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Table 2.

Table with the literature classification for 1416 objects among the 2116 candidate Cepheids in the MW by Clementini et al. (2019).

Source_id RA Dec DR2 Class. Lit. Name Lit. Class.
deg deg
(1) (2) (3) (4) (5) (6)
2947530506428832768 101.64608 −14.92456 DCEP_1O ASAS J064635-1455.5 DSCT/SXPHE
208360790657462144 79.45432 44.47322 WVIR ASASSN-V J051749.04+442823.6 RRAB
3315820030750497536 89.13874 1.70906 DCEP_1O CRTS J055633.2+014232 RRd
4044404165342126848 276.27275 −34.44904 DCEP_MULTI V3276 Sgr RRAB
4071594911751759872 280.72338 −28.62898 DCEP_1O [CAG2000] vs1f408 RRC
3045809872243862400 106.25278 −11.81071 DCEP_1O GDS_J0705006-114838 VAR
4122020821451345664 259.72364 −19.99288 DCEP_1O V1836 Oph RR
4051686608879712640 277.11621 −27.4369 DCEP_1O MACHO 175.30920.52 RRAB
3099348185775497728 101.98331 −7.41384 BLHER ASASSN-V J064755.99-072449.9 RRAB
4114405122877842688 257.82295 −23.27459 DCEP_MULTI 140805 RRAB
4077490291331290368 278.75571 −24.01232 DCEP_1O 124321 RRC
4043821561616680448 270.95217 −31.78211 RVTAU OGLE-BLG-RRLYR-12209 RRAB
4627678075752483584 65.96439 −76.91188 BLHER OGLE-GAL-ACEP-006 ACEP/DCEP_F
4072780464535420160 279.21002 −26.99927 DCEP_F [CAG2000] vs11f595 RRAB
4594729766718946304 265.52038 27.75574 DCEP_1O 28630 RRAB

Continuation

Lit. source P1 P2 P3 P1 source P2 source P3 source
days days days
(7) (8) (9) (10) (11) (12) (13)

VSX/ASAS_RICHARDS 0.0954 VSX/ASAS_RICHARDS
ASAS-SN 0.1849 ASAS-SN
CRTS 0.2731 CRTS
VSX 0.3565 VSX
VSX 0.3920 VSX
VSX/PS1 0.4276 PS1
VSX 0.4342 VSX
VSX 0.4675 VSX
ASAS-SN 0.4820 ASAS-SN
PS1 0.4838 PS1
PS1 0.4895 PS1
OGLE 0.4959 OGLE
OGLE/VSX 0.5042 1.8836 OGLE VSX
VSX 0.5048 VSX
PS1 0.5049 PS1

Notes. The different columns correspond to the following: (1) Gaia DR2 source identification; (2)-(3) RA-Dec (J2000); (4) variability classification according to Gaia DR2; (5) name of the object in the literature; (6) type(s) of variability found in the literature; (7) source for the different type of variability, separated by a “/” or “//” depending whether or not the period estimates of the two or more sources agree; (8)-(10) period(s) present in the literature; (11)-(13) sources of the period(s) in columns (8)-(10). A glossary of the variability types is reported Table A.1. The acronyms for the literature are given in the references of this table. The table is published in its entirety at the CDS. A portion including the first 15 lines is shown for guidance regarding its form and content.

References. ASAS3 (All Sky Automated Survey, Pojmanski 1997, 2002); ASAS_RICHARDS (All Sky Automated Survey re-classification, Richards et al. 2012); ASAS-SN (All-Sky Automated Survey for Supernovae, Jayasinghe et al. 2018); B15 (Berdnikov et al. 2015); C01 (Clement et al. 2001); CRTS (Catalina Real-Time Transient Survey, Drake et al. 2014, 2017); GCVS (General Catalogue of Variable Stars, Samus’ et al. 2017); DR1 (Clementini et al. 2016); EROS2_KIM (Kim et al. 2014); Hip11 (Dubath et al. 2011); IOMC (Integral Optical Monitoring Camera, Alfonso-Garzón et al. 2012); Kep11 (Debosscher et al. 2011); LINEAR (Lincoln Near-Earth Asteroid Research, Palaversa et al. 2013); NSVS (Northern Sky Variable Survey, Woźniak et al. 2004; Hoffman et al. 2009); OGLE (Optical Gravitational Lensing Experiment, Soszyński et al. 2015a,b, 2016, Soszyński et al. 2017a,b, 2018); PS1 (Panoramic Survey Telescope & Rapid Response System, Sesar et al. 2017); SDSS (Ivezić et al. 2007); Simbad (Wenger et al. 2000); VSX (The International Variable Star Index, Watson et al. 2006).

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