TY - JOUR
T1 - The Simons Observatory
T2 - science goals and forecasts for the enhanced Large Aperture Telescope
AU - The Simons Observatory collaboration
AU - Abitbol, M.
AU - Abril-Cabezas, I.
AU - Adachi, S.
AU - Ade, P.
AU - Adler, A. E.
AU - Agrawal, P.
AU - Aguirre, J.
AU - Ahmed, Z.
AU - Aiola, S.
AU - Alford, T.
AU - Ali, A.
AU - Alonso, D.
AU - Alvarez, M. A.
AU - An, R.
AU - Arnold, K.
AU - Ashton, P.
AU - Atkins, Z.
AU - Austermann, J.
AU - Azzoni, S.
AU - Baccigalupi, C.
AU - Baleato Lizancos, A.
AU - Barron, D.
AU - Barry, P.
AU - Bartlett, J.
AU - Battaglia, N.
AU - Battye, R.
AU - Baxter, E.
AU - Bazarko, A.
AU - Beall, J. A.
AU - Bean, R.
AU - Beck, D.
AU - Beckman, S.
AU - Begin, J.
AU - Beheshti, A.
AU - Beringue, B.
AU - Bhandarkar, T.
AU - Bhimani, S.
AU - Bianchini, F.
AU - Biermann, E.
AU - Biquard, S.
AU - Bixler, B.
AU - Boada, S.
AU - Boettger, D.
AU - Bolliet, B.
AU - Bond, J. R.
AU - Borrill, J.
AU - Borrow, J.
AU - Braithwaite, C.
AU - Brien, T. L.R.
AU - Galvez Ghersi, J. T.
N1 - Publisher Copyright:
© 2025 The Author(s).
PY - 2025/8/1
Y1 - 2025/8/1
N2 - We describe updated scientific goals for the wide-field, millimeter-wave survey that will be produced by the Simons Observatory (SO). Significant upgrades to the 6-meter SO Large Aperture Telescope (LAT) are expected to be complete by 2028, and will include a doubled mapping speed with 30,000 new detectors and an automated data reduction pipeline. In addition, a new photovoltaic array will supply most of the observatory’s power. The LAT survey will cover about 60% of the sky at a regular observing cadence, with five times the angular resolution and ten times the map depth of the Planck satellite. The science goals are to: (1) determine the physical conditions in the early universe and constrain the existence of new light particles; (2) measure the integrated distribution of mass, electron pressure, and electron momentum in the late-time universe, and, in combination with optical surveys, determine the neutrino mass and the effects of dark energy via tomographic measurements of the growth of structure at redshifts z ≲ 3; (3) measure the distribution of electron density and pressure around galaxy groups and clusters, and calibrate the effects of energy input from galaxy formation on the surrounding environment; (4) produce a sample of more than 30,000 galaxy clusters, and more than 100,000 extragalactic millimeter sources, including regularly sampled AGN light-curves, to study these sources and their emission physics; (5) measure the polarized emission from magnetically aligned dust grains in our Galaxy, to study the properties of dust and the role of magnetic fields in star formation; (6) constrain asteroid regoliths, search for Trans-Neptunian Objects, and either detect or eliminate large portions of the phase space in the search for Planet 9; and (7) provide a powerful new window into the transient universe on time scales of minutes to years, concurrent with observations from the Vera C. Rubin Observatory of overlapping sky.
AB - We describe updated scientific goals for the wide-field, millimeter-wave survey that will be produced by the Simons Observatory (SO). Significant upgrades to the 6-meter SO Large Aperture Telescope (LAT) are expected to be complete by 2028, and will include a doubled mapping speed with 30,000 new detectors and an automated data reduction pipeline. In addition, a new photovoltaic array will supply most of the observatory’s power. The LAT survey will cover about 60% of the sky at a regular observing cadence, with five times the angular resolution and ten times the map depth of the Planck satellite. The science goals are to: (1) determine the physical conditions in the early universe and constrain the existence of new light particles; (2) measure the integrated distribution of mass, electron pressure, and electron momentum in the late-time universe, and, in combination with optical surveys, determine the neutrino mass and the effects of dark energy via tomographic measurements of the growth of structure at redshifts z ≲ 3; (3) measure the distribution of electron density and pressure around galaxy groups and clusters, and calibrate the effects of energy input from galaxy formation on the surrounding environment; (4) produce a sample of more than 30,000 galaxy clusters, and more than 100,000 extragalactic millimeter sources, including regularly sampled AGN light-curves, to study these sources and their emission physics; (5) measure the polarized emission from magnetically aligned dust grains in our Galaxy, to study the properties of dust and the role of magnetic fields in star formation; (6) constrain asteroid regoliths, search for Trans-Neptunian Objects, and either detect or eliminate large portions of the phase space in the search for Planet 9; and (7) provide a powerful new window into the transient universe on time scales of minutes to years, concurrent with observations from the Vera C. Rubin Observatory of overlapping sky.
KW - CMBR experiments
KW - cosmological parameters from CMBR
KW - feedback in galaxies
KW - star explosions
UR - https://www.scopus.com/pages/publications/105013332246
U2 - 10.1088/1475-7516/2025/08/034
DO - 10.1088/1475-7516/2025/08/034
M3 - Article
AN - SCOPUS:105013332246
SN - 1475-7516
VL - 2025
JO - Journal of Cosmology and Astroparticle Physics
JF - Journal of Cosmology and Astroparticle Physics
IS - 8
M1 - 034
ER -