Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8063
Full metadata record
DC FieldValueLanguage
dc.contributor.authorSharma, Saurabh-
dc.contributor.authorOjha, Devendra. K-
dc.contributor.authorGhosh, Arpan-
dc.contributor.authorNinan, Joe. P-
dc.contributor.authorGhosh, Supriyo-
dc.contributor.authorGhosh, Swarna. K-
dc.contributor.authorManoj, P-
dc.contributor.authorNaik, Milind. B-
dc.contributor.authorD'Costa, Savio, L. A-
dc.contributor.authorReddy, B. Krishna-
dc.contributor.authorNanjappa, Nandish-
dc.contributor.authorPandey, Rakesh-
dc.contributor.authorSinha, Tirthendu-
dc.contributor.authorPanwar, Neelam-
dc.contributor.authorSusmitha, A-
dc.contributor.authorKaur, Harmeen-
dc.contributor.authorSahu, Sanjit-
dc.contributor.authorBangia, Tarun-
dc.contributor.authorPoojary, Satheesha S-
dc.contributor.authorJadhav, Rajesh. B-
dc.contributor.authorBhagat, Shailesh. B-
dc.contributor.authorMeshram, Ganesh. S-
dc.contributor.authorShah, Harshit-
dc.contributor.authorRayner, John. T-
dc.contributor.authorToome, Douglas. W-
dc.contributor.authorSandimani, Pradeep. R-
dc.date.accessioned2022-10-20T10:18:02Z-
dc.date.available2022-10-20T10:18:02Z-
dc.date.issued2022-08-
dc.identifier.citationPublications of the Astronomical Society of the Pacific, Vol. 134, No. 1038, 085002en_US
dc.identifier.issn0004-6280-
dc.identifier.urihttp://hdl.handle.net/2248/8063-
dc.descriptionOpen Accessen_US
dc.description.abstractWe present the design and performance of the TANSPEC, a medium-resolution 0.55–2.5 μm cryogenic spectrometer and imager, now in operation at the 3.6 m Devasthal Optical Telescope (DOT), Nainital, India. The TANSPEC provides three modes of operation, which include photometry with broad- and narrowband filters, spectroscopy with short slits of 20″ length and different widths (from 0.″5 to 4.″0) in cross-dispersed mode at a resolving power R of ∼2750, and spectroscopy with long slits of 60″ length and different widths (from 0.″5 to 4.″0) in prism mode at a resolving power R of ∼100–350. TANSPEC’s imager mode provides a field of view of 60″ × 60″ with a plate scale of 0.″245 pixel−1 on the 3.6 m DOT. The TANSPEC was successfully commissioned during 2019 April–May, and the subsequent characterization and astronomical observations are presented here. The TANSPEC was made available to the worldwide astronomical community for science observations from 2020 October.en_US
dc.language.isoenen_US
dc.publisherIOP Publishing Ltd on behalf of the Astronomical Society of the Pacificen_US
dc.relation.urihttps://doi.org/10.1088/1538-3873/ac81eb-
dc.rights© The Author(s)-
dc.subjectSpectrometersen_US
dc.subjectDirect imagingen_US
dc.subjectNear infrared astronomyen_US
dc.subjectOptical observationen_US
dc.titleTANSPEC: TIFR-ARIES Near-infrared Spectrometeren_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
TANSPEC TIFR-ARIES Near-infrared Spectrometer.pdf8.47 MBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.