The SEDIGISM survey: First Data Release and overview of the Galactic structure Article Swipe
F. Schüller
,
J. S. Urquhart
,
T. Csengeri
,
Dario Colombo
,
A. Duarte-Cabral
,
M. Mattern
,
Adam Ginsburg
,
Alex R. Pettitt
,
F. Wyrowski
,
L. D. Anderson
,
F. Azagra
,
Peter J. Barnes
,
M. T. Beltrán
,
H. Beuther
,
S. J. Billington
,
L. Bronfman
,
R. Cesaroni
,
Clare L. Dobbs
,
David Eden
,
Min-Young Lee
,
S-N. X. Medina
,
K. M. Menten
,
Toby Moore
,
F. M. Montenegro‐Montes
,
S. E. Ragan
,
A. J. Rigby
,
M. Riener
,
D. Russeil
,
E. Schisano
,
Á. Sánchez-Monge
,
A. Traficante
,
A. Zavagno
,
C. Agurto
,
Sylvain Bontemps
,
Ricardo Finger
,
A. Giannetti
,
Elizabeth Johana Gonzalez
,
Audra K. Hernández
,
Thomas Henning
,
J. Kainulainen
,
Jens Kauffmann
,
S. Leurini
,
Sebastián López
,
F. Mac-Auliffe
,
P. Mazumdar
,
S. Molinari
,
F. Motte
,
Erik Muller
,
Q. Nguyễn Lương
,
Rodrigo Parra
,
J-P Perez-Beaupuits
,
P. Schilke
,
N. Schneider
,
S. Suri
,
L. Testi
,
K. Torstensson
,
V. S. Veena
,
Paulina Venegas
,
Ke Wang
,
M. Wienen
·
YOU?
·
· 2020
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/staa2369
YOU?
·
· 2020
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/staa2369
The SEDIGISM (Structure, Excitation and Dynamics of the Inner Galactic Interstellar Medium) survey used the APEX telescope to map 84 deg2 of the Galactic plane between ℓ = −60° and +31° in several molecular transitions, including 13CO (2 – 1) and C18O (2 – 1), thus probing the moderately dense (∼103 cm−3) component of the interstellar medium. With an angular resolution of 30 arcsec and a typical 1σ sensitivity of 0.8–1.0 K at 0.25 km s−1 velocity resolution, it gives access to a wide range of structures, from individual star-forming clumps to giant molecular clouds and complexes. The coverage includes a good fraction of the first and fourth Galactic quadrants, allowing us to constrain the large-scale distribution of cold molecular gas in the inner Galaxy. In this paper, we provide an updated overview of the full survey and the data reduction procedures used. We also assess the quality of these data and describe the data products that are being made publicly available as part of this First Data Release (DR1). We present integrated maps and position–velocity maps of the molecular gas and use these to investigate the correlation between the molecular gas and the large-scale structural features of the Milky Way such as the spiral arms, Galactic bar and Galactic Centre. We find that approximately 60 per cent of the molecular gas is associated with the spiral arms and these appear as strong intensity peaks in the derived Galactocentric distribution. We also find strong peaks in intensity at specific longitudes that correspond to the Galactic Centre and well-known star-forming complexes, revealing that the 13CO emission is concentrated in a small number of complexes rather than evenly distributed along spiral arms.
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- Type
- article
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- en
- Landing Page
- https://doi.org/10.1093/mnras/staa2369
- https://academic.oup.com/mnras/article-pdf/500/3/3064/34659742/staa2369.pdf
- OA Status
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- Cited By
- 87
- References
- 136
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W3049114668
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Raw OpenAlex JSON
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https://openalex.org/W3049114668Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1093/mnras/staa2369Digital Object Identifier
- Title
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The SEDIGISM survey: First Data Release and overview of the Galactic structureWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2020Year of publication
- Publication date
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2020-08-14Full publication date if available
- Authors
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F. Schüller, J. S. Urquhart, T. Csengeri, Dario Colombo, A. Duarte-Cabral, M. Mattern, Adam Ginsburg, Alex R. Pettitt, F. Wyrowski, L. D. Anderson, F. Azagra, Peter J. Barnes, M. T. Beltrán, H. Beuther, S. J. Billington, L. Bronfman, R. Cesaroni, Clare L. Dobbs, David Eden, Min-Young Lee, S-N. X. Medina, K. M. Menten, Toby Moore, F. M. Montenegro‐Montes, S. E. Ragan, A. J. Rigby, M. Riener, D. Russeil, E. Schisano, Á. Sánchez-Monge, A. Traficante, A. Zavagno, C. Agurto, Sylvain Bontemps, Ricardo Finger, A. Giannetti, Elizabeth Johana Gonzalez, Audra K. Hernández, Thomas Henning, J. Kainulainen, Jens Kauffmann, S. Leurini, Sebastián López, F. Mac-Auliffe, P. Mazumdar, S. Molinari, F. Motte, Erik Muller, Q. Nguyễn Lương, Rodrigo Parra, J-P Perez-Beaupuits, P. Schilke, N. Schneider, S. Suri, L. Testi, K. Torstensson, V. S. Veena, Paulina Venegas, Ke Wang, M. WienenList of authors in order
- Landing page
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https://doi.org/10.1093/mnras/staa2369Publisher landing page
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https://academic.oup.com/mnras/article-pdf/500/3/3064/34659742/staa2369.pdfDirect link to full text PDF
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YesWhether a free full text is available
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hybridOpen access status per OpenAlex
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https://academic.oup.com/mnras/article-pdf/500/3/3064/34659742/staa2369.pdfDirect OA link when available
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Physics, Astrophysics, Galactic plane, Molecular cloud, Milky Way, Spiral galaxy, Galaxy, Star formation, Interstellar medium, Astronomy, Galactic Center, StarsTop concepts (fields/topics) attached by OpenAlex
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87Total citation count in OpenAlex
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2025: 14, 2024: 20, 2023: 17, 2022: 22, 2021: 11Per-year citation counts (last 5 years)
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136Number of works referenced by this work
- Related works (count)
-
10Other works algorithmically related by OpenAlex
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