Figure 18.
VLT/X–shooter average spectrum (black, upper panel UVB, central panel VIS, bottom panel NIR) of SDSS1238. Regions strongly affected by telluric absorption are drawn in grey. The two insets show the white dwarf Mg ii (4481 Å) and the secondary K i ($12\, 432/12\, 522$ Å) absorption features used to measure their radial velocities. For comparison, the SDSS spectrum is shown in blue (no offset in flux has been applied). The agreement between the two spectra illustrates the good relative and absolute flux calibration of the X-shooter data. The circles and the squares are the SDSS (blue, green, red, purple, and salmon for the u, g, i, r, and $z$ band filters) and 2MASS (grey, gold and cyan for the J, H, Ks band filters) photometry (obtained at different epochs).

VLT/X–shooter average spectrum (black, upper panel UVB, central panel VIS, bottom panel NIR) of SDSS1238. Regions strongly affected by telluric absorption are drawn in grey. The two insets show the white dwarf Mg ii (4481 Å) and the secondary K i (⁠|$12\, 432/12\, 522$| Å) absorption features used to measure their radial velocities. For comparison, the SDSS spectrum is shown in blue (no offset in flux has been applied). The agreement between the two spectra illustrates the good relative and absolute flux calibration of the X-shooter data. The circles and the squares are the SDSS (blue, green, red, purple, and salmon for the u, g, i, r, and |$z$| band filters) and 2MASS (grey, gold and cyan for the J, H, Ks band filters) photometry (obtained at different epochs).

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close