| Author dc.contributor.author | Suleiman, Nofoz | |
| Author dc.contributor.author | Toba, Yoshiki | |
| Author dc.contributor.author | Frey, Sándor | |
| Author dc.contributor.author | Tóth, L. Viktor | |
| Availability Date dc.date.accessioned | 2024-04-12T12:11:53Z | |
| Availability Date dc.date.available | 2024-04-12T12:11:53Z | |
| Release dc.date.issued | 2023 | |
| uri dc.identifier.uri | http://hdl.handle.net/10831/107812 | |
| Abstract dc.description.abstract | This work aims to represent the physical properties of a sample of infrared-bright dust-obscured galaxies (DOGs) studied by Suleiman et al. (2022) by fitting the spectral energy distributions (SEDs). Twenty-eight DOGs were examined at redshifts 0.47 ≤ z ≤ 1.63 discovered by combining images of the Subaru Hyper Suprime-Cam (HSC) survey, VISTA Kilo-degree Infrared Galaxy (VIKING) survey, and the Wide-field Infrared Survey Explorer ( WISE ) all-sky survey, and detected at Herschel Spectral and Photometric Imaging Receiver (SPIRE) bands. The results show a correlation between the star formation rate (SFR) and the dust luminosity of Suleiman et al. (2022) DOG sample, the SFR ranges of the sample according to different redshifts, and a comparison between Suleiman et al. (2022) sample and other samples of DOGs. | |
| Language dc.language | Angol | |
|
dc.rights | Nevezd meg! CC-BY | |
|
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | |
| Title dc.title | The physical properties of IR-bright Dust-Obscured Galaxies | |
| Type dc.type | folyóiratcikk | |
| Date Change dc.date.updated | 2024-04-12T12:05:32Z | |
| Scope dc.format.page | 67-69 | |
| Doi ID dc.identifier.doi | https://doi.org/10.1017/S1743921322003726 | |
| MTMT ID dc.identifier.mtmt | 34007520 | |
| Issue Number dc.identifier.issue | S373 | |
| abbreviated journal dc.identifier.jabbrev | PROC IAU | |
| Journal dc.identifier.jtitle | PROCEEDINGS OF THE INTERNATIONAL ASTRONOMICAL UNION | |
| Volume Number dc.identifier.volume | 17 | |
| Release Date dc.description.issuedate | 2023 | |
| department of Author dc.contributor.institution | Konkoly Thege Miklós Csillagászati Intézet | |
| department of Author dc.contributor.institution | Fizikai és Csillagászati Intézet | |
| Author institution dc.contributor.department | Konkoly Thege Miklós Csillagászati Intézet |
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Except where otherwise noted, this item's license is described as Nevezd meg! CC-BY