surveys and observing programs
a list of major surveys and observing programs
Major Surveys
- UNCOVER/MegaScience Survey (2022–)
Photometry and Catalog lead - Euclid Consortium Deep Field Survey (2018–)
LBG Work Package co-lead, US/NASA high redshift coordinator - Cosmic Dawn Survey (2018–)
Project Co-lead, Photometry and Catalog co-lead - Cosmic Evolution Survey (2018–)
COSMOS2020 Catalog lead
Observing Programs
In addition to large Hawaii-led programs on CFHT (17N), Subaru (28N), and Keck (25N):
2024 | Fulfilling the UV Legacy of the Hubble and Webb Deep Public Frontier Field HST Cycle 32 — 72 orbits, PI: K. Whitaker |
2024 | Clumpy Relics: The First Spectroscopic Confirmation of Globular Clusters at z≈3 JWST/NIRSpec IFU Cycle 3 — 20h, PI: S. Cutler |
2024 | A Deep Look into PAHs: Resolved PAH and Fine-Structure Emission in z=1 Main-Sequence Galaxies JWST/MIRI Cycle 3 — 48h, PI: A. Faisst |
2024 | Mirage or Miracle? Spectroscopic Confirmation of Remarkably Luminous Galaxies at z>10 JWST/NIRSpec Cycle 3 — 33.4h, PIs: R. Naidu & P. Oesch |
2023 | [OIII] Confirmation for Intrinsically Luminous z~12 Galaxy Candidates ALMA — 23.1h, PI: C. Casey |
2023 | On the formation of cosmic DUNES: The first dusty galaxies of the universe ALMA — 36.4h, PI: J. Zavala |
2023 | Chasing Giants: Discovering a Large Population of z>3 Massive Quiescent Galaxies ALMA — 29.2h, PI: A. Long |
2023 | Unveiling the Mpc-scale structure of a maturing protocluster at z=3.61 ALMA — 6.5h, PI: N. Sillassen |
2023 | Spatially Resolving Dust Obscured Star Formation ALMA — 29.7h, PI: V. Kokorev |
2023 | Caught in the Web: ALMA Data for Every Sub-Millimeter Galaxy Over the COSMOS-Web Survey Field ALMA — 6.7h, PI: J. McKinney |
2023 | Medium bands, Mega Science: spatially-resolved R~15 spectrophotometry at z=0.3–12 JWST/NIRCam Cycle 2 — 50.1h, PI: W. Suess |
2023 | MAGNIF: Medium-band Astrophysics with the Grism of NIRCam in Frontier Fields JWST/NIRCamWFSS Cycle 2 — 38.8h, PI: F. Sun |
2023 | A deep dive into the physics of the first massive quiescent galaxies in the Universe JWST/NIRCam/NIRSpec Cycle 2 — 47.6h, PI: F. Valentino |
2022 | A comprehensive study of the most massive proto-cluster in COSMOS ALMA — 23.3h, PI: J. Zavala |
2022 | Redshift scans for dusty star-forming galaxies at cosmic dawn ALMA — 8.7h, PI: R. Gobat |
2022 | Dust in galaxies at z=8–11 ALMA — 22.1h, PI: S. Fujimoto |
2022 | Unveiling the nature of a strong H₂O absorption in a dusty galaxy at z=4.1 ALMA — 3.3h, PI: S. Jin |
2022 | A joint ALMA and JWST public Legacy Field – Abell 2744 ALMA — 37.2h, PI: S. Fujimoto |
2022 | WERLS: Webb Epoch of Reionization Lyman-alpha Survey Keck/MOSFIRE+LRIS — 29N, PI: C. Casey & J. Kartaltepe |
2022 | Compact oddballs in COSMOS: The Faint End of the z>6 Quasar Luminosity Function HST Cycle 30 — 14 Orbits, PI: A. Faisst |
2022 | Beasts in the Bubbles: Characterizing ultra-luminous Galaxies at Cosmic Dawn JWST/NIRSpec IFU Cycle 1 — 14.4h, PI: J. Weaver |
2022 | Galaxy Protoclusters as Drivers of Cosmic Reionization JWST/NIRCam/NIRSpec Cycle 1 — 25.2/9.7h, PI: C. Martin |
2022 | Identifying protoclusters at z~4 in the Euclid Deep Field North NOEMA — 10.0h, PI: M. Shuntov |
2022 | Exploring UV-bright galaxies at z~9–10 Keck/MOSFIRE — 2N, PI: B. Mobasher |
2022 | Deep spectroscopy of bright red massive quiescent galaxies at z~2.5–3 VLT/X-Shooter — 56.0h, PI: F. Valentino |
2022 | First accurate constraint of cold dust and gas properties in the EoR NOEMA — 20.0h, PI: D. Liu |
2022 | Uncovering a unique population of gas giants at <z>=1.2 NOEMA — 8.0h, PI: V. Kokorev |
2022 | Deep [OIII] 88μm and dust cont. of two luminous galaxies at z~10 ALMA Cycle 8 — 17.8h, PI: T. Hashimoto |
2022 | Beasts in the Bubbles: Remarkably UV-bright Galaxies at z=9–10 Keck/MOSFIRE — 2N, PI: C. Casey |
2022 | Beasts in the Bubbles: Remarkably UV-bright Galaxies at z=9–10 Subaru/SWIMS — 1.5N, PI: S. Fujimoto |
2022 | Deep Subaru HSC z-band imaging of the Euclid/JWST/Roman Deep Field Subaru/HSC — 2N, PI: N. Suzuki |
2021 | Beasts in the Bubbles: Remarkably UV-bright Galaxies at z=9–10 VLT/XSHOOTER — 25.7h, PI: S. Fujimoto |
2021 | A pilot study of AGN disk reverberation mapping at redshift z=1 Liverpool Telescope — 26.0h, PI: J. Hernandez Santisteban |
2021 | Chasing big bubbles: the confirmation of a bright z=9.8 galaxy NOEMA — 30.0h, PI: F. Valentino |
2019 | Resolving the rapid quenching of star formation in the local Universe ALMA Cycle 7 — 10.7h, PI: K. Rowlands |