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A Partial Near-infrared Guide Star Catalog for Thirty Meter Telescope Operations

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dc.contributor.author Shah, Sarang
dc.contributor.author Subramanian, S
dc.contributor.author Avinash, Ck
dc.contributor.author Andersen, David R
dc.contributor.author Skidmore, Warren
dc.contributor.author Anupama, G. C
dc.contributor.author Delgado, Francisco
dc.contributor.author Gillies, Kim
dc.contributor.author Maheshwar, G
dc.contributor.author Ramaprakash, A. N
dc.contributor.author Reddy, B. E
dc.contributor.author Sivarani, T
dc.contributor.author Subramaniam, A
dc.date.accessioned 2024-08-30T05:09:10Z
dc.date.available 2024-08-30T05:09:10Z
dc.date.issued 2024-08-01
dc.identifier.citation The Astronomical Journal, Vol. 168, No. 2, 59 en_US
dc.identifier.issn 1538-3881
dc.identifier.uri http://hdl.handle.net/2248/8523
dc.description Open Access en_US
dc.description Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
dc.description.abstract At first light, the Thirty Meter Telescope (TMT) near-infrared (NIR) instruments will be fed by a multiconjugate adaptive optics instrument known as the Narrow Field Infrared Adaptive Optics System (NFIRAOS). NFIRAOS will use six laser guide stars to sense atmospheric turbulence in a volume corresponding to a field of view of 2', but natural guide stars (NGSs) will be required to sense tip/tilt and focus. To achieve high sky coverage (50% at the north Galactic pole), the NFIRAOS client instruments use NIR on-instrument wave front sensors that take advantage of the sharpening of the stars by NFIRAOS. A catalog of guide stars with NIR magnitudes as faint as 22 mag in the J band (Vega system), covering the TMT-observable sky, will be a critical resource for the efficient operation of NFIRAOS, and no such catalog currently exists. Hence, it is essential to develop such a catalog by computing the expected NIR magnitudes of stellar sources identified in deep optical sky surveys using their optical magnitudes. This paper discusses the generation of a partial NIR Guide Star Catalog (IRGSC), similar to the final IRGSC for TMT operations. The partial catalog is generated by applying stellar atmospheric models to the optical data of stellar sources from the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) optical data and then computing their expected NIR magnitudes. We validated the computed NIR magnitudes of the sources in some fields by using the available NIR data for those fields. We identified the remaining challenges of this approach. We outlined the path for producing the final IRGSC using the Pan-STARRS data. We have named the Python code to generate the IRGSC as irgsctool, which generates a list of NGS for a field using optical data from the Pan-STARRS 3pi survey and also a list of NGSs having observed NIR data from the UKIRT Infrared Deep Sky Survey if they are available. irgsctool is available in the public domain on this GitHub public repository (https://github.com/sshah1502/irgsc), while the generated and validated IRGSC for the 20 test fields and additional Pan-STARRS Medium Deep Survey fields can be found on Zenodo. en_US
dc.language.iso en en_US
dc.publisher American Astronomical Society en_US
dc.relation.uri https://doi.org/10.3847/1538-3881/ad517f
dc.rights © 2024. The Author(s)
dc.subject Catalogs en_US
dc.subject Surveys en_US
dc.subject Astronomy data analysis en_US
dc.subject Observational astronomy en_US
dc.subject Astronomical techniques en_US
dc.subject Interstellar extinction en_US
dc.subject Star counts en_US
dc.title A Partial Near-infrared Guide Star Catalog for Thirty Meter Telescope Operations en_US
dc.type Article en_US


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