{"id":538,"date":"2010-02-28T18:51:37","date_gmt":"2010-03-01T02:51:37","guid":{"rendered":"http:\/\/jazzistentialism.com\/blog\/?page_id=538"},"modified":"2018-07-18T08:49:47","modified_gmt":"2018-07-18T00:49:47","slug":"538-2","status":"publish","type":"page","link":"http:\/\/jazzistentialism.com\/blog\/?page_id=538","title":{"rendered":"Papers and Published Observations"},"content":{"rendered":"

Updated July 2018<\/p>\n

Shenton Park Observatory (MPC D21) has undertaken serious astronomical research since 2005. The primary areas include supernova discovery, minor planet (NEO) recovery and follow-up and spectroscopic observations and research of bright stars.<\/p>\n

Spectroscopy<\/strong><\/p>\n

ATel #6380<\/strong><\/em>  The stability of the He II 4686 line emission across periastron passages in eta Carinae<\/a><\/p>\n

ATel #6464<\/strong><\/em>  He II 4686 in eta Carinae: no significant changes between 2009.0 and 2014.6<\/a><\/p>\n

The <\/em>Astrophysical Journal (March, 2016)<\/em><\/strong>: He II 4686 emission from the massive binary system in eta Car: constraints to the orbital elements and the nature of the periodic minima – Teodoro et al.<\/a><\/p>\n

ATel #9658 (October, 2016)<\/strong><\/em>  Confirmation of TCP J18102829-2729590 in Sagittarius as a classical nova in the optically thick stage<\/a><\/p>\n

ATel #9678 (October 2016)<\/strong><\/em>  Spectroscopic confirmation of ASASSN-16ma as a classical nova in the Fe-curtain stage<\/a><\/p>\n

Monthly Notices of the Royal Astronomical Society (May, 2017)<\/strong>: <\/em>V473 Lyr, a modulated, period-doubled Cepheid, and U TrA, a double-mode Cepheid observed by MOST<\/a><\/p>\n

ATel #10399 (May, 2017)<\/strong><\/em>  Spectroscopic observations of ASASSN-17gk<\/a> (and errata ATel #10400<\/a>).<\/p>\n

Monthly Notices of the Royal Astronomical Society (July, 2017) <\/strong><\/em>The variability of the BRITE-est Wolf\u2013Rayet binary, \u03b32 Velorum\u2013I. Photometric and spectroscopic evidence for colliding winds<\/a><\/p>\n

ATel #10737 (September, 2017)<\/strong><\/em>  Continuing ARAS visible spectroscopic monitoring of the slow classical nova Sct 2017 = ASASSN-17hx<\/a>.<\/p>\n

Nature Astronomy (Sepember, 2017) <\/em><\/strong><\/span>A nova outburst powered by shocks<\/a><\/p>\n

ATel #10795 (September, 2017)<\/strong><\/em>  Spectroscopic confirmation of ASASSN-17mt as a classical nova in the optically thick (Fe curtain) stage<\/a>.<\/p>\n

Astronomy and Astrophysics (forthcoming paper)<\/em><\/span> <\/strong>A combined HST and XMM-Newton campaign for the magnetic O9.7 V star HD 54879. Constraining the weak-wind problem of massive stars<\/a><\/p>\n

Monthly Notices of the Royal Astronomical Society <\/strong><\/em>BRITE-Constellation high-precision time-dependent photometry of the early-O-type supergiant \u03b6 Puppis unveils the photospheric drivers of its small- and large-scale wind structures<\/a><\/p>\n

Journal of the British Astronomical Association <\/strong><\/em>Spectroscopic observation of planetary nebulae<\/a><\/p>\n

ATel #11460 <\/strong><\/em>Spectroscopic Observations of ASASSN-18fv as a Classical Nova in the Iron Curtain Phase<\/a><\/p>\n

Supernova Discoveries (2005 – 2008)<\/strong><\/p>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
Name<\/strong><\/td>\nType<\/strong><\/td>\nDiscovery date<\/strong><\/td>\nGalaxy<\/strong><\/td>\nReference<\/strong><\/td>\n<\/tr>\n
2008bq<\/td>\nType Ia<\/td>\nApril 2, 2008<\/td>\nESO 308-G25<\/td>\nCBET 1328<\/em><\/td>\n<\/tr>\n
2007as<\/td>\nType Ia<\/td>\nMarch 13, 2007<\/td>\nESO 18-G18<\/td>\nCBET 888, IAUC 8822<\/em><\/td>\n<\/tr>\n
2006du<\/td>\nType II<\/td>\nJuly 18, 2006<\/td>\nIC 1529<\/td>\nCBET 583,  IACU 8733<\/em><\/td>\n<\/tr>\n
2006ck<\/td>\nType Ic<\/td>\nMay 20, 2006<\/td>\nUGC 8238<\/td>\nCBET 518, IAUC 8713<\/em><\/td>\n<\/tr>\n
2006bs<\/td>\nType II<\/td>\nApril 19, 2006<\/td>\nMCG +0-27-14<\/td>\nCBET 484, IAUC 8705<\/em><\/td>\n<\/tr>\n
2006ai<\/td>\nType II<\/td>\nFebruary 17, 2006<\/td>\nESO 5-G9<\/td>\nCBET 406, IAUC 8674<\/em><\/td>\n<\/tr>\n
2006y<\/td>\nType II<\/td>\nFebruary 3, 2006<\/td>\nAnon<\/td>\nIAUC 8668<\/em><\/td>\n<\/tr>\n
2005my<\/td>\nType II<\/td>\nDecember 30, 2005<\/td>\nESO 302-G27<\/td>\nCBET 346<\/em><\/td>\n<\/tr>\n
2005gm<\/td>\nType IIn<\/td>\nOctober 9, 2005<\/td>\nNGC 1423<\/td>\nCBET 251, IAUC 8616<\/em><\/td>\n<\/tr>\n
2005dk<\/td>\nType II<\/td>\nAugust 21, 2005<\/td>\nIC 4882<\/td>\nIAUC 8586<\/em><\/td>\n<\/tr>\n
2005dc<\/td>\nType Ia<\/td>\nJuly 26, 2005<\/td>\nNGC 7107<\/td>\nCBET 187, IAUC 8575<\/em><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

 <\/p>\n

Minor Planet Discoveries (2007 – 2010)<\/strong><\/p>\n

2007 PG9<\/strong> \u2013 a bright main belt asteroid discovered at D21 Shenton Park. It currently has a 177 day observed arc.<\/p>\n

2009 TV9 <\/strong>\u2013 a bright Mars Crosser discovered at D21 Shenton Park on October 8th<\/sup>, 2009. It has a perihelion of 1.56AU and a relatively high eccentricity of 0.41.<\/p>\n

2010 OE100 <\/strong> – a main belt asteroid with an orbit that appears more eccentric and with a lower perihelion than typical main belt asteroids.<\/p>\n

Published NEO Observations<\/strong><\/p>\n

The list of published NEO observations for D21, Shenton Park stands at 950 and is too large to list here. A full updated list is published at the NEODys website:<\/p>\n

http:\/\/newton.dm.unipi.it\/neodys\/index.php?pc=2.1.2&o=D21&ab=0<\/a><\/p>\n

Published Minor Planet Observations<\/strong><\/p>\n

These are too numerous to list here, and can be found via the Minor Planet Circulars listed at the end of this section.<\/p>\n\n\n\n\n\n\n\n
Year<\/strong><\/td>\nNumber<\/strong><\/td>\n<\/tr>\n
2003<\/td>\n30<\/td>\n<\/tr>\n
2007<\/td>\n887<\/td>\n<\/tr>\n
2009<\/td>\n487<\/td>\n<\/tr>\n
2010<\/td>\n647*<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

Published NEO Recoveries<\/strong><\/p>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
Object<\/strong><\/td>\nDate<\/strong><\/td>\nReference<\/strong><\/td>\n<\/tr>\n
2002 SV<\/td>\nAugust 11, 2007<\/td>\nMPEC 2007-P41<\/em><\/td>\n<\/tr>\n
2000 TH1<\/td>\nOctober 2, 2007<\/td>\nMPEC 2007-T14<\/em><\/td>\n<\/tr>\n
2004 RK9<\/td>\nMay 25, 2009<\/td>\nMPEC 2009-K56<\/em><\/td>\n<\/tr>\n
2005 TY51<\/td>\nSept 4, 2009<\/td>\nMPEC 2009-R06<\/em><\/td>\n<\/tr>\n
2008 WB59<\/td>\nSept 25, 2009<\/td>\nMPEC 2009-S110<\/em><\/td>\n<\/tr>\n
2008 VK14<\/td>\nApril 18, 2010<\/td>\nMPEC 2010-H28<\/em><\/td>\n<\/tr>\n
2007 XB10<\/td>\nApril 20, 2010<\/td>\nMPEC 2010-H31<\/em><\/td>\n<\/tr>\n
2008 JP<\/td>\nMay 4, 2010<\/td>\nMPEC 2010-J15<\/em><\/td>\n<\/tr>\n
2002 BF25<\/td>\nJuly 4,2010<\/td>\nMPEC 2010-N10<\/em><\/td>\n<\/tr>\n
2002 AC9<\/td>\nJuly 20, 2010<\/td>\nMPEC 2010-O13<\/em><\/td>\n<\/tr>\n
2002 NE71<\/td>\nAugust 2, 2010<\/td>\nMPEC 2010-P05<\/em><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

 <\/p>\n

Published NEO Confirmations<\/strong><\/p>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
Object<\/strong><\/td>\nDate<\/strong><\/td>\nReference<\/strong><\/td>\n<\/tr>\n
2007 SP6<\/td>\nSeptember 22, 2007<\/td>\nMPEC 2007-S44<\/em><\/td>\n<\/tr>\n
2007 VG3<\/td>\nNovember 4, 2007<\/td>\nMPEC 2007-V22<\/em><\/td>\n<\/tr>\n
2007 VY7<\/td>\nNovember 4, 2007<\/td>\nMPEC 2007-V39<\/em><\/td>\n<\/tr>\n
2007 VD138<\/td>\nNovember 10, 2007<\/td>\nMPEC 2007-V85<\/em><\/td>\n<\/tr>\n
2007 VG184<\/td>\nNovember 13, 2007<\/td>\nMPEC 2007-V91<\/em><\/td>\n<\/tr>\n
2007 VJ184<\/td>\nNovember 13, 2007<\/td>\nMPEC 2007-V93<\/em><\/td>\n<\/tr>\n
2007 VK184<\/td>\nNovember 13, 2007<\/td>\nMPEC 2007-V94<\/em><\/td>\n<\/tr>\n
2007 VF189<\/td>\nNovember 13, 2007<\/td>\nMPEC 2007-V119<\/em><\/td>\n<\/tr>\n
2007 WP3<\/td>\nNovember 18, 2007<\/td>\nMPEC 2007-W27<\/em><\/td>\n<\/tr>\n
2007 WW4<\/td>\nNovember 21, 2007<\/td>\nMPEC 2007-W47<\/em><\/td>\n<\/tr>\n
2007 WZ4<\/td>\nNovember 21, 2007<\/td>\nMPEC 2007-W49<\/em><\/td>\n<\/tr>\n
2009 QF31<\/td>\nAugust 26, 2009<\/td>\nMPEC 2009-Q56<\/em><\/td>\n<\/tr>\n
2009 QD34<\/td>\nAugust 28, 2009<\/td>\nMPEC 2009-Q60<\/em><\/td>\n<\/tr>\n
2009 QE34<\/td>\nAugust 28, 2009<\/td>\nMPEC 2009-Q61<\/em><\/td>\n<\/tr>\n
2009 SM98<\/td>\nSeptember 24, 2009<\/td>\nMPEC 2009-S87<\/em><\/td>\n<\/tr>\n
2009 SN103<\/td>\nSeptember 25, 2009<\/td>\nMPEC 2009-S100<\/em><\/td>\n<\/tr>\n
2009 TL4<\/td>\nOctober 14, 2009<\/td>\nMPEC 2009-T52<\/em><\/td>\n<\/tr>\n
2009 TH8<\/td>\nOctober 15, 2009<\/td>\nMPEC 2009-T62<\/em><\/td>\n<\/tr>\n
2009 TN8<\/td>\nOctober 15, 2009<\/td>\nMPEC 2009-T66<\/em><\/td>\n<\/tr>\n
2009 UO3<\/td>\nOctober 20, 2009<\/td>\nMPEC 2009-U53<\/em><\/td>\n<\/tr>\n
2010 HA<\/td>\nApril 16, 2010<\/td>\nMPEC 2010-H10<\/em><\/td>\n<\/tr>\n
2010 HF<\/td>\nApril 19, 2010<\/td>\nMPEC 2010-H18<\/em><\/td>\n<\/tr>\n
2010 JF<\/td>\nMay 4, 2010<\/td>\nMPEC 2010-J20<\/em><\/td>\n<\/tr>\n
2010 JG<\/td>\nMay 4, 2010<\/td>\nMPEC 2010-J21<\/em><\/td>\n<\/tr>\n
2010 PJ<\/td>\nAugust 4, 2010<\/td>\nMPEC 2010-P13<\/em><\/td>\n<\/tr>\n
2010 PO2<\/td>\nAugust 4, 2010<\/td>\nMPEC 2010-P18<\/em><\/td>\n<\/tr>\n
2010 PH9<\/td>\nAugust 6, 2010<\/td>\nMPEC 2010-P27<\/em><\/td>\n<\/tr>\n
2010 PJ9<\/td>\nAugust 6, 2010<\/td>\nMPEC 2010-P28<\/em><\/td>\n<\/tr>\n
2010 PK9<\/td>\nAugust 6, 2010<\/td>\nMPEC 2010-P29<\/em><\/td>\n<\/tr>\n
2010 PL9<\/td>\nAugust 6, 2010<\/td>\nMPEC 2010-P30<\/em><\/td>\n<\/tr>\n
2010 PM10<\/td>\nAugust 8, 2010<\/td>\nMPEC 2010-P39<\/em><\/td>\n<\/tr>\n
2010 PQ10<\/td>\nAugust 8, 2010<\/td>\nMPEC 2010-P41<\/em><\/td>\n<\/tr>\n
2010 PR10<\/td>\nAugust 8, 2010<\/td>\nMPEC 2010-P42<\/em><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

Published Special Interest NEO Revisions<\/strong><\/p>\n\n\n\n
2010 DJ1<\/td>\nFebruary 21, 2010<\/td>\nMPEC 2010-D60<\/em><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

 <\/p>\n

Published observations of unusual, one opposition objects<\/strong> observed last by D21, Shenton Park is available via the Minor Planet Centre and includes:<\/p>\n\n\n\n\n\n\n\n
One-Opposition Unnumbered Objects<\/td>\n<\/tr>\n
 <\/td>\n <\/td>\n <\/td>\n <\/td>\n2007 PS25<\/td>\n<\/tr>\n
2007 TT18<\/td>\n2007 TR24<\/td>\n2007 TC66<\/td>\n2007 UT3<\/td>\n2007 UF6<\/td>\n<\/tr>\n
2007 UL12<\/td>\n2007 VF189<\/td>\n2007 VE191<\/td>\n2007 WA<\/td>\n2009 CR4<\/td>\n<\/tr>\n
2009 RH<\/td>\n2009 SW17<\/td>\n2009 UD<\/td>\n <\/td>\n <\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

 <\/p>\n

Minor Planet Circulars<\/strong><\/p>\n

MPCs containing published observations from D21, Shenton Park (2003 – 2010).<\/p>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
Minor Planet Circular<\/strong><\/td>\nNumber of Observations<\/strong><\/td>\n<\/tr>\n
2003 Nov. 9<\/td>\n30<\/td>\n<\/tr>\n
2007 Aug. 28<\/td>\n266<\/td>\n<\/tr>\n
2007 Sept. 26<\/td>\n179<\/td>\n<\/tr>\n
2007 Oct. 26<\/td>\n78<\/td>\n<\/tr>\n
2007 Nov. 24<\/td>\n136<\/td>\n<\/tr>\n
2007 Dec. 24<\/td>\n228<\/td>\n<\/tr>\n
2009 June 7<\/td>\n92<\/td>\n<\/tr>\n
2009 Sept. 4<\/td>\n82<\/td>\n<\/tr>\n
2009 Oct. 4<\/td>\n100<\/td>\n<\/tr>\n
2009 Nov. 2<\/td>\n213<\/td>\n<\/tr>\n
2010 Jan. 30<\/td>\n3<\/td>\n<\/tr>\n
2010 Feb. 28<\/td>\n79<\/td>\n<\/tr>\n
2010 Mar. 30<\/td>\n12<\/td>\n<\/tr>\n
2010 Apr. 28<\/td>\n28<\/td>\n<\/tr>\n
2010 May 27<\/td>\n71<\/td>\n<\/tr>\n
2010 July 20<\/td>\n106<\/td>\n<\/tr>\n
2010 Aug. 24<\/td>\n348<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

 <\/p>\n

Variable Star Photometry<\/b><\/span><\/p>\n

As of October 2017, 1,360  observations of variable stars have been submitted to the AAVSO from photometry acquired at SPO. These can be found searching WebObs at aavso.org<\/a> using observatory code LPAE.<\/p>\n","protected":false},"excerpt":{"rendered":"

Updated July 2018 Shenton Park Observatory (MPC D21) has undertaken serious astronomical research since 2005. The primary areas include supernova discovery, minor planet (NEO) recovery and follow-up and spectroscopic observations and research of bright stars. Spectroscopy ATel #6380  The stability of the He … Continue reading →<\/span><\/a><\/p>\n","protected":false},"author":4,"featured_media":0,"parent":0,"menu_order":1,"comment_status":"closed","ping_status":"open","template":"","meta":{"ngg_post_thumbnail":0},"_links":{"self":[{"href":"http:\/\/jazzistentialism.com\/blog\/index.php?rest_route=\/wp\/v2\/pages\/538"}],"collection":[{"href":"http:\/\/jazzistentialism.com\/blog\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"http:\/\/jazzistentialism.com\/blog\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"http:\/\/jazzistentialism.com\/blog\/index.php?rest_route=\/wp\/v2\/users\/4"}],"replies":[{"embeddable":true,"href":"http:\/\/jazzistentialism.com\/blog\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=538"}],"version-history":[{"count":62,"href":"http:\/\/jazzistentialism.com\/blog\/index.php?rest_route=\/wp\/v2\/pages\/538\/revisions"}],"predecessor-version":[{"id":1987,"href":"http:\/\/jazzistentialism.com\/blog\/index.php?rest_route=\/wp\/v2\/pages\/538\/revisions\/1987"}],"wp:attachment":[{"href":"http:\/\/jazzistentialism.com\/blog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=538"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}