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17"Peremennye Zvezdy", Prilozhenie, vol. 22, N 3 (2022)
Discovery of Six New Variables: Center a=23h58m d=+62°37r
O. Burkhonov#1'2. S. Egamberdiev#1,3. B. Satovskiv#4. F. Khamrakulov#1,2. R. Karimov#1. R. Gavsin#1. B. Khafizov#1
#1. Astronomical Institute of the Uzbekistan Academy of Sciences, Tashkent, Uzbekistan; #2. Samarkand State University, Samarkand, Uzbekistan; #3. National University of Uzbekistan, Tashkent, Uzbekistan; #4. State Space Corporation "Roscosmos", Moscow, Russia.
ISSN 2221-0474 DOI: 10.24412/2221-0474-2022-3
Received: 27.07.2022; accepted: 11.11.2022
(E-mail for contact: boa@astrin.uz')
# |Name | Other Coord (J2000) Type Max Min System Period Epoch (JD) tXP-e Sp. Comment L.Curve Find.Chart Data
1 USN0-B1.0 1524-0451378 23 58 19.525 +62 29 00.97 EA 15.57 15.87 R 2.730 2459471.366 min mao v1_ph.pne mao v1 map.pne mao v1 dat.txt
2 USNO-BI.O 1526-0460830 23 58 46.987 +62 36 51.50 EA 16.18 16.49 R min Comm. 2 mao v2 lc.pne mao v2 map.pne mao v2 dat.txt
3 USN0-B1.0 1528-0467698 23 57 05.425 +62 49 53.84 EA 17.00 17.57 R min Comm. 3 mao v3 lc.pne mao v3 map.pne mao v3 dat.txt
4 USNO-BI.O 1526-0458817 23 56 19.567 +62 36 04.59 EA 16.55 16.98 R 5.183 2459464.173 min mao v4_ph.pne mao v4 map.pne mao v4 dat.txt
5 USN0-B1.0 1526-0460762 23 58 41.428 +62 37 14.88 EA 16.05 16.27 R 1.5154 2459465.116 min mao v5_ph.pne mao v5 map.pne mao v5 dat.txt
6 USN0-B1.0 1528-0470117 23 59 57.470 +62 49 49.83 DSCT 16.10 16.22 R 0.07823 2459471.329 max mao v6_ph.pne mao v6 map.pne mao v6 dat.txt
Comments:
2. It was not possible to determine the period because only one minimum was observed. JDmin = 2459465.3624.
3. It was not possible to determine the period because only one minimum was observed. JDmin = 2459511.156. Remarks:
We present the results of searching for variable stars in a field in Cassiopea with the center a=23h58m S=+62°37' (2000.0) and the field of view of 30'. We did not find any reference to these stars being variable in the available star databases: GCVS (Samus et al. 2017), VSX, ZTF (Chen et al. 2020), and ASAS-SN Variable Stars Database.
Observations were carried out at the Maidanak Astronomical Observatory of the Astronomical Institute of the Academy of Sciences of the Republic of Uzbekistan (Ehgamberdiev 2018) using the 0.5-meter AMT-1 telescope with Mathis Instruments MI-750/1000 equatorial fork mount equipped with an Apogee Alta U16M (4K*4K) CCD camera. The physical size of a CCD pixel is 9 microns. We used 2^2 binning, which corresponds to 0.907 ''/pixel, and the field of view of 30.9'*30.9'. The exposure times were 180 seconds in the Bessel R filter. The temperature of the camera was set to -15°C. Calibration images as bias, dark and flat were also obtained for each observational date. Observations were obtained during the period from September 5 to October 30, 2021. The total number of observation nights was 28 during which 2593 images were taken.
All images were processed with master bias, dark, and flat frames using standard IRAF packages. We rejected low-quality images, and the final sample contained 2514 images. The VaST (Variability
Search Toolkit) software package (Sokolovsky and Lebedev 2018) was used to search for variable stars. To derive periods we used period search tool by Dr. K.V. Sokolovsky who incorporated it in his VaST package. Acknowledgments: We are grateful to the staff of the Maidanak Astronomical Observatory for their efforts to support observations.
References:
Chen, X., Wang, S., et al., 2020, Astron. J. Suppl. Ser., 249, 18 Ehgamberdiev, Sh., 2018, Nature Astronomy, 2, 349
Samus, N.N., Kazarovets, E.V., Durlevich, O.V., Kireeva, N.N., Pastukhova, E.N., 2017, Astron. Rep., 61, No. 1, 80 Sokolovsky, K. V., Lebedev, A. A., 2018, Astron. and Computing, 22, 28
