A dataset provided by the European Space Agency

Name 11227
Title The orbital period for an ultraluminous X-ray source in NGC1313
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=11227;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-j2n8j64
Author Liu, Jifeng
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=11227&mission=hst
Publication
  • Absence of nebular He II l4686 constrains the UV emission from the ultraluminous X-ray pulsar NGC 1313 X-2
  • Compact Optical Counterparts of Ultraluminous X-Ray Sources
  • Dynamical Mass Constraints on the Ultraluminous X-Ray Source NGC 1313 X-2
  • Hubble Space Telescope Monitoring Reveals a 6.1 Day Period for an Ultraluminous X-Ray Source in NGC 1313
  • Nuclear star clusters in 228 spiral galaxies in the HST/WFPC2 archive: catalogue and comparison to other stellar systems
  • Optical variability of the ultraluminous X-ray source NGC 1313 X-2
  • Searching for the orbital period of the ultraluminous X-ray source NGC 1313 X-2
  • The Distance Measurement of NGC 1313 with Cepheids
  • The Nature of the UV/Optical Emission of the Ultraluminous X-Ray Source in Holmberg II
Instrument WFPC2, WFPC2/PC
Temporal Coverage 2007-10-03T02:30:17Z/2008-08-13T01:32:37Z
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 2009-08-13T07:18:38Z
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, Liu comma Jifeng, 2009, 'The orbital period for an ultraluminous X-ray source in NGC1313', 1.0, European Space Agency, https://doi.org/10.5270/esa-j2n8j64