#
#   Copyright (c) 2021-2022 Lami Suleiman, Morgane Fortin
#
#   This file is part of CompOSE
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#   You should have received a copy of the GNU General Public License
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# Measured Neutron Star masses of X-ray optical sources
# Data used in Fig.1 of Suleiman et al. PRC 2021.
# We present 17 sources not in Double Neutron Star binary nor Milisecond pulsars nor Slowly rotating Pulsars.

#! 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

1.02	0.17	0.17     4U1538$-$52
1.073	0.358	0.358    Her$\,$X$-$1           
1.21	0.12	0.12     SMC$\,$X$-$1
1.30    0.26    0.40     XTE$\,$J$\,$2123$-$058
1.41	0.24	0.24     XTE$\,$J1855$-$026
1.44    0.1     0.1      2S$\,$0921$-$630
1.57	0.11	0.11     LMC$\,$X$-$4
1.57	0.16	0.16     Cen$\,$X$-$3
1.57	0.25	0.25     SAX$\,$J1802.7$-$2017
1.71	0.21 	0.21     Cyg$\,$X$-$2
1.74	0.3    	0.3      OAO$\,$1657$-$415
1.91	0.45	0.45     EXO$\,$1722$-$363
1.96    0.36    0.36     4U$\,$1822$-$371
2.0     0.4     0.4      J01326.7$+$303228
2.12	0.16	0.16     Vela$\,$X$-$1
2.27    0.15    0.17     PSR$\,$J2215$+$5135
2.40    0.12    0.12     PSR$\,$B1957$+$20