Table 6: PSR B0656+14 in the NIR-optical-NUV range.
Filter/ Log ${\nu}$ $F_{\nu}$ $F_{\nu}$
Telescope   observed dereddeneda
  Hz $\mu$Jy $\mu$Jy
NIR
${\it F187W}$/HST 14.204( $^{\rm +30}_{-28}$) 0.779(97)b 0.789(98)
${\it F160W}$/HST 14.273( $^{\rm +58}_{-51}$) 0.575(41)b 0.584(42)
${\it F110W}$/HST 14.436( $^{\rm +138}_{-105}$) 0.336(30)b 0.346(31)
Optical
I/Subaru 14.571( $^{\rm +44}_{-40}$) 0.371( +44-40)c 0.390( $^{\rm +46}_{-42}$)
R/Subaru 14.658( $^{\rm +55}_{-49}$) 0.417( +55-49)c 0.447( $^{\rm +59}_{-53}$)
${\it F555W}$/HST 14.734( $^{\rm +62}_{-54}$) 0.393(24)b 0.428(26)
B/Subaru 14.829( $^{\rm +52}_{-47}$) 0.313( +52-47)c 0.350( $^{\rm +58}_{-53}$)
${\it F430W}$/HST 14.882( $^{\rm +49}_{-44}$) 0.264(29)d 0.300(33)
NUV
${\it F342W}$/HST 14.944( $^{\rm +47}_{-43}$) 0.307(27)d 0.353(31)
${\it GRISM}$/HST 15.071( $^{\rm +170}_{-125}$) 0.354(31)e 0.429(38)
${\it F195W}$/HST 15.104( $^{\rm +159}_{-39}$) 0.349(43)d 0.438(54)

a  E(B-V)=0.03; b K (2001); c this work; d Pavlov et al. (1997); e Shibanov et al. (2005).

Source LaTeX | All tables | In the text