Table 2. Open in new tab For a given...

Observed properties of NSs
AXP 1E 1841−045	11.783	3.930		4.750	G27.4+0.0 (Kes 73)	0.750	2.100 [1]
AXP 1E 2259+586	6.979	4.843e − 2		228.317	G109.1−01.0 (CTB 109)	10.000	16.000 [2]
CXOU J171405.7−381031	3.825	6.400		0.947	G348.7+00.3	0.350	3.150 [3]
SGR 0526−66	8.054	3.800		3.358	N49	−	4.800 [4]
SGR 1627−41	2.595	1.900		2.164	G337.3−0.1	−	5.000 [5]
HBP J1119−6127	0.408	0.400	2.684 ± 0.002 [14]	1.616	G292.2−0.5	4.200	7.100 [6]
HBP J1734−3333	1.170	0.228	0.9 ± 0.2 [15]	8.131	G354.8−0.8	1.300	− [7]
HBP J1846−0258 A	0.325	0.709	2.64 ± 0.01 [16]	0.726	G029.7−0.3 (Kes 75)	0.900	4.300 [8]
HBP J1846−0258 B	0.327	0.711	2.16 ± 0.13 [17]	0.728
PSR J0537−6910	0.016	0.518	−1.5 ± 0.1 [18]	4.925	N157B	1.000	5.000 [9]
PSR B0833−45	0.089	1.250	1.4 ± 0.2 [19]	11.319	G263.9−03.3 (Vela)	5.400	16.000 [10]
RX J0822.0−4300	0.112	8.300e − 4		213.799	G260.4−3.4 (Puppis A)	3.700	5.200 [11]
1E 1207.4−5209	0.424	6.600e − 6		1.018e5	G296.5 +10.0 (PKS 1209−51/52)	2.000	20.000 [12]
CXOU J185238.6+004020	0.105	8.680e − 7		1.917e5	G033.6+00.1 (Kes 79)	5.400	7.500 [13]

Observed properties of NSs

PSR

|$\dot{P}$|

τ_PSR

SNR

τ_{SNR −}

τ_{SNR +}

(s)

(10⁻¹¹ss⁻¹)

(kyr)

AXP 1E 1841−045

11.783

3.930

4.750

G27.4+0.0 (Kes 73)

0.750

2.100 [1]

AXP 1E 2259+586

6.979

4.843e − 2

228.317

G109.1−01.0 (CTB 109)

10.000

16.000 [2]

CXOU J171405.7−381031

3.825

6.400

0.947

G348.7+00.3

0.350

3.150 [3]

SGR 0526−66

8.054

3.800

3.358

N49

−

4.800 [4]

SGR 1627−41

2.595

1.900

2.164

G337.3−0.1

−

5.000 [5]

HBP J1119−6127

0.408

0.400

2.684 ± 0.002 [14]

1.616

G292.2−0.5

4.200

7.100 [6]

HBP J1734−3333

1.170

0.228

0.9 ± 0.2 [15]

8.131

G354.8−0.8

1.300

− [7]

HBP J1846−0258 A

0.325

0.709

2.64 ± 0.01 [16]

0.726

G029.7−0.3 (Kes 75)

0.900

4.300 [8]

HBP J1846−0258 B

0.327

0.711

2.16 ± 0.13 [17]

0.728

PSR J0537−6910

0.016

0.518

−1.5 ± 0.1 [18]

4.925

N157B

1.000

5.000 [9]

PSR B0833−45

0.089

1.250

1.4 ± 0.2 [19]

11.319

G263.9−03.3 (Vela)

5.400

16.000 [10]

RX J0822.0−4300

0.112

8.300e − 4

213.799

G260.4−3.4 (Puppis A)

3.700

5.200 [11]

1E 1207.4−5209

0.424

6.600e − 6

1.018e5

G296.5 +10.0 (PKS 1209−51/52)

2.000

20.000 [12]

CXOU J185238.6+004020

0.105

8.680e − 7

1.917e5

G033.6+00.1 (Kes 79)

5.400

7.500 [13]

Observed properties of NSs
AXP 1E 1841−045	11.783	3.930		4.750	G27.4+0.0 (Kes 73)	0.750	2.100 [1]
AXP 1E 2259+586	6.979	4.843e − 2		228.317	G109.1−01.0 (CTB 109)	10.000	16.000 [2]
CXOU J171405.7−381031	3.825	6.400		0.947	G348.7+00.3	0.350	3.150 [3]
SGR 0526−66	8.054	3.800		3.358	N49	−	4.800 [4]
SGR 1627−41	2.595	1.900		2.164	G337.3−0.1	−	5.000 [5]
HBP J1119−6127	0.408	0.400	2.684 ± 0.002 [14]	1.616	G292.2−0.5	4.200	7.100 [6]
HBP J1734−3333	1.170	0.228	0.9 ± 0.2 [15]	8.131	G354.8−0.8	1.300	− [7]
HBP J1846−0258 A	0.325	0.709	2.64 ± 0.01 [16]	0.726	G029.7−0.3 (Kes 75)	0.900	4.300 [8]
HBP J1846−0258 B	0.327	0.711	2.16 ± 0.13 [17]	0.728
PSR J0537−6910	0.016	0.518	−1.5 ± 0.1 [18]	4.925	N157B	1.000	5.000 [9]
PSR B0833−45	0.089	1.250	1.4 ± 0.2 [19]	11.319	G263.9−03.3 (Vela)	5.400	16.000 [10]
RX J0822.0−4300	0.112	8.300e − 4		213.799	G260.4−3.4 (Puppis A)	3.700	5.200 [11]
1E 1207.4−5209	0.424	6.600e − 6		1.018e5	G296.5 +10.0 (PKS 1209−51/52)	2.000	20.000 [12]
CXOU J185238.6+004020	0.105	8.680e − 7		1.917e5	G033.6+00.1 (Kes 79)	5.400	7.500 [13]

Table 2.

Open in new tab

For a given PSR, P is the period, |$\dot{P}$| the period derivative. The characteristic age is τ_PSR and the lower and upper SNR age limits are τ_SNR− and τ_{SNR +}, respectively, from the McGill magnetar catalogue (http://www.physics.mcgill.ca/∼pulsar/magnetar/main.html). The SNR ages have been compiled in the U. of Manitoba's High-Energy SNR Catalogue (SNRcat, http://www.physics.umanitoba.ca/snr/SNRcat/). References to SNR ages in this table are [1]: Kumar et al. (2014), [2]: Nakano et al. (2015), [3]: Nakamura et al. (2009), [4]: Park et al. (2012), [5]: Corbel et al. (1999), [6]: Kumar et al. (2012), [7]: Ho & Anderson (2012), [8]: Gotthelf et al. (2000), [9]: Wang & Gotthelf (1998), [10]: Page et al. (2009), [11]: Becker et al. (2012), [12]: Zavlin et al. (2000), [13]: Sun et al. (2004). References to the braking indices included here are [14]: Weltevrede et al. (2011), [15]: Espinoza et al. (2011), [16]: Livingstone et al. (2006), [17]: Livingstone et al. (2011), [18]: Middleditch et al. (2006), [19]: Lyne et al. (1996), [20]: Olausen & Kaspi (2014).

Observed properties of NSs
PSR	P	\|$\dot{P}$\|	n	τ_PSR	SNR	τ_{SNR −}	τ_{SNR +}
	(s)	(10⁻¹¹ss⁻¹)		(kyr)		(kyr)	(kyr)
AXP 1E 1841−045	11.783	3.930		4.750	G27.4+0.0 (Kes 73)	0.750	2.100 [1]
AXP 1E 2259+586	6.979	4.843e − 2		228.317	G109.1−01.0 (CTB 109)	10.000	16.000 [2]
CXOU J171405.7−381031	3.825	6.400		0.947	G348.7+00.3	0.350	3.150 [3]
SGR 0526−66	8.054	3.800		3.358	N49	−	4.800 [4]
SGR 1627−41	2.595	1.900		2.164	G337.3−0.1	−	5.000 [5]
HBP J1119−6127	0.408	0.400	2.684 ± 0.002 [14]	1.616	G292.2−0.5	4.200	7.100 [6]
HBP J1734−3333	1.170	0.228	0.9 ± 0.2 [15]	8.131	G354.8−0.8	1.300	− [7]
HBP J1846−0258 A	0.325	0.709	2.64 ± 0.01 [16]	0.726	G029.7−0.3 (Kes 75)	0.900	4.300 [8]
HBP J1846−0258 B	0.327	0.711	2.16 ± 0.13 [17]	0.728
PSR J0537−6910	0.016	0.518	−1.5 ± 0.1 [18]	4.925	N157B	1.000	5.000 [9]
PSR B0833−45	0.089	1.250	1.4 ± 0.2 [19]	11.319	G263.9−03.3 (Vela)	5.400	16.000 [10]
RX J0822.0−4300	0.112	8.300e − 4		213.799	G260.4−3.4 (Puppis A)	3.700	5.200 [11]
1E 1207.4−5209	0.424	6.600e − 6		1.018e5	G296.5 +10.0 (PKS 1209−51/52)	2.000	20.000 [12]
CXOU J185238.6+004020	0.105	8.680e − 7		1.917e5	G033.6+00.1 (Kes 79)	5.400	7.500 [13]

Observed properties of NSs
PSR	P	\|$\dot{P}$\|	n	τ_PSR	SNR	τ_{SNR −}	τ_{SNR +}
	(s)	(10⁻¹¹ss⁻¹)		(kyr)		(kyr)	(kyr)
AXP 1E 1841−045	11.783	3.930		4.750	G27.4+0.0 (Kes 73)	0.750	2.100 [1]
AXP 1E 2259+586	6.979	4.843e − 2		228.317	G109.1−01.0 (CTB 109)	10.000	16.000 [2]
CXOU J171405.7−381031	3.825	6.400		0.947	G348.7+00.3	0.350	3.150 [3]
SGR 0526−66	8.054	3.800		3.358	N49	−	4.800 [4]
SGR 1627−41	2.595	1.900		2.164	G337.3−0.1	−	5.000 [5]
HBP J1119−6127	0.408	0.400	2.684 ± 0.002 [14]	1.616	G292.2−0.5	4.200	7.100 [6]
HBP J1734−3333	1.170	0.228	0.9 ± 0.2 [15]	8.131	G354.8−0.8	1.300	− [7]
HBP J1846−0258 A	0.325	0.709	2.64 ± 0.01 [16]	0.726	G029.7−0.3 (Kes 75)	0.900	4.300 [8]
HBP J1846−0258 B	0.327	0.711	2.16 ± 0.13 [17]	0.728
PSR J0537−6910	0.016	0.518	−1.5 ± 0.1 [18]	4.925	N157B	1.000	5.000 [9]
PSR B0833−45	0.089	1.250	1.4 ± 0.2 [19]	11.319	G263.9−03.3 (Vela)	5.400	16.000 [10]
RX J0822.0−4300	0.112	8.300e − 4		213.799	G260.4−3.4 (Puppis A)	3.700	5.200 [11]
1E 1207.4−5209	0.424	6.600e − 6		1.018e5	G296.5 +10.0 (PKS 1209−51/52)	2.000	20.000 [12]
CXOU J185238.6+004020	0.105	8.680e − 7		1.917e5	G033.6+00.1 (Kes 79)	5.400	7.500 [13]

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