prikaz prve stranice dokumenta Erratum: "Photometric Properties of Lyα Emitters at z ≈ 4.86 in the COSMOS 2 Square Degree Field"
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Erratum: "Photometric Properties of Lyα Emitters at z ≈ 4.86 in the COSMOS 2 Square Degree Field"
Astrophysical Journal, 700 (2009); 899-900. https://doi.org/10.1088/0004-637X/700/1/899
Shioya, Y.; Taniguchi, Y.; Sasaki, S.; Nagao, T.; Murayama, T.; Saito, T.; Ideue, Y.; Nakajima, A.; Matsuoka, K.; Trump, J.; Scoville, N. Z.; Sanders, D. B.; Mobasher, B.; Aussel, H.; Capak, P.; Kartaltepe, J.; Koekemoer, A.; Carilli, C.; Ellis, R. S.; Garilli, B.; Giavalisco, M.; Kitzbichler, M. G.; Impey, C.; LeFevre, O.; Schinnerer, E.; Smolčić, Vernesa Više autora...

Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

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Shioya, Y., Taniguchi, Y., Sasaki, S., Nagao, T., Murayama, T., Saito, T. ... Smolčić, V. (2009). Erratum: "Photometric Properties of Lyα Emitters at z ≈ 4.86 in the COSMOS 2 Square Degree Field". Astrophysical Journal, 700., 899-900. doi: 10.1088/0004-637X/700/1/899

Shioya, Y., et al. "Erratum: "Photometric Properties of Lyα Emitters at z ≈ 4.86 in the COSMOS 2 Square Degree Field"." Astrophysical Journal, vol. 700, 2009, str. 899-900. https://doi.org/10.1088/0004-637X/700/1/899

Shioya, Y., Y. Taniguchi, S. Sasaki, T. Nagao, T. Murayama, T. Saito, Y. Ideue, et al. "Erratum: "Photometric Properties of Lyα Emitters at z ≈ 4.86 in the COSMOS 2 Square Degree Field"." Astrophysical Journal 700 (2009): 899-900. https://doi.org/10.1088/0004-637X/700/1/899

Shioya, Y., et al. (2009) 'Erratum: "Photometric Properties of Lyα Emitters at z ≈ 4.86 in the COSMOS 2 Square Degree Field"', Astrophysical Journal, 700, str. 899-900. doi: 10.1088/0004-637X/700/1/899

Shioya Y, Taniguchi Y, Sasaki S, Nagao T, Murayama T, Saito T, i sur.. Erratum: "Photometric Properties of Lyα Emitters at z ≈ 4.86 in the COSMOS 2 Square Degree Field". Astrophysical Journal [Internet]. 2009. [pristupljeno 25.11.2024.];700:899-900. doi: 10.1088/0004-637X/700/1/899

Y. Shioya, et al., "Erratum: "Photometric Properties of Lyα Emitters at z ≈ 4.86 in the COSMOS 2 Square Degree Field"", Astrophysical Journal, vol. 700, str. 899-900, 2009. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:786492. [Citirano: 25.11.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:786492
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Naslov (engleski)Erratum: "Photometric Properties of Lyα Emitters at z ≈ 4.86 in the COSMOS 2 Square Degree Field"
AutorY. Shioya
AutorY. Taniguchi
AutorS. Sasaki
AutorT. Nagao
AutorT. Murayama
AutorT. Saito
AutorY. Ideue
AutorA. Nakajima
AutorK. Matsuoka
AutorJ. Trump
AutorN. Z. Scoville
AutorD. B. Sanders
AutorB. Mobasher
AutorH. Aussel
AutorP. Capak
AutorJ. Kartaltepe
AutorA. Koekemoer
AutorC. Carilli
AutorR. S. Ellis
AutorB. Garilli
AutorM. Giavalisco
AutorM. G. Kitzbichler
AutorC. Impey
AutorO. LeFevre
AutorE. Schinnerer
AutorVernesa Smolčić
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Astronomija i astrofizika
Sažetak (engleski)
We present results of a survey for Lyα emitters at z ≈ 4.86 based on optical narrowband (λ c = 7126 Å, Δλ = 73 Å) and broadband (B, V, r', i', and z') observations of the Cosmic Evolution Survey field using Suprime-Cam on the Subaru Telescope. We find 79 Lyα emitter (LAE) candidates at z ≈ 4.86 over a contiguous survey area of 1.83 deg2, down to the Lyα line flux of 1.47 × 10–17 erg s-1 cm–2. We obtain the Lyα luminosity function with a best-fit Schechter parameters of log L* = 42.9+0.5 –0.3 erg s-1 and phi* = 1.2+8.0 –1.1 × 10–4 Mpc-3 for α = –1.5 (fixed). The two-point correlation function for our LAE sample is ξ(r) = (r/4.4+5.7 –2.9 Mpc)–1.90±0.22. In order to investigate the field-to-field variations of the properties of Lyα emitters, we divide the survey area into nine tiles of 0fdg5 × 0fdg5 each. We find that the number density varies with a factor of sime2 from field to field with high statistical significance. However, we find no significant field-to-field variance when we divide the field into four tiles with 0fdg7 × 0fdg7 each. We conclude that at least 0.5 deg2 survey area is required to derive averaged properties of LAEs at z ~ 5, and our survey field is wide enough to overcome the cosmic variance.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Ostalo
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaAstrophysical Journal
Brojčani podacivol. 700, str. 899-900
p-ISSN0004-637X
e-ISSN1538-4357
DOIhttps://doi.org/10.1088/0004-637X/700/1/899
URN:NBNurn:nbn:hr:217:786492
Datum objave publikacije2009
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© 2009 American Astronomical Society. Published 2009 July 6.
Datum i vrijeme pohrane2019-10-19 19:28:33