Published October 20, 2020 | Version v1

Data for the paper 'WISDOM Project - VI. Exploring the relation between supermassive black hole mass and galaxy rotation with molecular gas '

Authors/Creators

  • 1. Sub-department of Astrophysics, Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH, UK

Description

This upload includes the data underlying the MNRAS paper Smith et al. (2020) entitled 'WISDOM Project - VI. Exploring the relation between supermassive black hole mass and galaxy rotation with molecular gas' (arXiv:2010.08565). The full author list is available from the paper, and we request that this paper is cited if this data is used in future publications.

The upload includes machine-readable versions (csv) of Tables 3, 4, A1 and A2 of the paper. The upload also includes the calibrated spectra from the two observing programmes (191-18 at the IRAM 30m telescope and 2018-04a at the OSO 20m telescope), and the homogenised spectra used in the project. Full descriptions are given in the paper. 

Table 3: CubeData.csv; The table contains the determined line widths, inclinations, and SMBH masses used for the resolved sample of this project. The references from which the cubes were obtained, are listed in Table 3 of the paper.

UnresolvedData.csv: Table 4; The table contains the determined line widths, inclinations, and SMBH masses used for the unresolved sample of this project. The references from which the spectra were obtained, are listed in Table 4 of the paper.

IRAMData.csv: Table A1; The table contains a list of galaxies observed using the IRAM 30m telescope as part of project 191-18. For each galaxy the rms noise is listed, and for detected galaxies the spectrally-integrated line intensity measured over the specified velocity range given. The inferred molecular gas mass is also listed. 

OSO20mData.csv: Table A2; The table contains a list of galaxies observed using the OSO 20m telescope as part of project 2018-04a. For each galaxy the rms noise is listed, and for detected galaxies the spectrally-integrated line intensity measured over the specified velocity range given. The inferred molecular gas mass is also listed. 

IRAM30m_191-18.tar: Calibrated spectra from programme 191-18.

OSO2018-04a.tar: Calibrated spectra from programme 2018-04a.

ResolvedSample.tar: Homogenised spectra for the spatially-resolved sample. Note that some spectra were sourced from other works, the original references are given in the fits headers.

UnresolvedSample.tar: Homogenised spectra for the spatially-unresolved sample. Note that some spectra were sourced from other works, the original references are given in the fits headers.

Files

CubeData.csv

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Additional details

Related works

Is documented by
Journal article: arXiv:2010.08565 (arXiv)

Funding

European Commission
RadioNet - Advanced Radio Astronomy in Europe 730562

References

  • Smith, Mark D. et al. (2020) WISDOM project - VI. Exploring the relation between supermassive black hole mass and galaxy rotation with molecular gas