Finding pulsars with LOFAR | Astronomy & Astrophysics (A&A)

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Table 3:

Name, declination (Dec), distance (d), dispersion measure (DM) observed or ⁺modeled after Taylor & Cordes (1993), core radius ( $r_{\rm c}$ ), collision number ( $\Gamma$ ) and number of detected pulsars (N) for the ten highest-ranking candidates for a LOFAR globular cluster survey.
Name	Dec	d	DM	$r_{\rm c}$	$\Gamma$	N
	deg	kpc	pc/cm³	arcmin
M15	+12	10.3	67.3	0.07	665	8
M92	+43	8.2	29⁺	0.23	106
M5	+02	7.5	30.0	0.42	79	5
M10	-04	4.4	43⁺	0.86	28
M13	+36	7.7	30.4	0.78	39	5
M3	+28	10.4	26.3	0.55	66	4
M2	-01	11.5	29⁺	0.34	120
M14	-03	9.3	76⁺	0.83	54
Pal 2	+31	27.6	97⁺	0.24	209
M12	-02	4.9	39⁺	0.72	10

Data from Harris (1996) and Freire (2008).

Source LaTeX | All tables | In the text

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