The 1-D flux (y axis) is in ergs/sec/cm2/angstrom.
The wavelength (x axis) is in angstroms.
The left part of the spectra are from the G430M data,
and the right part are from the G750M data -- note
that they are scaled differently in y (flux). The x axis
(wavelength) is scaled the same for all objects.
Spectra for individual objects are available via the LMC
flux page.
Maintained by the MCPN Project
Team, with
acknowledgements.
Some content is restricted (*) until publication. Send comments to
mutchler@stsci.edu.
Copyright
� 2001 The Association of Universities for Research in Astronomy, Inc.
All Rights Reserved.
