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