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Belissima 2012 :: MASTER Robotic Network Results and Perspectives of the MASTER Robotic Telescopes Network Denis V. Denisenko Sternberg Astronomical Institute Lomonosov Moscow State University on behalf of the large international collaboration of Universities, Institutes and Observatories
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Belissima 2012 :: MASTER Robotic Network MASTER team V. Lipunov, E. Gorbovskoy, V. Kornilov, D. Kuvshinov, A. Belinski, N. Tyurina, N. Shatskiy, P.Balanutsa, D. Zimnukhov, A. Kuznetsov, V.V. Chazov, A. Kuznetsov, A. Sankovich Lomonosov Moscow State University, Sternberg Astronomical Institute K. Ivanov, S. Yazev, N.M. Budnev, O. Gres, O. Chuvalaev, V.A. Poleshchuk Irkutsk State University A. Tlatov, A.V. Parhomenko, D. Dormidontov, V. Sennik Kislovodsk Solar Station of Pulkovo Observatory V. Krushinski, I. Zalozhnich, A. Popov, A. Bourdanov, A. Punanova Ural Federal University V. Yurkov, Yu. Sergienko, D. Varda, E. Sinyakov Blagoveschensk Educational State University, Blagoveschensk Volunteers: S. Shurpakov, V. Shumkov, P. Podvorotniy H. Levato and C. Saffe Instituto de Ciencias Astronomicas, de la Tierra y del Espacio (ICATE), Argentina C. Mallamaci, C. Lopez and F. Podest Observatorio Astronomico Felix Aguilar (OAFA), Argentina
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Belissima 2012 :: MASTER Robotic Network MASTER team
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Belissima 2012 :: MASTER Robotic Network Somewhere near Moscow 10 years ago
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Belissima 2012 :: MASTER Robotic Network Somewhere in Siberia, current days MASTER-II: D=400 mm, F=1000 mm, FOV=2*4 sq.deg., 20m in 180 sec MASTER-WFC: FOV=384 sq. deg, 7 frames per sec, 12m in 1 sec
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Belissima 2012 :: MASTER Robotic Network MASTER photometer
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Belissima 2012 :: MASTER Robotic Network Siberian Roof
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Belissima 2012 :: MASTER Robotic Network MASTER Net in 2008-2011
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Belissima 2012 :: MASTER Robotic Network Twin T.T.T.T. Optical scheme: Hamiltonian Optical scheme: Hamiltonian CCD: CCD: Alta U16M Q=25% S=940 sq. cm 4Kx4K pixels Scale: 1.85”/pixel FOV=2.1x2.1 deg
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Belissima 2012 :: MASTER Robotic Network MASTER Mount Manufacturer: ASTELCO Model: Model: NTM500 Pointing speed: up to 30 deg/sec Pointing accuracy: down to 10”
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Belissima 2012 :: MASTER Robotic Network MASTER sites SiteLong.Lat.Elev.Note Ural 03h58m11s.2+57◦02′13′′290Kourovka Tunka 06h52m16s.1+51◦48′34′′700 Tunka Valley Amur 08h29m56s.0+50◦19′07′′215 Ex-Latit. Station Kislovodsk 02h50m04s.0+43◦45′00′2067 GAS GAO Canarias 01h06m02s.3+28◦18′00′2390 Teide Obs.
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Belissima 2012 :: MASTER Robotic Network MASTER nights SiteFNT,hCNT,hCNT,% Sky BG Ural2659122346% 21.2-20.5 Tunka2984170057% 22.0-21.9 Amur3068214670% 20.5-19.5 Kislovodsk3291187657% 21.9-21.7 Canarias35342474~70% 21.9-21.7
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Belissima 2012 :: MASTER Robotic Network Night Control Center
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Belissima 2012 :: MASTER Robotic Network MASTER results GRB pointing statistics during the winter of 2010-2011 First PointingPrompt Pointing
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Belissima 2012 :: MASTER Robotic Network The first synchronous polarization observations of gamma-ray burst in the world (2010 Sep. 06, MASTER)
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Belissima 2012 :: MASTER Robotic Network GRB 100906: gamma-ray burst from the textbook
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Belissima 2012 :: MASTER Robotic Network MASTER Synoptic Sky Survey Sky Coverage Present: up to 2500 sq. deg/night By 2013: up to 5000 sq. deg/night Information Flow MASTER-II: 4x15 GB = 60 GB/night MASTER-WVF: 12x950 GB=10 TB/ngt
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Belissima 2012 :: MASTER Robotic Network
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Big Synoptic Survey Theorem by Prof. Lipunov If you design synoptic telescope with diameter D, You must have spectral telescope with diameter ~ 10 D.
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Belissima 2012 :: MASTER Robotic Network OT of unknown nature (19.4m): MASTER J082752.77+704606.0
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Belissima 2012 :: MASTER Robotic Network OT of unknown nature (19.4m): MASTER J082752.77+704606.0
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Belissima 2012 :: MASTER Robotic Network Supernova discoveries 2012de 22 15 05.32 +10 18 12.6 18.5 Ia Podvorotniy 2012dc 15 38 17.95 +25 44 17.3 18.6 Ia Shumkov (MASTER) 2012cd 13 22 35.25 +54 48 47.7 15.1 IIb Shurpakov (MASTER) 2012bp 16 18 12.44 +36 28 52.8 15.5 Ia Lipunov (MASTER) 2012bd 16 31 05.47 +61 55 48.4 18.1 IIP Lipunov (MASTER) 2012af 15 00 30.87 +23 55 45.1 16.7 Ia Lipunov (MASTER) 2012ae 08 58 55.88 +23 03 42.4 18.4 Ia Astrotel 2012K 00 34 30.79 +30 24 06.3 16.0 II Lipunov (MASTER) All Russian SNe discovered in 2012 so far
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Belissima 2012 :: MASTER Robotic Network Supernova discoveries 2011jy 10 53 57.03 +23 22 34.5 16.5 II Lipunov (MASTER) 2011iq 02 48 49.60 -08 04 30.0 18.3 Ia Lipunov (MASTER) 2011ip 01 13 47.59 -12 41 06.0 17.8 Ic Denisenko (Ka-Dar) 2011io 23 02 47.60 +08 48 09.8 16.2 Ia Balanutsa (MASTER) 2011il 07 35 08.62 +19 11 26.1 17.0 Ia Balanutsa (MASTER) 2011if 10 06 11.04 +25 09 01.5 18.5 II Astrotel 2011ib 11 44 39.27 +35 58 03.9 16.8 IIn Shumkov (MASTER) 2011hz 08 52 34.24 +55 15 14.2 18.2 Ia Denisenko (Ka-Dar) 2011hx 02 32 07.96 +41 05 00.5 18.3 II Astrotel 2011hh 02 57 04.61 +49 47 43.3 16.9 Ia Lipunov (MASTER) 2011ha 03 57 40.87 +10 09 55.2 18.5 Ia Balanutsa (MASTER) 2011ft 17 52 42.98 +29 04 10.6 17.1 Ib Balanutsa, Lipunov (MASTER) All Russian SNe discovered in 2011
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Belissima 2012 :: MASTER Robotic Network MASTER discoveries of CV (since the start of 2012) MASTER designationMag.SiteDate (UT)Telegram OT J061730.02+354036.614.5VAmur2011-12-28.572ATel 3843 OT J105123.02+672528.314.6VAmur2012-01-01.700ATel 3845 OT J061431.44+415904.418.4CKislo.2012-01-14.861ATel 3866 OT J124819.37+072049.616.8CKislo.2012-01-21.045ATel 3875 OT J021216.01+461154.514.4CTunka2012-01-29.577ATel 3898 OT J124346.19+160504.116.8CKislo.2012-02-16.027ATel 3935 OT J064757.28+594811.318.4CTunka2012-02-16.779ATel 3935 OT J072948.66+593824.413.3CTunka2012-02-17.626ATel 3935 OT J033006.27+181233.116.1CKislo.2012-02-21.717ATel 3938 OT J070737.08+104933.716.0RAmur2012-03-16.478ATel 3981
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Belissima 2012 :: MASTER Robotic Network MASTER discoveries of CV in 2012 (continued) MASTER designationMag.SiteDate (UT)Telegram OT J072351.31+635526.216.1CAmur2012-03-18.505ATel 4001 OT J063425.03+434513.418.4CTunka2012-03-25.653ATel 4003 OT J174305.70+231107.815.6CAmur2012-04-05.831ATel 4022 OT J182201.93+324906.715.4CAmur2012-04-29.791ATel 4084 OT J184809.40+395440.516.0CKislo.2012-04-30.953ATel 4084 OT J221621.91+705415.515.3CAmur2012-06-03.656ATel 4150 OT J221811.12+654219.914.3CAmur2012-06-03.655ATel 4150 OT J211258.65+242145.412.9CKislo.2012-06-24.859ATel 4208 OT J225350.78+364434.517.8CAmur2012-06-25.728ATel 4213 Note: 2 CVs on June 03 were discovered on 2 images separated by 96 sec.
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Belissima 2012 :: MASTER Robotic Network Results 2011-2012 More than 70 GCN Circulars posted More than 70 GCN Circulars posted ~150 OT detections (SNe, CVs, orphan OT, high-PM cool dwarf) published in Astronomer’s Telegram (ATel) ~150 OT detections (SNe, CVs, orphan OT, high-PM cool dwarf) published in Astronomer’s Telegram (ATel) More than 4000 Minor Planet positions reported to MPC More than 4000 Minor Planet positions reported to MPC 20 IAU Electronic Telegrams published 20 IAU Electronic Telegrams published
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Belissima 2012 :: MASTER Robotic Network Confirmation of outbursts discovered by other projects MIS V1448 in Cygnus On 2012 JuneS. Yoshida has reported the outburst of the new variable at mag 13.4 on 2012 May 27 images from MISAO project. On 2012 June 08 in [vsnet-alert 14643] S. Yoshida has reported the outburst of the new variable at mag 13.4 on 2012 May 27 images from MISAO project. Checking MASTER database has shown the star went into outburst at least on 2012 May 13 and was as bright as 12.1! Prediscovery photometry was reported in [vsnet-alert 14643] one hour later Checking MASTER database has shown the star went into outburst at least on 2012 May 13 and was as bright as 12.1! Prediscovery photometry was reported in [vsnet-alert 14643] one hour later.
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Belissima 2012 :: MASTER Robotic Network MIS V1448 = 2MASS 19591944+5625208
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Belissima 2012 :: MASTER Robotic Network Nova Sgr 2012 No.4 prediscovery image by MASTER-ICATE
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Belissima 2012 :: MASTER Robotic Network Brightest MASTER CV so far OT J211258.65+242145.4 Constellation: Vulpecula Range: 12.9C-20.8B Type: UGWZ Period: 0.0598d (86.1 min) Published: ATel 4208, 2012 June 25
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Belissima 2012 :: MASTER Robotic Network OT J211258.65+242145.4
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Belissima 2012 :: MASTER Robotic Network 10000 observations in 30 days since the discovery!
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Belissima 2012 :: MASTER Robotic Network 7 rebrightenings in the next 25 days!
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Belissima 2012 :: MASTER Robotic Network Perspectives Southern OTs with MASTER-Argentina Southern OTs with MASTER-Argentina Photometric follow-up with MASTER- Vostryakovo and University telescopes Photometric follow-up with MASTER- Vostryakovo and University telescopes Spectroscopic identification with future 2.5-m MSU telescope near Kislovodsk Spectroscopic identification with future 2.5-m MSU telescope near Kislovodsk Search for eclipses in our database Search for eclipses in our database Detailed statistical analysis Detailed statistical analysis
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Belissima 2012 :: MASTER Robotic Network Perspectives: 2013
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Belissima 2012 :: MASTER Robotic Network http://observ.pereplet.ru http://masternet.sai.msu.ru/ lipunov2007@gmail.com d.v.denisenko@gmail.com
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