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Table 3.
Contents of the SMC source catalog.
Column | Name | Description |
---|---|---|
1 | ID | Index |
2 | RA(J2000) | Right Ascension, J2000 (deg) |
3 | Dec(J2000) | Declination, J2000 (deg) |
4−9 | 2MASS_J, ..., e_2MASS_KS | 2MASS photometries with uncertainties (mag) |
10−19 | IRAC1, ..., e_MIPS24 | Spitzer photometries with uncertainties (mag) |
20−27 | WISE1, ..., e_WISE4 | WISE photometries with uncertainties (mag) |
28−33 | Gaia_parallax, ..., e_Gaia_pmdec | Gaia DR2 astrometric solutions with uncertainties (mas; mas/yr) |
34−36 | Gaia_G, ..., Gaia_RP | Gaia DR2 mean magnitudes (mag) |
37−38 | Gaia_RV, e_Gaia_RV | Gaia DR2 radial velocity with uncertainty (km s−1) |
39−44 | VMC_Y, ..., e_VMC_KS | VMC photometries with uncertainties (mag) |
45−50 | IRSF_J, ..., e_IRSF_KS | IRSF photometries with uncertainties (mag) |
51−62 | AKARI_N3, ..., e_AKARI_L24 | AKARI photometries with uncertainties (mag) |
63−72 | HERITAGE_f70, ..., e_HERITAGE_f350 | HERITAGE fluxes with uncertainties (mJy) |
73−84 | SkyMapper_u, ..., e_SkyMapper_z | SkyMapper photometries with uncertainties (mag) |
85−96 | NSC_u, ..., e_NSC_Y | NSC photometries with uncertainties (mag) |
97−104 | M2002_V, ..., e_M2002_V_R | M2002 photometries with uncertainties (mag) |
105−108 | GALEX_FUV, ..., e_GALEX_NUV | GALEX photometries with uncertainties (mag) |
109 | B2011_SAGE_Class | IR color classifications from Boyer et al. (2011) |
110 | S2013_YSO | YSO classifications from Sewiło et al. (2013) |
111 | R2015_IRS_Class | MIR spectral classifications from Ruffle et al. (2015) |
112 | B2010_MK_Class | Optical spectral classifications from Bonanos et al. (2010) |
113−115 | GF2015_MK_SpVar, ..., GF2015_MK_Class | Optical spectral classifications from González-Fernández et al. (2015) (km s−1) |
116−117 | N2018_RV, N2018_MK_Class | Optical spectral classifications from Neugent et al. (2018) (km s−1) |
118−121 | Simbad_RV, ..., Simbad_Other_Types | Simbad classifications (km s−1) |
122−127 | Median_WISE1, ..., Amp_WISE1 | WISE1-band variability statistics (mag) |
128−133 | Median_WISE2, ..., Amp_WISE2 | WISE2-band variability statistics (mag) |
134−137 | Median_IRAC1, ..., Amp_IRAC1 | IRAC1-band variability statistics (mag) |
138−141 | Median_IRAC2, ..., Amp_IRAC2 | IRAC2-band variability statistics (mag) |
142−145 | Median_VMC_Y, ..., Amp_VMC_Y | VMC Y-band variability statistics (mag) |
146−149 | Median_VMC_J, ..., Amp_VMC_J | VMC J-band variability statistics (mag) |
150−153 | Median_VMC_KS, ..., Amp_VMC_KS | VMC KS-band variability statistics (mag) |
154 | VMC_Type | VMC variable classifications |
155−158 | Median_IRSF_J, ..., Amp_IRSF_J | IRSF J-band variability statistics (mag) |
159−162 | Median_IRSF_H, ..., Amp_IRSF_H | IRSF H-band variability statistics (mag) |
163−166 | Median_IRSF_KS, ..., Amp_IRSF_KS | IRSF KS-band variability statistics (mag) |
167−170 | Median_Gaia_G, ..., Amp_Gaia_G | GaiaG-band variability statistics (mag) |
171−174 | Median_Gaia_BP, ..., Amp_Gaia_BP | GaiaBP-band variability statistics (mag) |
175−178 | Median_Gaia_RP, ..., Amp_Gaia_RP | GaiaRP-band variability statistics (mag) |
179−180 | Best_Class_Gaia, Best_Class_Score_Gaia | Gaia variable classifications |
181−184 | Median_NSC_u, ..., Amp_NSC_u | NSC u-band variability statistics (mag) |
185−188 | Median_NSC_g, ..., Amp_NSC_g | NSC g-band variability statistics (mag) |
189−192 | Median_NSC_r, ..., Amp_NSC_r | NSC r-band variability statistics (mag) |
193−196 | Median_NSC_i, ..., Amp_NSC_i | NSC i-band variability statistics (mag) |
197−200 | Median_NSC_z, ..., Amp_NSC_z | NSC z-band variability statistics (mag) |
201−204 | Median_NSC_Y, ..., Amp_NSC_Y | NSC Y-band variability statistics (mag) |
205−214 | OGLE_LPV_Type, ..., OGLE_LPV_Iamp3 | OGLE long period variables statistics (mag) |
215−225 | OGLE_CCep_Mode, ..., OGLE_CCep_phi31 | OGLE classical Cepheids statistics (mag) |
226−236 | OGLE_T2Cep_Type, ..., OGLE_T2Cep_phi31 | OGLE Type II Cepheids statistics (mag) |
237−243 | OGLE_Ecl_Type, ..., OGLE_Ecl_DS | OGLE eclipsing binaries statistics (mag) |
Notes. This table is available in its entirety in CDS.
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