biases in statistical tests, and argued that given nine redshift ranges were used, the probability threshold should actually be lower than p < 0.05, instead around p < 0.005.<ref name=":0"/> A 2020 paper (by the original group of discoverers and others) says that their analysis of the most reliable current dataset supports the structure's existence, but that the [[THESEUS (satellite)|THESEUS satellite]] will be needed to decide the question conclusively.<ref name="HS"/>


==See also==
==See also==
* [[CfA2 Great Wall]]
* [[CfA2 Great Wall]]
* [[The Giant Arc]], another large cosmic structure
* [[Pisces-Cetus Supercluster Complex]]
* [[Big Ring]], another large cosmic structure
* [[Observable universe#Large-scale structure]]
* [[Observable universe#Large-scale structure|Large-scale structure of the universe]]
* [[List of largest cosmic structures]]
* [[South Pole Wall]], a large "wall" of galaxies


==References==
==References==

{{reflist}}
{{reflist}}


{{2013 in space}}
{{Hercules (constellation)}}
{{Portal bar|Astronomy|Stars|Spaceflight|Outer space|Solar System}}

{{DEFAULTSORT:Hercules-Corona Borealis Great Wall}}
[[Category:Galaxy filaments]]
[[Category:Galaxy filaments]]
[[Category:Astronomical objects discovered in 2013]]
[[Category:Large-scale structure of the cosmos]]
[[Category:Astronomical objects discovered in 2013|20131105]]
[[Category:Hercules (constellation)]]
[[Category:Corona Borealis]]

Latest revision as of 18:52, 7 November 2024

Hercules–Corona Borealis Great Wall
Top: The total sample of 283 gamma-ray bursts (GRBs) recorded between 1997 and 2012 and examined by Horváth et al., shown as blue dots in galactic coordinates. The reduced instances of GRBs through the equator are due to the Zone of Avoidance of the Milky Way plane.
Bottom: The specific GRBs in group 4 of the sample lying at 1.6 < z < 2.1. The clustering at the upper-left quarter region is the suspected Hercules–Corona Borealis Great Wall.
Images credit: I. Horváth, Z. Bagoly, J. Hakkila and L. V. Tóth.
Observation data (Epoch J2000)
Constellation(s)Hercules, Corona Borealis, Lyra, Boötes and Draco[1]
Right ascension17h 0m
Declination+27° 45′
Major axisGpc (10 Gly)[2][3]
Minor axis2.2 Gpc (7 Gly) h−1
0.6780
Redshift1.6 to 2.1[2][3]
Distance9.612 to 10.538 billion light-years (light travel distance)[4]
15.049 to 17.675 billion light-years
(present comoving distance)[4]

The Hercules–Corona Borealis Great Wall (HCB)[1][5] or simply the Great Wall[6] is a galaxy filament that is the largest known structure in the observable universe, measuring approximately 10 billion light-years in length (the observable universe is about 93 billion light-years in diameter). This massive superstructure is a region of the sky seen in the data set mapping of gamma-ray bursts (GRBs) that has been found to have a concentration of similarly distanced GRBs that is unusually higher than the expected average distribution.[2][3] It was discovered in early November 2013 by a team of American and Hungarian astronomers led by István Horváth, Jon Hakkila and Zsolt Bagoly while analyzing data from the Swift Gamma-Ray Burst Mission, together with other data from ground-based telescopes.[2][3] It is the largest known formation in the universe, exceeding the size of the Huge-LQG by about a factor of two.[7]

The overdensity lies at the Second, Third and Fourth Galactic Quadrants (NGQ2, NGQ3 and NGQ4) of the sky. Thus, it lies in the Northern Hemisphere, centered on the border of the constellations Draco and Hercules. The entire clustering consists of around 19 GRBs with the redshift ranges between 1.6 and 2.1.[3]

Typically, the distribution of GRBs in the universe appears in the sets of less than the 2σ distribution, or with less than two GRBs in the average data of the point-radius system.[clarification needed] One possible explanation of this concentration is the Hercules–Corona Borealis Great Wall.[8][9] The wall has a mean size in excess of 2 billion to 3 billion parsecs (6 to 10 billion light-years).[5] Such a supercluster can explain the significant distribution of GRBs because of its tie to star formation.

Doubt has been placed on the existence of the structure in other studies, positing that the structure was found through biases in certain statistical tests, without considering the full effects of extinction.[10][11] A 2020 paper (by the original group of discoverers and others) says that their analysis of the most reliable current dataset supports the structure's existence, but that the THESEUS satellite will be needed to decide the question conclusively.[12]

Discovery

[edit]
Artist's interpretation of a gamma-ray burst, like the ones used to map the wall

The overdensity was discovered using data from different space telescopes operating at gamma-ray and X-ray wavelengths, plus some data from ground-based telescopes. By the end of 2012 they successfully recorded 283 GRBs and measured their redshifts spectroscopically. They subdivided them to different group subsamples of different redshifts, initially with five groups, six groups, seven groups and eight groups, but each group division in the tests suggest a weak anisotropy and concentration, but this is not the case when it is subdivided to nine groups, each containing 31 GRBs; they noticed a significant clustering of GRBs of the fourth subsample (z = 1.6 to 2.1) with 19 of the 31 GRBs of the subsample are concentrated within the vicinity of the Second, Third and Fourth Northern Galactic Quadrants (NGQ2, NGQ3 and NGQ4) spanning no less than 120 degrees of the sky.[2][13] Under current stellar evolutionary models GRBs are only caused by neutron star collision and collapse of massive stars, and as such, stars causing these events are only found in regions with more matter in general. Using the two-point Kolmogorov–Smirnov test, a nearest-neighbor test, and a Bootstrap point-radius method, they found the statistical significance of this observation to be less than 0.05 %. The possible binomial probability to find a clustering was p=0.0000055. It is later reported in the paper that the clustering may be associated with a previously unknown supermassive structure.[2]

Nomenclature

[edit]

The authors of the paper concluded that a structure was the possible explanation of the clustering, but they never associated any name with it.[14] Hakkila stated that "During the process, we were more concerned with whether it was real or not."[14] The term "Hercules–Corona Borealis Great Wall" was coined by Johndric Valdez, a Filipino teenager from Marikina on Wikipedia,[14][15] after reading a Discovery News report[16] three weeks after the structure's discovery in 2013. The nomenclature was used by Jacqueline Howard, on her "Talk Nerdy to Me" video series,[17] and Hakkila would later use the name.[1]

The term is misleading, since the clustering occupies a region much larger than the constellations Hercules and Corona Borealis. In fact, it covers the region from Boötes to as far as the Zodiac constellation Gemini. In addition, the clustering is somewhat roundish in shape, which is more likely a supercluster, in contrast to an elongated shape of a galaxy wall. Another name, the Great GRB Wall, was proposed in a later paper.[6]

Characteristics

[edit]

The paper states that "14 of the 31 GRBs are concentrated within 45 degrees of the sky",[3] which translates to the size of about 10 billion light-years (3 gigaparsecs) in its longest dimension,[original research?] which is approximately one ninth (10.7%) of the diameter of the observable universe. However, the clustering contains 19 to 22 GRBs, and spans a length three times longer than the remaining 14 GRBs. Indeed, the clustering crosses over 20 constellations and covers 125 degrees of the sky, or almost 15,000 square degrees in total area, which translates to about 18 to 23 billion light-years (5.5 to 7 gigaparsecs) in length. It lies at redshift 1.6 to 2.1.

Methods for discovery

[edit]

The team subdivides the 283 GRBs into nine groups in sets of 31 GRBs. At least three different methods have been used to reveal the significance of the clustering.

Two-dimensional Kolmogorov–Smirnov test

[edit]

The Kolmogorov–Smirnov test (K–S test) is a nonparametric test of the equality of continuous, one-dimensional probability distributions that can be used to compare a sample with a reference probability distribution (one-sample K–S test), or to compare two samples (two-sample K–S test), thus, it can be used to test the comparisons of the distributions of the nine subsamples. However, the K–S test can only be used for one dimensional data—it cannot be used for sets of data involving two dimensions such as the clustering. However, a 1983 paper by J. A. Peacock suggests that one should use all four possible orderings between ordered pairs to calculate the difference between the two distributions. Since the sky distribution of any object is composed of two orthogonal angular coordinates, the team used this methodology.[3]

Group no. 2 3 4 5 6 7 8 9
1 9 9 15 11 13 9 12 8
2 10 18 7 15 11 9 12
3 14 9 11 14 9 10
4 15 10 15 17 11
5 13 13 8 10
6 10 13 8
7 10 10
8 11

The above table shows the results of the 2D K–S test of the nine GRB subsamples. For example, the difference between group 1 and group 2 is 9 points. Values greater than 2σ (significant values equal to or greater than 14) are italicized and colored in yellow background. Note the six significant values in group 4.

The results of the test shows that out of the six largest numbers, five belong to group 4. Six of the eight numerical comparisons of group 4 belong to the eight largest numerical differences, that is, numbers greater than 14. To calculate the approximate probabilities for the different numbers, the team ran 40 thousand simulations where 31 random points are compared with 31 other random points. The result contains the number 18 twenty-eight times and numbers larger than 18 ten times, so the probability of having numbers larger than 17 is 0.095%. The probability of having numbers larger than 16 is p=0.0029, of having numbers larger than 15 is p=0.0094, and of having numbers larger than 14 is p=0.0246. For a random distribution, this means that numbers larger than 14 correspond to 2σ deviations and numbers larger than 16 correspond to 3σ deviations. The probability of having numbers larger than 13 is p=0.057, or 5.7%, which is not statistically significant.[3]

Nearest-neighbor test

[edit]

Using nearest neighbor statistics, a similar test to the 2D K–S test; 21 consecutive probabilities in group 4 reach the 2σ limit and 9 consecutive comparisons reach the 3σ limit. One can calculate binomial probabilities. For example, 14 out of the 31 GRBs in this redshift band are concentrated in approximately one eighth of the sky. The binomial probability of finding this deviation is p=0.0000055.

Bootstrap point-radius

[edit]

The team also used a bootstrapping statistic to determine the number of GRBs within a preferred angular area of the sky. The test showed that the 15–25% of the sky identified for group 4 contains significantly more GRBs than similar circles at other GRB redshifts. When the area is chosen to be 0.1125 × 4π, 14 GRBs out of the 31 lie inside the circle. When the area is chosen to be 0.2125 × 4π, 19 GRBs out of the 31 lie inside the circle. When the area is chosen to be 0.225 × 4π, 20 GRBs out of the 31 lie inside the circle. In this last case only 7 out of the 4,000 bootstrap cases had 20 or more GRBs inside the circle. This result is, therefore, a statistically significant (p=0.0018) deviation (the binomial probability for this being random is less than 10−6). The team built statistics for this test by repeating the process a large number of times (ten thousand). From the ten thousand Monte Carlo runs they selected the largest number of bursts found within the angular circle. Results show that only 7 out of the 4,000 bootstrap cases have 20 GRBs in a preferred angular circle.

Controversy

[edit]

Some studies have cast doubt on the existence of the HCB. A study in 2016 found that the observed distribution of GRBs was consistent with what could be derived from Monte Carlo simulations, but was below the 95% probability threshold (p < .05) of significance typically used in p-value analyses.[11] A study in 2020 found even higher probability levels when considering biases in statistical tests, and argued that given nine redshift ranges were used, the probability threshold should actually be lower than p < 0.05, instead around p < 0.005.[10] A 2020 paper (by the original group of discoverers and others) says that their analysis of the most reliable current dataset supports the structure's existence, but that the THESEUS satellite will be needed to decide the question conclusively.[12]

See also

[edit]

References

[edit]
  1. ^ a b c Horváth, István; Bagoly, Zsolt; Hakkila, Jon; Tóth, L. Viktor (2015). "New data support the existence of the Hercules-Corona Borealis Great Wall". Astronomy & Astrophysics. 584: A48. arXiv:1510.01933. Bibcode:2015A&A...584A..48H. doi:10.1051/0004-6361/201424829. S2CID 56073380.
  2. ^ a b c d e f Horváth, István; Hakkila, Jon; Bagoly, Zsolt (2014). "Possible structure in the GRB sky distribution at redshift two". Astronomy & Astrophysics. 561: id.L12. arXiv:1401.0533. Bibcode:2014A&A...561L..12H. doi:10.1051/0004-6361/201323020. S2CID 24224684.
  3. ^ a b c d e f g h Horváth I.; Hakkila J. & Bagoly Z. (2013). "The largest structure of the Universe, defined by Gamma-Ray Bursts". 7th Huntsville Gamma-Ray Burst Symposium, GRB 2013: Paper 33 in EConf Proceedings C1304143. 1311: 1104. arXiv:1311.1104. Bibcode:2013arXiv1311.1104H.
  4. ^ a b "Redshift-distance relation".
  5. ^ a b Horváth, István; Bagoly, Zsolt; Hakkila, Jon; Tóth, L. Viktor (2014). "Anomalies in the GRB spatial distribution". Proceedings of Science: 78. arXiv:1507.05528. Bibcode:2014styd.confE..78H. doi:10.22323/1.233.0078.
  6. ^ SciShow Space (21 July 2016). "The Impossibly Huge Quasar Group". YouTube.
  7. ^ Klotz, Irene (2013-11-19). "Universe's Largest Structure is a Cosmic Conundrum". discovery. Archived from the original on 2016-05-16. Retrieved 2013-11-22.
  8. ^ "Biggest Thing In The Universe Is So Gigantic It Shouldn't Exist At All". The Huffington Post. 27 May 2014.
  9. ^ a b Christian, Sam (2020-07-11). "Re-examining the evidence of the Hercules–Corona Borealis Great Wall". Monthly Notices of the Royal Astronomical Society. 495 (4): 4291–4296. arXiv:2006.00141. doi:10.1093/mnras/staa1448. ISSN 0035-8711. S2CID 219177572.
  10. ^ a b Ukwatta, T. N.; Woźniak, P. R. (2016-01-01). "Investigation of redshift- and duration-dependent clustering of gamma-ray bursts". Monthly Notices of the Royal Astronomical Society. 455 (1): 703–711. arXiv:1507.07117. doi:10.1093/mnras/stv2350. ISSN 0035-8711.
  11. ^ a b Horvath, I.; Szecsi, D.; Hakkila, J.; Szabo, A.; Racz, I.I.; Toth, L.V.; Pinter, S.; Bagoly, Z. (2020-08-22). "The clustering of gamma-ray bursts in the Hercules-Corona Borealis Great Wall: the largest structure in the Universe?". Monthly Notices of the Royal Astronomical Society. 498 (2): 2544–2553. arXiv:2008.03679. doi:10.1093/mnras/staa2460. ISSN 0035-8711. Our statistical analyses confirm the clustering's presence in the most reliable dataset currently available, ... We conclude from all this that the Hercules-Corona Borealis Great Wall may indeed be the largest structure in the Universe - but to be able to decide conclusively whether it actually exists, we need THESEUS.
  12. ^ "College of Charleston Professor Makes Discovery of Epic Proportions". The College Today. Ron Mehanca. 15 July 2014. Retrieved 14 November 2014.
  13. ^ a b c "Starstruck". College of Charleston Magazine. Mark Berry. 3 November 2014. Retrieved 14 November 2014.
  14. ^ "Hercules-Corona Borealis Great Wall". Wikipedia. 22 November 2013. Retrieved 12 January 2016.
  15. ^ Klotz, Irene (19 November 2013). "Universe's Largest Structure is a Cosmic Conundrum". Discovery News. Archived from the original on 16 May 2016. Retrieved 12 January 2016.
  16. ^ Howard, Jacqueline (27 May 2014). "The Biggest Thing In The Universe Is So Gigantic It Shouldn't Exist At All". The Huffington Post.