Dear colleagues,
I have just finished analysing my unfiltered observations of TCP
J19092450+3041330, obtained on 2021, September 04/05 at CBA Belgium
Observatory (0.40-m f/10.0 telescope, QHY-268M CMOS, clear then clouds) and
at CBA Extremadura Observatory (0.40-m f/5.1 telescope, SX-46 CCD, clear
skies).
Combining both observation sets, regular superhumps with an amplitude of
0.40 mag are clearly visible in the resulting light curve, establishing TCP
J19092450+3041330 as a new SU UMa-type dwarf nova. A period analysis using
the ANOVA, Lomb-Scargle, Generalized-Lomb-Scargle and PDM methods (Peranso
3.0), yields a combined superhump period of 0.0680 +/- 0.0002d. The object
was at mag CV = 16.1 on Sep 05th.
I will send my observations to AAVSO, CBA and VSNET for further analysis.
Best regards
Tonny
---
Tonny Vanmunster
CBA Belgium Observatory
CBA Extremadura Observatory
http://www.cbabelgium.com
PERANSO : The Light Curve and Period Analysis Software
http://www.peranso.com
Dear colleagues,
I have just finished analysing my unfiltered CMOS observations of MASTER OT
J052622.61+734629.7, obtained on 2021, September 03/04 at CBA Belgium
Observatory, using a 0.40-m f/10.0 telescope and QHY-268M CMOS camera under
clear skies.
Regular superhumps with an amplitude of 0.29 mag are clearly visible in the
resulting light curve, establishing MASTER OT J052622.61+734629.7 as a new
SU UMa-type dwarf nova. A period analysis using the ANOVA, Lomb-Scargle,
Generalized-Lomb-Scargle and PDM methods (Peranso 3.0), yields a combined
superhump period of 0.0665 +/- 0.0003d. The object was at mag CV = 16.2 on
Sep 04th.
I will send my observations to AAVSO, CBA and VSNET for further analysis.
Best regards
Tonny
---
Tonny Vanmunster
CBA Belgium Observatory
CBA Extremadura Observatory
http://www.cbabelgium.com
PERANSO : The Light Curve and Period Analysis Software
http://www.peranso.com
Dear friends,
Using my private system scraping MARS ( https://mars.lco.global/ ),
I've just found ZTF21abwplpy out as a CV candidate from the public ZTF data.
It's amplitude is > ~ 6.0 mag (assuming the limiting mag of PS1-g is 21.6).
(I'm sorry if someone has already discovered and reported it.)
Lasair: https://lasair.roe.ac.uk/object/ZTF21abwplpy/
ALeRCE: https://alerce.online/object/ZTF21abwplpy
MARS: https://mars.lco.global/?objectId=ZTF21abwplpy
According to ALeRCE, the position is (RA, Dec) = (19:15:25.637,
-13:31:07.56)
Last non-detections by ZTF:
g > 20.5191 on 2021-08-29.21 (ZTF, 'difference mag' via ALeRCE)
First detections by ZTF:
g = 15.601 +/- 0.024 on 2021-09-01.17 (ZTF, 'difference mag' via ALeRCE)
Second detections by ZTF:
r = 16.369 +/- 0.045 on 2021-09-03.23 (ZTF, 'difference mag' via ALeRCE)
g = 16.281 +/- 0.030 on 2021-09-03.25 (ZTF, 'difference mag' via ALeRCE)
The result of ASAS-SN Sky Patrol:
https://asas-sn.osu.edu/sky-patrol/coordinate/1713e323-474d-437d-aa0b-d65df…
It confirms a nearby star is contaminated.
There are no possible counterparts recorded in the PS1 mean object catalog.
No known minor planets are found by the Minor Planet Checker
(https://www.minorplanetcenter.net/cgi-bin/checkmp.cgi).
Best Regards and Clear Skies,
Kenta
--
________________________________________________________________
田口 健太 (TAGUCHI, Kenta)
京都大学大学院理学研究科宇宙物理学教室
(Department of Astronomy, Graduate School of Science, Kyoto University)
kentagch(a)kusastro.kyoto-u.ac.jp <mailto:kentagch@kusastro.kyoto-u.ac.jp>
09090536980
ASASSN-19wz possible superoutburst
Past ZTF data suggest an SU UMa star (possible superoutburst
in 2020 Nov.).
YYYYMMDD(UT) mag observer
20210901.2558 15.276zg (Zwicky Transient Facility Lasair (Masci+ 2019))