A dataset provided by the European Space Agency

Name 9727
Title Exploration of the SN Ia Hubble Diagram at z > 1.2
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=9727;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-8ci7o7v
Author Perlmutter, Saul
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=9727&mission=hst
Publication
  • A Census of Photometrically Selected Little Red Dots at 4 < z < 9 in JWST Blank Fields
  • A dusty compact object bridging galaxies and quasars at cosmic dawn
  • A New Determination of the High-Redshift Type Ia Supernova Rates with the Hubble Space Telescope Advanced Camera for Surveys
  • A Panchromatic Catalog of Early-type Galaxies at Intermediate Redshift in the Hubble Space Telescope Wide Field Camera 3 Early Release Science Field
  • A Probabilistic Approach to Classifying Supernovae Using Photometric Information
  • CANDELS Multi-wavelength Catalogs: Source Detection and Photometry in the GOODS-South Field
  • Clumpy Galaxies in CANDELS. I. The Definition of UV Clumps and the Fraction of Clumpy Galaxies at 0.5 < z < 3
  • Contamination of Broadband Photometry by Nebular Emission in High-redshift Galaxies: Investigations with Kecks MOSFIRE Near-infrared Spectrograph
  • Cosmic evolution of radio-excess active galactic nuclei in quiescent and star-forming galaxies across 0 < z < 4
  • Deep Large Binocular Camera r-band Observations of the GOODS-N Field
  • Differential attenuation in star-forming galaxies at 0.3 z 1.5 in the SHARDS/CANDELS field
  • Dust in Little Red Dots
  • Early Growth of the Star Formation Rate Function in the Epoch of Reionization: An Approach with Rest-frame Optical Emissions
  • Evaluating the Accuracy of Non-parametric Galaxy Morphological Indicator Measurements in the CSST Imaging Survey
  • Evolution of Intermediate Redshift Galaxies Physical Properties and Mass-Metallicity Relation
  • Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
  • HALO7D II: The Halo Velocity Ellipsoid and Velocity Anisotropy with Distant Main-sequence Stars
  • Identification of High-redshift Galaxy Overdensities in GOODS-N and GOODS-S
  • JWST/MIRI unveils the stellar component of the GN20 dusty galaxy overdensity at z = 4.05
  • Massive Quiescent Disk Galaxies at 0.5 <= z <= 1 in CANDELS: Color Gradients and Likely Origin
  • Metallicities of Emission-line Galaxies from HST ACS PEARS and HST WFC3 ERS Grism Spectroscopy at 0.6 < z < 2.4
  • Near-infrared Survey of the GOODS-North Field: Search for Luminous Galaxy Candidates at z >~ 6.5
  • Ne v emission from a faint epoch of reionization-era galaxy: evidence for a narrow-line intermediate-mass black hole
  • Not Just a Dot: The Complex UV Morphology and Underlying Properties of Little Red Dots
  • O II emitters at z ~ 4.6 in the GOODS field: a homogeneous measure of evolving star formation
  • On the Impact of Inclination-dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
  • Precision Measurement of The Most Distant Spectroscopically Confirmed Supernova Ia with the Hubble Space Telescope
  • Star Formation Rate Function at z 4.5: An Analysis from Rest UV to Optical
  • The CANDELS/SHARDS Multiwavelength Catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission-line Fluxes, and Star Formation Rates
  • The Effect of Surface Brightness Dimming in the Selection of High-z Galaxies
  • The Evolutionary Pathway of Low-mass Supermassive Black Holes at Intermediate Redshift: Insights from the JADES Survey
  • The First Photometric Evidence of a Transient/Variable Source at z > 5 with JWST
  • The Hubble Legacy Archive ACS grism data
  • The impact of satellite trails on Hubble Space Telescope observations
  • The mass evolution of the first galaxies: stellar mass functions and star formation rates at 4 < z < 7 in the CANDELS GOODS-South field
  • The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam
  • Thermonuclear supernova light curves: Progenitors and cosmology
  • The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z = 3.5
  • The z 9 Galaxy UV Luminosity Function from the JWST Advanced Deep Extragalactic Survey: Insights into Early Galaxy Evolution and Reionization
Instrument ACS, ACS/WFC, NICMOS, NICMOS/NIC2
Temporal Coverage 2004-04-02T01:59:13Z/2005-09-15T03:12:28Z
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 2006-09-15T12:49:22Z
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, Perlmutter et al., 2006, 'Exploration of the SN Ia Hubble Diagram at z > 1.2', 1.0, European Space Agency, https://doi.org/10.5270/esa-8ci7o7v