Open Access

Table B.2.

HST-ACS/WFC3, JWST-NIRCam and JWST-MIRI photometric data of the FXT XT2.

Telescope Instrument Filter AB mag. Flux (μJy)
(1) (2) (3) (4) (5)
Blanco MOSAIC II U > 26.63 > 0.081
VLT VIMOS U > 27.97 > 0.024
HST ACS F435W 26.58 ± 0.34 0.085 ± 0.027
HST ACS F606W 25.64 ± 0.21 0.201 ± 0.039
HST ACS F775W 24.99 ± 0.24 0.366 ± 0.079
HST ACS F814W 24.97 ± 0.15 0.372 ± 0.050
HST ACS F850LP 25.21 ± 0.35 0.301 ± 0.096
HST WFC3 F105W 24.99 ± 0.37 0.367 ± 0.126
HST WFC3 F125W 24.38 ± 0.17 0.642 ± 0.102
HST WFC3 F140W 24.4 ± 0.42 0.632 ± 0.246
HST WFC3 F160W 24.0 ± 0.14 0.910 ± 0.119

JWST NIRCam F090W 24.85 ± 0.03 0.418 ± 0.012
JWST NIRCam F115W 24.51 ± 0.02 0.570 ± 0.012
JWST NIRCam F150W 24.01 ± 0.01 0.903 ± 0.011
JWST NIRCam F200W 23.26 ± 0.01 1.803 ± 0.011
JWST NIRCam F277W 22.49 ± 0.01 3.652 ± 0.009
JWST NIRCam F335M 22.46 ± 0.01 3.753 ± 0.013
JWST NIRCam F356W 22.37 ± 0.01 4.089 ± 0.007
JWST NIRCam F410M 22.08 ± 0.01 5.359 ± 0.010
JWST NIRCam F444W 21.91 ± 0.0 6.255 ± 0.009

JWST MIRI F770W 21.38 ± 0.01 10.194 ± 0.094
JWST MIRI F1280W 21.65 ± 0.01 7.909 ± 0.073
JWST MIRI F1500W 21.38 ± 0.01 10.177 ± 0.094

Notes. Data were taken from Eisenstein et al. (2023b), while the VLT and Blanco data are the 5σ magnitude limit for the U−band photometry of Guo et al. (2013).

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