izpis_h1_title_alt

The GALAH survey : new diffuse interstellar bands found in residuals of 872 000 stellar spectra
ID Vogrinčič, Rok (Author), ID Kos, Janez (Author), ID Zwitter, Tomaž (Author), ID Traven, Gregor (Author), ID Beeson, Kevin Luke (Author), ID Čotar, Klemen (Author), et al.

.pdfPDF - Presentation file, Download (12,84 MB)
MD5: F4DF3D3FAD4B6559564A20458D9B9511
URLURL - Source URL, Visit https://academic.oup.com/mnras/article/521/3/3727/7085973 This link opens in a new window

Abstract
We use more than 872 000 mid- to high-resolution (R ∼ 20 000) spectra of stars from the GALactic Archaeology with HERMES (GALAH) survey to discern the spectra of diffuse interstellar bands (DIBs). We use four windows with the wavelength ranges 4718–4903, 5649–5873, 6481–6739, and 7590–7890 Å, giving a total coverage of 967 Å. We produce ∼400 000 spectra of interstellar medium (ISM) absorption features and correct them for radial velocities of the DIB clouds. Ultimately, we combine the 33 115 best ISM spectra into six reddening bins with a range of 0.1 < E(B − V) < 0.7 mag. A total of 183 absorption features in these spectra qualify as DIBs, and their fitted model parameters are summarized in a detailed catalogue. From these, 64 are not reported in the literature, of which 17 are certain, 14 are probable and 33 are possible. We find that the broad DIBs can be fitted with a multitude of narrower DIBs. Finally, we create a synthetic DIB spectrum at unit reddening. This should allow us to narrow down the possible carriers of DIBs, to explore the composition of the ISM, and ultimately to model dust and star formation better as well as to correct Galactic and extragalactic observations. The majority of certain DIBs show a significant excess of equivalent width when compared with reddening. We explain this with observed lines of sight penetrating more uniform DIB clouds compared with clumpy dust clouds.

Language:English
Keywords:catalogues, spectroscopic surveys, methods, data analysis, surveys, dust, extinction
Work type:Article
Typology:1.01 - Original Scientific Article
Organization:FMF - Faculty of Mathematics and Physics
Publication status:Published
Publication version:Version of Record
Year:2023
Number of pages:Str. 3727-3748
Numbering:Vol. 521, iss. 3
PID:20.500.12556/RUL-147271 This link opens in a new window
UDC:524.3
ISSN on article:1365-2966
DOI:10.1093/mnras/stad678 This link opens in a new window
COBISS.SI-ID:152621827 This link opens in a new window
Publication date in RUL:28.06.2023
Views:390
Downloads:26
Metadata:XML RDF-CHPDL DC-XML DC-RDF
:
Copy citation
Share:Bookmark and Share

Record is a part of a journal

Title:Monthly notices of the Royal Astronomical Society
Shortened title:Mon. not. R. Astron. Soc.
Publisher:Blackwell Science
ISSN:1365-2966
COBISS.SI-ID:1870180 This link opens in a new window

Licences

License:CC BY 4.0, Creative Commons Attribution 4.0 International
Link:http://creativecommons.org/licenses/by/4.0/
Description:This is the standard Creative Commons license that gives others maximum freedom to do what they want with the work as long as they credit the author.

Projects

Funder:ARRS - Slovenian Research Agency
Project number:P1-0188
Name:Astrofizika in fizika atmosfere

Funder:ARC - Australian Research Council
Project number:CE170100013
Name:Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions
Acronym:ASTRO 3D

Funder:ARC - Australian Research Council
Funding programme:Discovery Projects
Project number:DP180101791

Funder:Other - Other funder or multiple funders
Funding programme:UNSW, Scientia Fellowship

Similar documents

Similar works from RUL:
Similar works from other Slovenian collections:

Back