Journal article
Predicting the observability of population III stars with ELT-HARMONI via the helium 1640 Å emission line
- Abstract:
-
Population III (Pop. III) stars, as of yet, have not been detected, however as we move into the era of extremely large telescopes this is likely to change. One likely tracer for Pop. III stars is the He IIλ1640 emission line, which will be detectable by the HARMONI spectrograph on the European Extremely Large Telescope (ELT) over a broad range of redshifts (2 ≤ z ≤ 14). By post-processing galaxies from the cosmological, AMR-hydrodynamical simulation NEWHORIZON with theoretical spectral energy...
Expand abstract
- Publication status:
- Published
- Peer review status:
- Peer reviewed
Actions
Access Document
- Files:
-
-
(Preview, Accepted manuscript, 1.9MB, Terms of use)
-
- Publisher copy:
- 10.1093/mnras/stab013
Authors
Bibliographic Details
- Publisher:
- Oxford University Press
- Journal:
- Monthly Notices of the Royal Astronomical Society More from this journal
- Volume:
- 501
- Issue:
- 4
- Pages:
- 5517-5537
- Publication date:
- 2021-01-08
- Acceptance date:
- 2020-11-30
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
Item Description
- Language:
-
English
- Keywords:
- Pubs id:
-
1156543
- Local pid:
-
pubs:1156543
- Deposit date:
-
2021-02-22
Terms of use
- Copyright holder:
- Grisdale et al.
- Copyright date:
- 2021
- Rights statement:
- © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society
- Notes:
- This is the accepted manuscript version of the article. The final version is available from Oxford University Press at: https://doi.org/10.1093/mnras/stab013
Metrics
If you are the owner of this record, you can report an update to it here: Report update to this record