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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