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Table 3.

Photometry data for NGC 4593.

Observed band Flux Significance Systematic error (%) Ref.
Swift (2–10 keV) 3.16 × 10−11 erg cm−2 s−1 No uncertainty reported 10% (1)
Swift (14–195 keV) 3.4 × 10−10 erg cm−2 s−1 90% confidence 10% (1)
GALEX (FUV) 3.60 ± 0.05 mJy 1σ 5% (2)
GALEX (NUV) 5.91 ± 0.03 mJy 1σ 5% (2)
2MASS (J) 415.00 ± 7.71 mJy 1σ 2% (3)
2MASS (H) 494.00 ± 10.20 mJy 1σ 2% (3)
2MASS (Ks) 427.00 ± 12.40 mJy 1σ 2% (4)
IRAC (3.6 μm) 125.00 ± 8.03 mJy 1σ 5% (5)
IRAC (4.5 μm) 134.00 ± 21.00 mJy 1σ 5% (5)
IRAC (5.8 μm) 163.00 ± 23.95 mJy 1σ 5% (5)
IRAC (8.0 μm) 229.00 ± 33.16 mJy 1σ 5% (6)
IRAS (12 μm) 299.00 ± 73.00 mJy Uncertainty, confidence not specified 10% (7)
Spitzer MIPS (24 μm) 633.00 ± 89.00 mJy No uncertainty reported 10% (5)
ALMA (Band 6) 8.13 ± 0.22 mJy 1σ 10% (8)
ALMA (Band 3) 8.42 ± 0.06 mJy 1σ 10% (8)

Notes. This table presents the photometry data for NGC 4593 across a range of observed bands, including X-ray, UV, near-infrared, and mid-infrared wavelengths. Flux values are given in units of mJy, except for the Swift X-ray data, which are expressed in erg cm−2 s−1. The uncertainties listed in the flux column correspond to the statistical errors of the measurements. The significance column denotes the confidence level associated with the data, while the systematic error indicates the potential percentage uncertainty due to instrumental calibration or observational conditions.

(1) Ricci et al. (2017b); (2) Bouquin et al. (2018); (3) McAlary et al. (1983); (4) Jarrett et al. (2003); (5) Skrutskie et al. (2006); (6) Cutri et al. (2012); (7) Tommasin et al. (2010); (8) Obtained in this work based on ALMA observation project IDs: 2017.1.00236.S and 2018.1.00576.S.

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