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Thermal and Nonthermal Emission at Large Radii in the ... - HEASARC

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HXD/PIN
Observ<strong>at</strong>ion
of
NW<br />

Radio
Relic<br />

• 73.5
ksec
exposure
<strong>in</strong>
PIN<br />

• NXB
model
agrees
well
with<br />

Earth-blocked
flux
(2.1%)
<strong>and</strong><br />

spectrum<br />

• Model
CXB<br />

• Model
AGN
po<strong>in</strong>t
srcs<br />

• Relic
<strong>at</strong>
large
projected
radius
_<br />

<strong>the</strong>rmal
emission
weak
but
still<br />

very
important<br />

• Model
<strong>the</strong>rmal
based
on
XIS<br />

<strong>and</strong>/or
XMM
(see
also<br />

Nakazawa
poster)<br />

Earth-blocked
d<strong>at</strong>a
vs.<br />

NXB
model

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