prikaz prve stranice dokumenta 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
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Scientific paper - Original scientific paper
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. More authors...

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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, no. 1, 2007, pp. 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, no. 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), pp. 456-467. doi: 10.1086/518037

Takahashi MI, Shioya Y, Taniguchi Y, Murayama M, Ajiki M, Sasaki SS, and 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 [cited 2024 April 16];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, no. 1, pp. 456-467, 2007. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:507517. [Accessed: 16 April 2024]

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Metadata
Title (english)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
AuthorM. I. Takahashi
AuthorY. Shioya
AuthorY. Taniguchi
AuthorM. Murayama
AuthorM. Ajiki
AuthorS. S. Sasaki
AuthorO. Koizumi
AuthorT. Nagao
AuthorN. Z. Scoville
AuthorB. Mobasher
AuthorH. Aussel
AuthorP. Capak
AuthorC. Carilli
AuthorR. S. Ellis
AuthorB. Garilli
AuthorM. Giavalisco
AuthorL. Guzzo
AuthorG. Hasinger
AuthorC. Impey
AuthorM. G. Kitzbichler
AuthorA. Koekemoer
AuthorO. Le Fèvre
AuthorS. J. Lilly
AuthorD. Maccagni
AuthorA. Renzini
AuthorM. Rich
AuthorD. B. Sanders
AuthorE. Schinnerer
AuthorM. Scodeggio
AuthorP. Shopbell
AuthorVernesa Smolčić
AuthorS. Tribiano
AuthorY. Ideue
AuthorS. Mihara
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract (english)
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).
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. 456-467
p-ISSN0067-0049
e-ISSN1538-4365
DOIhttps://doi.org/10.1086/518037
URN:NBNurn:nbn:hr:217:507517
Publication2007
Type of resourceText
Access conditionsOpen access
Terms of useLicence In copyright icon
Public note© 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.
Created on2019-10-16 15:28:54