ARCADE ARCADE (Absolute Radiometer for Cosmology, Astrophysics, and Diffuse Emission) is a high altitude balloon payload designed to study the early universe.
Airships NASA is considering a stratospheric airship challenge to incentivize the demonstration of a long duration scientific platform for both Earth and space sciences.
BICEP BICEP (Background Imaging of Cosmic Extragalactic Polarization) is an experiment designed to measure the polarization of the cosmic microwave background (CMB) to unprecedented precision.
BICEP Array BICEP Array is the fourth stage of the BICEP2/Keck/BICEP3
BICEP2 / Keck Array BICEP2 and Keck Array follow BICEP and probe more deeply in the polarization of the CMB.
BICEP3 BICEP3 will provide the most sensitive map of the CMB & polarized foregrounds at 95 GHz at the spatial scales where the imprint of primordial Inflation may be found. It is supported by The Office of the Chief Scientist & Chief Technologist.
Boomerang The continuing mission of the Boomerang project is to study the properties of the Cosmic Microwave Background radiation (CMBR).
COMAP The CO Mapping Array Pathfinder (COMAP) will open a new window on both the Epoch of Reionization (EoR) and the Epoch of Galaxy Assembly by using carbon monoxide (CO) lines to trace the distribution of star-forming galaxies in both epochs.
Dark Energy Survey (DES) DES is a optical survey that covers 5000 square degree of the sky and aims at constraining dark energy through weak lensing, SN1A, galaxy clusters, and baryonic acoustic oscillations.
Euclid Euclid is a mission designed to study "dark energy", the hypothesized cause of the Universe's accelerated expansion. I am a member of the NASA-funded Euclid Science Team.
FIRS (Far Infrared Surveyor) The Far Infrared Surveyor is a large cryogenic space telescope envisioned as a follow-on to the Spitzer Space Telescope (Spitzer) and the Herschel Space Observatory.
GEMP Galactic Emission Mapping Project (GEMP) is a project located in Portugal aimed at mapping the polarised galactic emission at 5GHz and 10GHz.
Herschel The Herschel Space Observatory was a space-based telescope that studied the Universe in the light of the far-infrared and submillimeter portions of the spectrum.
Hyper Suprime-Cam (HSC) The Subaru HSC survey is an optical survey that covers 1400 square degrees of the sky with the depth of median redshift~1. One of the main science targets of the survey is weak lensing cosmology.
Juno Juno is in 53-day polar orbits, observing Jupiter in order to understand the planet's gross size and structural properties, as well as measuring its atmospheric composition, temperature and deep wind profiles.
Nancy Grace Roman Space Telescope The Nancy Grace Roman Space Telescope is a NASA observatory designed to unravel the secrets of dark energy and dark matter, search for and image exoplanets, and explore many topics in infrared astrophysics.
PASIPHAE A unique Astrophysics experiment is set to take place at the Skinakas Observatory, Crete, and the South African Astronomical Observatory in Sutherland, South Africa, aiming to clear the path towards the detection of the imprint on primordial light ..
Planck Planck is the first European mission to study the birth of the Universe. Planck was launched on May 14, 2009.
ROBO-AO Robo-AO is the first autonomous laser adaptive optics system and science instrument operating on sky.
Rosetta The Rosetta mission is designed to study the origin of comets, the relationship between cometary and interstellar material and its implications with regard to the origin of the Solar System.
SPHEREx SPHEREx will conduct an all-sky spectral survey in the near-infrared.
Spider Spider is a balloon borne observatory designed to probe the epoch of Inflation through measurements of the CMB polarization on the largest angular scales.
Spitzer The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003.
Square Kilometre Array (SKA) The Square Kilometre Array is the world's biggest radio telescope, to be built in South Africa and Western Australia over the coming decade.
SuperBIT SuperBIT is a mid-latitude (launch from Wanaka, NZ) ultra-long duration balloon (ULDB), which will provide 100 days of near space-quality imaging of selected galaxy clusters to study properties of dark energy and dark matter.