Update embright section; fixes #89

ligo/followup_advocate/templates/em_bright.jinja2

@@ -5,11 +5,15 @@
 estimation {{citeskymap_number(updated_skymap.pipeline, citation_index)}},
 under the assumption that the candidate {{gracedb_id}} is astrophysical in
 origin,{% else %}Assuming the candidate is astrophysical in origin, {% endif %}
-the probability that the lighter compact object has a mass
-< 3 solar masses (HasNS) is {{probability(prob_has_ns)}}.
-[{{citation_index['em_bright']}}] Using the
-masses and spins inferred from the signal, the probability of
-matter outside the final compact object (HasRemnant)
-is {{probability(prob_has_remnant)}}. [{{citation_index['em_bright']}}]
+the probability that the lighter compact object is consistent with a neutron star mass
+(HasNS) is {{probability(prob_has_ns)}}.
+[{{citation_index['em_bright']}}] Using the masses and spins inferred from the signal, the
+probability of matter outside the final compact object (HasRemnant) is
+{{probability(prob_has_remnant)}}. [{{citation_index['em_bright']}}]
+Both HasNS and HasRemnant consider the support of several neutron star
+equations of state. The probability that any one of the binary components
+lie between 3 to 5 solar mass (HasMassgap) is {{probability(prob_has_massgap)}}.
+
+
 
 {% endfilter %}