First scientific observations with MEGARA at GTC

dc.contributor.authorGil de Paz, Armando
dc.contributor.authorGallego Maestro, Jesús
dc.contributor.authorBouquin, A.
dc.contributor.authorCarbajo, J.
dc.contributor.authorCardiel López, Nicolás
dc.contributor.authorCastillo Morales, África
dc.contributor.authorEsteban San Román, Segundo
dc.contributor.authorLópez Orozco, José Antonioi
dc.contributor.authorPascual Ramírez, Sergio
dc.contributor.authorPicazo, P.
dc.contributor.authorSánchez Penim, Ainhoa
dc.contributor.authorZamorano Calvo, Jaime
dc.contributor.authorCatalán Torrecilla, Cristina
dc.contributor.authorDullo, Bililign
dc.contributor.authorPérez González, P.G.
dc.date.accessioned2023-06-17T22:39:04Z
dc.date.available2023-06-17T22:39:04Z
dc.date.issued2018
dc.description© 2018 SPIE. Artículo firmado por 82 autores. Conference on Ground-Based and Airborne Instrumentation for Astronomy (VII. 2018. Austin, TX, USA).
dc.description.abstractOn June 25th 2017, the new intermediate-resolution optical IFU and MOS of the 10.4-m GTC had its first light. As part of the tests carried out to verify the performance of the instrument in its two modes (IFU & MOS) and 18 spectral setups (identical number of VPHs with resolutions R=6000-20000 from 0.36 to 1 micron) a number of astronomical objects were observed. These observations show that MEGARA@GTC is called to fill a niche of high-throughput, intermediate resolution IFU & MOS observations of extremely-faint narrow-lined objects. Lyman-α absorbers, star-forming dwarfs or even weak absorptions in stellar spectra in our Galaxy or in the Local Group can now be explored to a new level. Thus, the versatility of MEGARA in terms of observing modes and spectral resolution and coverage will allow GTC to go beyond current observational limits in either depth or precision for all these objects. The results to be presented in this talk clearly demonstrate the potential of MEGARA in this regard.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/51309
dc.identifier.doi10.1117/12.2313299
dc.identifier.issn0277-786X
dc.identifier.officialurlhttps://doi.org/10.1117/12.2313299
dc.identifier.relatedurlhttps://www.spiedigitallibrary.org
dc.identifier.urihttps://hdl.handle.net/20.500.14352/18729
dc.journal.titleGround-based and airbone instrumentation for astronomy
dc.language.isoeng
dc.publisherSpie-Int Soc Optical Engineering
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordIntermediate-resolution IFU & MOS
dc.subject.keywordOptical spectrograph
dc.subject.keywordResolved stellar populations
dc.subject.keywordCosmis web
dc.subject.keywordLyman-alpha forest
dc.subject.keywordKinematics and dynamics
dc.subject.keywordNearby galaxies
dc.subject.keywordOptical fibers.
dc.subject.ucmAstrofísica
dc.titleFirst scientific observations with MEGARA at GTC
dc.typejournal article
dc.volume.number10702
dspace.entity.typePublication
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