Peremennye Zvezdy

Article in PDF
"Peremennye Zvezdy",
Prilozhenie
,
vol. 17, N 1 (2017)

Light Curves of Variable Active Galactic Nuclei from the Catalina Sky Survey

K. Bernhard#1,2, S. Huemmerich#1,3
#1. Bundesdeutsche Arbeitsgemeinschaft fuer Veraenderliche Sterne e.V. (BAV), Berlin, Germany;
#2. Linz, Austria;
#3. Braubach, Germany;

ISSN 2221–0474

Received:   9.05.2014;   accepted:   26.01.2017
(E-mail for contact: klaus.bernhard@liwest.at , ernham@rz-online.de)


#NameOtherCoord (J2000)TypeMaxMinSystemPeriodEpoch (JD)typeSpCommentL.CurveFind.ChartData
1 2MASS 00185977+061931900 18 59.776, +06 19 31.99AGN16.917.9CV  other Comm. 1lc01.jpgchart01.pngdata01.txt
2 2MASS 00305804-115305900 30 58.043, -11 53 05.90AGN16.817.3CV  other Comm. 2lc02.jpgchart02.pngdata02.txt
3 2MASS 01594908-035200001 59 49.082, -03 52 00.04AGN16.116.7CV  other Comm. 3lc03.jpgchart03.pngdata03.txt
4 2MASS 02221804-062511102 22 18.046, -06 25 11.18AGN17.017.9CV  other Comm. 4lc04.jpgchart04.pngdata04.txt
5 2MASS 07034450+510042307 03 44.502, +51 00 42.33AGN16.717.6CV  other Comm. 5lc05.jpgchart05.pngdata05.txt
6 2MASS 07113788+241130007 11 37.889, +24 11 30.07AGN17.518.1CV  other Comm. 6lc06.jpgchart06.pngdata06.txt
7 2MASS 07380702+212729507 38 07.029, +21 27 29.54AGN16.216.5CV  other Comm. 7lc07.jpgchart07.pngdata07.txt
8 2MASS 07424005+354025007 42 40.053, +35 40 25.07AGN17.018.0CV  other Comm. 8lc08.jpgchart08.pngdata08.txt
9 2MASS 08290463+074339108 29 04.633, +07 43 39.15AGN15.415.5CV  other Comm. 9lc09.jpgchart09.pngdata09.txt
10 2MASS 08542951-070056808 54 29.512, -07 00 56.88AGN16.817.9CV  other Comm. 10lc10.jpgchart10.pngdata10.txt
11 2MASS 09055360-042611909 05 53.609, -04 26 11.97AGN15.916.5CV  other Comm. 11lc11.jpgchart11.pngdata11.txt
12 2MASS 09332405-293955909 33 24.055, -29 39 55.96AGN16.016.7CV  other Comm. 12lc12.jpgchart12.pngdata12.txt
13 2MASS 10503791+170208410 50 37.911, +17 02 08.48AGN16.518.0CV  other Comm. 13lc13.jpgchart13.pngdata13.txt
14 2MASS 11414222-023253311 41 42.228, -02 32 53.39AGN14.214.5CV  other Comm. 14lc14.jpgchart14.pngdata14.txt
15 2MASS 14031941-264427514 03 19.419, -26 44 27.51AGN16.717.8CV  other Comm. 15lc15.jpgchart15.pngdata15.txt
16 2MASS 15442601-201634215 44 26.012, -20 16 34.26AGN14.314.8CV  other Comm. 16lc16.jpgchart16.pngdata16.txt
17 2MASS 16593988+510726916 59 39.883, +51 07 26.98AGN16.617.8CV  other Comm. 17lc17.jpgchart17.pngdata17.txt
18 2MASS 17252982+380451017 25 29.828, +38 04 51.08AGN17.017.8CV  other Comm. 18lc18.jpgchart18.pngdata18.txt
19 2MASS 17375730+343252517 37 57.306, +34 32 52.56AGN17.317.9CV  other Comm. 19lc19.jpgchart19.pngdata19.txt
20 2MASS 20515533-233641520 51 55.339, -23 36 41.52AGN16.519.8CV  other Comm. 20lc20.jpgchart20.pngdata20.txt
21 2MASS 21021057-092904621 02 10.579, -09 29 04.69AGN16.617.1CV  other Comm. 21lc21.jpgchart21.pngdata21.txt
22 2MASS 21042191-021238921 04 21.912, -02 12 38.92AGN17.318.3CV  other Comm. 22lc22.jpgchart22.pngdata22.txt
23 2MASS 21560164+181837121 56 01.641, +18 18 37.18AGN17.117.8CV  other Comm. 23lc23.jpgchart23.pngdata23.txt
24 2MASS 21572678-061017621 57 26.782, -06 10 17.64AGN14.414.9CV  other Comm. 24lc24.jpgchart24.pngdata24.txt
25 2MASS 22373222-033808522 37 32.228, -03 38 08.60AGN17.218.7CV  other Comm. 25lc25.jpgchart25.pngdata25.txt
26 2MASS 23391553-225757323 39 15.538, -22 57 57.38AGN17.418.4CV  other Comm. 26lc26.jpgchart26.pngdata26.txt

Comments:


1. J–K = 0.686 (2MASS), 1RXS J001859.8+061937, HR1 = 0.24, HR2 = 0.24, probably quasar (Flesch 2010); SDSS, Release 9: star-like object; CSS light curve: very slow variations, confirmed as quasar.

2. J–K = 1.412 (2MASS), 1RXS J003059.3–115300, HR1 = –0.41, HR2 = 0.33, 6dF J0030580–115306, z = 0.240540 (Jones, Read, Saunders et al. 2009), AGN candidate (Kouzuma and Yamaoka 2010); CSS light curve: slow variations, possible period ~2200 d, confirmed as quasar.

3. J–K = 1.728 (2MASS), 1RXS J015948.9–035206, HR1 = –0.51, HR2 = 0.00, probably quasar (Flesch 2010), AGN candidate (Kouzuma and Yamaoka, 2010); SDSS, Release 9: star-like object; CSS light curve: slow, irregular variations, confirmed as quasar.

4. J–K = 1.32 (2MASS), 1RXS J022218.0–062513, HR1 = –0.40, HR2 = –0.16, probably quasar (Flesch 2010), AGN candidate (Kouzuma and Yamaoka 2010); SDSS, Release 9: star-like object; CSS light curve: very slow variations, confirmed as quasar.

5. J–K = 1.74 (2MASS), 1RXS J070344.4+510040, HR1 = 0.60, HR2 = –0.28, probably quasar (Flesch 2010); CSS light curve: very slow variations, confirmed as quasar.

6. J–K = 1.493 (2MASS), 1RXS J071136.5+241124, HR1 = 0.66, HR2 = –0.27, AGN candidate (Kouzuma and Yamaoka 2010); CSS light curve: very slow variations, confirmed as quasar.

7. J–K = 1.512 (2MASS), 1RXS J073806.9+212726, HR1 = 0.13, HR2 = –0.49, probably quasar (Flesch 2010; Abraham, Philip, Kembhavi et al. 2012), AGN candidate (Kouzuma and Yamaoka 2010); SDSS, Release 9: star-like object; CSS light curve: very slow variations, confirmed as quasar.

8. J–K = 1.616 (2MASS), 1RXS J074240.3+354023, HR1 = 0.38, HR2 = –0.07, probably quasar (Flesch 2010), AGN candidate (Kouzuma and Yamaoka 2010); SDSS, Release 9: star-like object; CSS light curve: slow, irregular variations, confirmed as quasar.

9. J–K = 0.542 (2MASS), 1RXS J082904.3+074335, HR1 = 0.54, HR2 = 0.61, probably quasar (Flesch 2010); SDSS, Release 9: star-like object; CSS light curve: slow variations, possible period ~1550 d, confirmed as quasar.

10. J–K = 1.661 (2MASS), 1RXS J085429.8–070046, HR1 = 0.57, HR2 = 0.20, probably quasar (Flesch 2010); CSS light curve: slow, irregular variations, confirmed as quasar.

11. J–K = 1.753 (2MASS), 1RXS J090553.8–042608, HR1 = –0.21, HR2 = 0.14, probably quasar (Flesch 2010), AGN candidate (Kouzuma and Yamaoka 2010); CSS light curve: slow, irregular variations, confirmed as quasar.

12. J–K = 1.579 (2MASS), 1RXS J093322.7–293956, HR1 = 0.80, HR2 = 0.13, AGN candidate (Kouzuma and Yamaoka 2010); CSS light curve: slow, irregular variations, confirmed as quasar.

13. J–K = 1.768 (2MASS), 1RXS J105038.2+170220, HR1 = 0.33, HR2 = 0.28, quasar or Seyfert galaxy (Flesch 2010), AGN candidate (Kouzuma and Yamaoka 2010),