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The [O II] λ3727 Luminosity Function and Star Formation Rate at z ≈ 1.2 in the COSMOS 2 Square Degree Field and the Subaru Deep Field
Astrophysical Journal Supplement Series, 172 (2007), 1; 456-467. https://doi.org/10.1086/518037
Takahashi, M. I.; Shioya, Y.; Taniguchi, Y.; Murayama, M.; Ajiki, M.; Sasaki, S. S.; Koizumi, O.; Nagao, T.; Scoville, N. Z.; Mobasher, B.; Aussel, H.; Capak, P.; Carilli, C.; Ellis, R. S.; Garilli, B.; Giavalisco, M.; Guzzo, L.; Hasinger, G.; Impey, C.; Kitzbichler, M. G.; Koekemoer, A.; Le Fèvre, O.; Lilly, S. J.; Maccagni, D.; Renzini, A.; Rich, M.; Sanders, D. B.; Schinnerer, E.; Scodeggio, M.; Shopbell, P.; Smolčić, Vernesa; Tribiano, S.; Ideue, Y.; Mihara, S. Više autora...

Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

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Takahashi, M. I., Shioya, Y., Taniguchi, Y., Murayama, M., Ajiki, M., Sasaki, S. S. ... Mihara, S. (2007). The [O II] λ3727 Luminosity Function and Star Formation Rate at z ≈ 1.2 in the COSMOS 2 Square Degree Field and the Subaru Deep Field. Astrophysical Journal Supplement Series, 172. (1), 456-467. doi: 10.1086/518037

Takahashi, M. I., et al. "The [O II] λ3727 Luminosity Function and Star Formation Rate at z ≈ 1.2 in the COSMOS 2 Square Degree Field and the Subaru Deep Field." Astrophysical Journal Supplement Series, vol. 172, br. 1, 2007, str. 456-467. https://doi.org/10.1086/518037

Takahashi, M. I., Y. Shioya, Y. Taniguchi, M. Murayama, M. Ajiki, S. S. Sasaki, O. Koizumi, et al. "The [O II] λ3727 Luminosity Function and Star Formation Rate at z ≈ 1.2 in the COSMOS 2 Square Degree Field and the Subaru Deep Field." Astrophysical Journal Supplement Series 172, br. 1 (2007): 456-467. https://doi.org/10.1086/518037

Takahashi, M. I., et al. (2007) 'The [O II] λ3727 Luminosity Function and Star Formation Rate at z ≈ 1.2 in the COSMOS 2 Square Degree Field and the Subaru Deep Field', Astrophysical Journal Supplement Series, 172(1), str. 456-467. doi: 10.1086/518037

Takahashi MI, Shioya Y, Taniguchi Y, Murayama M, Ajiki M, Sasaki SS, i sur.. The [O II] λ3727 Luminosity Function and Star Formation Rate at z ≈ 1.2 in the COSMOS 2 Square Degree Field and the Subaru Deep Field. Astrophysical Journal Supplement Series [Internet]. 2007. [pristupljeno 25.11.2024.];172(1):456-467. doi: 10.1086/518037

M. I. Takahashi, et al., "The [O II] λ3727 Luminosity Function and Star Formation Rate at z ≈ 1.2 in the COSMOS 2 Square Degree Field and the Subaru Deep Field", Astrophysical Journal Supplement Series, vol. 172, br. 1, str. 456-467, 2007. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:507517. [Citirano: 25.11.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:507517
Podaci o radu
Naslov (engleski)The [O II] λ3727 Luminosity Function and Star Formation Rate at z ≈ 1.2 in the COSMOS 2 Square Degree Field and the Subaru Deep Field
AutorM. I. Takahashi
AutorY. Shioya
AutorY. Taniguchi
AutorM. Murayama
AutorM. Ajiki
AutorS. S. Sasaki
AutorO. Koizumi
AutorT. Nagao
AutorN. Z. Scoville
AutorB. Mobasher
AutorH. Aussel
AutorP. Capak
AutorC. Carilli
AutorR. S. Ellis
AutorB. Garilli
AutorM. Giavalisco
AutorL. Guzzo
AutorG. Hasinger
AutorC. Impey
AutorM. G. Kitzbichler
AutorA. Koekemoer
AutorO. Le Fèvre
AutorS. J. Lilly
AutorD. Maccagni
AutorA. Renzini
AutorM. Rich
AutorD. B. Sanders
AutorE. Schinnerer
AutorM. Scodeggio
AutorP. Shopbell
AutorVernesa Smolčić
AutorS. Tribiano
AutorY. Ideue
AutorS. Mihara
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
We have carried out a wide-field imaging survey for [O II] λ3727 emitting galaxies at z ≈ 1.2 in the HST COSMOS 2 square degree field using the Suprime-Cam on the Subaru Telescope. The survey covers a sky area of 6700 arcmin 2 in the COSMOS field, and a redshift range between 1.17 and 1.20 (Δz = 0.03), corresponding to a survey volume of 5.56 × 105 Mpc3. We obtain a sample of 3176 [O II] emitting galaxies with observed emission-line equivalent widths greater than 26 Å. Since our survey tends to sample brighter [O II] emitting galaxies, we also analyze a sample of fainter [O II] emitting galaxies found in the Subaru Deep Field (SDF).
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. 456-467
p-ISSN0067-0049
e-ISSN1538-4365
DOIhttps://doi.org/10.1086/518037
URN:NBNurn:nbn:hr:217:507517
Datum objave publikacije2007
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© 2007 American Astronomical Society. Received 2006 September 15; accepted for publication 2007 March 3; published September 2007. Based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan.
Datum i vrijeme pohrane2019-10-16 15:28:54