Measuring Planck beams with planets | Astronomy & Astrophysics (A&A)

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Table 2:

Planck detector properties used for modeling.
Band	Sample rate	White noise	Knee for 1/f	Low-f	Bolometer	FWHM
(GHz)	(Hz)	( $\mu$ K s^-1/2)	(mHz)	index $\alpha$	$\tau$ (ms)	(arcmin)
Low-Frequency Instrument
30	32.5	170	50	1.7	...	32
44	46.5	200	50	1.7	...	20
70	78.8	270	50	1.7	...	13
High-Frequency Instrument
100	185	50	30	2	10.3	9.2
143	185	62	30	2	4.5	6.5
217	185	91	30	2	3.2	4.5
353	185	277	30	2	4.2	4.2
545	185	1998	30	2	1.5	4.2
857	185	91 000	30	2	1.9	4.0

The HFI sampling rate is approximate and subject to on-orbit tuning. Noise figures give values in CMB thermodynamic units. FWHM based on a Gaussian fit to the realistic beam models mentioned in text. References: Ashdown et al. (2009); Holmes et al. (2008); Planck Collaboration (2006).

Source LaTeX | All tables | In the text

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