A dataset provided by the European Space Agency

Name 11339
Title A deep observation of NGC4261: understanding its unique X-ray source population, gas morphology, and jet properties
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=11339;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-lwm4j3s
Author Zezas, Andreas
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=11339&mission=hst
Publication
  • Circumnuclear Dust in Luminous Early-type Galaxies. I. Sample Properties and Stellar Luminosity Models
  • Studying the asymmetry of the globular cluster population of NGC 4261
  • The Two-dimensional Projected Spatial Distribution of Globular Clusters. I. Method and Application to NGC 4261
  • The X-ray point source population hosted by globular clusters in the elliptical galaxy NGC 4261
Instrument WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage 2007-12-26T09:51:17Z/2008-03-10T22:53:57Z
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 2009-03-11T11:47:04Z
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, Zezas comma Andreas, 2009, 'A deep observation of NGC4261: understanding its unique X-ray source population, gas morphology, and jet properties', 1.0, European Space Agency, https://doi.org/10.5270/esa-lwm4j3s