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

[vsnet-alert 26563] ASASSN-22bs: likely dwarf nova outburst (mag. 12.2, in Canis Major)
by Patrick Schmeer 08 Feb '22

08 Feb '22

ASASSN-22bs (UG:) https://www.aavso.org/vsx/index.php?view=detail.top&oid=2226032 Complete 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/2f8a4b69-9191-4256-a3ef-a8e9b… ASASSN-22bs 20220205.8444 <16.91g ASN ASASSN-22bs 20220208.2927 12.15g ASN Transient Name Server (TNS): https://www.wis-tns.org/object/2022bqs Outburst amplitude of more than 8.0 magnitudes. Time-resolved photometry is urgently required. Spectroscopy is also encouraged. Clear skies, Patrick

1 0

[vsnet-alert 26561] NSV 5031: new SU UMa-type dwarf nova
by tonny.vanmunster＠gmail.com 08 Feb '22

08 Feb '22

Dear colleagues, I have just finished analysing my unfiltered CCD observations of NSV 5031, obtained on 2022, February 07/08 at CBA Extremadura Observatory (Spain), using a 0.40-m f/5.1 telescope and SX-46 CCD camera under clear skies. My observations were triggered by Rob Stubbings' vsnet-alert message 26557. Regular superhumps with an amplitude of 0.35 mag are very clearly visible in the resulting light curve, establishing NSV 5031 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 0.0764 +/- 0.0013d. The object was at mag CV = 14.1 on Feb 08th. 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

2 1

[vsnet-alert 26560] ASASSN-14fe superoutburst
by Taichi Kato 08 Feb '22

08 Feb '22

ASASSN-14fe superoutburst (Superhumps have not yet been detected) YYYYMMDD(UT) mag observer 20220130.485 140 (Rod Stubbings) 20220131.546 140 (Rod Stubbings) 20220202.1637 14.03C (Masao Funada) 20220202.544 145 (Rod Stubbings) 20220203.478 144 (Rod Stubbings) 20220204.544 143 (Rod Stubbings) 20220205.542 145 (Rod Stubbings) 20220206.544 147 (Rod Stubbings)

1 0

[vsnet-alert 26559] V393 Hya fading (VY Scl)
by Taichi Kato 08 Feb '22

08 Feb '22

V393 Hya fading (VY Scl) http://gsaweb.ast.cam.ac.uk/alerts/alert/Gaia22amb/ Novalike CV V393 Hya fades by ~1 mag over ~1 year

1 0

[vsnet-alert 26558] NSV 5031 precursor and superoutburst
by Taichi Kato 08 Feb '22

08 Feb '22

NSV 5031 precursor and superoutburst Time-resolved observations are encourgaged. (Superhumps have not yet been detected). YYYYMMDD(UT) mag observer 20220202.578 <160 (Rod Stubbings) 20220203.574 138 (Rod Stubbings) 20220204.551 140 (Rod Stubbings) 20220205.1947 14.76C (Masao Funada) 20220205.558 147 (Rod Stubbings) 20220206.1081 16.06C (Masao Funada) 20220206.551 160 (Rod Stubbings) 20220207.526 134 (Rod Stubbings) location: 105749.916 -215658.74 (2000.0) Gaia_DR2_3549823111895468672 plx=1.522(0.150) dismod=9.1 pmra=6.517(0.240) pmdec=-15.902(0.210) G=17.958 BP=17.940 RP=17.394 105749.917 -215658.75 (2000.0) Gaia_EDR3_3549823111895468672 plx=1.596(0.079) dismod=9.0 pmra=6.694(0.117) pmdec=-15.865(0.100) G=17.822 BP=17.959 RP=17.301 105749.887 -215658.52 (2000.0) GALEX_DR5_6382315538213766389 NUV=18.979(0.077) FUV=19.093(0.117)

1 0

[vsnet-alert 26557] NSV 5031 rebrightened!
by Rod Stubbings 07 Feb '22

07 Feb '22

NSV 5031 is a possible SU-UMa star but not yet confirmed. The rebrightening observed tonight could be a superoutburst. object YYMMDD(UT) mag code NSV 5031 220202.579 <160 Stu.RASNZ 20220203.574 138 (Rod Stubbings) 20220204.551 140 (Rod Stubbings) 20220205.1947 14.76C ### (Masao Funada) 20220205.558 147 ### (Rod Stubbings) 20220206.551 160 ### (Rod Stubbings) object YYMMDD(UT) mag code NSV 5031 220207.526 134 Stu.RASNZ rebrightened! -- Rod Stubbings Tetoora Road Observatory Victoria, Australia Telescope: "Infinity" 22" f/3.8 stubbo(a)dcsi.net.au http://rodstubbingsobservatory.wordpress.com/

1 0

[vsnet-alert 26556] ASASSN-20pv third rebrightening
by Taichi Kato 07 Feb '22

07 Feb '22

ASASSN-20pv third rebrightening YYYYMMDD(UT) mag observer 20220119.2103 <16.15g (ASAS-SN survey (Shappee+ 2014; Kochanek+ 2017)) 20220120.1483 12.29g (ASAS-SN survey (Shappee+ 2014; Kochanek+ 2017)) 20220120.1495 12.34g (ASAS-SN survey (Shappee+ 2014; Kochanek+ 2017)) 20220120.535 123 (Rod Stubbings) 20220121.494 124 (Rod Stubbings) 20220122.533 125 (Rod Stubbings) 20220124.492 128 (Rod Stubbings) 20220125.524 131 (Rod Stubbings) 20220126.2222 13.52C (Eddy Muyllaert) 20220126.2225 13.61C (Masao Funada) 20220127.2257 13.41C (Eddy Muyllaert) 20220127.2267 13.52C (Masao Funada) 20220128.2638 13.88C (Masao Funada) 20220128.2639 13.78C (Eddy Muyllaert) 20220129.3576 13.83C (Eddy Muyllaert) 20220129.3580 13.42C (Masao Funada) 20220130.535 154 (Rod Stubbings) 20220131.533 156 (Rod Stubbings) (0201 first) 20220203.496 154 (Rod Stubbings) 20220204.519 144 (Rod Stubbings) second 20220205.510 156 (Rod Stubbings) 20220206.498 143 (Rod Stubbings) third 20220206.542 145 (Rod Stubbings) 20220206.556 147 (Rod Stubbings) 20220206.571 148 (Rod Stubbings) 20220206.594 148 (Rod Stubbings) 20220206.697 154 (Rod Stubbings)

1 0

[vsnet-alert 26548] Re: ASASSN-20pv: no major variations yet
by Taichi Kato 04 Feb '22

04 Feb '22

> Observations on Jan 20 showed a transition to the early modulation with > 'growing' superhumps of still small amplitude and a hint of a 0.0095d alt. > 0.019d period around a mean magnitude of 12.49CR. Ordinary superhumps, yes. The amplitudes were too small to be directly visible in Hambsch's data.

2 1

[vsnet-alert 26554] QZ Vir: rapidly fading but bright peak
by Taichi Kato 01 Feb '22

01 Feb '22

QZ Vir: rapidly fading but bright peak Precursor outburst? YYYYMMDD(UT) mag observer 20220129.9444 <138 (Eddy Muyllaert) 20220130.576 156 (Rod Stubbings) 20220130.8202 150C (Masayuki Moriyama) 20220131.567 98 (Rod Stubbings) 20220131.803 108 (Hiroyuki Maehara) 20220131.9340 108 (Eddy Muyllaert) 20220201.828 120 (Hiroyuki Maehara)

1 0

[vsnet-alert 26531] TCP J07094936+1412280: appearance of ordinary superhumps
by 反保雄介 01 Feb '22

01 Feb '22

TCP J07094936+1412280: appearance of ordinary superhumps Kiyota-san, Itoh-san, Tonny Vanmunster, Stephen M. Brincat, Sano-san, Tamás Tordai, and Kyoto Univ. Obs. have reported further observations of TCP J07094936+1412280. The data on 15th Jan at Kyoto Univ. Obs. showed clear ordinary superhumps with an amplitude of ~0.15 mag. The baseline was still too short to determine its period. Continuous observations are encouraged. Best, Yusuke

2 1

2025

2024

2023

2022

2021

vsnet-alert