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The 3 columns in color are computed by VizieR, and are not part of the original data.
J/AJ/133/665/stars
Post annotation
Photometry of type II Cepheid candidates (Schmidt+, 2007)
Program stars and light curve parameters (tables 1 and 3 of paper) (205 rows)
img(gal)
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Full

LC

Seq

n_

Per
d
<Vmag>
mag
<V-R>
mag
Vamp
mag
Slope

n_

St

PerA
d
_RA
deg
_DE
deg
1LCR001   57.00000013.90 1.40 0.38 0.11RE   0.98333800287.05458+38.49967
2LCR002  320.00000014.00 1.00 0.29 0.08REB 1.01634800269.93921+31.58869
3LCR003    13.70 1.90 0.44 0.33IR,RE   1.02233303265.71950+23.01789
4LCR004   78.00000013.30 1.10 0.30 0.15IR,RE   1.02267396263.32167+25.92403
5LCR005    12.50 1.00 0.20 0.14IR,RE   1.02331805280.54596+39.12647
6LCR006   37.30000012.59 0.54 0.04 0.23  A 1.03392696251.26087+08.00961
7LCR007*  13.40 0.40 0.00  CO   1.05063200274.79408+53.42700
8LCR008* 0.52294012.32 0.29 0.21 0.09SP   1.09815705293.22058+45.84389
9LCR009   9.23000014.08 0.64 0.08 0.36  A 1.12023306249.91392+38.49525
10LCR010    14.50 0.32 0.00  CO   1.22454298262.14962+18.22625
11LCR011   4.81100012.61 0.48 0.13-0.16SL   1.25945902262.95579+44.41575
12LCR012   1.38535012.31 0.52 0.15 0.01  A 1.38528705219.52812+35.82814
13LCR013   1.43340011.76 0.47 0.16 0.19  A 1.43157601256.61896+41.25208
14LCR014    12.00 0.10 0.32-0.04IR,BL   1.52315104243.38267+32.57767
15LCR015   0.18636111.21 0.39 0.10-0.11SP   1.58459103264.11733+49.08889
16LCR016   1.70070013.55 0.04 1.22 0.09BL   1.70195496254.45725+35.34233
17LCR017   3.50260011.90 0.40 0.67 0.07EC   1.75260699263.61229+32.22531
18LCR018   1.89400012.24 0.45 0.12 0.12  A 1.86349797258.99504+43.90736
19LCR019    13.66 0.36 0.00  CO   1.93418396266.77887+38.54822
20LCR020   1.96320013.68 0.66 0.16 0.18  A 1.98090005252.91687+09.63611
21LCR021    13.10 0.20 2.30 0.16CV   2.09508109251.03887+25.25103
22LCR022   4.44830012.06 0.48 0.31 0.10EC   2.22385812284.39996+45.13125
23LCR023   2.42930011.76 0.60 0.21 0.03  A 2.43277502259.60483+52.92475
24LCR024   2.75120010.52 0.46 0.02 0.20  A 2.75598693258.37887+23.34064
25LCR025   2.78160012.70 0.81 0.09 0.02  B 2.77758694207.74250+26.55578
26LCR026   2.87730013.19 0.67 0.22 0.11  A 2.86190510285.88833+38.48681
27LCR027   2.93420011.45 0.29 0.07-0.27SL   2.93369293257.32350+31.46658
28LCR028   3.02660012.03 0.51 0.14 0.16  A 3.01902199252.84637+23.92769
29LCR029   3.05017012.87 0.96 0.03 0.16  B 3.05227089227.53504+25.64136
30LCR030   3.07600012.09 0.70 0.38 0.10  A 3.07779503256.99158+29.32081
31LCR031   3.09890012.03 0.60 0.12 0.19  A 3.14013791259.29937+08.25594
32LCR032   1.60070010.71 0.52 0.08 0.10  A 3.19838595195.94142+28.62200
33LCR033   3.31650013.48-0.08 0.25-0.23SL,BL   3.31412601207.71996+36.70069
34LCR034   3.68000012.27 0.49 0.07 0.02  A 3.68630409262.95687+33.07897
35LCR035   3.75500013.04 0.60 0.29 0.11  A 3.73737597252.80333+09.87750
36LCR036   3.87710011.82 0.62 0.10 0.18  A 3.85980892264.58033+34.53258
37LCR037   4.11700012.81 0.65 0.30 0.06  A 4.12298489289.72337+43.82500
38LCR038   0.72150013.94 0.52 0.11 0.40SP   4.25137091258.01546+52.89850
39LCR039   4.36030012.38 0.45 0.13-0.02  A 4.38333082278.49129+42.62261
40LCR040   0.40430011.82 0.53 0.14 0.41SP   4.41973782242.92575+36.49125
41LCR041   4.62200012.77 0.62 0.15 0.12  A 4.54563000271.88854+40.25836
42LCR042   4.58230011.67 0.55 0.27-0.07  A 4.59007000251.76404+09.76706
43LCR043   5.07800011.89 0.61 0.36 0.07  A 5.09124000281.63875+48.90981
44LCR044   5.77300011.62 0.49 0.14-0.03  A 5.77376000256.40783+33.84792
45LCR045   5.91100012.23 0.47 0.06 0.26  A 5.88170000241.32579+37.43986
46LCR046   6.21400010.25 0.44 0.03 0.02  A 6.07072020270.44787+27.65206
47LCR047   6.36300011.72 0.62 0.32 0.11  A 6.33070993265.79596+33.83003
48LCR048   6.31100012.95 0.58 0.19-0.07  A 6.33694077204.37471+30.34125
49LCR049   6.85900013.06 0.65 0.20 0.15  A 6.89707613256.48550+10.35617
50LCR050   6.52300011.35 0.50 0.06 0.40  A 6.93244696261.63250+40.63769
Result truncated to 50 rows
J/AJ/133/665/notes
Post annotation
Photometry of type II Cepheid candidates (Schmidt+, 2007)
Individual notes (20 rows)
 
Full

Seq

Note

1R007Only one photometric night so the zero point of the magnitude and color are
2R007 uncertain.
3R008Excess scatter may suggest that this star exhibits the Blazhko effect or
4R008 multiperiodicity.
5R069The Akerlof period was used for this star since a period could not be
6R069 determined from the Behlen data.
7R074This star appears to have undergone a sudden period change during the
8R074 interval covered by the NSVS data. By the epoch of the Behlen data the
9R074 period had reverted to the original value. The period listed in the table
10R074 is valid for the NSVS data prior to JD 2451320 and the Behlen data.
11R092The adjusted period satisfies both the first season of the NSVS data
12R092 (JD2451274-JD2451322) and the Behlen data. However, the amplitude of the
13R092 former is much larger. No well defined period could be found for the
14R092 second season of the NSVS data (JD2451512-JD2451633).
15R122We are unable to find a period which satisfies all of the data. However,
16R122 there is some indication of RV Tau behavior with a double period of about
17R122 83 days in the NSVS data.
18R137The NSVS data only covers part of the cycle of this star. The cited period
19R137 fits both the Behlen data and the NSVS data but must be regarded as
20R137 tentative.
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