MediaWiki API result

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            "*": "Subscribe to the mediawiki-api-announce mailing list at <https://lists.wikimedia.org/mailman/listinfo/mediawiki-api-announce> for notice of API deprecations and breaking changes."
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            "203": {
                "pageid": 203,
                "ns": 0,
                "title": "Status of the verification partners",
                "revisions": [
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                        "*": "= Status of the partners preparing for the Gaia Alerts verification =\n\n== Information about the requirements ==\nIn order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are:\n\n# take part in the test observations\n# react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h\n# reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*)\n# flux calibrations better than 10% (0.1 mag)\n\n(*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.''\n\n[[Verification:tests|Test observing campaigns and results]]\n\n= Partners in test=\n\n=== '''NORTH''' ===\n\n==== Loiano ====\n* Contact person: Gisella Clementini, Giuseppe Altavilla\n* Location: Loiano, Bologna, Italy\n* 1.5m\n\n<big>Status: <span style=\"color:#FFFFFF; background:#00ff00\">automated data upload</span></big>\n\n==== Asiago====\n* Contact person: Gisella Clementini, Lina Tomasella\n* Location: Padova, Italy\n* 1.82m\n\n<big>Status: <span style=\"color:#FFFFFF; background:#ff0000\">no data uploaded</span></big>\n\n\n==== APT2====\n* Contact person: Gisella Clementini, Giuseppe Leto,\n* Location: Serra la Nave, Catania, Sicily\n* robotic 80cm Ritchey-Cretien\n\n<big>Status: <span style=\"color:#FFFFFF; background:#00ff00\">automated data upload</span></big>\n\n==== TNT ====\n* Contact person: Anna Piersimoni\n* Location: Teramo, Italy, \n* 72cm Ritchey-Cretien\n\n<big>Status: <span style=\"color:#FFFFFF; background:#ff0000\">no data uploaded</span></big>\n\n==== Belgian Mercator ====\n* Contact person: Laurent Eyer, Lovro Palaversa\n* La Palma (Swiss time)\n* 1.2m\n\n<big>Status: <span style=\"color:#FFFFFF; background:#00ff00\">automated data upload</span></big>\n\n====Konkoly====\n* Contact person: Laszlo Szabados, Gabor Marschalko\n* Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary\n* 1m RCC,  60/90/180 cm Schmidt, 50 cm Cassegrain\n\n<big>Status: <span style=\"color:#FFFFFF; background:#5500ff\">manual data upload</span></big>\n\n\n====PIRATE====\n* Contact person: Ulrich Kolb, Richard.Busuttil\n* Location: Mallorca\n* 43cm corr.D-K, remote and robotic controlled\n\n<big>Status: <span style=\"color:#FFFFFF; background:#00ff00\">automated data upload</span></big>\n\n''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)''\n\n==== pt5m ====\n* Contact person: Stuart Littlefair\n* Location: La Palma\n* 50cm mod.D-K, robotic\n\n<big>Status: <span style=\"color:#FFFFFF; background:#00ff00\">automated data upload</span></big>\n\n====Vienna====\n* Contact person: Werner Zeilinger\n* Location: Austria\n* 1.5m RC\n\n<big>Status: <span style=\"color:#FFFFFF; background:#00ff00\">automated data upload</span></big>\n\nSmall FoV: occasional problems with calibrations.\n\n====ASV Serbia====\n* Contact person: Goran Damljanovic, Oliver Vince\n* Location: Serbia\n* 60cm reflector\n\n<big>Status: <span style=\"color:#FFFFFF; background:#00ff00\">automated data upload</span></big>\n\n''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)''\n\n==== Tubitak Turkey ====\n* Contact person: Irek Khamitov\n* Location: Turkey\n* 150cm (RTT150), 100cm, 60cm\n\n<big>Status: <span style=\"color:#FFFFFF; background:#0000ff\">manual data upload within 24h</span></big>\n\n''Names and affiliations: Khamitov I.M.(1,3 ), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4)\n\n1. T\u00dcB\u0130TAK National Observatory, Antalya, Turkey\n2. \u0130stanbul University, Istanbul, Turkey\n3. Kazan Federal University, Kazan, Russia \n4. Academy of Sciences of Tatarstan, Kazan, Russia\n''\n\n==== Bialkow/Wroclaw Poland ====\n* Contact person: Zbyszek Kolaczkowski\n* Location: Poland\n* 60cm\n\n<big>Status: <span style=\"color:#FFFFFF; background:#00ff00\">automated data upload</span></big>\n\n==== Italian Supernova Project ====\n* Contact person: Simone Leonini\n* Location: Italy\n* 53cm\n\n<big>Status: <span style=\"color:#FFFFFF; background:#5500ff\">manual data upload</span></big>\n\n''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, \nMontarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)''\n\n==== Wise Observatory ====\n* Contact person: Yossi Shvarzvald, Dani Maoz\n* Location: Israel\n* 1m, 71cm, 45cm\n\n<big>Status: <span style=\"color:#FFFFFF; background:#00ff00\">automated data upload</span></big>\n\n==== Ostrowik Observatory ====\n* Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak\n* Location: Poland\n* 60cm\n\n<big>Status: <span style=\"color:#FFFFFF; background:#00ff00\">automated data upload</span></big>\n\n==== OHP ====\n* Contact person: Michel Dennefeld\n* Location: France\n* 1.2m\n\n<big>Status: <span style=\"color:#FFFFFF; background:#ff0000\">no data uploaded</span></big>\n\n==== Vega Slovenia ====\n* Contact person: Jure Japelj\n* Location: Ljubljana, Slovenia\n* 0.7m\n\n<big>Status: <span style=\"color:#FFFFFF; background:#5500ff\">manual data upload</span></big>\n\n----\n\n=== '''SOUTH''' ===\n\n==== Swiss Euler ====\n* Contact person: Laurent Eyer, Lovro Palaversa\n* La Silla, Chile\n* 1.2m\n\n<big>Status: <span style=\"color:#FFFFFF; background:#5500ff\">manual data upload</span></big>\n\n====Danish/Czech Telescope ====\n* Contact person: Pavel Koubsky and Uffe Jorgensen\n* La Silla\n* 1.54m, remotely controlled by Czechs\n\n<big>Status: <span style=\"color:#FFFFFF; background:#ff0000\">no data uploaded</span></big>\n\nSome data collected.\n\n==== GROND ====\n* Contact person: Jochen Greiner, MPIE\n* 2.2m La Silla\n* 7 channels: Optical/NIR: grizJHK\n\n<big>Status: <span style=\"color:#FFFFFF; background:#ff0000\">no data uploaded</span></big>\n\nSome data collected.\n\n==== SAAO ====\n* Contact person: Patricia Whitelock\n* 1.9m, 1.0m\n\n<big>Status: <span style=\"color:#FFFFFF; background:#ff0000\">no data uploaded</span></big>"
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            "8": {
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                "title": "Triggers",
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                        "*": "''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.'''\n\n===Possible triggers for Science Alerts===\n\n* [[Triggers:Asteroids | Asteroids]]\n\n* [[Triggers:Be | Be-type stars]]\n\n* [[Triggers:CVs | Cataclysmic Variables (CVs)]]\n\n* [[Triggers:CNe | Classical novae]]\n\n* [[Triggers:DNe | Dwarf novae]]\n\n* [[Triggers:GRBs | Gamma Ray Bursts Optical Counterparts]]\n\n* [[Triggers:LensedSNe | Gravitationally lensed supernovae]]\n\n* [[Triggers:LBVs | Luminous Blue Variables]]\n\n* [[Triggers:Flares | M-dwarf flares]]\n\n* [[Triggers:Microlensing | Microlensing events]]\n\n* [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]]\n\n* [[Triggers:Supernovae | Supernovae]]\n\n* [[Triggers:TTau | T Tauri stars and other Young variables]]\n\n** [[Triggers:FUOri | Eruptive young stellar objects]]\n\n** [[Triggers:YSOecl | Eclipsing young stellar objects]]\n\n* [[Triggers:XBs | X-ray binaries (XBs)]]\n\n\n* [[Triggers:Other | Other rare transients]]\n\n* [[Triggers:Theoretical | Exotic/theoretical events]]\n\n== Table of transients ==\nThis table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF).\nMR is an absolute magnitude in R, tau is time of a decline by 2 mag.\nNote, these are not all the types of transites Gaia will detect.\n \n{| border=\"1\" cellspacing=\"0\" cellpadding=\"5\" align=\"center\"\n! Class\n! MR\n! tau\n! Universal rate\n! Gaia rate\n|- \n| Dwarf Novae\n| 9..4\n| 3..20\n| <math>3\\times10^{-5} \\textrm{pc}^{-3} \\textrm{yr}^{-1}</math>\n|\n|-\n|Classical Novae\n| -5..-10\n|2..100\n|<math>2\\times10^{-10} \\textrm{yr}^{-1}\\textrm{L}_{\\odot,K}^{-1}</math>\n|\n|-\n|Luminous Red Novae\n| -10..-14\n|20..60\n|<math>1.5\\times10^{-13} \\textrm{yr}^{-1}\\textrm{L}_{\\odot,K}^{-1}</math>\n|\n|-\n|Fallback SNe\n| -4..-21\n|0.5..2\n|<math>10^{-13} \\textrm{yr}^{-1}\\textrm{L}_{\\odot,K}^{-1}</math>\n|\n|-\n|Macronovae\n| -13..-15\n|0.3..3\n|<math>10^{-4..-8} \\textrm{Mpc}^{-3} \\textrm{yr}^{-1}</math>\n|\n|-\n|SN .Ia\n| -15..-17\n|2..5\n|<math>(4..10)\\times 10^{-6} \\textrm{Mpc}^{-3} \\textrm{yr}^{-1}</math>\n|\n|-\n|SNe Ia\n| -17..-19.5\n|30..70\n|<math>3\\times 10^{-5} \\textrm{Mpc}^{-3} \\textrm{yr}^{-1}</math>\n|\n|-\n|Tidal disruption flares\n| -15..-19\n|30..350\n|<math>10^{-6} \\textrm{Mpc}^{-3} \\textrm{yr}^{-1}</math>\n|\n|-\n|Core-collapse SNe\n| -14..-21\n|20..300\n|<math>5\\times 10^{-5} \\textrm{Mpc}^{-3} \\textrm{yr}^{-1}</math>\n|\n|-\n|Luminous SNe\n| -19..-23\n|50..400\n|<math>10^{-7} \\textrm{Mpc}^{-3} \\textrm{yr}^{-1}</math>\n|\n|-\n|Orphan afterglows (SGRB)\n| -14..-18\n|5..15\n|<math>3\\times 10^{-7..-9} \\textrm{Mpc}^{-3} \\textrm{yr}^{-1}</math>\n|\n|-\n|Orphan afterglows (LGRB)\n| -22..-26\n|2..15\n|<math>3\\times 10^{-7..-9} \\textrm{Mpc}^{-3} \\textrm{yr}^{-1}</math>\n|\n|-\n|On-axis LGRB afterglows\n| ..-37\n|1..15\n|<math>4\\times 10^{-10} \\textrm{Mpc}^{-3} \\textrm{yr}^{-1}</math>\n|\n|-\n|}\n\n----\n== CMD of selected variables and transients ==\nCMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009]\n\n[[File:VariablesPathsCMDLMC.png|650px]]\n\n----\n== Time scales and amplitudes ==\n[[File:Kulkarni-absmag-timescale.png|400px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]]\n\n[[File:plot_transients_tau_ampl.png|400px]]\n[[File:plot_transients_trise_ampl.png|400px]]\n[[File:plot_transients_tdecline_ampl.png|400px]]\n[[File:plot_transients_trise_tdecline.png|400px]]"
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