We have observed linear polarization of the Sgr A* at band 3, 6, 7, 8, and 9 using ALMA. I will outline our method, and compare our measurements with the records taken since 2005 by Geoffrey Bower and Dan Marrone
We report on the submillimeter properties of Sagittarius A* derived from observations with the Submi...
Sgr A* is variable at radio and submillimeter wavelengths on hourly timescales, showing time delays ...
The Atacama Large mm-submm Array (ALMA) is, by far, the most sensitive mm/submm telescope in the Wor...
We have observed linear polarization of the Sgr A* at band 3, 6, 7, 8, and 9 using ALMA. I will outl...
Aims. Our aim is to characterize the polarized continuum emission properties including intensity, po...
Aims. Our aim is to characterize the polarized continuum emission properties including int...
Aims. Our aim is to characterize the polarized continuum emission properties including intensity, po...
International audienceWe present the results from a full polarization study carried out with the Ata...
Aims. Our aim is to characterize the polarized continuum emission properties including int...
Contains fulltext : 35198.pdf ( ) (Open Access) ...
The role of magnetic field in the AGN jet physics is still not fully determined. At pc scale, it is ...
We report linearly polarized continuum emission properties of Sgr A* at $\sim$492 GHz, based on the ...
The role of magnetic field in the AGN jet physics is still not fully determined. At pc scale, it is ...
International audienceWe characterize the accuracy of linear-polarization mosaics made using the Ata...
Contains fulltext : 198798pub.pdf (publisher's version ) (Open Access) ...
We report on the submillimeter properties of Sagittarius A* derived from observations with the Submi...
Sgr A* is variable at radio and submillimeter wavelengths on hourly timescales, showing time delays ...
The Atacama Large mm-submm Array (ALMA) is, by far, the most sensitive mm/submm telescope in the Wor...
We have observed linear polarization of the Sgr A* at band 3, 6, 7, 8, and 9 using ALMA. I will outl...
Aims. Our aim is to characterize the polarized continuum emission properties including intensity, po...
Aims. Our aim is to characterize the polarized continuum emission properties including int...
Aims. Our aim is to characterize the polarized continuum emission properties including intensity, po...
International audienceWe present the results from a full polarization study carried out with the Ata...
Aims. Our aim is to characterize the polarized continuum emission properties including int...
Contains fulltext : 35198.pdf ( ) (Open Access) ...
The role of magnetic field in the AGN jet physics is still not fully determined. At pc scale, it is ...
We report linearly polarized continuum emission properties of Sgr A* at $\sim$492 GHz, based on the ...
The role of magnetic field in the AGN jet physics is still not fully determined. At pc scale, it is ...
International audienceWe characterize the accuracy of linear-polarization mosaics made using the Ata...
Contains fulltext : 198798pub.pdf (publisher's version ) (Open Access) ...
We report on the submillimeter properties of Sagittarius A* derived from observations with the Submi...
Sgr A* is variable at radio and submillimeter wavelengths on hourly timescales, showing time delays ...
The Atacama Large mm-submm Array (ALMA) is, by far, the most sensitive mm/submm telescope in the Wor...