Table:
text: List of astronomical interferometers at visible and infrared wavelengths
Current performance of ground-based interferometers
Current Performance of Existing Astronomical Interferometers
Interferometer_and_observing_mode Waveband Limiting_magnitude Minimum_baseline_m_un_projected Maximum_baseline_m Approx_no_visibility_measurements_per_year_measurements_per_night_x_nights_used_per_year Max_ratio_of_no_phase_no_amplitude_measurements_measure_of_imaging_performance_0_is_none Accuracy_of_amplitude2_measurements Accuracy_of_phase_measurements_milli_radians Number_of_spectral_channels_max_in_use_simultaneously Comments_
CHARA Array V, R, I, J, H, K 8 34 330 7500 0.7 1% 10 30000 Yes... 30000 in the visible band; maxiumum baseline 330-m
COAST visible R, I 7 4 60 2000 0.5 4% 10 4? 300 cloudy nights per year, maximum baseline 100-m
COAST infrared J, H 3 4 60 100 0.5 20% 10 1 300 cloudy nights per year, maximum baseline 100-m
GI2T visible R, I 5 10 65 2000 0 10% - 400? CLOSED in 2006
IOTA J, H, K 7 6 30 10000 0.3 2% 10 1? Integrated optics beam combiner. CLOSED.

Question: What has a limiting magnitude higher than visible coastal light, chara array, or coastal infrared among the list of astronomical interferometers at visible and infrared wavelengths?