
A quasar whose central black hole is hidden by a thick shroud of gas and dust.An obscured quasar is a type of active galactic nucleus where the supermassive black hole at the center of a galaxy is accreting matter at a furious rate, but this activity is hidden from direct view by a dense, dusty shroud. While a typical quasar outshines its entire host galaxy, an obscured quasar appears much dimmer at optical and ultraviolet wavelengths because the dust absorbs that light and re-emits it as infrared radiation. These objects are crucial for understanding the 'big picture' of black hole growth, as they may represent a common, hidden phase in the life cycle of galaxies.
The concept of obscured quasars emerged in the 1980s and 1990s, largely through the work of astronomers like Robert Antonucci, who proposed the unified model of active galactic nuclei, explaining that many apparent differences between objects are due to viewing angle.
The obscuring material is thought to form a torus or clumpy ring of gas and dust on a scale of a few parsecs around the central engine. When viewed from certain angles, this torus blocks the direct light from the accretion disk and the broad emission lines from the hot gas near the black hole. However, the infrared glow from the heated dust and the narrow emission lines from more distant gas can still be detected, revealing the quasar's presence.
Surveys in the infrared and X-ray bands, such as those conducted with the Spitzer Space Telescope and NuSTAR, are used to find and count obscured quasars, providing a census of black hole growth across cosmic time.
Some of the most luminous obscured quasars are so heavily hidden that they are completely invisible in optical surveys, and were only discovered through their intense infrared emission, which can outshine the entire galaxy.














