The DESI Experiment, a whitepaper for Snowmass 2013
The Dark Energy Spectroscopic Instrument (DESI) is a massively multiplexed fiber-fed spectrograph that will make the next major advance in dark energy in the timeframe 2018-2022. On the Mayall telescope, DESI will obtain spectra and redshifts for at least 18 million emission-line galaxies, 4 million...
Gespeichert in:
| Veröffentlicht in: | arXiv.org 2013-08 |
|---|---|
| Hauptverfasser: | , , , , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | |
| container_start_page | |
| container_title | arXiv.org |
| container_volume | |
| creator | Levi, Michael Bebek, Chris Beers, Timothy Blum, Robert Cahn, Robert Eisenstein, Daniel Flaugher, Brenna Honscheid, Klaus Kron, Richard Lahav, Ofer McDonald, Patrick Roe, Natalie Schlegel, David representing the DESI collaboration |
| description | The Dark Energy Spectroscopic Instrument (DESI) is a massively multiplexed fiber-fed spectrograph that will make the next major advance in dark energy in the timeframe 2018-2022. On the Mayall telescope, DESI will obtain spectra and redshifts for at least 18 million emission-line galaxies, 4 million luminous red galaxies and 3 million quasi-stellar objects, in order to: probe the effects of dark energy on the expansion history using baryon acoustic oscillations (BAO), measure the gravitational growth history through redshift-space distortions, measure the sum of neutrino masses, and investigate the signatures of primordial inflation. The resulting 3-D galaxy maps at z2 will make 1%-level measurements of the distance scale in 35 redshift bins, thus providing unprecedented constraints on cosmological models. |
| format | Article |
| fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2086132636</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2086132636</sourcerecordid><originalsourceid>FETCH-proquest_journals_20861326363</originalsourceid><addsrcrecordid>eNqNirEKwjAUAIMgWLT_8MDVQvKejd01onO7lwwpbbFJTFLq59vBD3A6uLsNy5BIFNUZccfyGEfOOcoLliVljJrewE3VT1Afb8IwGZtOoGHph2S8XhV0LkBt3TLpGAG5oAPbdvoVTf7jnh3vqrk-Ch_cezYxtaObg11Ti7ySglCSpP-uL1I2Mnc</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2086132636</pqid></control><display><type>article</type><title>The DESI Experiment, a whitepaper for Snowmass 2013</title><source>Free E- Journals</source><creator>Levi, Michael ; Bebek, Chris ; Beers, Timothy ; Blum, Robert ; Cahn, Robert ; Eisenstein, Daniel ; Flaugher, Brenna ; Honscheid, Klaus ; Kron, Richard ; Lahav, Ofer ; McDonald, Patrick ; Roe, Natalie ; Schlegel, David ; representing the DESI collaboration</creator><creatorcontrib>Levi, Michael ; Bebek, Chris ; Beers, Timothy ; Blum, Robert ; Cahn, Robert ; Eisenstein, Daniel ; Flaugher, Brenna ; Honscheid, Klaus ; Kron, Richard ; Lahav, Ofer ; McDonald, Patrick ; Roe, Natalie ; Schlegel, David ; representing the DESI collaboration</creatorcontrib><description>The Dark Energy Spectroscopic Instrument (DESI) is a massively multiplexed fiber-fed spectrograph that will make the next major advance in dark energy in the timeframe 2018-2022. On the Mayall telescope, DESI will obtain spectra and redshifts for at least 18 million emission-line galaxies, 4 million luminous red galaxies and 3 million quasi-stellar objects, in order to: probe the effects of dark energy on the expansion history using baryon acoustic oscillations (BAO), measure the gravitational growth history through redshift-space distortions, measure the sum of neutrino masses, and investigate the signatures of primordial inflation. The resulting 3-D galaxy maps at z<2 and Lyman-alpha forest at z>2 will make 1%-level measurements of the distance scale in 35 redshift bins, thus providing unprecedented constraints on cosmological models.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Astronomical models ; Constraint modelling ; Cosmology ; Dark energy ; Galaxies ; Neutrinos ; Quasars ; Red shift</subject><ispartof>arXiv.org, 2013-08</ispartof><rights>2013. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>776,780</link.rule.ids></links><search><creatorcontrib>Levi, Michael</creatorcontrib><creatorcontrib>Bebek, Chris</creatorcontrib><creatorcontrib>Beers, Timothy</creatorcontrib><creatorcontrib>Blum, Robert</creatorcontrib><creatorcontrib>Cahn, Robert</creatorcontrib><creatorcontrib>Eisenstein, Daniel</creatorcontrib><creatorcontrib>Flaugher, Brenna</creatorcontrib><creatorcontrib>Honscheid, Klaus</creatorcontrib><creatorcontrib>Kron, Richard</creatorcontrib><creatorcontrib>Lahav, Ofer</creatorcontrib><creatorcontrib>McDonald, Patrick</creatorcontrib><creatorcontrib>Roe, Natalie</creatorcontrib><creatorcontrib>Schlegel, David</creatorcontrib><creatorcontrib>representing the DESI collaboration</creatorcontrib><title>The DESI Experiment, a whitepaper for Snowmass 2013</title><title>arXiv.org</title><description>The Dark Energy Spectroscopic Instrument (DESI) is a massively multiplexed fiber-fed spectrograph that will make the next major advance in dark energy in the timeframe 2018-2022. On the Mayall telescope, DESI will obtain spectra and redshifts for at least 18 million emission-line galaxies, 4 million luminous red galaxies and 3 million quasi-stellar objects, in order to: probe the effects of dark energy on the expansion history using baryon acoustic oscillations (BAO), measure the gravitational growth history through redshift-space distortions, measure the sum of neutrino masses, and investigate the signatures of primordial inflation. The resulting 3-D galaxy maps at z<2 and Lyman-alpha forest at z>2 will make 1%-level measurements of the distance scale in 35 redshift bins, thus providing unprecedented constraints on cosmological models.</description><subject>Astronomical models</subject><subject>Constraint modelling</subject><subject>Cosmology</subject><subject>Dark energy</subject><subject>Galaxies</subject><subject>Neutrinos</subject><subject>Quasars</subject><subject>Red shift</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNqNirEKwjAUAIMgWLT_8MDVQvKejd01onO7lwwpbbFJTFLq59vBD3A6uLsNy5BIFNUZccfyGEfOOcoLliVljJrewE3VT1Afb8IwGZtOoGHph2S8XhV0LkBt3TLpGAG5oAPbdvoVTf7jnh3vqrk-Ch_cezYxtaObg11Ti7ySglCSpP-uL1I2Mnc</recordid><startdate>20130804</startdate><enddate>20130804</enddate><creator>Levi, Michael</creator><creator>Bebek, Chris</creator><creator>Beers, Timothy</creator><creator>Blum, Robert</creator><creator>Cahn, Robert</creator><creator>Eisenstein, Daniel</creator><creator>Flaugher, Brenna</creator><creator>Honscheid, Klaus</creator><creator>Kron, Richard</creator><creator>Lahav, Ofer</creator><creator>McDonald, Patrick</creator><creator>Roe, Natalie</creator><creator>Schlegel, David</creator><creator>representing the DESI collaboration</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20130804</creationdate><title>The DESI Experiment, a whitepaper for Snowmass 2013</title><author>Levi, Michael ; Bebek, Chris ; Beers, Timothy ; Blum, Robert ; Cahn, Robert ; Eisenstein, Daniel ; Flaugher, Brenna ; Honscheid, Klaus ; Kron, Richard ; Lahav, Ofer ; McDonald, Patrick ; Roe, Natalie ; Schlegel, David ; representing the DESI collaboration</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20861326363</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Astronomical models</topic><topic>Constraint modelling</topic><topic>Cosmology</topic><topic>Dark energy</topic><topic>Galaxies</topic><topic>Neutrinos</topic><topic>Quasars</topic><topic>Red shift</topic><toplevel>online_resources</toplevel><creatorcontrib>Levi, Michael</creatorcontrib><creatorcontrib>Bebek, Chris</creatorcontrib><creatorcontrib>Beers, Timothy</creatorcontrib><creatorcontrib>Blum, Robert</creatorcontrib><creatorcontrib>Cahn, Robert</creatorcontrib><creatorcontrib>Eisenstein, Daniel</creatorcontrib><creatorcontrib>Flaugher, Brenna</creatorcontrib><creatorcontrib>Honscheid, Klaus</creatorcontrib><creatorcontrib>Kron, Richard</creatorcontrib><creatorcontrib>Lahav, Ofer</creatorcontrib><creatorcontrib>McDonald, Patrick</creatorcontrib><creatorcontrib>Roe, Natalie</creatorcontrib><creatorcontrib>Schlegel, David</creatorcontrib><creatorcontrib>representing the DESI collaboration</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>ProQuest Engineering Database</collection><collection>Publicly Available Content (ProQuest)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Levi, Michael</au><au>Bebek, Chris</au><au>Beers, Timothy</au><au>Blum, Robert</au><au>Cahn, Robert</au><au>Eisenstein, Daniel</au><au>Flaugher, Brenna</au><au>Honscheid, Klaus</au><au>Kron, Richard</au><au>Lahav, Ofer</au><au>McDonald, Patrick</au><au>Roe, Natalie</au><au>Schlegel, David</au><au>representing the DESI collaboration</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>The DESI Experiment, a whitepaper for Snowmass 2013</atitle><jtitle>arXiv.org</jtitle><date>2013-08-04</date><risdate>2013</risdate><eissn>2331-8422</eissn><abstract>The Dark Energy Spectroscopic Instrument (DESI) is a massively multiplexed fiber-fed spectrograph that will make the next major advance in dark energy in the timeframe 2018-2022. On the Mayall telescope, DESI will obtain spectra and redshifts for at least 18 million emission-line galaxies, 4 million luminous red galaxies and 3 million quasi-stellar objects, in order to: probe the effects of dark energy on the expansion history using baryon acoustic oscillations (BAO), measure the gravitational growth history through redshift-space distortions, measure the sum of neutrino masses, and investigate the signatures of primordial inflation. The resulting 3-D galaxy maps at z<2 and Lyman-alpha forest at z>2 will make 1%-level measurements of the distance scale in 35 redshift bins, thus providing unprecedented constraints on cosmological models.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2013-08 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_proquest_journals_2086132636 |
| source | Free E- Journals |
| subjects | Astronomical models Constraint modelling Cosmology Dark energy Galaxies Neutrinos Quasars Red shift |
| title | The DESI Experiment, a whitepaper for Snowmass 2013 |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-07T17%3A04%3A16IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=document&rft.atitle=The%20DESI%20Experiment,%20a%20whitepaper%20for%20Snowmass%202013&rft.jtitle=arXiv.org&rft.au=Levi,%20Michael&rft.date=2013-08-04&rft.eissn=2331-8422&rft_id=info:doi/&rft_dat=%3Cproquest%3E2086132636%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2086132636&rft_id=info:pmid/&rfr_iscdi=true |