Search: onr:"swepub:oai:DiVA.org:su-168579" >
Emission-line Metal...
Emission-line Metallicities from the Faint Infrared Grism Survey and VLT/MUSE
- Article/chapterEnglish2019
Publisher, publication year, extent ...
-
2019-03-29
-
American Astronomical Society,2019
-
printrdacarrier
Numbers
-
LIBRIS-ID:oai:DiVA.org:su-168579
-
https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-168579URI
-
https://doi.org/10.3847/1538-4357/ab08ecDOI
Supplementary language notes
-
Language:English
-
Summary in:English
Part of subdatabase
Classification
-
Subject category:ref swepub-contenttype
-
Subject category:art swepub-publicationtype
Notes
-
We derive direct-measurement gas-phase metallicities of 7.4 < 12 + log (O/H) < 8.4 for 14 low-mass emissionline galaxies at 0.3 < z < 0.8 identified in the Faint Infrared Grism Survey. We use deep slitless G102 grism spectroscopy of the Hubble Ultra Deep Field, dispersing light from all objects in the field at wavelengths between 0.85 and 1.15 mu m. We run an automatic search routine on these spectra to robustly identify 71 emission-line sources, using archival data from Very Large Telescope (VLT)/Multi-Unit Spectroscopic Explorer (MUSE) to measure additional lines and confirm redshifts. We identify 14 objects with 0.3 < z < 0.8 with measurable [O Iota Iota Iota] lambda 4363 angstrom emission lines in matching VLT/MUSE spectra. For these galaxies, we derive direct electron-temperature gas-phase metallicities with a range of 7.4 < 12 + log (O/H) < 8.4. With matching stellar masses in the range of 10(7.9) M-circle dot < M* < 10(10.4) M-circle dot, we construct a mass-metallicity (MZ) relation and find that the relation is offset to lower metallicities compared to metallicities derived from alternative methods (e.g., R-23,O3N2, N2O2) and continuum selected samples. Using star formation rates derived from the H alpha emission line, we calculate our galaxies' position on the Fundamental Metallicity Relation, where we also find an offset toward lower metallicities. This demonstrates that this emission-line-selected sample probes objects of low stellar masses but even lower metallicities than many comparable surveys. We detect a trend suggesting galaxies with higher Specific Star Formation (SSFR) are more likely to have lower metallicity. This could be due to cold accretion of metal-poor gas that drives star formation, or could be because outflows of metal-rich stellar winds and SNe ejecta are more common in galaxies with higher SSFR.
Subject headings and genre
Added entries (persons, corporate bodies, meetings, titles ...)
-
Malhotra, Sangeeta
(author)
-
Rhoads, James
(author)
-
Christensen, Lise
(author)
-
Finkelstein, Steven L.
(author)
-
Grogin, Norman
(author)
-
Harish, Santosh
(author)
-
Jiang, Tianxing
(author)
-
Kim, Keunho
(author)
-
Koekemoer, Anton
(author)
-
Pirzkal, Norbert
(author)
-
Smith, Mark
(author)
-
Yang, Huan
(author)
-
Cimatti, Andrea
(author)
-
Ferreras, Ignacio
(author)
-
Hathi, Nimish
(author)
-
Hibon, Pascale
(author)
-
Meurer, Gerhardt
(author)
-
Östlin, GöranStockholms universitet,Institutionen för astronomi(Swepub:su)ostlin
(author)
-
Pasquali, Anna
(author)
-
Ryan, Russell
(author)
-
Straughn, Amber
(author)
-
Windhorst, Rogier
(author)
-
Stockholms universitetInstitutionen för astronomi
(creator_code:org_t)
Related titles
-
In:Astrophysical Journal: American Astronomical Society874:20004-637X1538-4357
Internet link
Find in a library
To the university's database
- By the author/editor
-
Pharo, John
-
Malhotra, Sangee ...
-
Rhoads, James
-
Christensen, Lis ...
-
Finkelstein, Ste ...
-
Grogin, Norman
-
show more...
-
Harish, Santosh
-
Jiang, Tianxing
-
Kim, Keunho
-
Koekemoer, Anton
-
Pirzkal, Norbert
-
Smith, Mark
-
Yang, Huan
-
Cimatti, Andrea
-
Ferreras, Ignaci ...
-
Hathi, Nimish
-
Hibon, Pascale
-
Meurer, Gerhardt
-
Östlin, Göran
-
Pasquali, Anna
-
Ryan, Russell
-
Straughn, Amber
-
Windhorst, Rogie ...
-
show less...
- About the subject
-
- NATURAL SCIENCES
-
NATURAL SCIENCES
-
and Physical Science ...
-
and Astronomy Astrop ...
- Articles in the publication
-
Astrophysical Jo ...
- By the university
-
Stockholm University