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Table 1

Photometry, including non-detections, used to construct the SED of BLG-360.

MJD Instrument Filter λc (μm) Flux1 (Jy)
59 564 ASAS-SN g 0.46 <0.0013
58 270 ASAS-SN V 0.55 <0.0013
59 421 SkyMapper i 0.77 <5.8 × 10−6
59 421 SkyMapper z 0.91 <1.2 × 10−5
58 304 Keck-NIRC2 Ks 2.15 (3.94 ± 0.40) × 10−4
59 506 Gemini+NIRI Ks 2.15 <1.6 × 10−5
59 571 NEOWISE2 W1 3.40 (1.46 ± 0.03) × 10−2
59 506 Gemini+NIRI L′ 3.77 0.071 ± 0.008
59 571 NEOWISE2 W2 4.60 0.32 ± 0.020
59 508 Gemini+NIRI M′ 4.68 0.41 ± 0.075
59 403 FORCAST F056 5.61 1.22 ± 0.09
59 403 FORCAST F064 6.35 2.00 ± 0.13
59 403 FORCAST F077 7.72 4.60 ± 0.27
59 403 FORCAST F088 8.64 4.68 ± 0.28
59 403 FORCAST F111 11.01 2.69 ± 0.18
57 935 COMICS N12.4 12.40 5.43 ± 0.28
59 403 FORCAST F197 19.70 7.29 ± 0.44
59 403 FORCAST F253 25.24 5.81 ± 0.37
59 403 FORCAST F315 31.36 6.58 ± 0.44
59 403 FORCAST F336 33.57 3.65 ± 0.41
59 403 FORCAST F348 34.64 7.76 ± 0.52
59 403 FORCAST F371 36.98 6.44 ± 0.43
59 739 HAWC+ Band A 53.0 3.22 ± 0.45
59 739 HAWC+ Band C 89.0 2.11 ± 0.46
59 739 HAWC+ Band D 154.0 0.49 ± 0.13
59 739 HAWC+ Band E 214.0 0.67 ± 0.15
59 715 ACA Band 7 867 0.034 ± 0.001
58 304 SMA 230 GHz 1273 0.012 ± 0.005
59 154 VLASS 3 GHz 105 <7.72 × 10−4
58 795 ASKAP 1.37 GHz 2.19e5 <1.30 × 10−3
59 228 ASKAP 0.89 GHz 3.37e5 <1.95 × 10−3

Notes. 1Non-detection fluxes are given as 5σ upper limits, where σ is the root-mean-square noise in a region where BLG-360 should be observed. We refer to the flux errors as 1σ uncertainties. 2These fluxes were obtained using interpolation between observations epochs to match the MJD mid-point between the SOFIA FORCAST and HAWC+ observations epochs.

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