id:"swepub:oai:DiVA.org:su-146940"
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 02998naa a2200517 4500 | |
| 001 | oai:DiVA.org:su-146940 | |
| 003 | SwePub | |
| 008 | 170919s2017 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1469402 URI |
| 024 | 7 | a https://doi.org/10.1093/mnras/stx16772 DOI |
| 040 | a (SwePub)su | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Diener, C.4 aut |
| 245 | 1 0 | a The MUSE-Wide survey :b detection of a clustering signal from Lyman alpha emitters in the range 3 < z < 6 |
| 264 | c 2017-07-05 | |
| 264 | 1 | b Oxford University Press (OUP),c 2017 |
| 338 | a print2 rdacarrier | |
| 520 | a We present a clustering analysis of a sample of 238 Ly alpha emitters at redshift 3 less than or similar to z less than or similar to 6 from the MUSE-Wide survey. This survey mosaics extragalactic legacy fields with 1h MUSE pointings to detect statistically relevant samples of emission line galaxies. We analysed the first year observations from MUSE-Wide making use of the clustering signal in the line-of-sight direction. This method relies on comparing pair-counts at close redshifts for a fixed transverse distance and thus exploits the full potential of the redshift range covered by our sample. A clear clustering signal with a correlation length of r(0) = 2.9(-1.1)(+1.0) Mpc (comoving) is detected. Whilst this result is based on only about a quarter of the full survey size, it already shows the immense potential of MUSE for efficiently observing and studying the clustering of Ly alpha emitters. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 653 | a galaxies: high-redshift | |
| 653 | a cosmology: observations | |
| 700 | 1 | a Wisotzki, L.4 aut |
| 700 | 1 | a Schmidt, K. B.4 aut |
| 700 | 1 | a Herenz, Edmund C.u Stockholms universitet,Institutionen för astronomi,Leibniz-Institut für Astrophysik Potsdam (AIP), Germany4 aut0 (Swepub:su)ehere |
| 700 | 1 | a Urrutia, T.4 aut |
| 700 | 1 | a Garel, T.4 aut |
| 700 | 1 | a Kerutt, J.4 aut |
| 700 | 1 | a Saust, R. L.4 aut |
| 700 | 1 | a Bacon, R.4 aut |
| 700 | 1 | a Cantalupo, S.4 aut |
| 700 | 1 | a Contini, T.4 aut |
| 700 | 1 | a Guiderdoni, B.4 aut |
| 700 | 1 | a Marino, R. A.4 aut |
| 700 | 1 | a Richard, J.4 aut |
| 700 | 1 | a Schaye, J.4 aut |
| 700 | 1 | a Soucail, G.4 aut |
| 700 | 1 | a Weilbacher, P. M.4 aut |
| 710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
| 773 | 0 | t Monthly notices of the Royal Astronomical Societyd : Oxford University Press (OUP)g 471:3, s. 3186-3192q 471:3<3186-3192x 0035-8711x 1365-2966 |
| 856 | 4 | u http://arxiv.org/pdf/1707.01109 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-146940 |
| 856 | 4 8 | u https://doi.org/10.1093/mnras/stx1677 |
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