{"title":"盖亚科学警报和塞尔维亚-保加利亚迷你网络望远镜的观测设施","authors":"G. Damljanovic, O. Vince, S. Boeva","doi":"10.2298/SAJ1488085D","DOIUrl":null,"url":null,"abstract":"The astrometric European Space Agency (ESA) Gaia mission was launched in \n December 19, 2013. One of the tasks of the Gaia mission is production of an \n astrometric catalog of over one billion stars and more than 500000 \n extragalactic sources. The quasars (QSOs), as extragalactic sources and radio \n emitters, are active galactic nuclei objects (AGNs) whose coordinates are \n well determined via Very Long Baseline Interferometry (VLBI) technique and \n may reach sub-milliarcsecond accuracy. The QSOs are the defining sources of \n the quasi-inertial International Celestial Reference Frame (ICRF) because of \n their core radio morphology, negligible proper motions (until \n sub-milliarcsecond per year), and apparent point-like nature. Compact AGNs, \n visible in optical domain, are useful for a direct link of the future Gaia \n optical reference frame with the most accurate radio one. Apart from the \n above mentioned activities, Gaia has other goals such as follow-up of \n transient objects. One of the most important Gaia's requirements for \n photometric alerts is a fast observation and reduction response, that is, \n submition of observations within 24 hours. For this reason we have developed \n a pipeline. In line with possibilities of our new telescope \n (D(cm)/F(cm)=60/600) at the Astronomical Station Vidojevica (ASV, of the \n Astronomical Observatory in Belgrade), we joined the Gaia-Follow-Up Network \n for Transients Objects (Gaia-FUN-TO) for the photometric alerts. Moreover, in \n view of the cooperation with Bulgarian colleagues (in the frst place, SV), \n one of us (GD) initiated a local mini-network of Serbian { Bulgarian \n telescopes useful for the Gaia-FUN-TO and other astronomical purposes. During \n the next year we expect a new 1.4 m telescope at ASV site. The speed of data \n processing (from observation to calibration server) could be one day. Here, \n we present an overview of our activities in the Gaia-FUN-TO which includes \n establishing Serbian { Bulgarian mini-network (of five telescopes at three \n sites, ASV in Serbia, Belogradchik and Rozhen in Bulgaria), the Gaia-FUN-TO \n test observations, and some results. [Projekat Ministarstva nauke Republike \n Srbije, br. 176011: Dynamics and kinematics of celestial bodies and systems, \n br. 176004: Stellar physics, i br. 176021: Visible and invisible matter in \n nearby galaxies: theory and observations]","PeriodicalId":48878,"journal":{"name":"Serbian Astronomical Journal","volume":"188 1","pages":"85-93"},"PeriodicalIF":0.8000,"publicationDate":"2014-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.2298/SAJ1488085D","citationCount":"1","resultStr":"{\"title\":\"Gaia science alerts and the observing facilities of the Serbian-Bulgarian mini-network telescopes\",\"authors\":\"G. Damljanovic, O. Vince, S. Boeva\",\"doi\":\"10.2298/SAJ1488085D\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The astrometric European Space Agency (ESA) Gaia mission was launched in \\n December 19, 2013. One of the tasks of the Gaia mission is production of an \\n astrometric catalog of over one billion stars and more than 500000 \\n extragalactic sources. The quasars (QSOs), as extragalactic sources and radio \\n emitters, are active galactic nuclei objects (AGNs) whose coordinates are \\n well determined via Very Long Baseline Interferometry (VLBI) technique and \\n may reach sub-milliarcsecond accuracy. The QSOs are the defining sources of \\n the quasi-inertial International Celestial Reference Frame (ICRF) because of \\n their core radio morphology, negligible proper motions (until \\n sub-milliarcsecond per year), and apparent point-like nature. Compact AGNs, \\n visible in optical domain, are useful for a direct link of the future Gaia \\n optical reference frame with the most accurate radio one. Apart from the \\n above mentioned activities, Gaia has other goals such as follow-up of \\n transient objects. One of the most important Gaia's requirements for \\n photometric alerts is a fast observation and reduction response, that is, \\n submition of observations within 24 hours. For this reason we have developed \\n a pipeline. In line with possibilities of our new telescope \\n (D(cm)/F(cm)=60/600) at the Astronomical Station Vidojevica (ASV, of the \\n Astronomical Observatory in Belgrade), we joined the Gaia-Follow-Up Network \\n for Transients Objects (Gaia-FUN-TO) for the photometric alerts. Moreover, in \\n view of the cooperation with Bulgarian colleagues (in the frst place, SV), \\n one of us (GD) initiated a local mini-network of Serbian { Bulgarian \\n telescopes useful for the Gaia-FUN-TO and other astronomical purposes. During \\n the next year we expect a new 1.4 m telescope at ASV site. The speed of data \\n processing (from observation to calibration server) could be one day. 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Gaia science alerts and the observing facilities of the Serbian-Bulgarian mini-network telescopes
The astrometric European Space Agency (ESA) Gaia mission was launched in
December 19, 2013. One of the tasks of the Gaia mission is production of an
astrometric catalog of over one billion stars and more than 500000
extragalactic sources. The quasars (QSOs), as extragalactic sources and radio
emitters, are active galactic nuclei objects (AGNs) whose coordinates are
well determined via Very Long Baseline Interferometry (VLBI) technique and
may reach sub-milliarcsecond accuracy. The QSOs are the defining sources of
the quasi-inertial International Celestial Reference Frame (ICRF) because of
their core radio morphology, negligible proper motions (until
sub-milliarcsecond per year), and apparent point-like nature. Compact AGNs,
visible in optical domain, are useful for a direct link of the future Gaia
optical reference frame with the most accurate radio one. Apart from the
above mentioned activities, Gaia has other goals such as follow-up of
transient objects. One of the most important Gaia's requirements for
photometric alerts is a fast observation and reduction response, that is,
submition of observations within 24 hours. For this reason we have developed
a pipeline. In line with possibilities of our new telescope
(D(cm)/F(cm)=60/600) at the Astronomical Station Vidojevica (ASV, of the
Astronomical Observatory in Belgrade), we joined the Gaia-Follow-Up Network
for Transients Objects (Gaia-FUN-TO) for the photometric alerts. Moreover, in
view of the cooperation with Bulgarian colleagues (in the frst place, SV),
one of us (GD) initiated a local mini-network of Serbian { Bulgarian
telescopes useful for the Gaia-FUN-TO and other astronomical purposes. During
the next year we expect a new 1.4 m telescope at ASV site. The speed of data
processing (from observation to calibration server) could be one day. Here,
we present an overview of our activities in the Gaia-FUN-TO which includes
establishing Serbian { Bulgarian mini-network (of five telescopes at three
sites, ASV in Serbia, Belogradchik and Rozhen in Bulgaria), the Gaia-FUN-TO
test observations, and some results. [Projekat Ministarstva nauke Republike
Srbije, br. 176011: Dynamics and kinematics of celestial bodies and systems,
br. 176004: Stellar physics, i br. 176021: Visible and invisible matter in
nearby galaxies: theory and observations]
期刊介绍:
Serbian Astronomical Journal publishes original observations and researches in all branches of astronomy. The journal publishes:
Invited Reviews - review article on some up-to-date topic in astronomy, astrophysics and related fields (written upon invitation only),
Original Scientific Papers - article in which are presented previously unpublished author''s own scientific results,
Preliminary Reports - original scientific paper, but shorter in length and of preliminary nature,
Professional Papers - articles offering experience useful for the improvement of professional practice i.e. article describing methods and techniques, software, presenting observational data, etc.
In some cases the journal may publish other contributions, such as In Memoriam notes, Obituaries, Book Reviews, as well as Editorials, Addenda, Errata, Corrigenda, Retraction notes, etc.