A dataset provided by the European Space Agency

Name 7826
Title Near-IR Photometry of M31s Metal-Rich Globular Clusters
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=7826;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-h4xy20i
Author Frogel, Jay A.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=7826&mission=hst
Publication
  • Deep ALTAIR+NIRI Imaging of the Disk and Bulge of M31
  • Hubble Space Telescope NICMOS Color Transformations and Photometric Calibrations
  • Hubble Space Telescope-NICMOS Observations of M31S Metal-Rich Globular Clusters and Their Surrounding Fields. II. Results
  • Hubble Space Telescope-NICMOS Observations of M31S Metal-Rich Globular Clusters and Their Surrounding Fields. I. Techniques
  • Prospects for Measuring Supermassive Black Hole Masses with Future Extremely Large Telescopes
  • The Star Formation Histories of the Bulge and Disk of M31 from Resolved Stars in the Near-Infrared
  • The Stellar Content of the Bulge of M31
  • Transformations between the Theoretical and Observational Planes in the Hubble Space Telescope NICMOS and WFPC2 Photometric Systems
Instrument NICMOS/NIC1, NICMOS/NIC2, NICMOS/NIC3
Temporal Coverage 1998-07-18T18:51:52Z/1998-10-28T16:15:29Z
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 1999-10-29T18:54:49Z
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, Frogel comma Jay A., 1999, 'Near-IR Photometry of M31's Metal-Rich Globular Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-h4xy20i