A dataset provided by the European Space Agency

Name 11677
Title Is 47 Tuc Young? Measuring its White Dwarf Cooling Age and Completing a Hubble Legacy
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=11677;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-sqgmtq5
Author Richer, Harvey B.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=11677&mission=hst
Publication
  • A comparative analysis of the observed white dwarf cooling sequence from globular clusters
  • A Deep, Wide-field, and Panchromatic View of 47 Tuc and the SMC with HST: Observations and Data Analysis Methods
  • A Dynamical Signature of Multiple Stellar Populations in 47 Tucanae
  • A JWST Project on 47 Tucanae. Overview, Photometry, and Early Spectroscopic Results of M Dwarfs and Observations of Brown Dwarfs
  • An age difference of two billion years between a metal-rich and a metal-poor globular cluster
  • An Empirical Measure of the Rate of White Dwarf Cooling in 47 Tucanae
  • A new visual - near-infrared diagnostic to estimate the metallicity of cluster and field dwarf stars
  • Comparing the White Dwarf Cooling Sequences in 47 Tuc and NGC 6397
  • Constraining Globular Cluster Age Uncertainties using the IR Color-Magnitude Diagram
  • Deep HST Imaging in 47 Tucanae: A Global Dynamical Model
  • Hubble Space Telescope Proper Motion (HSTPROMO) Catalogs of Galactic Globular Clusters. V. The Rapid Rotation of 47 Tuc Traced and Modeled in Three Dimensions
  • Implications of the Milky Way Travel Velocity for Dynamical Mass Estimates of the Local Group
  • JWST unveils the brown dwarf sequence of 47 Tucanae
  • Multiple stellar populations in globular clusters with JWST: an NIRCam view of 47 Tucanae
  • New PARSEC data base of a-enhanced stellar evolutionary tracks and isochrones - I. Calibration with 47 Tuc (NGC 104) and the improvement on RGB bump
  • Solo dwarfs - III. Exploring the orbital origins of isolated Local Group galaxies with Gaia Data Release 2
  • Sum of the masses of the Milky Way and M31: A likelihood-free inference approach
  • The age of the Galactic stellar halo from Gaia white dwarfs
  • The Blue Turn in the White Dwarf Stars of Globular Clusters
  • The impact of satellite trails on Hubble Space Telescope observations
  • The M31 Velocity Vector. I. Hubble Space Telescope Proper-motion Measurements
  • The M31 Velocity Vector. II. Radial Orbit toward the Milky Way and Implied Local Group Mass
  • The onset of convective coupling and freezing in the white dwarfs of 47 Tucanae
  • The outskirts of M33: Tidally induced distortions versus signatures of gas accretion
  • The Spectral Energy Distributions of White Dwarfs in 47 Tucanae: The Distance to the Cluster
  • The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. III. NGC 4038/39 and NGC 5584
  • The white dwarf cooling sequence of 47 Tucanae
  • Ultra-Deep Hubble Space Telescope Imaging of the Small Magellanic Cloud: The Initial Mass Function of Stars with M <~ 1 M
  • Updated BaSTI Stellar Evolution Models and Isochrones. II. a-enhanced Calculations
  • Validation of PSF models for HST and other space-based observations
Instrument ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage 2010-01-15T05:11:16Z/2010-10-01T21:00:10Z
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 2011-10-02T01:30:39Z
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Richer comma Harvey B., 2011, 'Is 47 Tuc Young? Measuring its White Dwarf Cooling Age and Completing a Hubble Legacy', 1.0, European Space Agency, https://doi.org/10.5270/esa-sqgmtq5