Lynx Supercluster

The Lynx Supercluster was discovered in 1999

{{cite journal

|author=Rosati, P.

|display-authors=etal

|date=1999

|title=An X-Ray-Selected Galaxy Cluster at z = 1.26

|journal=The Astronomical Journal

|volume=118 |issue=1 |pages=76–85

|arxiv=astro-ph/9903381

|bibcode=1999AJ....118...76R

|doi=10.1086/300934

|s2cid=2560006

}} as ClG J0848+4453, a name now used to describe the western cluster, with ClG J0849+4452 being the eastern one.

{{cite web

|title=Lynx Supercluster

|url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NAME%20LYNX%20SUPERCLUSTER

|work=SIMBAD

}} It contains at least two clusters, designated RXJ 0848.9+4452 (at redshift z=1.26) and RXJ 0848.6+4453 (redshift z=1.27) . At the time of discovery, it was the most distant known supercluster{{cite journal |author=Nakata, F. |display-authors=etal |date=2004 |title=Discovery of a large-scale clumpy structure of the Lynx supercluster at z~1.27 |journal=Proceedings of the International Astronomical Union |volume=2004 |pages=29–33 |publisher=Cambridge University Press |bibcode=2004ogci.conf...29N |doi=10.1017/S1743921304000080 |doi-broken-date=1 November 2024 |isbn=0-521-84908-X|doi-access=free }} with a comoving distance of 12.9 billion light years. Additionally, seven smaller groups of galaxies are associated with the supercluster.

{{cite journal

|author=Ohta, K.

|display-authors=etal

|date=2003

|title=Optical Identification of the ASCA Lynx Deep Survey: An Association of Quasi-Stellar Objects and a Supercluster at z = 1.3?

|journal=The Astrophysical Journal

|volume=598 |issue=1

|pages=210–215

|arxiv=astro-ph/0308066

|bibcode=2003ApJ...598..210O

|doi=10.1086/378690

|s2cid=117171639

}} Through electromagnetic radiation and how it reacts with matter, we have been able to find three groupings of stars and two x-ray clusters within the Lynx.{{Cite journal|last1=Kim|first1=Jae-Woo|last2=Im|first2=Myungshin|last3=Lee|first3=Seong-Kook|last4=Edge|first4=Alastair C.|last5=Hyun|first5=Minhee|last6=Kim|first6=Dohyeong|last7=Choi|first7=Changsu|last8=Jueun Hong|last9=Jeon|first9=Yiseul|date=2016|title=Discovery of a Supercluster at z 0.91 and Testing the ΛCDM Cosmological Model|journal=The Astrophysical Journal Letters|language=en|volume=821|issue=1|pages=L10|doi=10.3847/2041-8205/821/1/L10|issn=2041-8205|arxiv=1604.03254|bibcode=2016ApJ...821L..10K|s2cid=118568359 |doi-access=free }}

The observation of the Lynx Supercluster has allowed other locations in proximity to be found. These locations are of special interest because of their high density, which has turned into the discovery of the seven smaller groups of galaxies mentioned above.{{Cite journal|last1=Nakata|first1=F.|last2=Kodama|first2=T.|last3=Shimasaku|first3=K.|last4=Doi|first4=M.|last5=Furusawa|first5=H.|last6=Hamabe|first6=M.|last7=Kimura|first7=M.|last8=Komiyama|first8=Y.|last9=Miyazaki|first9=S.|date=2005-03-11|title=Discovery of a large-scale clumpy structure around the Lynx supercluster at z 1.27|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=357|issue=4|pages=1357–1362|doi=10.1111/j.1365-2966.2005.08756.x|doi-access=free |issn=0035-8711|arxiv=astro-ph/0412460|bibcode=2005MNRAS.357.1357N|s2cid=15053608}}

A study has been conducted between the clusters in the Lynx, to examine and compare their color and shift.