Name
9479
Title
The Field Stellar Populations of M33s Outer Halo
URL
https://hst.esac.esa.int/ehst/#/pages/search;proposal=9479;TAPCLIENT=DOI
DOI
https://doi.org/10.5270/esa-jpyfycy
Author
Sarajedini, Ata
Description
This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=9479&mission=hst
Publication
A Catalog of New M33 Star Clusters Based on Hubble Space Telescope WFPC2 Images Ages of M33 Star Clusters Based on the Hubble Space Telescope/WFPC2 Photometry A New Distance to M33 Using Blue Supergiants and the FGLR Method CLUES about M33: the reversed radial stellar age gradient in the outskirts of Triangulum galaxy Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies The Detection of Inside-Out Disk Growth in M33 The impact of satellite trails on Hubble Space Telescope observations The Stellar Populations in the Outer Regions of M33. II. Deep ACS Imaging The Stellar Populations in the Outer Regions of M33. III. Star Formation History The stellar populations of M33s outer regions - IV. Inflow history and chemical evolution
Instrument
ACS, ACS/WFC, NICMOS, NICMOS/NIC2, STIS/CCD, WFPC2, WFPC2/PC
Temporal Coverage
2003-01-12T05:56:38Z/2003-01-12T12:27:13Z
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
2006-12-20T06:03:19Z
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, Sarajedini comma Ata, 2006, 'The Field Stellar Populations of M33's Outer Halo', 1.0, European Space Agency, https://doi.org/10.5270/esa-jpyfycy Copy Example
