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

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

Belissima 2012 :: MASTER Robotic Network MASTER team

Belissima 2012 :: MASTER Robotic Network Somewhere near Moscow 10 years ago

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

Belissima 2012 :: MASTER Robotic Network MASTER photometer

Belissima 2012 :: MASTER Robotic Network Siberian Roof

Belissima 2012 :: MASTER Robotic Network MASTER Net in

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

Belissima 2012 :: MASTER Robotic Network MASTER Mount Manufacturer: ASTELCO Model: Model: NTM500 Pointing speed: up to 30 deg/sec Pointing accuracy: down to 10”

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.

Belissima 2012 :: MASTER Robotic Network MASTER nights SiteFNT,hCNT,hCNT,% Sky BG Ural % Tunka % Amur % Kislovodsk % Canarias ~70%

Belissima 2012 :: MASTER Robotic Network Night Control Center

Belissima 2012 :: MASTER Robotic Network MASTER results GRB pointing statistics during the winter of First PointingPrompt Pointing

Belissima 2012 :: MASTER Robotic Network The first synchronous polarization observations of gamma-ray burst in the world (2010 Sep. 06, MASTER)

Belissima 2012 :: MASTER Robotic Network GRB : gamma-ray burst from the textbook

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

Belissima 2012 :: MASTER Robotic Network

Big Synoptic Survey Theorem by Prof. Lipunov If you design synoptic telescope with diameter D, You must have spectral telescope with diameter ~ 10 D.

Belissima 2012 :: MASTER Robotic Network OT of unknown nature (19.4m): MASTER J

Belissima 2012 :: MASTER Robotic Network OT of unknown nature (19.4m): MASTER J

Belissima 2012 :: MASTER Robotic Network Supernova discoveries 2012de Ia Podvorotniy 2012dc Ia Shumkov (MASTER) 2012cd IIb Shurpakov (MASTER) 2012bp Ia Lipunov (MASTER) 2012bd IIP Lipunov (MASTER) 2012af Ia Lipunov (MASTER) 2012ae Ia Astrotel 2012K II Lipunov (MASTER) All Russian SNe discovered in 2012 so far

Belissima 2012 :: MASTER Robotic Network Supernova discoveries 2011jy II Lipunov (MASTER) 2011iq Ia Lipunov (MASTER) 2011ip Ic Denisenko (Ka-Dar) 2011io Ia Balanutsa (MASTER) 2011il Ia Balanutsa (MASTER) 2011if II Astrotel 2011ib IIn Shumkov (MASTER) 2011hz Ia Denisenko (Ka-Dar) 2011hx II Astrotel 2011hh Ia Lipunov (MASTER) 2011ha Ia Balanutsa (MASTER) 2011ft Ib Balanutsa, Lipunov (MASTER) All Russian SNe discovered in 2011

Belissima 2012 :: MASTER Robotic Network MASTER discoveries of CV (since the start of 2012) MASTER designationMag.SiteDate (UT)Telegram OT J VAmur ATel 3843 OT J VAmur ATel 3845 OT J CKislo ATel 3866 OT J CKislo ATel 3875 OT J CTunka ATel 3898 OT J CKislo ATel 3935 OT J CTunka ATel 3935 OT J CTunka ATel 3935 OT J CKislo ATel 3938 OT J RAmur ATel 3981

Belissima 2012 :: MASTER Robotic Network MASTER discoveries of CV in 2012 (continued) MASTER designationMag.SiteDate (UT)Telegram OT J CAmur ATel 4001 OT J CTunka ATel 4003 OT J CAmur ATel 4022 OT J CAmur ATel 4084 OT J CKislo ATel 4084 OT J CAmur ATel 4150 OT J CAmur ATel 4150 OT J CKislo ATel 4208 OT J CAmur ATel 4213 Note: 2 CVs on June 03 were discovered on 2 images separated by 96 sec.

Belissima 2012 :: MASTER Robotic Network Results 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

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.

Belissima 2012 :: MASTER Robotic Network MIS V1448 = 2MASS

Belissima 2012 :: MASTER Robotic Network Nova Sgr 2012 No.4 prediscovery image by MASTER-ICATE

Belissima 2012 :: MASTER Robotic Network Brightest MASTER CV so far OT J Constellation: Vulpecula Range: 12.9C-20.8B Type: UGWZ Period: d (86.1 min) Published: ATel 4208, 2012 June 25

Belissima 2012 :: MASTER Robotic Network OT J

Belissima 2012 :: MASTER Robotic Network observations in 30 days since the discovery!

Belissima 2012 :: MASTER Robotic Network 7 rebrightenings in the next 25 days!

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

Belissima 2012 :: MASTER Robotic Network Perspectives: 2013

Belissima 2012 :: MASTER Robotic Network