prikaz prve stranice dokumenta Lyα Emitters at Redshift 5.7 in the COSMOS Field
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Scientific paper - Original scientific paper
Lyα Emitters at Redshift 5.7 in the COSMOS Field
Astrophysical Journal Supplement Series, 172 (2007), 1; 523-544. https://doi.org/10.1086/516597
Murayama, T.; Taniguchi, Y.; Scoville, N. Z.; Ajiki, M.; Sanders, D. B.; Mobasher, B.; Aussel, H.; Capak, P.; Koekemoer, A.; Shioya, Y.; Nagao, T.; Carilli, C.; Ellis, R. S.; Garilli, B.; Giavalisco, M.; Kitzbichler, M. G.; Le Fèvre, O.; Maccagni, D.; Schinnerer, E.; Smolčić, Vernesa; Tribiano, S.; Cimatti, A.; Komiyama, Y.; Miyazaki, S.; Sasaki, S. S.; Koda, J.; Karoji, H. More authors...

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Murayama, T., Taniguchi, Y., Scoville, N. Z., Ajiki, M., Sanders, D. B., Mobasher, B. ... Karoji, H. (2007). Lyα Emitters at Redshift 5.7 in the COSMOS Field. Astrophysical Journal Supplement Series, 172. (1), 523-544. doi: 10.1086/516597

Murayama, T., et al. "Lyα Emitters at Redshift 5.7 in the COSMOS Field." Astrophysical Journal Supplement Series, vol. 172, no. 1, 2007, pp. 523-544. https://doi.org/10.1086/516597

Murayama, T., Y. Taniguchi, N. Z. Scoville, M. Ajiki, D. B. Sanders, B. Mobasher, H. Aussel, et al. "Lyα Emitters at Redshift 5.7 in the COSMOS Field." Astrophysical Journal Supplement Series 172, no. 1 (2007): 523-544. https://doi.org/10.1086/516597

Murayama, T., et al. (2007) 'Lyα Emitters at Redshift 5.7 in the COSMOS Field', Astrophysical Journal Supplement Series, 172(1), pp. 523-544. doi: 10.1086/516597

Murayama T, Taniguchi Y, Scoville NZ, Ajiki M, Sanders DB, Mobasher B, and sur.. Lyα Emitters at Redshift 5.7 in the COSMOS Field. Astrophysical Journal Supplement Series [Internet]. 2007 [cited 2024 August 30];172(1):523-544. doi: 10.1086/516597

T. Murayama, et al., "Lyα Emitters at Redshift 5.7 in the COSMOS Field", Astrophysical Journal Supplement Series, vol. 172, no. 1, pp. 523-544, 2007. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:885096. [Accessed: 30 August 2024]

Metadata
Title (english)Lyα Emitters at Redshift 5.7 in the COSMOS Field
AuthorT. Murayama
AuthorY. Taniguchi
AuthorN. Z. Scoville
AuthorM. Ajiki
AuthorD. B. Sanders
AuthorB. Mobasher
AuthorH. Aussel
AuthorP. Capak
AuthorA. Koekemoer
AuthorY. Shioya
AuthorT. Nagao
AuthorC. Carilli
AuthorR. S. Ellis
AuthorB. Garilli
AuthorM. Giavalisco
AuthorM. G. Kitzbichler
AuthorO. Le Fèvre
AuthorD. Maccagni
AuthorE. Schinnerer
AuthorVernesa Smolčić
AuthorS. Tribiano
AuthorA. Cimatti
AuthorY. Komiyama
AuthorS. Miyazaki
AuthorS. S. Sasaki
AuthorJ. Koda
AuthorH. Karoji
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract (english)
We present results from a narrowband optical survey of a contiguous area of 1.95 deg2, covered by the Cosmic Evolution Survey (COSMOS). Both optical narrowband (λc = 8150 Å and Δλ = 120 Å) and broadband (B , V, g', r', i', and z') imaging observations were performed with the Subaru prime-focus camera, Suprime-Cam on the Subaru Telescope. We provide the largest contiguous narrowband survey, targeting Lyα emitters (LAEs) at z ≈ 5.7. We find a total of 119 LAE candidates at z ~ 5.7. Over the wide-area covered by this survey, we find no strong evidence for large-scale clustering of LAEs. We estimate a star formation rate (SFR) density of ~7 × 10-4 M☉ yr-1 Mpc-3 for LAEs at z ≈ 5.7 and compare it with previous measurements.
Keywords (english)
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titleAstrophysical Journal Supplement Series
Numberingvol. 172, no. 1, pp. 523-544
p-ISSN0067-0049
DOIhttps://doi.org/10.1086/516597
URN:NBNurn:nbn:hr:217:885096
Publication2007
Type of resourceText
Access conditionsOpen access
Terms of useLicence In copyright icon
Public note© 2007 American Astronomical Society. Received 2006 September 21; accepted for publication 2007 February 14; published 2007 September. Based on data collected at the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan.
Created on2019-10-16 15:24:46