Light Curves of NGC 7469

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• UV light curves from 1996 Campaign
  • Data: UV continuum and line light curves from Wanders et al. (1997)
    [continuum at 1315 Å]
    [continuum at 1485 Å]
    [continuum at 1740 Å]
    [continuum at 1825 Å]
    [Ly alpha+N V]
    [Ly alpha]
    [C IV]
    [C III]]
    [N V]
    [Si IV]
    [He II 1640]
    
  • Reference: Wanders et al. 1997, ApJS, 113, 69 [Abstract]
  • Format of Data:
    • Column (1): JD - 2450000
    • Column (2): Flux. Continuum in units of 10^-14 ergs s^-1 cm^-2 A^-1, emission lines in units of 10^-14 ergs s^-1 cm^-2.
    • Column (3): Uncertainty in flux, same units as column (2).
  • Additional Notes: From Tables 2 and 3 of Wanders et al. (1997), based on TOMSIPS extracted IUE SWP spectra.

• Optical light curves from 1996 Campaign
  • Data: Continuum and Balmer line light curves from Collier et al. (1998)
    [continuum at 4845 Å]
    [continuum at 6962 Å]
    [H alpha]
    [H beta]
    
  • Reference: Collier et al. (1998), ApJ, 500, 162 [Abstract]
  • Format of Data:
    • Column (1): JD - 2450000
    • Column (2): Flux. Continuum in units of 10^-14 ergs s^-1 cm^-2 Å^-1, emission lines in units of 10^-14 ergs s^-1 cm^-2.
    • Column (3): Uncertainty in flux, same units as column (2).
  • Additional Notes: From Tables 1 (continuum) and 2 (lines) of Collier et al. (1998).

• Revised UV light curves from 1996 Campaign
  • Data: UV continuum and line light curves from Kriss et al. (2000)
    [continuum at 1315 Å]
    [continuum at 1485 Å]
    [continuum at 1740 Å]
    [continuum at 1825 Å]
    [Ly alpha 1215 +N V 1240]
    [Ly alpha 1215]
    [N V 1240]
    [Si II 1260]
    [O I 1304]
    [C II 1335]
    [Si IV 1400]
    [N IV] 1486]
    [C IV 1549]
    [He II 1640]
    [O III 1663]
    [N III 1750]
    [Si III] 1892 + C III] 1909]
    [Si III] 1892]
    [C III] 1909]
    
  • Reference: Kriss et al. 2000, ApJ, 535, 38 [Abstract]
  • Format of Data:
    • Column (1): JD - 2450000
    • Column (2): Flux. Continuum in units of 10^-14 ergs s^-1 cm^-2 A^-1, emission lines in units of 10^-14 ergs s^-1 cm^-2.
    • Column (3): Uncertainty in flux, same units as column (2).

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Updated 29 November 2001
peterson@astronomy.ohio-state.edu