Searching for anomalous microwave emission in nearby galaxies - K-band observations with the Sardinia Radio Telescope

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Volume 658 (February 2022)

A&A, 658 (2022) L8

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Table A.1.

Data of Fig. 4 and Fig. 5.

names	distance^a		S_1.4GHz	T_d	M_d	M_⋆	SFR
	Mpc		Jy	K	M_⊙	M_⊙	M_⊙ yr⁻¹
NGC 3627	11.5	< 2.3 × 10⁻⁴^c	0.50 ± 0.01^h	25.3±0.8^m	2.9 ± 0.3 × 10⁷	6.7 ± 1.2 × 10¹⁰	2.9 ± 1.0
NGC 4254	12.9	< 3.1 × 10⁻⁴^c	0.51 ± 0.02^h	24.3±0.8^m	2.6 ± 0.2 × 10⁷	1.3 ± 0.2 × 10¹⁰	5.1 ± 0.5
NGC 4736	4.4	< 1.8 × 10⁻⁴^c	0.295 ± 0.005^h	26±1^m	2.7 ± 0.4 × 10⁶	2.5 ± 0.4 × 10¹⁰	0.55 ± 0.19
NGC 5055	9.0	< 2.2 × 10⁻⁴^c	0.460 ± 0.005^h	21.3±0.7^m	4.7 ± 0.5 × 10⁷	5.9 ± 1.1 × 10¹⁰	2.5 ± 0.7

MW	-	3.4 ± 0.3 × 10⁻⁴^d	-	18.3 ± 0.3ⁿ	-	-	-
LMC	0.05^b	1.4 ± 0.2 × 10⁻⁴^d	530 ± 30ⁱ	21.1 ± 0.4^o	1.5 ± 0.1 × 10⁶	2.0 ± 0.5 × 10⁹^q	0.4 ± 0.2
SMC	0.062^b	7.5 ± 2.4 × 10⁻⁵^d	42 ± 6ⁱ	20.2 ± 0.8^o	2.6 ± 0.4 × 10⁵	3.2 ± 0.8 × 10⁹^q	0.015 ± 0.010
M 31	0.79^b	4.2 ± 0.6 × 10⁻⁴^e	5.2 ± 0.4^j	17.3 ± 0.1^o	3.1 ± 0.1 × 10⁷	5.5 ± 0.1 × 10¹⁰^r	0.2 ± 0.1^s
M 33	0.04^b	< 3.5 × 10⁻⁵^f	2.7 ± 0.6^k	18.9 ± 0.3^o	5.6 ± 0.4 × 10⁶	4.5 ± 1.5 × 10⁹^t	0.25 ± 0.10^u
NGC 253	3.7	< 3.1 × 10⁻⁵^g	6.2 ± 0.1^l	26.2 ± 0.2^p	3.3 ± 0.1 × 10⁷	7.6 ± 0.8 × 10¹⁰^v	5.8 ± 0.8
NGC 3034	3.6	< 4.0 × 10⁻⁵^g	8.4 ± 0.3^l	35 ± 1^p	6.6 ± 0.5 × 10⁶	1.3 ± 0.3 × 10¹⁰^w	4.5 ± 0.6
NGC 4945	3.5	< 4.2 × 10⁻⁵^g	6.4 ± 0.2^l	26.4 ± 0.4^m	2.1 ± 0.3 × 10⁷	1.4 ± 0.6 × 10¹⁰	6.5 ± 3.6

Notes.

Unless otherwise specified, distances are from the DustPedia database, available at http://dustpedia.astro.noa.gr/.

From Clark et al. (2021).

From this work and the HerschelS_3THz in DustPedia.

Estimated at 22.8 GHz in PLA16.

Estimated at 30 GHz in Battistelli et al. (2019).

From the upper limit of Tibbs et al. (2018) at 30 GHz and S_3THz in Clark et al. (2021).

From the upper limit of P11 between 23 and ≈100 GHz and HerschelS_3THz in DustPedia, with the exception of NGC 3034, for which S_3THz was estimated from the SED fit.

T17; for NGC 3627 we used S_{1.36 GHz}.

ⁱ

For et al. (2018).

Battistelli et al. (2019).

Tibbs et al. (2018).

P11.

T_d and M_d from FIR-submm MBB fits, M_⋆ and SFR from optical-to-submm fits (Nersesian et al. 2019).

ⁿ

This work; MBB fits of the MW diffuse dust emissivity for 100 ≤ λ/ μm ≤ 850 from Hensley & Draine (2021).

This work; T_d and M_d from MBB fits of Herschel flux densities from Clark et al. (2021).

This work; T_d and M_d from MBB fits of Herschel flux densities in DustPedia.

M_⋆ and SFR from Skibba et al. (2012).

Viaene et al. (2014).

Viaene et al. (2017).

Corbelli (2003).

Williams et al. (2019).

M_⋆ and SFR from de los Reyes & Kennicutt (2019).

M_⋆ and SFR from Nersesian et al. (2019).

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