McGill Online Magnetar Catalog

Associations and distances

This table is available in ASCII and CSV format.
Back to main catalog.

Name	Assoc?	SNR Age	Distance	Measured To	z{a}	L_x{b}
		(kyr)	(kpc)		(pc)	(10³³ erg/s)
CXOU J010043.1−721134	SMC [lfmp02]	...	62.4(1.6) [hgd12b]	SMC	...	65
4U 0142+61	...	...	3.6(4) [dv06b]	0142+61	−27.1(3.0)	105
SGR 0418+5729	...	...	~2 [vck+10]	Perseus Arm	~180	0.00096
SGR 0501+4516	SNR HB 9? [GCN8149]	4 — 7 [lt07]	~2 [lkb+11]	Perseus Arm	~68	0.81
SGR 0526−66	LMC, SNR N49?, SL 463 [cdt+82] [khg+04]	~4.8 [phs+12]	53.6(1.2) [hgd12a]	LMC	...	189
1E 1048.1−5937	GSH 288.3−0.5−28? [gmo+05]	...	9.0(1.7) [dv06b]	1048.1−5937	−82(15)	49
1E 1547.0−5408	SNR G327.24−0.13 [gg07]	...	4.5(5) [tve+10]	1547.0−5408	−10.3(1.1)	1.3
PSR J1622−4950	SNR G333.9+0.0 [ags+12]	<6 [ags+12]	~9 [lbb+10]	J1622−4950	~−16	0.44
SGR 1627−41	CTB 33, MC −71, SNR G337.0−0.1 [ccdd99] [wkv+99b]	...	11.0(3) [ccdd99]	G337.0−0.1	−21.41(58)	3.6
CXOU J164710.2−455216	Westerlund 1 [mcc+06]	...	3.9(7) [kd07]	Westerlund 1	−29.3(5.3)	0.45
1RXS J170849.0−400910	...	...	3.8(5) [dv06b]	J170849.0−400910	2.39(31)	42
CXOU J171405.7−381031	SNR CTB 37B [hg10a]	0.65^+2.50_−0.30 [nbi+09]	~13.2 [tl12]	CTB 37B	~86	56

Name	Assoc?	SNR Age	Distance	Measured To	z{a}	L_x{b}
		(kyr)	(kpc)		(pc)	(10³³ erg/s)
SGR J1745−2900	Galactic Center [mgz+13]	...	8.3(3) [bdd+14]	Galactic Center	−6.78(25)	<0.11
SGR 1806−20	W31, Star cluster, MC 13A [cwd+97] [fmc+99] [ce04]	...	8.7^+1.8_−1.5 [bcfc08]	Star cluster	−36.7^+6.3_−7.6	163
XTE J1810−197	...	...	3.5^+0.5_−0.4 [mcr+08]	J1810−197	−9.7^+1.1_−1.4	0.043
Swift J1818.0−1607	...	...	~4.8 [ATel13553]	J1818.0−1607	~−12	...
Swift J1822.3−1606	M17 [snl+12]	...	1.6(3) [snl+12]	M17	−28.5(5.3)	<0.00040
SGR 1833−0832	...	...	...	...	~3.6	<2.4
Swift J1834.9−0846	SNR W41 [kkp+12]	~100 [tllw07]	4.2(3) [lt08a]	W41	−25.0(1.8)	<0.0084
1E 1841−045	SNR Kes 73 [vg97]	0.5 — 1 [tl08]	8.5^+1.3_−1.0 [tl08]	Kes 73	−0.97^+0.11_−0.15	184
3XMM J185246.6+003317	...	...	~7.1 [zcl+14]	Kes 79	~−5.6	<0.0060
SGR 1900+14	Star cluster [vhl+00]	...	12.5(1.7) [dfk+09]	Star cluster	167(23)	90
SGR 1935+2154	SNR G57.2+0.8 [GCN16533]	...	...	...	~140	...
1E 2259+586	SNR CTB 109 [fg81]	14(2) [spgb13]	3.2(2) [kf12]	CTB 109	−55.6(3.5)	17

Name	Assoc?	SNR Age	Distance	Measured To	z{a}	L_x{b}
		(kyr)	(kpc)		(pc)	(10³³ erg/s)
SGR 0755−2933	...	...	...	...	~−110	...
SGR 1801−23	...	...	...	...	~12	...
SGR 1808−20	...	...	...	...	~−45	...
AX J1818.8−1559	...	...	...	...	~−44	20
AX J1845.0−0258	SNR G29.6+0.1 [ggv99]	<8 [ggv99]	~8.5 [tkk+98]	Scutum Arm	~16	2.9
SGR 2013+34	W58 [sbb+11]	...	~8.8 [sbb+11]	W58	~−16	...

Name	Assoc?	SNR Age	Distance	Measured To	z{a}	L_x{b}
		(kyr)	(kpc)		(pc)	(10³³ erg/s)
PSR J1846−0258	SNR Kes 75 [gvbt00]	...	6.0^+1.5_−0.9 [lt08b]	Kes 75	−25.1^+3.8_−6.3	19

Footnotes:

{a}: The height above the Galactic plane, z, is calculated from the Galactic latitudes given in Table 1, assuming a distance of 10 kpc if none is known.
{b}: L_x is in the 2–10 keV range and is calculated using the fluxes given in Table 3, assuming a distance of 10 kpc if none is known.

Go to the McGill Pulsar Group website.