When using GALAH DR4 data, please acknowledge the work of the people involved and provide credits and necessary citations.
- GALAH Survey papers to cite
- The GALAH DR4 overview
- The motivation and planned execution of the GALAH survey, and first-light performance of HERMES
- The HERMES description paper
- Descriptions of the data reduction
- For stars from TESS-HERMES survey (
survey_name == tess_hermes) - For stars from K2-HERMES survey (
survey_name == k2_hermes)
- Acknowledgement
GALAH Survey papers to cite
If you have used public GALAH data in your paper, please cite the following papers describing the instruments, survey, and data analysis as appropriate:
The GALAH DR4 overview
- The GALAH Survey: Data Release 4
Buder et al. (2024) (https://arxiv.org/abs/2409.19858v1
The motivation and planned execution of the GALAH survey, and first-light performance of HERMES
- The GALAH survey: scientific motivation
De Silva et al. (2015) MNRAS 449 2604 (doi:10.1093/mnras/stv327, arXiv:1502.04767)
The HERMES description paper
- First light results from the High Efficiency and Resolution Multi-Element Spectrograph at the Anglo-Australian Telescope
Sheinis et al. (2015) JATIS 1 035002 (doi:10.1117/1.JATIS.1.3.035002)
Descriptions of the data reduction
- The GALAH survey: the data reduction pipeline
Kos et al. (2017) MNRAS 464 1259 (doi:10.1093/mnras/stw2064, arXiv:1608.04391) - The GALAH+ survey: a new library of observed stellar spectra improves radial velocities and hints at motions within M67
Zwitter et al. (2021) MNRAS 508 4202 (doi:10.1093/mnras/stab2673, arXiv:2012.12201)
For stars from TESS-HERMES survey (survey_name == tess_hermes)
- The TESS-HERMES survey data release 1: high-resolution spectroscopy of the TESS southern continuous viewing zone
Sharma et al. (2018) MNRAS 473 2004 (doi:10.1093/mnras/stx2582, arXiv:1707.05753)
For stars from K2-HERMES survey (survey_name == k2_hermes)
- The K2-HERMES Survey: age and metallicity of the thick disc
Sharma et al. (2019) MNRAS 490 5335 (doi:10.1093/mnras/stz2861, arXiv:1904.12444)small>
Acknowledgement
We also ask that you include the following acknowledgement in your works:
This work made use of the Fourth Data Release of the GALAH Survey (Buder et al. 2021). The GALAH Survey is based on data acquired through the Australian Astronomical Observatory, under programs: A/2013B/13 (The GALAH pilot survey); A/2014A/25, A/2015A/19, A2017A/18 (The GALAH survey phase 1); A2018A/18 (Open clusters with HERMES); A2019A/1 (Hierarchical star formation in Ori OB1); A2019A/15, A/2020B/23, R/2022B/5, R/2023A/4, R2023B/5 (The GALAH survey phase 2); A/2015B/19, A/2016A/22, A/2016B/10, A/2017B/16, A/2018B/15 (The HERMES-TESS program); A/2015A/3, A/2015B/1, A/2015B/19, A/2016A/22, A/2016B/12, A/2017A/14, A/2020B/14 (The HERMES K2-follow-up program); R/2022B/02 and A/2023A/09 (Combining asteroseismology and spectroscopy in K2); A/2023A/8 (Resolving the chemical fingerprints of Milky Way mergers); and A/2023B/4 (s-process variations in southern globular clusters). We acknowledge the traditional owners of the land on which the AAT stands, the Gamilaraay people, and pay our respects to elders past and present. This paper includes data that has been provided by AAO Data Central (datacentral.org.au).
Gaia Acknowledgement
The GALAH Survey relies on the work of the Gaia mission, so please consider including their acknowledgements:
This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.