#
#   Copyright (c) 2021-2022 Lami Suleiman, Morgane Fortin
#
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#   You should have received a copy of the GNU General Public License
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# Measured Neutron Star masses in Double Neutron Star binary systems
# Data used in Fig.1 of Suleiman et al. PRC 2021.
# We present 24 sources in Double Neutron Star binary

#! The columns are:
#! (i) pulsar mass (in solar masses)
#! (ii) minus error in mass (in solar masses)
#! (iii) plus error in mass (in solar masses)
#! (iv) pulsar name

1.174	  0.004	0.004   J0453$+$1559c
1.2064  0.002   0.002   J1807$-$2500Bc
1.23	0.007	0.007   J1756$-$2251c
1.248868	0.000011	0.000013  J0737$-$3039B
1.27    0.03    0.03    J1913$+$1102c
1.291	0.011	0.011   J1906$+$0746
1.299   0.0035  0.0035  J1829$+$2456
1.306   0.0035  0.0035  J1829$+$2456c
1.322	0.011	0.011   J1906$+$0746c
1.333	0.0002	0.0002  B1534$+$12
1.338185	0.000014	0.000012  J0737$-$3039A
1.3406  0.0005  0.0005  J1757$-$1854
1.34    0.08    0.08    J0509$+$3801
1.341	0.007	0.007   J1756$-$2251  
1.3455	0.0002	0.0002  B1534$+$12c 
1.354	0.01	0.01    B2127$+$11Cc
1.358	0.01	0.01    B2127$+$11C
1.3655  0.0021  0.0021  J1807$-$2500B
1.390   0.001   0.001   B1913$+$16c  
1.3917  0.0004  0.0004  J1757$-$1854c
1.438   0.001   0.001   B1913$+$16  
1.46    0.08    0.08    J0509$+$3801c
1.559	0.004	0.004   J0453$+$1559  
1.62    0.03   0.03     J1913$+$1102