The WST science drivers encompass a very broad range of areas, across the full electromagnetic spectrum and beyond. The WST will be pivotal, in synergy with other major astronomical facilities in the 2040s, to tackle some of the key open questions in modern astrophysics:
What are the extreme physical conditions that govern transient events (explosions, eruptions, and disruptions)?
Was the Universe re-ionized by few very highly star-forming galaxies or from a larger population of galaxies with more modest rate of star-formation?
The WST will uniquely combine the required panoramic coverage and sensitivity with the ability to characterise the galaxies’ ionising capability. By cross-correlating the fluctuating 21 cm signal with the large-scale galaxy distribution in the same cosmic volumes, it will test whether rare luminous or abundant sub-luminous sources drive reionisation.
What is the interplay between dark, stellar, and gaseous material in galaxies, and how does primordial and metal-enriched gas flow in and out of galaxies at various scales during different epochs?
Understanding the interplay between galaxies, their dark matter haloes, and the large-scale structures has long been limited by observational gaps across these regimes. The WST will bridge these scales with unprecedented accuracy and statistical power, offering a unified view of galaxy evolution.
How do black holes form and grow over cosmic time?
The statistical power of the WST, combined with its operational approach, will be key in investigating intermediate mass black holes and constrain the whole range of black hole population and their influence on galaxies.
What is the origin of the chemical elements that are crucial to trace the evolution of galaxies?
Is the accelerated expansion of the Universe due to an unknown form of energy or to a modification of General Relativity on large scales?
The WST will provide this essential multiprobe view, combining local and high redshift galaxy surveys, cosmic web mapping, and gravitational wave counterparts to reveal deviations from standard cosmology.
How do environmental conditions affect the formation and evolution of stars and planets?
The WST will perform a large-scale, high-resolution spectroscopic survey of planet-host stars and white dwarfs, spanning a broad range of Galactic environments.
What can we learn from multi-messenger observations (e.g., gravitational waves and photons) about the nature of compact objects? How can the extreme conditions during mergers of such objects test the laws of physics?
The wide field of view and high multiplexing of WST are ideal for pinpointing the electromagnetic counterparts of gravitational wave events, which can have initial localization uncertainties of several square degrees.
What are the extreme physical conditions that govern transient events (explosions, eruptions, and disruptions)?
Was the Universe re-ionized by few very highly star-forming galaxies or from a larger population of galaxies with more modest rate of star-formation?
The WST will uniquely combine the required panoramic coverage and sensitivity with the ability to characterise the galaxies’ ionising capability. By cross-correlating the fluctuating 21 cm signal with the large-scale galaxy distribution in the same cosmic volumes, it will test whether rare luminous or abundant sub-luminous sources drive reionisation.
What is the interplay between dark, stellar, and gaseous material in galaxies, and how does primordial and metal-enriched gas flow in and out of galaxies at various scales during different epochs?
Understanding the interplay between galaxies, their dark matter haloes, and the large-scale structures has long been limited by observational gaps across these regimes. The WST will bridge these scales with unprecedented accuracy and statistical power, offering a unified view of galaxy evolution.
How do black holes form and grow over cosmic time?
The statistical power of the WST, combined with its operational approach, will be key in investigating intermediate mass black holes and constrain the whole range of black hole population and their influence on galaxies.
What is the origin of the chemical elements that are crucial to trace the evolution of galaxies?
Is the accelerated expansion of the Universe due to an unknown form of energy or to a modification of General Relativity on large scales?
The WST will provide this essential multiprobe view, combining local and high redshift galaxy surveys, cosmic web mapping, and gravitational wave counterparts to reveal deviations from standard cosmology.
How do environmental conditions affect the formation and evolution of stars and planets?
The WST will perform a large-scale, high-resolution spectroscopic survey of planet-host stars and white dwarfs, spanning a broad range of Galactic environments.
What can we learn from multi-messenger observations (e.g., gravitational waves and photons) about the nature of compact objects? How can the extreme conditions during mergers of such objects test the laws of physics?
The wide field of view and high multiplexing of WST are ideal for pinpointing the electromagnetic counterparts of gravitational wave events, which can have initial localization uncertainties of several square degrees.
What are the extreme physical conditions that govern transient events (explosions, eruptions, and disruptions)?
Was the Universe re-ionized from few very highly star-forming galaxies or from a larger population of galaxies with more modest rate of star-formation?
The WST will uniquely combine the required panoramic coverage and sensitivity with the ability to characterise the galaxies’ ionising capability. By cross-correlating the fluctuating 21 cm signal with the large-scale galaxy distribution in the same cosmic volumes, it will test whether rare luminous or abundant sub-luminous sources drive reionisation.
What is the interplay between dark, stellar, and gaseous material in galaxies, and how does primordial and metal-enriched gas flow in and out of galaxies at various scales during different epochs?
Understanding the interplay between galaxies, their dark matter haloes, and the large-scale structures has long been limited by observational gaps across these regimes. The WST will bridge these scales with unprecedented accuracy and statistical power, offering a unified view of galaxy evolution.
How do black holes form and grow over cosmic time?
The statistical power of the WST, combined with its operational approach, will be key in investigating intermediate mass black holes and constrain the whole range of black hole population and their influence on galaxies.
What is the origin of the chemical elements that are crucial to trace the evolution of galaxies?
Is the accelerated expansion of the Universe due to an unknown form of energy or to a modification of General Relativity on large scales?
The WST will provide this essential multiprobe view, combining local and high redshift galaxy surveys, cosmic web mapping, and gravitational wave counterparts to reveal deviations from standard cosmology.
How do the environment conditions affect the formation and evolution of stars and planets?
The WST will perform a large-scale, high-resolution spectroscopic survey of planet-host stars and white dwarfs, spanning a broad range of Galactic environments.
What multiple messengers (e.g. gravitational waves, photons) tell us on the nature of compact objects and the extreme physics at play during their merging?
The wide field of view and high multiplexing of WST is ideally suited to the several square degrees uncertainty on the location on sky of the electromagnetic counterpart of gravitational waves events.
The WST will fill a critical gap in the global astronomical infrastructure of the 2040s.
The WST was conceived to transform our understanding of the Universe through large-scale spectroscopy.
Addressing outstanding science
Issue #1 The WST Chronicle