A census of the pulsar population observed with the international LOFAR station FR606 at low frequencies (25–80 MHz)

Open Access

Table A.1.

Pulsars that were not detected in this census.

J2000	Discovery	P0	DM	/P0	Duration	elev	Upper limit for the
name	name	s	pc.cm⁻³	%	min	degree	mean flux density [mJy]
J0117+5914	B0114+58	0.1014	49.4230	95.3	255	64	344 ^(τ)
J0139+5814	B0136+57	0.2725 ^(ϵ)	73.7790	172.6	225	63	366 ^(τ)
J0231+7026	B0226+70	1.4668 ^(ϵ)	46.6400	5.3	240	45	329
J0304+1932	B0301+19	1.3876 ^(ϵ)	15.7370	0.1	240	53	121
J0324+5239	J0324+5239	0.3366	119.0000	984.6	240	56	281 ^(τ)
J0415+6954	B0410+69	0.3907^ϵ	27.4650	2.9	360	44	253
J0534+2200	B0531+21	0.0334	56.7875	497.4	60	43	705^(η),(τ)
J0543+2329	B0540+23	0.2460 ^(ϵ)	77.7115	235.8	120	61 ^(τ)	428 ^(τ)
J0612+3721	B0609+37	0.2980 ^(ϵ)	27.1350	3.7	110	42	664
J0614+2229	B0611+22	0.3350 ^(ϵ)	96.9100	426.0	240	61	337 ^(τ)
J0629+2415	B0626+24	0.4766 ^ϵ	84.1950	168.4	180	48	540 ^(τ)
J0653+8051	B0643+80	1.2144 ^(ϵ)	33.3320	1.8	240	56	316
J0659+1414	B0656+14	0.3849 ^(ϵ)	13.9770	0.4	240	53	77
J0921+6254	B0917+63	1.5680 ^(ϵ)	13.1580	0.1	275	51	58
J0943+1631	B0940+16	1.0874 ^(ϵ)	20.3200	0.4	115	58	430
J0943+22	J0943+22	0.5329	25.1000	1.6	360	65	24
J0947+27	J0947+27	0.8510 ^(ϵ)	29.0000	1.6	220	65	1344
J1503+2111	J1503+2111	3.3140	3.2600	0.0	360	48	57
J1612+2008	J1612+2008	0.4266	19.5440	0.9	240	56	298
J1627+1419	J1627+1419	0.4909	33.8000	4.8	180	55	415
J1649+2533	J1649+2533	1.0153 ^(ϵ)	35.5000	2.8	240	64	303
J1720+2150	J1720+2150	1.6157	41.1000	3.0	240	57	292
J1740+1000	J1740+1000	0.1541 ^(ϵ)	23.8500	4.6	120	43	501
J1752−2806	B1749−28	0.5626	50.3720	18.5	60	14	4533
J1841+0912	B1839+09	0.3813 ^(ϵ)	49.1070	24.8	120	50	521
J1851−0053	J1851−0053	1.4091	24.0000	0.5	240	38	578
J1907+4002	B1905+39	1.2358 ^(ϵ)	30.9600	1.4	250	53	262
J1908+0734	J1908+0734	0.2124	11.1040	0.4	360	45	203
J1933+2421	B1931+24	0.8137	105.9251	252.3	120	64	468^(τ)
J1946+1805	B1944+17	0.4406 ^(ϵ)	16.2200	0.5	120	59	110
J1948+3540	B1946+35	0.7173	129.0750	646.7	120	77	391^(τ)
J1954+2923	B1952+29	0.4267 ^(ϵ)	7.9320	0.1	115	54	124
J2043+2740	J2043+2740	0.0961 ^(ϵ)	21.0000	4.9	115	56	425
J2055+2209	B2053+21	0.8152 ^(ϵ)	36.3610	3.8	120	64	419
J2139+2242	J2139+2242	1.0835	44.1000	5.8	115	57	427
J2149+6329	B2148+63	0.3801 ^(ϵ)	128.0000	1178.8	120	72	1798^(τ)
J2157+4017	B2154+40	1.5253 ^(ϵ)	70.8570	26.2	180	36	399
J2229+6205	B2227+61	0.4431	124.6140	905.6	180	47	400^(τ)

Notes. J2000 name, discovery name: pulsar name. P0: pulsar period. DM: the DM used to coherently disperse the observations from Zakharenko et al. (2013) Stovall et al. (2015) and Bilous et al. (2016), and ATNF to complete. /P0 : the scattering time (estimated using YMW16 Yao et al. (2017) at 60 MHz) divided by the pulsar period. Duration: total duration of the observation in minutes. elev: the average elevation of the observation. Upper limit for the mean flux: the upper limit for the mean flux density 1. ^η: excluding the contribution of the nebula to T_sky. ^τ: upper limit for the mean flux density is not valid (/P0 > 100%). ^ϵ: the file is folded using an ephemeris file from either Jodrell Bank Observatory or Nançay Radio Observatory (see Sect. 3.3).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.