Ten years of speckle interferometry at SOAR
arXiv:1801.04772 · doi:10.1088/1538-3873/aaa7d9
Abstract
Since 2007, close binary and multiple stars are observed by speckle interferometry at the 4.1 m Southern Astrophysical Research (SOAR) telescope. The HRCam instrument, observing strategy and planning, data processing and calibration methods, developed and improved during ten years, are presented here in a concise way. Thousands of binary stars were measured with diffraction-limited resolution (29mas at 540nm wavelength) and a high accuracy reaching 1mas; two hundred new pairs or subsystems were discovered. To date, HRCam has performed over 11000 observations with a high efficiency (up to 300 stars per night). An overview of the main results delivered by this instrument is given.
Accepted by PASP. 12 pages, 11 figures
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Cited by in corpus (132)
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- The inflated, eccentric warm Jupiter TOI-4914 b orbiting a metal-poor star, and the hot Jupiters TOI-2714 b and TOI-2981 b
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- TESS discovery of a super-Earth and two sub-Neptunes orbiting the bright, nearby, Sun-like star HD 22946
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- TOI-3288 b and TOI-4666 b: two gas giants transiting low-mass stars characterised by NIRPS
- A Transiting Super-Earth in the Radius Valley and An Outer Planet Candidate Around HD 307842
- Migration and Evolution of giant ExoPlanets (MEEP) II: Super-Jupiters and Lithium-rich Host Stars
- Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. VI: Confirmation of a Long-Period Giant Planet Discovered with a Single TESS Transit
- Confirmation of four hot Jupiters detected by TESS using follow-up spectroscopy from MaHPS at Wendelstein together with NEID and TRES
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- TOI-1743 b, TOI-5799 b, TOI-5799 c and TOI-6223 b: TESS discovery and validation of four super-Earth to Neptune-sized planets around M dwarfs
- TOI-2458 b: A mini-Neptune consistent with in situ hot Jupiter formation
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- Detection and characterisation of a 106-day transiting Jupiter : TOI-2449 b / NGTS-36 b
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