[HTML][HTML] First Sagittarius A* event horizon telescope results. III. Imaging of the galactic center supermassive black hole
First Sagittarius A* Event Horizon Telescope Results. III. Imaging of the Galactic Center
Supermassive Black Hole - IOPscience Skip to content IOP Science home Accessibility Help …
Supermassive Black Hole - IOPscience Skip to content IOP Science home Accessibility Help …
First Sagittarius A* event horizon telescope results. IV. Variability, morphology, and black hole mass
In this paper we quantify the temporal variability and image morphology of the horizon-scale
emission from Sgr A*, as observed by the EHT in 2017 April at a wavelength of 1.3 mm. We …
emission from Sgr A*, as observed by the EHT in 2017 April at a wavelength of 1.3 mm. We …
First M87 event horizon telescope results. VII. Polarization of the ring
Abstract In 2017 April, the Event Horizon Telescope (EHT) observed the near-horizon region
around the supermassive black hole at the core of the M87 galaxy. These 1.3 mm …
around the supermassive black hole at the core of the M87 galaxy. These 1.3 mm …
[HTML][HTML] First M87 event horizon telescope results. IV. Imaging the central supermassive black hole
First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
- IOPscience This site uses cookies. By continuing to use this site you agree to our use of …
- IOPscience This site uses cookies. By continuing to use this site you agree to our use of …
First M87 event horizon telescope results. VI. The shadow and mass of the central black hole
We present measurements of the properties of the central radio source in M87 using Event
Horizon Telescope data obtained during the 2017 campaign. We develop and fit geometric …
Horizon Telescope data obtained during the 2017 campaign. We develop and fit geometric …
First M87 event horizon telescope results. I. The shadow of the supermassive black hole
Event Horizon Telescope Collaboration - arXiv preprint arXiv …, 2019 - arxiv.org
When surrounded by a transparent emission region, black holes are expected to reveal a
dark shadow caused by gravitational light bending and photon capture at the event horizon …
dark shadow caused by gravitational light bending and photon capture at the event horizon …
On the application of machine learning in astronomy and astrophysics: A text‐mining‐based scientometric analysis
JV Rodríguez, I Rodríguez‐Rodríguez… - … Reviews: Data Mining …, 2022 - Wiley Online Library
Since the beginning of the 21st century, the fields of astronomy and astrophysics have
experienced significant growth at observational and computational levels, leading to the …
experienced significant growth at observational and computational levels, leading to the …
Silhouettes of invisible black holes
VI Dokuchaev, NO Nazarova - Physics-Uspekhi, 2020 - iopscience.iop.org
In general relativity, isolated black holes are invisible due to the infinitely large redshift of
photons propagating from the event horizon to a remote observer. However, the dark …
photons propagating from the event horizon to a remote observer. However, the dark …
First M87 event horizon telescope results. IV. Imaging the central supermassive black hole
Event Horizon Telescope Collaboration - arXiv preprint arXiv …, 2019 - arxiv.org
We present the first Event Horizon Telescope (EHT) images of M87, using observations from
April 2017 at 1.3 mm wavelength. These images show a prominent ring with a diameter of …
April 2017 at 1.3 mm wavelength. These images show a prominent ring with a diameter of …
Interferometric imaging directly with closure phases and closure amplitudes
Interferometric imaging now achieves angular resolutions as fine as∼ 10 μas, probing
scales that are inaccessible to single telescopes. Traditional synthesis imaging methods …
scales that are inaccessible to single telescopes. Traditional synthesis imaging methods …