Wide-band simultaneous observations of pulsars: disentangling dispersion measure and profile variations

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Table 7

Parameters of the models used in the dynamic templates.

PSR B0329+54
Component 1	Position	−ν^-0.22
	Amplitude	ν^-0.018
	Width	1.7°
Component 2	Position	ν^-0.022
	Amplitude	ν^0.48
	Width	2.4°
Component 3^a	Position	ν⁰
	Amplitude	ν⁰
	Width	1.8°
Component 4	Position	−ν^0.015
	Amplitude	ν^0.022
	Width	2.4°
Component 5	Position	ν^1.5
	Amplitude	ν^0.48
	Width	1.2°

PSR B0809+74
Component 1	Position	ν^-0.43
	Amplitude (<100 MHz)	−ν^-0.055
	Amplitude (>100 MHz)	−ν^0.013
	Width	14.9°
Component 2^a	Position	ν⁰
	Amplitude	ν⁰
	Width	7.7°

PSR B1133+16
Component 1	Position	ν^-0.62
	Amplitude	ν^-3.28
	Width	ν^-3.55
Component 2^a	Position	ν⁰
	Amplitude	ν⁰
	Width	3.2°
Component 3	Position	ν^-0.62
	Amplitude	ν^-3.11
	Width	ν^-3.98

PSR B1919+21^b
Component 1	Width	ν^0.04
Component 2	Width	−ν^0.01
Separation		ν^0.05
Ratio of Peaks	ν < 100 MHz	ν^-0.07
	100 MHz < ν < 300 MHz	ν^0.54
	ν > 300 MHz	1.2

Notes. The functions given are appropriate for frequencies measured in MHz, and pulse phase measured in degrees. Component brightnesses are defined relative to a fiducial component.

^(a)

Component used as the fiducial component.

^(b)

Midpoint between components used as fiducial point.

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