Table A.2.
Sample of bona fide stellar sources with a period analysis based on WISE data, period information (first entries).
| Ra | Dec | Periods literature | P refit | P1 | σP1 | P2 | σP2 | Amp1 | σA1 | W1 | σW1 |  |
Amp2 | σA2 | W2 | σW2 |  |
Com | Class | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (deg) | (deg) | (d) | (d) | (d) | (d) | (d) | (d) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | |||||
| 19.463942 | 67.231448 | 1060 (24) | 1053 | 4.1 | 1042 | 4.2 | 1.85 | 0.13 | 8.874 | 0.019 | 139.9 | 1.52 | 0.05 | 4.767 | 0.026 | 2.2 | ERO LPV | |||
| 124.826307 | -21.737399 | 944 | 7.4 | 937 | 5.8 | 1.52 | 0.09 | 7.251 | 0.059 | 50.0 | 1.39 | 0.08 | 3.811 | 0.047 | 2.1 | ERO LPV | ||||
| 237.773837 | -56.890007 | no (8) 453 (3) | 925 ± 3 (43) | 942 | 7.6 | 974 | 11.4 | 1.43 | 0.09 | 7.321 | 0.057 | 42.6 | 1.49 | 0.15 | 3.718 | 0.061 | 4.2 | ERO LPV | ||
| 287.486914 | 9.447611 | 1068 | 8.9 | 1075 | 9.7 | 1.19 | 0.06 | 6.144 | 0.078 | 9.7 | 1.55 | 0.12 | 2.496 | 0.062 | 1.9 | ERO LPV | ||||
| 323.345002 | 56.743063 | 924 | 4.3 | 962 | 9.6 | 1.14 | 0.04 | 7.390 | 0.022 | 40.1 | 1.51 | 0.14 | 3.700 | 0.066 | 7.0 | ERO LPV | ||||
| 349.802533 | 17.192628 | 696. (28) 520? (26) 700. (22) | 747 | 4.6 | 705 | 674.4 | 0.89 | 0.04 | 5.283 | 0.032 | 1.7 | 0.63 | 2.01 | 1.813 | 2.042 | 6.0 | ERO LPV | |||
| 89.161446 | -67.892776 | 1197 ± 32 (1) 1209 (2) | 1223 | 1.2 | 1217 | 1.3 | 1.24 | 0.04 | 11.978 | 0.003 | 37.3 | 1.02 | 0.05 | 8.971 | 0.002 | 80.4 | ERO LPV | |||
| 82.407959 | -72.831322 | 680 (2) | 679 | 1.0 | 677 | 1.1 | 0.62 | 0.01 | 14.119 | 0.008 | 7.9 | 0.61 | 0.02 | 10.709 | 0.006 | 38.6 | ERO LPV | |||
| 87.608788 | -69.934212 | 1052 (2) | 1104 | 4.1 | 1113 | 2.6 | 0.65 | 0.01 | 15.485 | 0.012 | 2.8 | 0.72 | 0.03 | 11.466 | 0.005 | 35.4 | ERO LPV | |||
| 79.701599 | -69.559563 | no (2) | 0.00 | 0.00 | 15.307 | 0.070 | 0.3 | 0.00 | 0.00 | 12.700 | 0.015 | 10.2 | ERO | |||||||
| 87.249886 | -70.556229 | no (2) | 4453 | 1288 | 3429 | 98.6 | 0.06 | 0.05 | 15.502 | 0.011 | 2.1 | 0.12 | 0.01 | 13.502 | 0.007 | 1.6 | ERO | |||
| 75.631233 | -68.093285 | no (2) | 1739 | 111.8 | 1890 | 20.7 | 0.76 | 0.26 | 15.662 | 0.125 | 19.8 | 0.31 | 0.02 | 13.074 | 0.007 | 4.4 | ERO LPV | |||
| 76.023376 | -68.394501 | no (2) | 0.00 | 0.00 | 16.213 | 0.140 | 0.2 | 0.00 | 0.00 | 13.194 | 0.007 | 4.5 | ERO | |||||||
| 81.419411 | -70.140877 | no (2) | 0.00 | 0.00 | 15.703 | 0.351 | 4.4 | 0.00 | 0.00 | 13.313 | 0.016 | 5.2 | ERO | |||||||
| 78.257469 | -69.564110 | no (2) | 9094 | 3214 | 0.00 | 0.00 | 15.547 | 0.087 | 0.1 | 0.28 | 0.15 | 13.871 | 0.046 | 1.2 | ERO | |||||
| 79.548790 | -70.507469 | no (2) | 8188 | 2519 | 4666 | 81.4 | 0.63 | 0.34 | 14.815 | 0.285 | 2.5 | 0.48 | 0.01 | 11.941 | 0.004 | 4.2 | ERO LPV | |||
| 82.684006 | -71.716766 | no (2) | 969 | 16.4 | 944 | 13.8 | 0.05 | 0.02 | 13.812 | 0.004 | 2.8 | 0.04 | 0.00 | 11.957 | 0.003 | 2.4 | ERO | |||
| 281.468597 | -1.778703 | 1140 ± 30 (31) | 1176 | 43.1 | 1125 | 17.4 | 1.05 | 0.10 | 5.754 | 0.184 | 31.7 | 1.35 | 0.10 | 2.518 | 0.106 | 0.5 | LPV | |||
| 282.174774 | -2.841357 | 2013 ± 243 (32) 1730 ± 200 (31) 2173 (30) | 1952 | 45.9 | 1524 | 16.8 | 0.67 | 0.06 | 7.430 | 0.031 | 8.0 | 0.88 | 0.08 | 2.966 | 0.053 | 1.3 | LPV | |||
| 282.859344 | -1.064581 | 1417 ± 108 (32) 1519 (30) no (4) | 1632 | 14.0 | 1605 | 21.6 | 0.89 | 0.07 | 7.506 | 0.060 | 9.0 | 1.34 | 0.12 | 3.400 | 0.068 | 2.5 | LPV | |||
| 283.092775 | -0.236713 | 1539 ± 31 (32) 1750 ± 130 (31) 1691 (30) no (4) | 1436 | 32.6 | 1666 | 25.8 | 0.67 | 0.07 | 7.296 | 0.048 | 10.5 | 1.32 | 0.13 | 2.694 | 0.087 | 2.8 | LPV | |||
| 287.284637 | 8.276116 | 2475 | 69.6 | 1976 | 51.4 | 0.68 | 0.09 | 7.659 | 0.056 | 73.0 | 0.88 | 0.15 | 4.566 | 0.100 | 5.0 | LPV | ||||
| 23.463343 | 62.448162 | 759 (12) 1540 ± 16 (21) 1638 ± 57 (32) 1592 (30) | 0.00 | 0.00 | 3.864 | 0.024 | 2.1 | 0.00 | 0.00 | 1.445 | 0.054 | 0.5 | ||||||||
| 53.377491 | 60.335957 | 1800 ± 400 (25) 2210 (30) | 1445 | 45.2 | 1833 | 293.3 | 0.62 | 0.09 | 4.502 | 0.097 | 2.4 | 0.33 | 0.29 | 2.418 | 0.152 | 5.7 | LPV | |||
| 79.197746 | 45.567860 | 1100 ± 100 (25) 1051 (30) | 1182 | 16.0 | 1133 | 35.3 | 1.05 | 0.09 | 4.439 | 0.057 | 2.0 | 0.72 | 0.16 | 2.404 | 0.099 | 3.6 | LPV | |||
| 111.101738 | -20.198791 | 5746/1411 (6) 1200 ± 200 (25) 7 (4) | 1447 | 24.3 | 1488 | 21.0 | 0.62 | 0.10 | 4.016 | 0.104 | 0.8 | 1.09 | 0.11 | 2.999 | 0.082 | 3.8 | LPV | |||
| 266.099701 | -31.927624 | 1440: (25) 1440 (33) 1 (3) | 1766 ± 47 (43) | 2054 | 58.6 | 0.72 | 0.11 | 4.086 | 0.134 | 0.8 | 0.00 | 0.00 | 0.708 | 0.106 | 0.0 | 1 | PER | |||
| 280.309784 | -6.250149 | 1172 ± 94 (32) 1330 ± 50 (31) | 1372 | 22.3 | 1206 | 66.3 | 0.62 | 0.09 | 4.485 | 0.120 | 0.4 | 0.48 | 0.16 | 2.468 | 0.132 | 2.4 | LPV | |||
| 277.128905 | -9.970644 | 1785 ± 114 (32) | 1548 | 96.5 | 1702 | 67.1 | 1.59 | 0.19 | 8.564 | 0.142 | 99.5 | 1.64 | 0.15 | 3.848 | 0.075 | 3.4 | LPV | |||
| 51.285198 | 65.535362 | 1276 ± 150 (32) 1410 (30) | 1431 | 26.2 | 1300 | 77.7 | 0.53 | 0.05 | 4.075 | 0.059 | 0.8 | 0.30 | 0.12 | 2.009 | 0.103 | 1.5 | LPV | |||
| 0.441592 | 62.748863 | 731 | 1.5 | 720 | 3.8 | 1.02 | 0.03 | 5.201 | 0.015 | 0.9 | 1.06 | 0.07 | 3.209 | 0.036 | 2.5 | LPV | ||||
| 3.853554 | 54.906147 | 613 | 6.4 | 627 | 6.4 | 0.46 | 0.04 | 3.738 | 0.033 | 0.6 | 0.59 | 0.12 | 2.268 | 0.079 | 2.9 | LPV | ||||
| 4.963700 | 65.991821 | 0.00 | 0.00 | 3.746 | 0.037 | 2.8 | 0.00 | 0.00 | 2.475 | 0.047 | 3.1 | nvoh |
Notes. References for Cols. 3-4: (1) = Groenewegen et al. (2020), (2) = Groenewegen & Sloan (2018), (3) = Ferreira Lopes et al. (2020), (4) = Shappee et al. (2014), Kochanek et al. (2017), (5) = Gaia Collaboration (2018), (6) = Heinze et al. (2018), (7) = Price et al. (2010), (8) = Whitelock et al. (2006), (9) = Pojmanski (2002), (10) = Contreras Peña et al. (2017) (11) = Alfonso-Garzón et al. (2012) (12) = Urago et al. (2020) (13) = Woźniak et al. (2004) (14) = Drake et al. (2009) (20) = Kiss et al. (2007) (21) = Suh & Kim (2002) (22) = Whitelock et al. (1994) (23) = Kerschbaum et al. (2006) (24) = Groenewegen et al. (1998) (25) = Jiménez-Esteban et al. (2006) (26) = Jones et al. (1990) (27) = Le Bertre (1993) (28) = Le Bertre (1992) (29) = Nakashima et al. (2000) (30) = Engels et al. (2015) (31) = Engels et al. (1983) (32) = van Langevelde et al. (1990) (33) = Olivier et al. (2001) (41) = Refit of VMC K-band data from Groenewegen et al. (2020) with initial period from the present work, (43) = Refit of VVV K-band (Ferreira Lopes et al. 2020), (44) = Refit of ASAS-SN V-band data (Shappee et al. 2014; Kochanek et al. 2017). (46) = Refit of ATLAS o-band data (Heinze et al. 2018). (47) = Refit of DIRBE 4.9 μm data (Price et al. 2010) (For the source with Ra = 204.411850 data at 3.5 μm data is used). (51) = Fit of OMC data (Alfonso-Garzón et al. 2012). (54) = Fit of CSS data (Drake et al. 2009). (63) = Fit to the data from Kerschbaum et al. (2006) with K-band photometry from the literature added. (70) = Fit to data from the Bochum Galactic Disk Survey (Hackstein et al. 2015). (71) = Fit to r-type data from the ZTF (Masci et al. 2019). Column 19, Comments: (1) W2 data is dummy. (2) Possibly a real source. IRAS 02408+5458 is located at 3″. (3) ASAS-SN: LC is peculiar. (4) Palt = 572. (5) ZTF: LC is peculiar. (6) Clones of VY CMa (110.7430362 -25.7675659). (7) Source is getting fainter with time. (8) Clones of IRAS 08074-3615 (122.334335 -36.407444). (9) Clones of HD 76220 (133.849921103 +19.6998172)? (10) Palt = 262. (11) Peculiar LC. (12) Palt = 491. (13) Source is getting brighter with time. (14) A clone of CW Leo (146.989203 +13.278759). (15) Source is getting brighter with time. (16) Clones of HD 97300 (167.4575881 -76.6130701). (17) Possibly a clone of IRAS 11145-6534, located at 75″. (18) ASAS-SN: bizarre LC. (19) Possibly a real source. Not an obvious clone. (20) A clone of IRAS 15194-5115 (230.7711108 -51.4329088). (21) Source (W2) is getting fainter with time. (22) Source (W2) is getting fainter with time. (23) Palt = 580, 780. (24) Palt = 1280. (25) Palt = 800. (26) Source is getting fainter with time. (27) Palt = 303. (28) Palt = 460. (29) P = 34.48 ± 0.16 days. (30) Palt = 460. (31) A clone of IRC +20 326 (262.9805754 +17.7558379). (32) Palt = 480, 730. (33) W1 data is dummy. (34) Palt = 314. (35) Palt = 969. (36) Sakurai’s object. Continueously brightening in K (VVV) and WISE filters. (37) Palt = 460 301. (38) Palt = 355. (39) A clone of AFGL 2135 (275.644226 -27.108224). (40) ASAS-SN: Burst, then nearly constant. (41) Source is getting fainter with time. (42) ZTF: peculiar LC (period fixed to 600 days). (43) ATLAS: Slowly getting brighter, with burst (?). (44) ZTF: very peculiar LC. (45) Palt = 1900. (46) ATLAS, ZTF: peculiar LC. Strong drop in brightness. (47) Source (W1) is getting brighter with time. (48) Palt = 330. (49) Clones of IRC +10 420 (291.700408 +11.354634). (50) OMC, ZTF: Slow change in both datasets. (51) ZTF: very peculiar LC. (52) P = 30.58 ± 0.02 days. (53) ASAS-SN: constant but then strong brightening. (54) ZTF: very peculiar LC. (55) Clones of AFGL 3068 (349.802533 +17.192628). (56) A clone of AFGL 3116 (353.61467 +43.55036). The full table is available at the CDS.
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