First Very Long Baseline Interferometry Detections at 870 μm

dc.contributor.authorRaymond, Alexander W.
dc.contributor.organizationfi=Suomen ESO-keskus|en=Finnish Centre for Astronomy with ESO|
dc.contributor.organizationfi=Tuorlan observatorio|en=Tuorla Observatory|
dc.contributor.organization-code1.2.246.10.2458963.20.54954054844
dc.contributor.organization-code1.2.246.10.2458963.20.90670098848
dc.converis.publication-id458464042
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/458464042
dc.date.accessioned2025-08-28T00:45:54Z
dc.date.available2025-08-28T00:45:54Z
dc.description.abstract<p>The first very long baseline interferometry (VLBI) detections at 870 μm wavelength (345 GHz frequency) are reported, achieving the highest diffraction-limited angular resolution yet obtained from the surface of the Earth and the highest-frequency example of the VLBI technique to date. These include strong detections for multiple sources observed on intercontinental baselines between telescopes in Chile, Hawaii, and Spain, obtained during observations in 2018 October. The longest-baseline detections approach 11 Gλ, corresponding to an angular resolution, or fringe spacing, of 19 μas. The Allan deviation of the visibility phase at 870 μm is comparable to that at 1.3 mm on the relevant integration timescales between 2 and 100 s. The detections confirm that the sensitivity and signal chain stability of stations in the Event Horizon Telescope (EHT) array are suitable for VLBI observations at 870 μm. Operation at this short wavelength, combined with anticipated enhancements of the EHT, will lead to a unique high angular resolution instrument for black hole studies, capable of resolving the event horizons of supermassive black holes in both space and time.<br></p>
dc.identifier.eissn1538-3881
dc.identifier.jour-issn0004-6256
dc.identifier.olddbid206364
dc.identifier.oldhandle10024/189391
dc.identifier.urihttps://www.utupub.fi/handle/11111/45547
dc.identifier.urlhttps://iopscience.iop.org/article/10.3847/1538-3881/ad5bdb
dc.identifier.urnURN:NBN:fi-fe2025082791225
dc.language.isoen
dc.okm.affiliatedauthorRamakrishnan, Venkatessh
dc.okm.affiliatedauthorWiik, Kaj
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherInstitute of Physics Publishing
dc.publisher.countryUnited Statesen_GB
dc.publisher.countryYhdysvallat (USA)fi_FI
dc.publisher.country-codeUS
dc.relation.articlenumber130
dc.relation.doi10.3847/1538-3881/ad5bdb
dc.relation.ispartofjournalThe Astronomical Journal
dc.relation.issue3
dc.relation.volume168
dc.source.identifierhttps://www.utupub.fi/handle/10024/189391
dc.titleFirst Very Long Baseline Interferometry Detections at 870 μm
dc.year.issued2024

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