Table 1
IR data from VO archives used to build the SEDs.
| Survey | Facility/instrument (filters)(c) | Quality flags |
|---|---|---|
| 2MASS | 2MASS (J, H, Ks) | Qflg ∈ (A, B, C, D) |
| UKIDSS | UKIRT/WFCAM (J, H, K) | |ppErrBits| < 256 |
| VISTA | Paranal/VIRCAM (J, H, Ks) | |ppErrBits| < 256 |
| WISE | WISE (W1, W2) | – |
| Spitzer | IRAC (I1, I2, I3, I4) MIPS (24 µm, 70 µm, 160 µm) | (a)q = 0 or (b)n = 0 |
Notes. The catalogues used from each survey were: i) 2MASS: 2MASS All-Sky Catalog of Point Sources; ii) UKIDSS: Large Area Survey (LAS) DR10, Galactic Clusters Survey (GCS) DR10, Galactic Plane Survey (GPS) DR7, Deep Extragalactic Survey (DXS) DR10; iii) VISTA: VISTA Variables in the Via Lactea (VVV) DR5, VISTA Kilo-Degree Infrared Galaxy (VIKING) DR4, VISTA Hemisphere Survey (VHS) DR6, VISTA Magellanic Survey (VMS) DR4; iv) WISE: CatWISE2020 (Marocco et al. 2021); v) Spitzer: (a)Galactic Legacy Infrared Midplane Survey Extraordinaire (GLIMPSE) I, II & 3D, (b)The Spitzer Enhanced Imaging Products (SEIP) source list. (c)Detailed information on the mentioned filters can be found at the SVO Filter Profile Service “Carlos Rodrigo”5 (Rodrigo et al. 2024).
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