IR spectroscopy in the range 12â\u80\u93230 μm with the SPace IR telescope for Cosmology and Astrophysics (SPICA) will reveal the physical processes governing the formation and evolution of galaxies and black holes through cosmic time, bridging the gap between the James Webb Space Telescope and the upcoming Extremely Large Telescopes at shorter wavelengths and the Atacama Large Millimeter Array at longer wavelengths. The SPICA, with its 2.5-m telescope actively cooled to below 8 K, will obtain the first spectroscopic determination, in the mid-IR rest-frame, of both the star-formation rate and black hole accretion rate histories of galaxies, reaching lookback times of 12 Gyr, for large statistically significant samples. Densities, temperatu...
The evolution of galaxies at Cosmic Noon (redshift 1<3) passed through a dust-obscured phase, dur...
Measurements in the infrared wavelength domain allow us to assess directly the physical state and en...
Measurements in the infrared wavelength domain allow us to assess directly the physical state and en...
IR spectroscopy in the range 12â230 μm with the SPace IR telescope for Cosmology and Astrophysics (...
IR spectroscopy in the range 12-230 mu m with the SPace IR telescope for Cosmology and Astrophysics ...
IR spectroscopy in the range 12-230 μm with the SPace IR telescope for Cosmology and Astrophysics (S...
IR spectroscopy in the range 12-230 μm with the SPace IR telescope for Cosmology and Astrophysics (S...
IR spectroscopy in the range 12–230μm with the SPace IR telescope for Cosmology and Astrophysics (S...
To study the dust obscured phase of the galaxy evolution during the peak of the Star Formation Rate ...
We use the SPace Infrared telescope for Cosmology and Astrophysics (SPICA) project as a template to ...
The evolution of galaxies at Cosmic Noon (redshift 1<3) passed through a dust-obscured phase, dur...
Measurements in the infrared wavelength domain allow us to assess directly the physical state and en...
Measurements in the infrared wavelength domain allow us to assess directly the physical state and en...
IR spectroscopy in the range 12â230 μm with the SPace IR telescope for Cosmology and Astrophysics (...
IR spectroscopy in the range 12-230 mu m with the SPace IR telescope for Cosmology and Astrophysics ...
IR spectroscopy in the range 12-230 μm with the SPace IR telescope for Cosmology and Astrophysics (S...
IR spectroscopy in the range 12-230 μm with the SPace IR telescope for Cosmology and Astrophysics (S...
IR spectroscopy in the range 12–230μm with the SPace IR telescope for Cosmology and Astrophysics (S...
To study the dust obscured phase of the galaxy evolution during the peak of the Star Formation Rate ...
We use the SPace Infrared telescope for Cosmology and Astrophysics (SPICA) project as a template to ...
The evolution of galaxies at Cosmic Noon (redshift 1<3) passed through a dust-obscured phase, dur...
Measurements in the infrared wavelength domain allow us to assess directly the physical state and en...
Measurements in the infrared wavelength domain allow us to assess directly the physical state and en...