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
{"title":"位于双子座南区的双子座高分辨率光学摄谱仪(GHOST):仪器性能和集成、首次科学实验以及下一步工作","authors":"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","doi":"arxiv-2409.05855","DOIUrl":null,"url":null,"abstract":"The Gemini South telescope is now equipped with a new high-resolution\nspectrograph called GHOST (the Gemini High-resolution Optical SpecTrograph).\nThis instrument provides high-efficiency, high-resolution spectra covering\n347-1060 nm in a single exposure of either one or two targets simultaneously,\nalong with precision radial velocity spectroscopy utilizing an internal\ncalibration source. It can operate at a spectral element resolving power of\neither 76000 or 56000, and can reach a SNR$\\sim$5 in a 1hr exposure on a\nV$\\sim$20.8 mag target in median site seeing, and dark skies (per resolution\nelement). GHOST was installed on-site in June 2022, and we report performance\nafter full integration to queue operations in November 2023, in addition to\nscientific results enabled by the integration observing runs. These results\ndemonstrate the ability to observe a wide variety of bright and faint targets\nwith high efficiency and precision. With GHOST, new avenues to explore\nhigh-resolution spectroscopy have opened up to the astronomical community.\nThese are described, along with the planned and potential upgrades to the\ninstrument.","PeriodicalId":501068,"journal":{"name":"arXiv - PHYS - Solar and Stellar Astrophysics","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2024-09-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Gemini High-resolution Optical SpecTrograph (GHOST) at Gemini-South: Instrument performance and integration, first science, and next steps\",\"authors\":\"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\",\"doi\":\"arxiv-2409.05855\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The Gemini South telescope is now equipped with a new high-resolution\\nspectrograph called GHOST (the Gemini High-resolution Optical SpecTrograph).\\nThis instrument provides high-efficiency, high-resolution spectra covering\\n347-1060 nm in a single exposure of either one or two targets simultaneously,\\nalong with precision radial velocity spectroscopy utilizing an internal\\ncalibration source. It can operate at a spectral element resolving power of\\neither 76000 or 56000, and can reach a SNR$\\\\sim$5 in a 1hr exposure on a\\nV$\\\\sim$20.8 mag target in median site seeing, and dark skies (per resolution\\nelement). GHOST was installed on-site in June 2022, and we report performance\\nafter full integration to queue operations in November 2023, in addition to\\nscientific results enabled by the integration observing runs. These results\\ndemonstrate the ability to observe a wide variety of bright and faint targets\\nwith high efficiency and precision. With GHOST, new avenues to explore\\nhigh-resolution spectroscopy have opened up to the astronomical community.\\nThese are described, along with the planned and potential upgrades to the\\ninstrument.\",\"PeriodicalId\":501068,\"journal\":{\"name\":\"arXiv - PHYS - Solar and Stellar Astrophysics\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-09\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Solar and Stellar Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.05855\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Solar and Stellar Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.05855","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Gemini High-resolution Optical SpecTrograph (GHOST) at Gemini-South: Instrument performance and integration, first science, and next steps
The Gemini South telescope is now equipped with a new high-resolution
spectrograph called GHOST (the Gemini High-resolution Optical SpecTrograph).
This instrument provides high-efficiency, high-resolution spectra covering
347-1060 nm in a single exposure of either one or two targets simultaneously,
along with precision radial velocity spectroscopy utilizing an internal
calibration source. It can operate at a spectral element resolving power of
either 76000 or 56000, and can reach a SNR$\sim$5 in a 1hr exposure on a
V$\sim$20.8 mag target in median site seeing, and dark skies (per resolution
element). GHOST was installed on-site in June 2022, and we report performance
after full integration to queue operations in November 2023, in addition to
scientific results enabled by the integration observing runs. These results
demonstrate the ability to observe a wide variety of bright and faint targets
with high efficiency and precision. With GHOST, new avenues to explore
high-resolution spectroscopy have opened up to the astronomical community.
These are described, along with the planned and potential upgrades to the
instrument.