- vsnet-alert - ooruri.kusastro.kyoto-u.ac.jp

[vsnet-alert 26861] CRTS J202857.1-061803 likely superoutburst
by Taichi Kato 04 Jul '22

04 Jul '22

CRTS J202857.1-061803 likely superoutburst Type from ZTF data. YYYYMMDD(UT) mag observer 20220615.4097 <164C (Masao Funada) 20220626.1150 151cG (Masao Funada) 20220629.7143 152:cG (Yutaka Maeda) 20220630.7076 153:cG (Yutaka Maeda) 20220701.2036 158cG (Masao Funada)

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[vsnet-alert 26860] ASASSN-18su superhump period
by Taichi Kato 04 Jul '22

04 Jul '22

ASASSN-18su superhump period Berto Monard, Josch Hambsch and Itoh-san have reported observations. The superhump period is 0.05815(2) d. The amplitude is large (0.23 mag). Ordinary SU UMa star.

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[vsnet-alert 26859] Blazar 1308+326 optical superoutburst
by Stefan Karge 03 Jul '22

03 Jul '22

Blazar 1308+326 (OP +313, AU CVn, B2 1308+32; z=0.997) optical superoutburst object date (UTC) mag comment -------------------------------------------------- 1308+326 20220630.001 13.03C active (1) 1308+326 20220701.913 12.88C active (1) 1308+326 20220701.944 12.95V active (2) 1308+326 20220702.728 13.18V active (3) 1308+326 20220702.767 12.98V active (4) -------------------------------------------------- Brightest optical state ever. Second optical flare in just two month [vsnet-alert 26762]. See also ATel #15476 and ATel #15474. -------------------------------------------------- (1) 30cm-Refl. + CCD + Clear (2) 43cm-Refl. + CCD + V-Johnson (remote) (3) 50cm-Refl. + CCD + V-Johnson (remote) (4) 36cm-Refl. + CCD + V-Johnson (remote) Stefan Karge (SKA) http://quasar.square7.ch/fqm/1308+326.html _______________________________________________

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[vsnet-alert 26858] ASASSN-18su observed at KKO
by Berto Monard 02 Jul '22

02 Jul '22

Hello, two nights of observations at CBA KKO show ASASSN-18su to be in an active stage of outburst Clear superhumps with amplitude of 0.27CR and period of 0.0582d +/- 0.0001d hint at an UGSU type CV . The unfiltered magnitude of the object was around 12.0CR on both nights, 29 and 30 June 2022. There has been a four year interval since the previous outburst. Berto Monard / KKO

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[vsnet-alert 26857] New follow-up observations of TCP J15244460-6059200 = FQ Cir
by Filipp Romanov 30 Jun '22

30 Jun '22

Observer: Filipp Romanov (Russia). Remotely using T30 (iTelescope.Net) 0.50-m f/6.8 reflector of Siding Spring Observatory (Australia): CIRFQ 20220625.67985 11.28V RFD CIRFQ 20220625.68264 12.02B RFD CIRFQ 20220625.68532 10.42R RFD CIRFQ 20220625.68843 9.69I RFD Color image: https://www.flickr.com/photos/filipp-romanov/52182779263 or https://twitter.com/romanov_filipp/status/1542218300897230848

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[vsnet-alert 26856] Re: ASASSN-18su
by Taichi Kato 29 Jun '22

29 Jun '22

Re: ASASSN-18su Superhumps were already detected during the 2018 superoutburst by Berto Monard. Superhumps appeared on 2018 Aug. 25. Due to the short visibility, the period was not determined.

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[vsnet-alert 26854] ASASSN-18su (super?)outburst (since June 24)
by Patrick Schmeer 28 Jun '22

28 Jun '22

ASASSN-18su (UG) https://www.aavso.org/vsx/index.php?view=detail.top&oid=623474 ASASSN-18su was discovered on 2018 August 17. Unfortunately that outburst could be followed for only few days. After the seasonal gap a very long fading tail can be seen in ATLAS forced photometry data. T. Kato wrote (vsnet-alert 22429): "The Gaia proper motion is comparable to that of OV Boo ... ASASSN-18su looks likely a population II CV candidate." The current outburst was detected by Rod Stubbings at mv= 11.3 on 2022 June 28.537 UT (vsnet-outburst 28822, vsnet-alert 26852). It had already started on June 24 and is 1.5 magnitudes fainter than the 2018 outburst according to ASAS-SN Sky Patrol data: https://asas-sn.osu.edu/sky-patrol/coordinate/52d16cd1-3548-431f-a7fc-326e3… Time-resolved photometry is urgently required. Clear skies, Patrick ------- References: All-Sky Automated Survey for Supernovae (ASAS-SN) Sky Patrol: - Shappee et al., 2014ApJ...788...48S - Kochanek et al., 2017PASP..129j4502K Asteroid Terrestrial-impact Last Alert System (ATLAS): - Tonry et al., 2018PASP..130f4505T

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[vsnet-alert 26853] QZ Vir (= T Leo) superoutburst (since June 21)
by Patrick Schmeer 28 Jun '22

28 Jun '22

QZ Virginis = T Leonis (UGSU) https://www.aavso.org/vsx/index.php?view=detail.top&oid=17034 Outburst first detected on 2022 June 22.981 UT at V= 10.36 by Carlos Colesanti (CCT): https://app.aavso.org/webobs/results/?star=000-BBS-294 Observed on June 28.424 UT at mv= 10.4 by Rod Stubbings (vsnet-outburst 28822). Recent ASAS-SN Sky Patrol (Shappee et al. 2014ApJ...788...48S and Kochanek et al. 2017PASP..129j4502K) light curve and data: https://asas-sn.osu.edu/sky-patrol/coordinate/c371f339-8e10-448c-98f5-e234f… The current superoutburst started on 2022 June 20 or 21. A normal outburst was observed from 2022 Jan. 31 to Feb. 3. Clear skies, Patrick

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[vsnet-alert 26852] ASASSN-18su outburst
by Rod Stubbings 28 Jun '22

28 Jun '22

ASASSN-18su is in outburst. Last known outburst was in 2018. ASASSN-18su 220628.537 113 -- Rod Stubbings Tetoora Road Observatory Victoria, Australia Telescope: "Infinity" 22" f/3.8 stubbo(a)dcsi.net.au http://rodstubbingsobservatory.wordpress.com/

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[vsnet-alert 26851] TCP J15244460-6059200: strange Galactic nova (mag. 11) in Circinus
by Patrick Schmeer 27 Jun '22

27 Jun '22

TCP J15244460-6059200 (N) (submitted to VSX) RA 15h24m47.62s DE -60°59'47.3" (Gaia DR3, equinox and epoch J2000.0) Discoverer: Andrew Pearce (Nedlands, Western Australia) http://www.cbat.eps.harvard.edu/unconf/followups/J15244460-6059200.html Elias Aydi et al.: "SOAR spectroscopic follow-up of the Galactic optical transient TCP J15244460-6059200" (ATel #15473): https://www.astronomerstelegram.org/?read=15473 Quote: "The spectrum resembles that of a very fast classical nova after optical peak. The low amplitude of the transient raises questions about its nature and the possible progenitor match. TCP J15244460-6059200 could be an unusually low-amplitude, ultra-fast nova or a more exotic phenomenon. There is a slight chance that the actual progenitor system is much fainter and coincides with the bright (~14 mag) match, which would explain the unusually low- amplitude of the transient." The likely progenitor is the Gaia DR3 source 5875610751015084544 (Gmag. 13.75, BP-RP= 0.73, Teff ~22500 K, parallax 0.11 ± 0.02 mas, distance 6.5 ± 0.8 kpc). SMSS data: gPSF= 13.98, rPSF= 13.70, iPSF= 13.74 APASS data: V= 13.88, B= 14.35, g'= 14.08, r'= 13.70, i'= 13.65 So the eruption amplitude seems to be only 3 magnitudes! And the likely progenitor does not look like a typical CV in quiescence. ASAS-SN Sky Patrol (Shappee et al. 2014ApJ...788...48S and Kochanek et al. 2017PASP..129j4502K) light curves and data: https://asas-sn.osu.edu/sky-patrol/coordinate/63cd3b67-9d82-41da-869e-4d122… https://asas-sn.osu.edu/sky-patrol/coordinate/a61c2edb-9cab-4d5c-b9cf-f886b… TCPJ15244460-6059200 20220619.1200 14.00g ASN TCPJ15244460-6059200 20220625.2002 10.91g ASN TCPJ15244460-6059200 20220625.2015 10.92g ASN TCPJ15244460-6059200 20220625.2027 10.97g ASN TCPJ15244460-6059200 20220625.9486 12.00g ASN TCPJ15244460-6059200 20220625.9498 11.96g ASN TCPJ15244460-6059200 20220625.9510 12.00g ASN TCPJ15244460-6059200 20220626.2656 12.28g ASN TCPJ15244460-6059200 20220626.2668 12.27g ASN TCPJ15244460-6059200 20220626.2682 12.28g ASN TCPJ15244460-6059200 20220626.9602 12.71g ASN TCPJ15244460-6059200 20220626.9615 12.65g ASN TCPJ15244460-6059200 20220626.9628 12.81g ASN Could the apparent fading trend in ASAS-3 data be real? http://www.astrouw.edu.pl/cgi-asas/asas_variable/152448-6059.8,asas3,0,9755… Further spectroscopy and multiband photometry are required. Clear skies, Patrick

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