[vsnet-alert 17913] Re: PNV J03093063+2638031:likely a dwarf nova?
Tonny Vanmunster
tonny.vanmunster at gmail.com
Fri Oct 31 08:28:54 JST 2014
Dear colleagues,
I just concluded a time-resolved unfiltered CCD photometry session of this
target at my new CBA Belgium Observatory, using a 14" telescope with
STT-3200ME CCD (Paramount ME II, ScopeDome 3m). Clouds prevented me from
continuing the run. So far, the data show a 0.05 mag 'hump', which is
consistent with Gianluca's message below. Unfortunately, the run has not
been sufficiently long to allow a more accurate analysis nor period
determination.
Data will be made available to the Kyoto and CBA teams.
If sky conditions improve during the course of this night, I will resume the
session.
Best regards
Tonny
www.cbabelgium.com
www.peranso.com
-----Original Message-----
From: vsnet-alert-bounces at ooruri.kusastro.kyoto-u.ac.jp
[mailto:vsnet-alert-bounces at ooruri.kusastro.kyoto-u.ac.jp] On Behalf Of
Gianluca Masi
Sent: donderdag 30 oktober 2014 23:44
To: ALERT, VSNET
Subject: [vsnet-alert 17912] PNV J03093063+2638031:likely a dwarf nova?
Dear Colleagues,
we performed low-res spectroscopy of this transient, remotely using the 14"
robotic unit part of the Virtual Telescope in Italy.
300-seconds exposures were taken on 30.8125 Oct. UT, using a 100 lines/mm
grating, with a dispersion of 34.5 angstroms/pixel: we do NOT see evidence
of strong H-alpha emission.
We also performed time-resolved photometry of the source with the same
telescope, found at mag 11.1 (R, unfiltered), seeing a 0.05 large modulation
(early superhumps?).
Observations are ongoing.
Regards
Gianluca Masi
Pier Luigi Catalano
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