id:"swepub:oai:DiVA.org:su-211069"
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 04478naa a2200541 4500 | |
| 001 | oai:DiVA.org:su-211069 | |
| 003 | SwePub | |
| 008 | 221110s2022 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-2110692 URI |
| 024 | 7 | a https://doi.org/10.3847/1538-3881/ac93112 DOI |
| 040 | a (SwePub)su | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Sirressi, Mattiau Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)masi1109 |
| 245 | 1 0 | a CLusters in the UV as EngineS (CLUES). I. Survey Presentation and FUV Spectral Analysis of the Stellar Light |
| 264 | c 2022-10-21 | |
| 264 | 1 | b American Astronomical Society,c 2022 |
| 338 | a print2 rdacarrier | |
| 520 | a The CLusters in the Uv as EngineS (CLUES) survey is a Cosmic Origins Spectrograph (COS) campaign aimed at acquiring the 1130–1770 Å rest-frame spectroscopy of very young (<20 Myr) and massive (>104 M⊙) star clusters in galaxies that are part of the Hubble treasury program Legacy ExtraGalactic UV Survey. In this first paper of a series, we describe the CLUES sample consisting of 20 young star clusters and report their physical properties as derived by both multiwavelength photometry and far-UV (FUV) spectroscopy with Hubble Space Telescope. Thanks to the synergy of the two different data sets, we build a coherent picture of the diverse stellar populations found in each region (with sizes of 40–160 pc). We associate the FUV-brightest stellar population to the central targeted star cluster and the other modeled population to the diffuse stars that are included in the COS aperture. We observe better agreement between photometric and spectroscopic ages for star clusters younger than 5 Myr. For clusters older than 5 Myr, photometry and spectroscopy measurements deviate, with the latter producing older ages, due to the degeneracy of photometric models. FUV spectroscopy enables us to better constrain the stellar metallicities, a parameter that optical colors are insensitive to. Finally, the derived E(B − V) are quite similar, with a tendency for FUV spectroscopy to favor solutions with higher extinctions. The recovered masses are in agreement within a factor of 2 for all of the clusters. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 700 | 1 | a Adamo, Angela,d 1981-u Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)anad2127 |
| 700 | 1 | a Hayes, Matthewu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)mhaye |
| 700 | 1 | a Osborne, Shannon4 aut |
| 700 | 1 | a Hernandez, Svea4 aut |
| 700 | 1 | a Chisholm, John4 aut |
| 700 | 1 | a Messa, Matteo,d 1988-u Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC),Université de Genève, Switzerland4 aut0 (Swepub:su)mame4466 |
| 700 | 1 | a Smith, Linda J.4 aut |
| 700 | 1 | a Aloisi, Alessandra4 aut |
| 700 | 1 | a Wofford, Aida4 aut |
| 700 | 1 | a Fox, Andrew J.4 aut |
| 700 | 1 | a Mizener, Andrew4 aut |
| 700 | 1 | a Usher, Christopheru Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)chus3594 |
| 700 | 1 | a Bik, Arjanu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)abik |
| 700 | 1 | a Calzetti, Daniela4 aut |
| 700 | 1 | a Sabbi, Elena4 aut |
| 700 | 1 | a Schinnerer, Eva4 aut |
| 700 | 1 | a Östlin, Göranu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)ostlin |
| 700 | 1 | a Grasha, Kathryn4 aut |
| 700 | 1 | a Cignoni, Michele4 aut |
| 700 | 1 | a Fumagalli, Michele4 aut |
| 710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
| 773 | 0 | t Astronomical Journald : American Astronomical Societyg 164:5q 164:5x 0004-6256x 1538-3881 |
| 856 | 4 | u https://doi.org/10.3847/1538-3881/ac9311y Fulltext |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-211069 |
| 856 | 4 8 | u https://doi.org/10.3847/1538-3881/ac9311 |
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