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
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________________________________________________________________
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))
The AM CVn-type object NSV 1440 is in bright outburst.
NSV 1440 210830.519 129
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Rod Stubbings
Tetoora Road Observatory
Victoria, Australia
Telescope: "Infinity" 22" f/3.8
stubbo(a)dcsi.net.au
http://rodstubbingsobservatory.wordpress.com/
ASASSN-V J205543.90+240033.5: combination of three periods
Josch Hambsch and Tonny Vanmunster have reported
observations.
See
https://arxiv.org/abs/2108.09060http://vsolj.cetus-net.org/vsoljno80.pdf
"ASASSN-V J205543.90+240033.5: another white dwarf pulsar?"
Their observations indicate that the global
variation is a combination of the longer period 10.803 d
and a shorter period 0.203424(1) d (determined from
the ZTF data). These variations create the dispersion
in figure 2 of the above paper.
Their data also confirmed the short period of
0.0067876(7) d (amplitude 0.07 mag).
This must be a very interesting CV-like object
and further observations (including spectroscopy)
are requested.