Peremennye Zvezdy

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"Peremennye Zvezdy",
Prilozhenie
,
vol. 21, N 3 (2021)

New Variable Stars in Lacerta: Area of 2°.3×2°.3, Center α=22h50m δ=54°00′ (2000.0). Part II

E. G. Lapukhin#1, A. M. Zubareva#2,3, E. Kryukova#1, F. Khamrakulov#4
#1. Siberian State Aerospace University, Krasnoyarsk, Russia;
#2. Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia
#3. Sternberg Astronomical Institute, Lomonosov Moscow State University, Moscow, Russia;
#4. Samarkand State University, Samarkand, Republic of Uzbekistan.

ISSN 2221–0474 DOI: 10.24412/2221-0474-2021-3

Received:   3.12.2016;   accepted:   31.08.2021
(E-mail for contact: slovoktk@mail.ru)


#NameOtherCoord (J2000)TypeMaxMinSystemPeriodEpoch (JD)typeSpCommentL.CurveFind.ChartData
1 2MASS 22484859+531840522 48 48.599 +53 18 40.59EW15.8616.26 0.506442456928.181min Comm. 1lc12353.pngch12353.pngout12353.dat
2 2MASS 22485138+550120922 48 51.381 +55 01 20.96DSCT13.3913.43 0.09297172456929.171max Comm. 2lc34651.pngch34651.pngout34651.dat
3 2MASS 22485457+540521922 48 54.570 +54 05 21.97SR:14.3314.44 27.7:2456926.3max Comm. 3lc31653.pngch31653.pngout31653.dat
4FR Lac2MASS 22485788+541235422 48 57.884 +54 12 35.46EA14.5815.51 0.8319212456927.263min  lc40513.pngch40513.pngout40513.dat
5 2MASS 22485911+542137922 48 59.120 +54 21 37.99EA15.0315.35 2.37077:2456934.259min  lc55093.pngch55093.pngout55093.dat
6 2MASS 22490253+531506222 49 02.536 +53 15 06.21EA16.0416.77 2.3795:2456934.145min  lc10853.pngch10853.pngout10853.dat
7 2MASS 22490279+534533622 49 02.797 +53 45 33.61EW1515.3 0.405292456928.087min Comm. 7lc23315.pngch23315.pngout23315.dat
8 2MASS 22490710+533055622 49 07.103 +53 30 55.66EB16.116.49 2.2387:2456893.309min  lc17416.pngch17416.pngout17416.dat
9 2MASS 22490859+532535522 49 08.600 +53 25 35.54EW15.0815.28 0.634682456892.253min Comm. 9lc15069.pngch15069.pngout15069.dat
10 2MASS 22490968+535640822 49 09.681 +53 56 40.86EW15.5515.78 0.377782456929.136min  lc28001.pngch28001.pngout28001.dat
11 2MASS 22491471+532808522 49 14.715 +53 28 08.57LB12.8713.05   other Comm. 11lc15391.pngch15391.pngout15391.dat
12 2MASS 22491672+544249622 49 16.730 +54 42 49.68LB13.7713.34   other Comm. 12lc46726.pngch46726.pngout46726.dat
13 2MASS 22492261+530835522 49 22.610 +53 08 35.52DSCT15.6915.83 0.158362456892.295max Comm. 13lc08104.pngch08104.pngout08104.dat
14 2MASS 22492581+544502022 49 25.814 +54 45 02.07LB14.4214.54   other Comm. 14lc45569.pngch45569.pngout45569.dat
15 2MASS 22494092+541956622 49 40.921 +54 19 56.66LB13.1313.56   other Comm. 15lc55954.pngch55954.pngout55954.dat
16 2MASS 22494380+542129522 49 43.805 +54 21 29.55EA15.1415.6 0.875212456894.348min  lc55167.pngch55167.pngout55167.dat
17 2MASS 22500123+544740622 50 01.232 +54 47 40.65LB12.5612.74   other Comm. 17lc44797.pngch44797.pngout44797.dat
18 2MASS 22500557+542427322 50 05.571 +54 24 27.37EW16.4217.24 0.970452456917.192min  lc54221.pngch54221.pngout54221.dat
19 2MASS 22501251+541559122 50 12.511 +54 15 59.18L14.3214.69   other Comm. 19lc39266.pngch39266.pngout39266.dat
20 2MASS 22501628+550131122 50 16.281 +55 01 31.14BY13.0513.09 0.931982456928.198max  lc34827.pngch34827.pngout34827.dat
21 2MASS 22503120+535134122 50 31.209 +53 51 34.14EA13.713.81 1.8013:2456894.289min  lc25506.pngch25506.pngout25506.dat
22 2MASS 22503213+545102022 50 32.140 +54 51 02.07EA14.0514.52 4.60365:2456928.041min  lc43517.pngch43517.pngout43517.dat
23 2MASS 22503320+532549022 50 33.201 +53 25 49.07EW15.0315.42 0.821472456928.277min Comm. 23lc14791.pngch14791.pngout14791.dat
24 2MASS 22505128+540747722 50 51.282 +54 07 47.76EA13.7513.93 1.06512456928.127min  lc31633.pngch31633.pngout31633.dat
25 2MASS 22510239+540008122 51 02.396 +54 00 08.19EA14.7815.11 1.74912456928.332min Comm. 25lc29067.pngch29067.pngout29067.dat
26 2MASS 22510683+532605922 51 06.832 +53 26 05.94SR:12.6512.74 43.92456933.2max Comm. 26lc14746.pngch14746.pngout14746.dat
27 2MASS 22511398+542627022 51 13.983 +54 26 27.07EA13.9<14.44 2.0753:2456927.129min  lc53384.pngch53384.pngout53384.dat
28 2MASS 22511431+533528722 51 14.318 +53 35 28.77LB14.1716.29   other Comm. 28lc18645.pngch18645.pngout18645.dat
29 2MASS 22511552+545518322 51 15.528 +54 55 18.39LB13.7613.85   other Comm. 29lc37609.pngch37609.pngout37609.dat
30 2MASS 22511969+530430322 51 19.696 +53 04 30.35LB11.9312.14   other Comm. 30lc05840.pngch05840.pngout05840.dat
31 2MASS 22513364+545620722 51 33.642 +54 56 20.74EW13.3813.66 0.840192456928.335min Comm. 31lc37254.pngch37254.pngout37254.dat
32 2MASS 22514191+540552022 51 41.913 +54 05 52.08LB13.0313.19   other Comm. 32lc31096.pngch31096.pngout31096.dat
33 2MASS 22514326+532820522 51 43.269 +53 28 20.53EA15.8116.9 0.743862456927.222min Comm. 33lc15790.pngch15790.pngout15790.dat
34 2MASS 22514494+550544122 51 44.949 +55 05 44.11EA15.08<15.6 0.833072456927.717min  lc33418.pngch33418.pngout33418.dat
35 2MASS 22514555+545541722 51 45.558 +54 55 41.73LB13.3913.59   other Comm. 35lc37536.pngch37536.pngout37536.dat
36 2MASS 22515655+530320922 51 56.554 +53 03 20.95DSCT13.1213.17 0.0854272456928.241max Comm. 36lc05358.pngch05358.pngout05358.dat
37 2MASS 22515812+542649722 51 58.128 +54 26 49.77DSCT13.14113.201 0.19081762456927.228max Comm. 37lc53610.pngch53610.pngout53610.dat
38 2MASS 22515854+531850522 51 58.540 +53 18 50.55EA14.8515.03 0.7271912456928.199min  lc11656.pngch11656.pngout11656.dat
39 2MASS 22522038+533550522 52 20.386 +53 35 50.59EW16.0416.36 0.326262456928.272min  lc18805.pngch18805.pngout18805.dat
40 2MASS 22523182+525349622 52 31.824 +52 53 49.68EA15.2415.55 1.40042456917.141min  lc01612.pngch01612.pngout01612.dat
41 2MASS 22523236+532931822 52 32.361 +53 29 31.85EW12.9212.94 0.353132456894.207min  lc15889.pngch15889.pngout15889.dat
42 2MASS 22523396+542730322 52 33.964 +54 27 30.33EA13.8213.96 1.228152456892.163min Comm. 42lc53207.pngch53207.pngout53207.dat
43 2MASS 22524069+532622822 52 40.690 +53 26 22.88EW16.316.71 0.262472456928.1min  lc14721.pngch14721.pngout14721.dat
44 2MASS 22524379+535536522 52 43.793 +53 55 36.51EA13.713.83 1.29230:2456927.263min  lc26282.pngch26282.pngout26282.dat
45 2MASS 22524756+543124222 52 47.562 +54 31 24.21RRAB:14.6714.76 0.773422456927.222max  lc51885.pngch51885.pngout51885.dat
46 2MASS 22530286+545352522 53 02.868 +54 53 52.52LB12.2512.37   other Comm. 46lc42777.pngch42777.pngout42777.dat
47 2MASS 22530429+544530022 53 04.299 +54 45 30.05EA15.0915.33 1.030472456917.705min  lc46299.pngch46299.pngout46299.dat
48 2MASS 22530709+543534622 53 07.098 +54 35 34.66LB14.1814.35   other Comm. 48lc50206.pngch50206.pngout50206.dat
49 2MASS 22532119+540736922 53 21.194 +54 07 36.99EW15.5815.85 0.307592456928.171min  lc31794.pngch31794.pngout31794.dat

Comments:


1. MinII = 16m.21.

2. Possible DSCT type with P = 0.08506 d and JD0 = 2456928.241.

3. J = 11m.870, H = 11m.199, K = 10m.991 (2MASS).

7. MinII = 15m.26.

9. MinII = 15m.27.

11. J = 9m.384, H = 8m.392, K = 8m.079 (2MASS).

12. J = 8m.352, H = 7m.613, K = 7m.256 (2MASS).

13. EW type with twice longer period is possible (0.31671 d, JD0 = 2456934.179).

14. J = 12m.425, H = 11m.904, K = 11m.762 (2MASS).

15. J = 8m.256, H = 7m.217, K = 6m.809 (2MASS).
The object is in the NSVS database: ID 3468452.

17. J = 8m.819, H = 7m.774, K = 7m.414 (2MASS).

19. J = 11m.476, H = 11m.770, K = 11m.541 (2MASS).

23. MinII = 15m.36.

25. MinII = 15m.07.

26. J = 9m.648, H = 8m.659, K = 8m.387 (2MASS).

28. J = 10m.214, H = 8m.472, K = 7m.177 (2MASS).

29. J = 8m.760, H = 7m.695, K = 7m.241 (2MASS).

30. J = 6m.969, H = 5m.924, K = 5m.470 (2MASS).
The object is in the NSVS database: ID 3470780.

31. MinII = 13m.65.

32. J = 8m.588, H = 7m.616, K = 7m.219 (2MASS).

33. MinII = 16m.03.

35. J = 9m.788, H = 8m.713, K = 8m.385 (2MASS).

36. EW type with twice longer period (0.17079 d) is possible.

37. Twice longer period (0.572456 d) is possible.

42. MinII = 13m.90.

46. J = 8m.812, H = 7m.825, K = 7m.439 (2MASS).

48. J = 10m.510, H = 9m.486, K = 9m.074 (2MASS).

Remarks:
We present the second part of new discoveries of variable stars in Lacerta: area of 2°.3×2°.3, center α=22h50m δ=54°00′(2000.0). Some of the objects are newly discovered, some are already known from massive surveys like ZTF and ASAS-SN.

Our observations of an area in Lacerta were performed in the observatory of the Reshetnev Siberian State University of Science and Technology with a Hamilton telescope (D = 400 mm, F = 915 mm), equipped with an FLI ML9000 CCD chip (3056 × 3056 pixels, pixel size 12 μm). Exposures of all frames were 30 seconds. A CCD image covers 2.3 × 2.3 of the sky.
We obtained all unfiltered CCD observations during two time intervals: August–October 2012 and September–October 2014.
The magnitudes were referred to those of comparison stars (in unfiltered red band) from the UCAC4 catalog (Zacharias et al. 2013). We used VaST software (Sokolovsky & Lebedev 2018) to search for variable stars. To perform periodogram analysis, we applied WinEfk software provided by V.P. Goranskij.
This work was supported by Ministry of Education and Science of Russian Federation within the framework of state contract 3.6822.2017/7.8.

Acknowledgements: The authors are grateful to Dr. V.P. Goranskij for providing his efficient period-search software and Dr. K.V. Sokolovsky for providing VaST (a software package for detection of variable objects on a series of astronomical images).

References:
Sokolovsky, K. V., Lebedev, A. A., 2018, Astron. and Computing, 22, 28
Zacharias, N., Finch, C. T., Girard, T. M. et al., 2013, Astron. J., 145, 44, The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)



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