Table 5: Geminga in the NIR-optical-NUV-FUV range.
Filter/ Log ${\nu}$ $F_{\nu}$ $F_{\nu}$
Telescope   observed dereddeneda
  Hz $\mu$Jy $\mu$Jy
NIR
${\it F160W}$/HST 14.273( $^{\rm +58}_{-51}$) 0.230(25)b,c 0.233(25)
${\it F110W}$/HST 14.436( $^{\rm +138}_{-105}$) 0.166(21)b,c 0.170(21)
Optical
I/Subaru 14.571( $^{\rm +44}_{-40}$) 0.193 +19-21c 0.201 $^{\rm +20}_{-22}$
R/Subaru 14.658( $^{\rm +55}_{-49}$) 0.172 +17-18c $\rm0.181^{+18}_{-19}$
${\it F555W}$/HST 14.734( $^{\rm +62}_{-54}$) 0.170(20)d 0.182(21)
${\it F555W}$/HST 14.734( $^{\rm +62}_{-54}$) 0.146(13)c 0.156(14)
${\it F430W}$/HST 14.882( $^{\rm +49}_{-44}$) 0.146(11)c 0.160(12)
NUV
${\it F342W}$/HST 14.944( $^{\rm +47}_{-43}$) 0.201(10)c 0.224(11)
${\it F25SRF}$/HST 15.116( $^{\rm +122}_{-95}$) 0.261(26)d 0.315(31)
F195W/HST 15.104( $^{\rm +159}_{-39}$) 0.288(30)c 0.344(36)
FUV
G140L/HST 15.322(84) 0.455(29)d 0.546(35)
a  E(B-V)=0.023; b Harlow et al.  (1998); c this work; d Kargaltsev et al.  (2005)
using ACS and STIS/MAMA NUV and FUV.

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