Gemini High-resolution Optical SpecTrograph (GHOST) at Gemini-South: Instrument Performance and Integration, First Science, and Next Steps
V. M. Kalari, R. J. Diaz, G. Robertson, A. McConnachie,M. Ireland,R. Salinas, P. Young, C. Simpson, C. Hayes, J. Nielsen,G. Burley,J. Pazder, M. Gomez-Jimenez,E. Martioli,S. B. Howell, M. Jeong,S. Juneau, R. Ruiz-Carmona,S. Margheim,A. Sheinis, A. Anthony, G. Baker,T. A. M. Berg, T. Cao,E. Chapin, T. Chin, K. Chiboucas,V. Churilov, E. Deibert, A. Densmore, J. Dunn, M. L. Edgar, J. Heo, D. Henderson,T. Farrell, J. Font,V. Firpo, J. Fuentes,K. Labrie, S. Lambert,J. Lawrence, J. Lothrop,R. Mcdermid, B. W. Miller, G. Perez,V. M. Placco, P. Prado, C. Quiroz, F. Ramos,R. Rutten, K. M. G. Silva, J. Thomas-Osip, C. Urrutia, W. D. Vacca,K. Venn, F. Waller,L. Waller, M. White,S. Xu, R. Zhelem ASTRONOMICAL JOURNAL（2024）
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High resolution spectroscopy,Astronomical instrumentation,Optical observatories
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