A dataset provided by the European Space Agency

Name 16252
Title TREASUREHUNT: Hubbles UV-Visible treasury imaging of the JWST NEP Time-Domain Field
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=16252;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-cqsn994
Author Jansen, Rolf A.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=16252&mission=hst
Publication
  • An Atlas of Color-selected Quiescent Galaxies at z > 3 in Public JWST Fields
  • EPOCHS. III. Unbiased UV Continuum Slopes at 6.5 < z < 13 from Combined PEARLS GTO and Public JWST/NIRCam Imaging
  • EPOCHS. II. The Ultraviolet Luminosity Function from 7.5 < z < 13.5 Using 180 arcmin2 of Deep, Blank Fields from the PEARLS Survey and Public JWST Data
  • EPOCHS. I. The Discovery and Star-forming Properties of Galaxies in the Epoch of Reionization at 6.5 < z < 18 with PEARLS and Public JWST Data
  • EPOCHS. IV. SED Modeling Assumptions and Their Impact on the Stellar Mass Function at 6.5 <= z <= 13.5 Using PEARLS and Public JWST Observations
  • Even redder than we knew: Color and AV evolution up to z = 2.5 from JWST/NIRCam photometry
  • Galaxy mergers in the epoch of reionization - I. A JWST study of pair fractions, merger rates, and stellar mass accretion rates at z = 4.5-11.5
  • Galaxy-scale lens search in the PEARLS NEP TDF and CEERS JWST fields
  • J-NEP: 60-band photometry and photometric redshifts for the James Webb Space Telescope North Ecliptic Pole Time-Domain Field
  • JWSTs PEARLS: NIRCam imaging and NIRISS spectroscopy of a z = 3.6 star-forming galaxy lensed into a near-Einstein ring by a z = 1.258 massive elliptical galaxy
  • Lonely Little Red Dots: Challenges to the Active Galactic Nucleus Nature of Little Red Dots through Their Clustering and Spectral Energy Distributions
  • Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
  • PEARLS: Discovery of Point-source Features within Galaxies in the North Ecliptic Pole Time Domain Field
  • PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-domain Field II
  • The impact of satellite trails on Hubble Space Telescope observations
  • TREASUREHUNT: Transients and Variability Discovered with HST in the JWST North Ecliptic Pole Time-domain Field
Instrument ACS/WFC, WFC3/UVIS
Temporal Coverage 2020-09-25T04:55:57Z/2022-10-31T07:42:02Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2022-10-31T18:40:32Z
Last Update 2026-03-09
Keywords Hubble Space Telescope data, HST observations dataset, NASA ESA Hubble mission data, space-based optical imaging data, ultraviolet astronomy observations, near-infrared imaging dataset, Hubble spectroscopy data, Wide Field Camera 3 WFC3 data, Advanced Camera for Surveys ACS data, Space Telescope Imaging Spectrograph STIS data, Cosmic Origins Spectrograph COS data, Hubble deep field imaging dataset, extragalactic survey observations, galaxy evolution imaging data, star formation observations HST, stellar photometry dataset, globular cluster imaging data, supernova Hubble observations, exoplanet transit HST data, interstellar medium spectroscopy data, calibrated level 2 HST data products, drizzled image mosaics, FITS files astronomy, flux-calibrated spectra, photometric time-series Hubble data, redshift measurements dataset, Hubble Legacy Archive data, Mikulski Archive for Space Telescopes MAST dataset
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Jansen et al., 2022, 'TREASUREHUNT: Hubble's UV-Visible treasury imaging of the JWST NEP Time-Domain Field', 1.0, European Space Agency, https://doi.org/10.5270/esa-cqsn994