# # Copyright (c) 2021-2022 Lami Suleiman, Morgane Fortin # # This file is part of CompOSE # # CompOSE is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 2 of the License, or # (at your option) any later version. # # CompOSE is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with CompOSE; if not, write to the Free Software # Foundation, Inc., 59 Temple Place, Suite 330, Boston, MA 02111-1307 USA # # Measured Neutron Star masses for Slowly rotating pulsars # Data used in Fig.1 of Suleiman et al. PRC 2021. # We present sources not in Double Neutron Star binary and with frequency f<50 Hz (P>20ms) #! 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 1.251 0.021 0.021 J2045$+$3633 1.27 0.01 0.01 J1141$-$6545 1.34 0.10 0.10 B2303$+$46 1.3406 0.005 0.005 J1757$-$1854 1.40 0.18 0.21 J2053$+$4650 1.53 0.2 0.1 J0621$+$1002 1.831 0.01 0.01 J2222$-$0137 2.01 0.04 0.04 J0348$+$0432