Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Redshift
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
===Redshift surveys=== {{Main|Redshift survey}} [[File:2dfgrs.png|thumb|Rendering of the 2dFGRS data]] With advent of automated [[telescope]]s and improvements in [[astronomical spectroscopy|spectroscopes]], a number of collaborations have been made to map the universe in redshift space. By combining redshift with angular position data, a redshift survey maps the 3D distribution of matter within a field of the sky. These observations are used to measure properties of the [[Observable universe|large-scale structure]] of the universe. The [[CfA2 Great Wall|Great Wall]], a vast [[supercluster]] of galaxies over 500 million [[light-year]]s wide, provides a dramatic example of a large-scale structure that redshift surveys can detect.<ref>{{cite journal | title=Mapping the Universe | first1=M. J. | last1=Geller | first2=J. P. | last2=Huchra | journal=Science | volume=246 | issue=4932 | pages=897β903 | year=1989 | doi=10.1126/science.246.4932.897 | pmid=17812575 | bibcode=1989Sci...246..897G | s2cid=31328798 }}</ref> The first redshift survey was the [[CfA Redshift Survey]], started in 1977 with the initial data collection completed in 1982.<ref>See the CfA website for more details: {{cite web | title=The CfA Redshift Survey | first=John P. | last=Huchra | author-link=John Huchra | publisher=Harvard & Smithsonian Center for Astrophysics | url=https://lweb.cfa.harvard.edu/~dfabricant/huchra/zcat/ | access-date=2023-03-20 }}</ref> More recently, the [[2dF Galaxy Redshift Survey]] determined the large-scale structure of one section of the universe, measuring redshifts for over 220,000 galaxies; data collection was completed in 2002, and the final [[data set]] was released 30 June 2003.<ref>{{cite journal |title=The 2dF galaxy redshift survey: Power-spectrum analysis of the final dataset and cosmological implications | first1=Shaun | last1=Cole | author-link=Shaun Cole | last2=Percival | first2=Will J. | last3=Peacock | first3=John A. | last4=Norberg | first4=Peder | last5=Baugh | first5=Carlton M. | last6=Frenk | first6=Carlos S. | last7=Baldry | first7=Ivan | last8=Bland-Hawthorn | first8=Joss | last9=Bridges | first9=Terry | last10=Cannon | first10=Russell | last11=Colless | first11=Matthew | last12=Collins | first12=Chris | last13=Couch | first13=Warrick | last14=Cross | first14=Nicholas J. G. | last15=Dalton | first15=Gavin | last16=Eke | first16=Vincent R. | last17=De Propris | first17=Roberto | last18=Driver | first18=Simon P. | last19=Efstathiou | first19=George | last20=Ellis | first20=Richard S. | last21=Glazebrook | first21=Karl | last22=Jackson | first22=Carole | last23=Jenkins | first23=Adrian | last24=Lahav | first24=Ofer | last25=Lewis | first25=Ian | last26=Lumsden | first26=Stuart | last27=Maddox | first27=Steve | last28=Madgwick | first28=Darren | last29=Peterson | first29=Bruce A. | last30=Sutherland | first30=Will | last31=Taylor | first31=Keith | journal=Monthly Notices of the Royal Astronomical Society | volume=362 | issue=2 | pages=505β34 | date=2005 | bibcode=2005MNRAS.362..505C | arxiv=astro-ph/0501174 | doi=10.1111/j.1365-2966.2005.09318.x | doi-access=free | s2cid=6906627| display-authors=4 }} [http://msowww.anu.edu.au/2dFGRS/ 2dF Galaxy Redshift Survey homepage] {{Webarchive|url=https://web.archive.org/web/20070205010241/http://msowww.anu.edu.au/2dFGRS/ |date=2007-02-05 }}</ref> The [[Sloan Digital Sky Survey]] (SDSS) began collecting data in 1998<ref>{{cite journal |last1=Gunn |first1=James E. |last2=Siegmund |first2=Walter A. |last3=Mannery |first3=Edward J. |last4=Owen |first4=Russell E. |last5=Hull |first5=Charles L. |last6=Leger |first6=R. French |display-authors=etal |date=April 2006 |title=The 2.5 m Telescope of the Sloan Digital Sky Survey |journal=The Astronomical Journal |volume=131 |issue=4 |pages=2332β2359 |doi=10.1086/500975 |doi-access=free |arxiv=astro-ph/0602326 |bibcode=2006AJ....131.2332G }}</ref> and published its eighteenth data release in 2023.<ref>{{cite journal|last1=Almeida |first1=AndrΓ©s |display-authors=etal |title=The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V |journal=The Astrophysical Journal Supplement Series |date=2023 |volume=267 |number=2 |page=44 |doi=10.3847/1538-4365/acda98 |doi-access=free |arxiv=2301.07688 |bibcode=2023ApJS..267...44A}}</ref> SSDS has measured redshifts for galaxies as high as 0.8, and has recorded over 100,000 [[quasar]]s at {{math|''z'' {{=}} 3}} and beyond.<ref>{{cite web|url=https://www.sdss4.org/science/ |title=Science Results |website=SSDS |access-date=2025-05-20 }}</ref> The [[DEEP2 Redshift Survey]] used the [[Keck telescopes]] with the "DEIMOS" [[spectrograph]]; a follow-up to the pilot program DEEP1, DEEP2 was designed to measure faint galaxies with redshifts 0.7 and above, and it recorded redshifts of over 38,000 objects by its conclusion in 2013.<ref>{{cite conference | title=Science objectives and early results of the DEEP2 redshift survey| first1=Marc | last1=Davis |collaboration=DEEP2 collaboration |date=2002 | conference=Conference on Astronomical Telescopes and Instrumentation, Waikoloa, Hawaii, 22β28 Aug 2002 | arxiv=astro-ph/0209419 | bibcode=2003SPIE.4834..161D | doi=10.1117/12.457897 }}</ref><ref>{{cite journal|first1=Jeffrey A. |last1=Newman |display-authors=etal |title=The DEEP2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts |journal=The Astrophysical Journal Supplement Series |year=2013 |volume=208 |number=1 |page=5 |doi=10.1088/0067-0049/208/1/5|arxiv=1203.3192 |bibcode=2013ApJS..208....5N }}</ref>
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)