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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. Više autora...

Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

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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, br. 1, 2007, str. 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, br. 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), str. 523-544. doi: 10.1086/516597

Murayama T, Taniguchi Y, Scoville NZ, Ajiki M, Sanders DB, Mobasher B, i sur.. Lyα Emitters at Redshift 5.7 in the COSMOS Field. Astrophysical Journal Supplement Series [Internet]. 2007. [pristupljeno 24.12.2024.];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, br. 1, str. 523-544, 2007. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:885096. [Citirano: 24.12.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:885096
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Naslov (engleski)Lyα Emitters at Redshift 5.7 in the COSMOS Field
AutorT. Murayama
AutorY. Taniguchi
AutorN. Z. Scoville
AutorM. Ajiki
AutorD. B. Sanders
AutorB. Mobasher
AutorH. Aussel
AutorP. Capak
AutorA. Koekemoer
AutorY. Shioya
AutorT. Nagao
AutorC. Carilli
AutorR. S. Ellis
AutorB. Garilli
AutorM. Giavalisco
AutorM. G. Kitzbichler
AutorO. Le Fèvre
AutorD. Maccagni
AutorE. Schinnerer
AutorVernesa Smolčić
AutorS. Tribiano
AutorA. Cimatti
AutorY. Komiyama
AutorS. Miyazaki
AutorS. S. Sasaki
AutorJ. Koda
AutorH. Karoji
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
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.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaAstrophysical Journal Supplement Series
Brojčani podacivol. 172, br. 1, str. 523-544
p-ISSN0067-0049
DOIhttps://doi.org/10.1086/516597
URN:NBNurn:nbn:hr:217:885096
Datum objave publikacije2007
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© 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.
Datum i vrijeme pohrane2019-10-16 15:24:46