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Prossime Aperture
APERTURE PUBBLICHE DA APRILE 2019  PER TUTTO IL PERIODO DELL'ANNO L'OSSERVATORIO ASTRONOMICO APRE SOLO SU PRENOTAZIONE per gruppi con minimo di 20 ad un massimo di 50 persone INFO: 334-7313710 | APERTURA STRAORDINARIA SABATO 29 DICEMBRE 2018 ORE 18:00  LA STELLA DI BETLEMME tra realtà storica, religiosa e astronomica per riscoprire il Santo Natale Osservazione, visita attrezzature e meteoriti SOLO SU PRENOTAZIONE: max 50 persone | APERTURA STRAORDINARIA SABATO 5 GENNAIO 2019 ORE 18:00 LA STELLA DI BETLEMME tra realtà storica, religiosa e astronomica per riscoprire il Santo Natale Osservazione, visita attrezzature e meteoriti SOLO SU PRENOTAZIONE: max 50 persone | APERTURE PUBBLICHE DA APRILE 2019 PER TUTTO IL PERIODO DELL'ANNO L'OSSERVATORIO ASTRONOMICO APRE SOLO SU PRENOTAZIONE per gruppi con minimo di 20 ad un massimo di 50 persone INFO: 334-7313710 | ||
Prossime Aperture Pubbliche 2018
PRIMA APERTURA PUBBLICA SABATO 13 APRILE 2019 ORE 21:00  LE COSTELLAZIONI Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | SECONDA APERTURA PUBBLICA SABATO 11 MAGGIO 2019 ORE 21:00  IL SISTEMA SOLARE INTERNO Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | TERZA APERTURA PUBBLICA SABATO 1 GIUGNO 2019 ORE 21:00 IL SISTEMA SOLARE ESTERNO Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | QUARTA APERTURA PUBBLICA SABATO 8 GIUGNO 2019 ORE 21:00 IL SOLE: LA NOSTRA STELLA Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | QUINTA APERTURA PUBBLICA SABATO 29 GIUGNO 2019 ORE 21:00 LA VITA DELLE STELLE Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | SESTA APERTURA PUBBLICA SABATO 6 LUGLIO 2019 ORE 21:00  LA VIA LATTEA Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | SETTIMA APERTURA PUBBLICA SABATO 13 LUGLIO 2019 ORE 21:00 LA LUNA Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | OTTAVA APERTURA PUBBLICA SABATO 20 LUGLIO 2019 ORE 21:00  APOLLO 11: 50 ANNIVERSARIO Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | NONA APERTURA PUBBLICA SABATO 3 AGOSTO 2019 ORE 21:00  CORPI MINORI DEL SISTEMA SOLARE Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | TRE APERTURE PUBBLICHE 10-11-12 AGOSTO 2019 ORE 21:00 LE PERSEIDI: NOTTE DI SAN LORENZO Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | TREDICESIMA APERTURA PUBBLICA SABATO 24 AGOSTO 2019 ORE 21:00 IL PROFONDO CIELO Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | QUATTORDICESIMA APERTURA PUBBLICA SABATO 31 AGOSTO 2019 ORE 21:00  LE GALASSIE Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | QUINDICESIMA APERTURA PUBBLICA SABATO 7 SETTEMBRE 2018 ORE 21:00  STELLE, BUCHI NERI, WORMHOLE: L'ULTIMA FRONTIERA DELLA FISICA Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | SEDICESIMA APERTURA PUBBLICA SABATO 21 SETTEMBRE 2018 ORE 21:00  LA VITA AL DI LA' DELLA TERRA Visita Osservatorio, attrezzature e meteoriti Meteo permettendo spiegazione del cielo e osservazione con i telescopi NON SERVE PRENOTAZIONE | ||
Ultimi eventi (Ml > 2.0) rilevati dalla rete INGV, filtrati per una distanza di da Osservatorio Astronomico Monte Baldo
Eventi registrati dalla stazione sismografica MBAL - Osservatorio Astronomico Monte Baldo "A.Gelodi" - Novezzina
Evento | Data | Ora Locale | Magnitudo | Coordinate | Località | Profondità | Distanza | Direzione |
20:17:36 | 2.0 | 45.81,10.95 | Brentonico (TN) | 13 km | 1.0 km | S | ||
11:22:11 | 2.2 | 45.73,10.66 | Gargnano (BS) | 5 km | 4.0 km | N | ||
| 11:18:00 | 2.3 | 45.74,10.66 | Gargnano (BS) | 5 km | 5.0 km | N | ||
11:15:46 | 3.4 | 45.73,10.68 | Tignale (BS) | 3 km | 3.0 km | W | ||
11:31:00 | 2.4 | 45.65,10.72 | San Zeno di Montagna (VR) | 7 km | 2.0 km | NW | ||
11:18:35 | 2.2 | 45.65,10.70 | San Zeno di Montagna (VR) | 8 km | 3.0 km | W | ||
19:03:55 | 3.2 | 45.66,10.70 | San Zeno di Montagna (VR) | 10 km | 4.0 km | NW | ||
20:00:56 | 3.6 | 45.67,10.69 | Gargnano (BS) | 8 km | 3.3 km | SE | ||
Evento: Link su eventi INGV - Data: link su News OMB - Eventi registrati stazione MBAL >=2 | ||||||||
Rivivi con noi la Festa dell'astronomia
ASTROVEN III - 13/10/2018 VERONA
2020 The optical counterpart of the X-ray source 2SXPS J173508.4-292958 is a new, yellow-type symbiotic star. U. Munari (INAF Padova), P. Valisa, S. Dallaporta, A. Vagnozzi, V. Andreoli, F. Castellani (ANS Collaboration) With an assortment of telescopes operated by ANS Collaboration, we have obtained optical spectroscopy (low and high resolution) and BVRI photometry of the optical counterpart of 2SXPS J173508.4-292958, the source recently reported by Heinke et al. (ATel #13648) to have brightened in the X-rays. (Atel13660) (PDF) LAMOST J202629.80+423652.0 is not a symbiotic star - V. Andreoli and U. Munari Abstract. LAMOST J202629.80+423652.0 has been recently classi ed as a new symbiotic star containing a long-period Mira, surrounded by dust (D- type) and displaying in the optical spectra high ionization emission lines, in- cluding the Raman-scattered OVI at 6825 A. We have observed LAMOST J202629.80+423652.0 photometrically in the BVRI bands and spectroscopically over the 3500-8000 A range. (CAOSP Vol.50) (PDF) The OMB-supernova monitoring (ISSP collaboration), R.Belligoli, F.Castellani, C.Marangoni, F.Marziali reports the discovery of a PSN J16393220+6602141 SN2020gpe in NGC6214 by a Moravian G4-9000 KAF unfiltered CCD frames taken on '2020-04-12T03:21:49' UT on the 0.4m f.8 Ritchey-Chrétien telescope. The object observed is located at RA= '16 39 32.19' DEC= '+66 02 14.01' (equinox 2000.0) Offset 2"W 9"S from the center of NGC6214 galaxy (see link to discovery image below). Apparent magnitude 17.0 Clear (err +/- 0,5). (Atel13640) (PDF) We report the independent discovery of a probable nova in M31 on a co-added 810-s R-band CCD frame taken on 2020 Mar. 15.768 UT with the 0.65-m telescope at Ondrejov. The object was independently discovered and first announced by F. Castellani and R. Belligoli and designated as PNV J00424612+4111362 = AT 2020emi. The object was designated by us as M31N 2020-03c and is located at R.A. = 0h42m52s.16, Decl. = +41o13'37".2 (equinox 2000.0), which is 88.4" east and 151.3" south of the center of M31 ... (ATel_13561) (PDF) Remarks: F. Castellani, Verona, Italy reports the discovery by Flavio Castellani, Raffaele Belligoli and Claudio Marangoni, in the course of the ISSP Italian Supernovae Search Project, of an apparent nova in two images taken with a Moravian G4-9000 KAF CCD unfiltered, from Monte Baldo Observatory (Ferrara di Monte Baldo, Verona, Italy), with the 0.4m f.8 Ritchey-Chrétien telescope, obtained on 2020 March 04.7596. The new object is located at RA 00 42 08.56 DEC +41 26 00.8 (equinox 2000.0) Apparent magnitude about 18.0 in host Galaxy M31 Nothing is visible at this position on the reference image taken on 2020-02-28.769... (TNS Astronomical Transient Report No. 63512) 2019 The 2018 eruption and long-term evolution of the new high-mass Herbig Ae/Be object Gaia-18azl = VES 263 MNRAS U. Munari, V. Joshi, D. P. K. Banerjee, K. Cotar, S. Y. Shugarov, R. Jurdana-Sepi, R. Belligoli, A. Bergamini, M. Graziani, G. L. Righetti, A. Vagnozzi and P. Valisa We have been monitoring, at high cadence, the photometric and spectroscopic evolution of VES 263 following the discovery in 2018 of a brightening labelled as event Gaia-18azl. VES 263 is so far a neglected emission-line object discovered in the 1960s on objective prism plates, tentatively classified as a semiregular AGB cool giant by automated analysis of ASASSN light curves. We have discovered that VES 263 is a bona fide massive pre-mainsequence object (∼12 M), of the Herbig AeBe type. (MNRAS 488, 5536–5550 (2019) (PDF) 2018 Liverpool Telescope classification of optical transients AT2018hho and AT2018hhy ATel #12138; S. C. Williams (Lancaster), M. J. Darnley (LJMU), M. W. Healy (LJMU) on 22 Oct 2018; 22:36 UT Credential Certification: Steven Williams (s.williams7@lancaster.ac.uk) A faint continuum is detected in each case, but the S/N is too low for a classification. AT2018hho was observed at 2018-10-16.94 UT. We detect a Hα emission line with FWHM ~ 3100 km/s. We obtained a spectrum of AT2018hhy at 2018-10-17.99 UT, which shows TiO absorption bands on a red continuum, indicating that this object is a red LPV. We also note that there is a variable coincident with the position of AT2018hhy in Macri et al. (2001) and Hartman et al. (2006). (Atel_12138) (PDF) Independent INT/WFC discovery, improved position and IAC80/CAMELOT photometry of AT2018hho (= PNV J00424012+4117273) in M31 ATel #12127; Credential Certification: Ismael Perez-Fournon (ipf@iac.es) We report the independent discovery of a nova candidate in M31 on CCD images taken from 2018 Oct 13.937 to 2018 Oct 14.176 with the Wide Field Camera of the Isaac Newton Telescope. The discovery of this nova candidate was reported to TNS by Raffaele Belligoli, Flavio Castellani and Claudio Marangoni. We also observed AT2018hho with the CAMELOT CCD camera of the IAC80 telescope at Teide Observatory in Tenerife on the same night. (Atel_12127) (PDF) Independent Discovery of PNV J00424012+4117273 and Confirmation of PNV J01334673+3032181 ATel #12113; K. Hornoch (Astronomical Institute, Ondrejov, Czech Republic) on 15 Oct 2018; 07:55 UT Credential Certification: Matt Darnley (M.J.Darnley@ljmu.ac.uk) I report the independent discovery of a probable nova in M31 on a co-added 770-s R-band CCD frame taken on 2018 Oct. 14.740 UT with the 0.65-m telescope at Ondrejov. The object was independently discovered by R. Belligoli et al. (designated as PNV J00424012+4117273 = AT2018hfs) and is located at R.A. = 0h42m40s.11, Decl. = +41o17'26".9 (equinox 2000.0), which is 47.5" west and 78.4" north of the center of M31. (Atel_12113) (PDF) The Mass Accretion Rate of the Young Variable Star GM Cep Authors: Giannini, T.; Munari, U.; Lorenzetti, D.; Antoniucci, S.; Castellani, F.; Dallaporta, D.; Jurdana-Šepić, R. Affiliation: AA(INAF—Osservatorio Astronomico di Roma—Via Frascati, 33—Monte Porzio Catone I-00078, Italy Electronic On-line Article (HTML) - (PDF) The super-soft X-ray and CH/Ba-enhanced symbiotic star StHa 32 is in outburst ATel #11304; U. Munari (INAF Padova), S. Dallaporta, M. Graziani, G. L. Righetti, S. Tomaselli, S. Moretti, A. Maitan, F. Castellani, P. Valisa, L. Baldinelli (ANS Collaboration) on 15 Feb 2018; 11:12 UT Credential Certification: U. Munari (ulisse.munari@oapd.inaf.it) The supersoft X-ray source, Barium-enhanced, metal-deficient and Halo symbiotic star StHa 32 in going into outburst, the first ever recorded to the best of our knowledge.(ATel_11304) Asiago spectroscopic classification of 3 transients The Asiago Transient Classification Program (Tomasella et al. 2014, AN, 335, 841) reports the spectroscopic classification of AT 2018eq discovered by R. Belligoli (ISSP) in the direction of M31; PS18bq (AT2018bi) discovered by J. Grzegorzek and Pan-STARRS1 in UGC1791; and AT2018C (= Gaia18aak), a blue hostless transient discovered by Gaia. The observations were performed with the Asiago 1.82 m Copernico Telescope equipped with AFOSC (range 340-820 nm; resolution 1.4 nm).(ATel_11168) 2017 Spectroscopic classification AT 2017jdm as a nova, and likely recurrent eruption of M31N 2007-10b We obtained a spectrum of the transient AT 2017jdm (discovered by F. Castellani, R. Belligoli, C. Marangoni and F. Marziali; see TNS) with the SPRAT spectrograph (resolution R ~ 350; Piascik et al. 2014) on the 2-m Liverpool Telescope (Steele et al. 2004) on 2017 Dec 24.86 UT. (Atel_11088) A sudden brightness decrease of the young pre-MS object GM Cep U. Munari (INAF - Osservatorio Astronomico di Padova, Italy), F. Castellani (ANS Collaboration, Italy), T. Giannini, S. Antoniucci, D. Lorenzetti (INAF - Osservatorio Astronomico di Roma, Monte Porzio, Italy) on 24 Nov 2017; 14:38 UT Credential Certification: Simone Antoniucci (antoniucci@oa-roma.inaf.it) (Atel_11004) Nova ASASSN-17hx fast returning to maximum brightness, now at much larger velocities U. Munari (INAF Padova), P. Ochner (Univ. Padova), F.-J. Hambsch, A. Frigo, F. Castellani, A. Milani, P. Valisa, A. Vagnozzi (ANS Collaboration) on 11 Sep 2017; 21:54 UT Credential Certification: U. Munari (ulisse.munari@oapd.inaf.it) Nova ASASSN-17hx continues its unexpected and rapid re-brightening (ATel #10725), approaching the brightness attained at primary maximum when it peaked at B=9.65, V=8.44, R=7.79, I=7.05 around July 30.1 UT (ATel #10641)... (ATel_10736) "Photometry and spectroscopy of declining Nova ASASSN-17hx, now passing at t_2" U. Munari (INAF Padova), G. Traven (Univ. Ljubljana), F.-J. Hambsch, F. Castellani, A. Frigo, A. Milani, P. Valisa (ANS Collaboration), P. Ochner (Univ. Padova) ASASSN-17hx was discovered (Atel #10524) when still >4 mag below and ~41 days before maximum. Spectral classification and pre-maximum evolution have been reported (Atel #10527, #10558, #10572, #10613), as well as the identification in the VVVX survey of a Ks=16.7 mag star as the likely progenitor of the nova, and recently UV observations and an upper limit to X-ray flux obtained with Swift (Atel 10636) (ATel_10641) "Photometry and spectroscopy of FeII nova ASASSN-17hx, finally passing through maximum" U. Munari (INAF Padova), F.-J. Hambsch, A. Frigo, F. Castellani (ANS Collaboration),G. La Mura (Univ. Padova), G. Traven (Univ. Ljubljana), M. Ozbey Arabaci, T. Saguner (Ataturk Univ.) on 13 Jul 2017; 10:08 UT Credential Certification: U. Munari (ulisse.munari@oapd.inaf.it) More than two weeks past its discovery, nova ASASSN-17hx has finally reached what appears to be its peak optical brightness. Announced as a candidate nova on June 23.7 UT (ATel #10523), we begun daily photometric monitoring of ASASSN-17hx on June 24.07 UT when we measured V=12.39, B-V=+0.72, V-I=+1.19. After a monotonic - although structured - rise toward maximum, peak brightness has been reached at V=10.90, B-V=+0.85 on June 10, followed by a slow decline. (ATel_10572) After 23 years the yellow symbiotic star LT Del is again in outburst U. Munari (INAF Padova), P. Ochner (Univ. Padova), S. Dallaporta and R.Belligoli (ANS Collaboration) The ANS Collaboration photometric and spectroscopic monitoring of symbiotic stars has detected LT Del (= Hen 2467 = PK 06312.1 = StHa 179) in outburst. This is the first recorded outburst since the last one of 19941995, which was discovered by Passuello et al. (1994, IAUC 6065 ) and described by Arkhipova et al. (1995a, ALett 21, 339; 1995b, ALett 21, 391). LT Del is steeply rising in brightness. Last ANS photometric observation on UT (ATel 10361) NOVA 2017-04b (= PNV J09551279+6900093) IN M81 The extended M81 nova monitoring collaboration reports the discovery of a probable nova in M81 on pair of co-added 3900-s and 4200-s unfiltered CCD frames taken on 2017 Apr. 18.799 UT and 18.848 UT, respectively with the 0.4-m telescope at the Monte Baldo Observatory, Verona, Italy (MBO). The object designated PNV J09551279+6900093 is located at R.A. = 9h55m12s.79, Decl. = +69o00'09".3 (equinox 2000.0), which is 109.4" west and 225.8" south of the center of M81 (see link to discovery image below). (see link to discovery image). Atel#10290 NOVA AT2017blf in M81 The M81 nova monitoring collaboration reports the independent discovery of an apparent nova in M81 on a coadded 3510s unfiltered CCD frame taken on 2017 Feb. 24.119 UT with the 0.65m telescope at Ondrejov.The object designated PNV J09563149+6907301 was first announced and designated AT2017blf by F. Castellani et al. (see here) and is located at R.A. = 9h56m31s.49, Decl. = +69o07'30".1 (equinox 2000.0), which is 312.1" east and 215.0" north of the center of M81 (see link to discovery image below). Atel#10133 NOVA AT2017axz in M81 The M81 nova monitoring collaboration reports the independent discovery of an apparent nova in M81 on a co-added 5400-s unfiltered CCD frame taken on 2017 Feb. 19.962 UT with the 0.65-m telescope at Ondrejov (OND). The object designated PNV J09553619+6906210 was first announced and designated AT2017axz by F. Castellani et al. NOVA AT2017axi in M31 Nova M31 2017-02a? (= AT2017axi), TNS discovered 2017/02/18.746 by Raffaele Belligoli et al.(ISSP) Found in M31 at R.A. = 00h42m38s.120, Decl. = +41°14'10".70 Located 3".0 east and 115".0 south of the center of M31 (Discovery image) (ISSP image) Mag 18.3:2/18, Type unknown (References: CBAT TOCP) 2016 MASTER Independent Detection: Possible Nova in M31 After our detection we found discovery information at Bishop pages by Emmanuel Conseil (see at TNS https://wis-tns.weizmann.ac.il/object/2016jbx ) Atel#9912 Indipendent and prediscovery nova AT2016jbx by R.Belligoli, F.Castellani, C.Marangoni and F.Marziali on TNS UAI AT2016jbx. Confirmation and Photometry of M31 Transients AT2016jbg and AT2016ize Roughly 2.9' almost directly west of AT2016jbg lies the transient AT2016ize, reported to the IAU-TNS by Belligoli et al. on 2016 December 21.7139 UT with an unfiltered magnitude of 18.5 from observations conducted with ISSP. ATel#9915 NOVA AT2016ize in M31 The object designated PNV J00424659+4116578 was first announced and designated AT2016ize by R. Belligoli et al. (see here) and is located at R.A. = 0h42m46s.59, Decl. = +41o16'57".8 (equinox 2000.0), which is 25.5" east and 49.3" north of the center of M31 (see link to discovery image below). Atel#9896 Congratulations! Your paper is one of the 5 most highly cited papers published in New Astronomy. Dear Dr. Munari, The editors of New Astronomy are delighted to inform you that your paper, BVRI lightcurves of supernovae SN 2011fe in M101, SN 2012aw in M95, and SN 2012cg in NGC 4424, published in 2013 is one of the most highly cited papers during 2014, 2015 and up until June 2016. We would like to take this opportunity to thank you for publishing with us and to congratulate you. See more... The 2016 outburst of the unique symbiotic star MWC 560 ( = V694 Mon), its long-term BVRI evolution and a marked 331 days periodicity U. Munari, S. Dallaporta, F. Castellani, L. Baldinelli, G.L. Righetti, M. Graziani, G. Cherini, A. Maitan, S. Moretti, S. Tomaselli, A. Frigo NewAstronomy_49_43.pdf SUPERNOVA AT2016bry IN UGC 11635 The Asiago Transient Classification Program (Tomasella et al. 2014, AN, 335, 841) reports the spectroscopic classification of AT2016bry, discovered by V. Tinella in UGC 11635, and preliminary photometric follow-up. Additional CCD magnitudes for AT2016bry: 2016-04-27.35 | Bj 15.87 +- 0.02 | Vj 15.57 +- 0.01 | Rc15.17 +- 0.01 (R. Belligoli, F. Castellani, Verona, Italy) ATel#9018; (2016) |
2015 SUPERNOVA 2015Q IN NGC 3888 = PSN J11473508+5558147 Additional CCD magnitudes for 2015Q: 19.905, 16.3 (R. Belligoli, F. Castellani, and C. Marangoni, Verona, Italy) CBET4128; (2015) "The symbiotic binary and super-soft X-ray source AG Dra is going into outburst" U. Munari (INAF Padova-Asiago), G. L. Righetti, U. Sollecchia, F. Castellani (ANS Collaboration) ATel #7582; (2015) 2014 “The symbiotic star Hen 2-468 is undergoing a rare and bright outburst” U. Munari (INAF-Padova), S. Dallaporta and F. Castellani (ANS Collaboration) ATel 6841; (2014) "The prototype symbiotic star AX Per is in outburst" U. Munari (INAF Padova-Asiago), S. Dallaporta, G. L. Righetti, F. Castellani, G. Cherini (ANS Collaboration) ATel 6382 (2014) Study of three 2013 novae: V1830 Aql, V556 Ser and V809 Cep U. Munari, P. Ochner, S. Dallaporta, P. Valisa, M. Graziani, G.L. Righetti, G. Cherini, F. Castellani, G. Cetrulo and A., Englaro MNRAS 440, 3402–3415 (2014) NOVA SCORPII 2014 = TCP J17154683-3128303 U. Munari, S. Dallaporta, F. Castellani, R. Belligoli Electronic Telegram No. 3841* NOVA CYGNI 2014 = PNV J20214234+3103296 U. Munari, G. Cetrulo, D. Degano, and F. Castellani Electronic Telegram No. 3842* Optical photometry of the rapidly declining Nova Scorpii 2014 U. Munari (INAF Padova-Asiago), S. Dallaporta, F. Castellani, C. Marangoni (ANS Collaboration) on 1 Apr 2014; 09:05 UT Credential Certification: U. Munari (ulisse.munari@oapd.inaf.it) Nova Scorpii 2014 was discovered as optical transient TCP J17154683-3128303 by Nishiyama and Kabashima, and classified from optical spectra as a nova by Jelinek et al (ATEL #6025). X-ray emission was detected on Swift observations by Kuulkers et al. (ATEL #6015),... (ATel_6034) NOVA CEPHEI 2014 = TCP J20542386+6017077 U. Munari, A. Milani, P. Valisa, F. Castellani, and R. Belligoli Electronic Telegram No. 3825 SUPERNOVA 2014J IN M82 = PSN J09554214+6940260 U. Munari, F. Castellani, R. Belligoli, G. L. Righetti Electronic Telegram No. 3792 The symbiotic star TX CVn has entered an active state. U. Munari, F. Castellani, P. Valisa, S. Dallaporta, G. Cherini, A. Vagnozzi, G. L. Righetti, R. Belligoli 14 Jan 2014; 15:56 UT ATel 5761 (2014) The Metrology of Supernova Lightcurves 223rd American Astronomical Society Meeting Authors: Rust, Bert W.1; Mullen, Katharine M.2 Institutions: 1. NIST, Gaithersburg, MD, United States. 2. UCLA, Los Angeles, CA, United States. 3. ANS Collaboration: U.Munari, Italia AAS 223_ 354abstract ASS223_354poster 2013 SUPERNOVA 2013ff IN NGC 2748 = PSN J09133888+7628108 Belligoli R, Castellani F. Cbet 3647 Cbet3656 Photometric evolution, orbital modulation and progenitor of Nova Mon 2012. Munari, U., Dallaporta, S., Castellani, F., Valisa, P., Frigo, A., Chomiuk, L., Ribeiro, V.A.R.M. MNRAS 435, 771 (2013) An ongoing active phase for the old symbiotic nova AG Peg Munari, U., Valisa, P., Dallaporta, S., Cherini, G.L. Righetti, G., Castellani, F. ATel 5258 (2013) BVRI lightcurves of supernovae SN 2011fe in M101, SN 2012aw in M95, and SN 2012cg in NGC 4424. Munari, U., Henden, A., Belligoli, R., Castellani, F., Cherini, G., Righetti, G.L., Vagnozzi, A. NewAstronomy 20, 30 (2013NewA...20...30M) Nova Cephei 2013 has emerged from dust obscuration U. Munari, P. Ochner, A. Siviero, M. Graziani, S. Dallaporta, G. L. Righetti, G. Cherini, F. Castellani ATel 5389 (2013) An ongoing active phase for the old symbiotic nova AG Peg Munari, U., Valisa, P., Dallaporta, S., Cherini, G.L. Righetti, G., Castellani, F. ATel 5258 (2013) The symbiotic star YY Her is in outburst Munari, U., Dallaporta S., Castellani F., Belligoli R., Cherini G., Righetti G.L., Graziani M., Valisa P., Milani A. ATel 4996 (2013) Is Nova Cep 2013 currently forming dust ? Munari, U., Dallaporta, S., Cherini, G., Castellani, F., Cetrulo, G., Valisa, P., Graziani, M. ATel 4893 (2013) The decline of the super-soft X-ray source in Nova Mon 2012. 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Frigo 2011, CBET, 2861 SUPERNOVA 2011fe IN M101 Magnitude estimates: B. Mikuz and J. Vales, Crni Vrh Observatory, W. Souza, F. Castellani and R. Belligoli, Monte Baldo, G. Masi, J. Carvajal,P. Schmeer, Bischmisheim. 2011 CBET 2804 2010 BVRcIc Photometric Evolution and Flickering during the 2010 Outburst of the Recurrent Nova U Scorpii Munari, U., Dallaporta, S., Castellani, F. 2010, IBVS, 5930, 1M AX Persei Munari U., Siviero, A., R.L.M. Corradi R.L.M., Valisa P., Cherini G., Castellani F., Dallaporta S. 2010, CBET, 2555. COMET C/2010 G1 (BOATTINI) A. Boattini, R. Ligustri , E. Pettarin, F. Castellani and C. Marangoni, P. Birtwhistle, L. Buzzi, J. E. McGaha 2010, IAUC 9133 CI Cygni U. Munari, (INAF Padova-Asiago, Italy), P. Valisa, A. Milani, G. Cherini, F. Castellani, S. Dallaporta, A. Siviero, A. Frigo (ANS Collaboration) 2010 (09 October), ATEL, 2913 2009 The 2006-2008 Outburst of AG Draconis Munari, U., Siviero, A., Ochner, P., Wallerstein, G., Castellani, F., Righetti, G., Cherini, G., Valisa, P., Cetrulo, G. 2009, PASP, 121, 1070 AX PERSEI Munari, U., Siviero, A., Dallaporta, S., Cherini, G., Valisa, P., Castellani, F., Frigo, A., Vagnozzi, A., Bacci, S., Righetti, G., Moretti, S., Tomaselli, S. 2009, CBET, 1757 Ongoing meteor work - A Comprehensive List of Meteor Showers Obtained from 10 Years of Observations with the IMO Video Meteor Network WGN, the Journal of the IMO 37:4 (2009) 2008 NOVA SAGITTARII 2008 Munari, U., Siviero, A., Moretti, S., Tomaselli, S., Maitan, A., Baldinelli, L., Castellani, F., Dallaporta, S., Ochner, P. 2008, CBET, 1352 V2468 CYGNI Munari, U., Siviero, A., Valisa, P., Dallaporta, S., Cherini, G., Ochner, P., Castellani, F., Buzzi, L., Brienza, M., Luppi, V. 2008, CBET, 1431 Characterization of the HD 17156 planetary system M. Barbieri, R. Alonso, S. Desidera, A. Sozzetti, A.F. Martinez Fiorenzano, J. M. Almenara, M. Cecconi, R.U.Claudi, D. Charbonneau, M. Endl, V. Granata, R. Gratton, G. Laughlin, B. Loeillet, Amateur Consortium ⋆⋆ E.A.C. observations obtained by: F. Castellani (Mt. BaldoObservatory), B. Gary, J. Gregorio, C. Lopresti, A. Marchini (SienaUniversity Observatory),M. Nicolini (Cavezzo Observatory), R. Papini, C. Vallerani 2008 Astronomy & Astrophysics manuscript no. barbieri˙hd17156 c arXiv:0812.0785v1 2007 V2467 Cygni (Nova Cyg 2007) Munari, U., Dalla Via, G., Valisa, P., Dallaporta, S., Castellani, F. 2007, CBET, 897 V919 Sgr Munari, U., Siviero, A., Navasardyan H., Castellani, F., Bortolotti M., Valisa, P., Luppi V. 2007, CBET, 999 AG DRACONIS Munari, U., Siviero, A., Castellani, F., Valisa, P., Cherini, G., Bano, I., Englaro, A., Cetrulo, G. 2007, CBET, 1091 The 2006 outburst of the recurrent nova RS Oph U. Munari, A. 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