prikaz prve stranice dokumenta Quest for COSMOS Submillimeter Galaxy Counterparts using CARMA and VLA: Identifying Three High-redshift Starburst Galaxies
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Quest for COSMOS Submillimeter Galaxy Counterparts using CARMA and VLA: Identifying Three High-redshift Starburst Galaxies
Astrophysical Journal Supplement Series, 200 (2012), 1; 10-21. https://doi.org/10.1088/0067-0049/200/1/10
Smolčić, Vernesa; Navarrete, F.; Aravena, M.; Ilbert, O.; Yun, M. S.; Sheth, K.; Salvato, M.; McCracken, H. J.; Diener, C.; Aretxaga, I.; Riechers, D. A.; Finoguenov, A.; Bertoldi, F.; Capak, P.; Hughes, D.; Karim, A.; Schinnerer, E.; Scoville, N. Z.; Wilson, G. Više autora...

Institucijski repozitorij: Repozitorij Prirodoslovno-matematičkog fakulteta

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Smolčić, V., Navarrete, F., Aravena, M., Ilbert, O., Yun, M. S., Sheth, K. ... Wilson, G. (2012). Quest for COSMOS Submillimeter Galaxy Counterparts using CARMA and VLA: Identifying Three High-redshift Starburst Galaxies. Astrophysical Journal Supplement Series, 200. (1), 10-21. doi: 10.1088/0067-0049/200/1/10

Smolčić, Vernesa, et al. "Quest for COSMOS Submillimeter Galaxy Counterparts using CARMA and VLA: Identifying Three High-redshift Starburst Galaxies." Astrophysical Journal Supplement Series, vol. 200, br. 1, 2012, str. 10-21. https://doi.org/10.1088/0067-0049/200/1/10

Smolčić, Vernesa, F. Navarrete, M. Aravena, O. Ilbert, M. S. Yun, K. Sheth, M. Salvato, et al. "Quest for COSMOS Submillimeter Galaxy Counterparts using CARMA and VLA: Identifying Three High-redshift Starburst Galaxies." Astrophysical Journal Supplement Series 200, br. 1 (2012): 10-21. https://doi.org/10.1088/0067-0049/200/1/10

Smolčić, V., et al. (2012) 'Quest for COSMOS Submillimeter Galaxy Counterparts using CARMA and VLA: Identifying Three High-redshift Starburst Galaxies', Astrophysical Journal Supplement Series, 200(1), str. 10-21. doi: 10.1088/0067-0049/200/1/10

Smolčić V, Navarrete F, Aravena M, Ilbert O, Yun MS, Sheth K, i sur.. Quest for COSMOS Submillimeter Galaxy Counterparts using CARMA and VLA: Identifying Three High-redshift Starburst Galaxies. Astrophysical Journal Supplement Series [Internet]. 2012. [pristupljeno 22.11.2024.];200(1):10-21. doi: 10.1088/0067-0049/200/1/10

V. Smolčić, et al., "Quest for COSMOS Submillimeter Galaxy Counterparts using CARMA and VLA: Identifying Three High-redshift Starburst Galaxies", Astrophysical Journal Supplement Series, vol. 200, br. 1, str. 10-21, 2012. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:310093. [Citirano: 22.11.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:310093
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Naslov (engleski)Quest for COSMOS Submillimeter Galaxy Counterparts using CARMA and VLA: Identifying Three High-redshift Starburst Galaxies
AutorVernesa Smolčić
AutorF. Navarrete
AutorM. Aravena
AutorO. Ilbert
AutorM. S. Yun
AutorK. Sheth
AutorM. Salvato
AutorH. J. McCracken
AutorC. Diener
AutorI. Aretxaga
AutorD. A. Riechers
AutorA. Finoguenov
AutorF. Bertoldi
AutorP. Capak
AutorD. Hughes
AutorA. Karim
AutorE. Schinnerer
AutorN. Z. Scoville
AutorG. Wilson
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
We report on interferometric observations at 1.3 mm at 2"-3" resolution using the Combined Array for Research in Millimeter-wave Astronomy. We identify multi-wavelength counterparts of three submillimeter galaxies (SMGs; F_(1mm) > 5.5 mJy) in the COSMOS field, initially detected with MAMBO and AzTEC bolometers at low, ~10"-30", resolution. All three sources—AzTEC/C1, Cosbo-3, and Cosbo-8—are identified to coincide with positions of 20 cm radio sources. Cosbo-3, however, is not associated with the most likely radio counterpart, closest to the MAMBO source position, but with that farther away from it. This illustrates the need for intermediate-resolution (~2") mm-observations to identify the correct counterparts of single-dish-detected SMGs. All of our three sources become prominent only at NIR wavelengths, and their mm-to-radio flux based redshifts suggest that they lie at redshifts z ≳ 2. As a proof of concept, we show that photometric redshifts can be well determined for SMGs, and we find photometric redshifts of 5.6 ± 1.2, 1.9^(+0.9)_(–0.5), and ~4 for AzTEC/C1, Cosbo-3, and Cosbo-8, respectively. Using these we infer that these galaxies have radio-based star formation rates of ≳ 1000 M_☉ yr^(–1) and IR luminosities of ~10^(13) L_☉ consistent with properties of high-redshift SMGs. In summary, our sources reflect a variety of SMG properties in terms of redshift and clustering, consistent with the framework that SMGs are progenitors of z ~ 2 and today's passive galaxies.
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. 200, br. 1, str. 10-21
p-ISSN0067-0049
DOIhttps://doi.org/10.1088/0067-0049/200/1/10
URN:NBNurn:nbn:hr:217:310093
Datum objave publikacije2012
URL dokumentahttps://iopscience.iop.org/article/10.1088/0067-0049/200/1/10
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© 2012 American Astronomical Society. Received 2011 May 10; accepted 2012 March 21; published 2012 May 4.
Datum i vrijeme pohrane2019-11-15 19:24:15