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Table 2.

X-rays, optical, and radio photometry of EP250207b.

X-rays

Mid-time Exposure Telescope Instrument Band Unabsorbed flux
(days) (ks) (keV) (10−14 erg cm−2 s−1)
0.71 3 EP FXT 0.3–10 28.0 ± 5.0
1.86 5 EP FXT 0.3–10 4.0 ± 1.0
2.5 9 EP FXT 0.3–10 3.2 ± 0.7
4.90 24 Chandra ACIS-S 0.3–10 0.4 ± 0.2

Optical/nIR

Mid-time Exposure Telescope Instrument Filter Magnitude
(days) (s) (AB)

4.31 480 GTC OSIRIS z > 23.8
7.42 2020 HST 1 WFC3 F606W 28.0 ± 0.5
7.42 2212 HST WFC3 F105W 26.6 ± 0.2
7.42 2212 HST WFC3 F125W 26.8 ± 0.3
8.74 2212 HST WFC3 F160W 27.1 ± 0.3
8.66 819 GTC EMIR J > 23.5
8.70 1461 GTC EMIR Ks > 23.7
9.16 462 GTC EMIR H > 24.0
11.27 1404 GTC EMIR Ks > 23.2
12.48 1800 LBT LBC r > 25.8
12.48 1800 LBT LBC i > 24.9
23.26 1800 VLT FORS2 i > 25.1
23.28 1800 VLT HAWKI Ks > 23.8

Radio

Mid-time Exposure Telescope Array Band Flux Density
(days) (h) (μJy)

4.40 0.50 VLA A 6.0 GHz < 21
7.41 0.67 VLA A −> D 6.0 GHz < 174
11.78 6.65 ATCA 6D 5.5 GHz < 39
11.78 6.65 ATCA 6D 9.0 GHz < 27
38.54 3.92 ATCA 6D 5.5 GHz < 45
38.54 3.92 ATCA 6D 9.0 GHz < 42
1

Notes. Magnitudes are corrected by Galactic Extinction. Upper limits correspond to a 3σ confidence level.

The magnitudes quoted in the table were obtained via image subtraction (Hu et al. 2022). The values derived from aperture photometry are (AB mag): F606W = 26.41 ± 0.09, F105W = 25.75 ± 0.13, F125W = 26.83 ± 0.08, F160W = 25.82 ± 0.11. In the second epoch, we estimate F606W = 26.90 ± 0.10, F105W = 26.59 ± 0.16, F125W = 26.67 ± 0.19, F160W = 26.29 ± 0.16.

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