ВНИМАНИЕ! На форуме начался конкурс - астрофотография месяца АПРЕЛЬ!
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ASTEROIDAL OCCULTATION - REPORT FORM +------------------------------+ +------------------------------+ | EAON | | IOTA/ES | | | | INTERNATIONAL OCCULTATION | | EUROPEAN ASTEROIDAL | | TIMING ASSOCIATION | | OCCULTATION NETWORK | | EUROPEAN SECTION | +------------------------------+ +------------------------------+1 DATE: STAR: ASTEROID: N°: 2 OBSERVER: Name: Abbr: E-mail: Address:3 OBSERVING STATION: Nearest city: Station: Latitude: Longitude: Altitude: Datum (WGS84 preferred): Single, OR Double or Multiple station (Specify observer's name): +----------------------------------+4 TIMING OF EVENTS: | | | OCCULTATION RECORDED: xxxxTIVE | | | +----------------------------------+ Type of event Start observation Interrupt-start Disappearance Blink Flash End observation Jnterrupt-end Reappearance Other (specify) Comments Event Time (UT) P.E. Acc. Code HH MM SS.ss S.ss S.ss S - - - : - - - : D - - - : R - - - : - - - : E - - - : Duration : Mid-event : Was your reaction time applied to the above timings?5 TELESCOPE: Type: Aperture: Magnification: Mount: Motor drive:6 TIMING & RECORDING: Time source: Sensor: Recording: Time insertion (specify): Event insertion (specify):7 OBSERVING CONDITIONS: Atmospheric transparency: Wind: Temperature: Star image stability: Minor planet visible:8 ADDITIONAL COMMENTS:
-------------------------------------------------------------- ASTERIODAL OCCULTATION - REPORT FORM--------------------------------------------------------------1.DATE: 2008 July 27, predicted time: 00:04 UT STAR: HIP520 Mv = 7.7 ASTEROID: (4505) Okamura Mv = 16.42.OBSERVER, Abbr: Name: Vitalij Mechinskij Address: 220004, Belarus, Minsk E-mail: lupus@belastro.net3.OBSERVING STATION: Lipa. Nearest city: Baranovichi(BY) Latitude: N 53°16'36.5" Longitude: E 26°27'20.6" Altitude: 190 Datum: WGS 84 Single station4.TIMING OF EVENTS Occultation recorded: NEGATIVE Type of event: "S"tart observation; "I"nterrupt-"s"tart; "D"isappearance; "B"link; "F"lash; "E"nd observation; "I"nterrupt-"e"nd; "R"eappearance; "O"ther (specify) Event Time (UT) P.E. Accuracy + Comments code HH:MM:SS.00 0.ss S.ss S 00:04:00 -.-- 1.0 - : : . . D : : . . R : : . . - : : . . E 00:06:32 -.-- 1.0 Duration: -.-- s Mid-event: --:--:--.--5.TELESCOPE Type: Newton Aperture: 114mm Magnification: 45x Focal length: 900mm Mount: Equatorial Motor drive: no6.TIMING & RECORDING Time-signal Station: RWM station Mode of recording: Stopwatch Device of recording: no, visual7.OBSERVING CONDITIONS Atmospheric transparency: good Wind: no Star image stability: good Temperature: 10°C Minor planet visible: no before/during/after event8.ADDITIONAL COMMENTS -
-------------------------------------------------------------- ASTERIODAL OCCULTATION - REPORT FORM--------------------------------------------------------------1.DATE: 2008 July 27, predicted time: 00:04 UT STAR: HIP520 Mv = 7.7 ASTEROID: (4505) Okamura Mv = 16.42.OBSERVER, Abbr: Name: Ivan BRUHANOV Address: E-mail:3.OBSERVING STATION: Gorodische. Nearest city: Minsk(BY) Latitude: N 53°59'22" Longitude: E 27°51'07" Altitude: 220 Datum: WGS 84 Single station4.TIMING OF EVENTS Occultation recorded: POSITIVE Type of event: "S"tart observation; "I"nterrupt-"s"tart; "D"isappearance; "B"link; "F"lash; "E"nd observation; "I"nterrupt-"e"nd; "R"eappearance; "O"ther (specify) Event Time (UT) P.E. Accuracy + Comments code HH:MM:SS.00 0.ss S.ss S 23:57:00 1.0 - : : . . D 00:04:30.8 0.2 . 0.01 . F 00:04:32.4 0.2 0.01 R 00:04:32.6 0.2 . 0.01 . - : : . . E 00:05:00 1.0 Duration: 1.8 s Mid-event: 00:04:31.75.TELESCOPE Type: Refractor Aperture: 45mm Magnification: 25x Focal length: - Mount: Azimuthal Motor drive: no6.TIMING & RECORDING Time-signal Station: RWM Mode of recording: Stopwatch Device of recording: no, visual7.OBSERVING CONDITIONS Atmospheric transparency: good Wind: no Star image stability: good Temperature: 10°C Minor planet visible: no before/during/after event8.ADDITIONAL COMMENTS Reappearance was in two steps. First step was appearance of star with m=10-10.5, second step was reappearance of star with m=7.7. Time of reaction is already applied: from the reading of stopwatch was subtracted time of reaction (0.2 sec).
Чисто ИМХО - лучше делать одну большую таблицу, нежели бланк под каждое покрытие (их за ночь может быть более 10). Но это - как кому удобнее. А форма самого отчёта, кстати, будет зависеть от того, куда отчёт отправляется.Цитата: ГК от 23 Апр 2010 [16:01:46]Предлагаю свой бланк.Сразу есть несколько существенных претензий:1) высота над у.м. точки наблюдения; и, желательно, точность определения 3-х координат, если это не стационарный телескоп2) ЛИЧНОЕ УРАВНЕНИЕ! (каким образом учтено, величина, и т.п.)3) ПРИВЯЗКА к абсолютной шкале ВРЕМЕНИ! (источник, метод привязки, метод фиксации покрытия)4) поле для комментариев (условия наблюдения и прочее при необходимости)... необязательно, но неплохо бы иметьЦитата: ГК от 23 Апр 2010 [15:11:30]Расскажите и представьте пожалуйста бланк- отчет о наблюдении покрытии звезды луной.Более подробно рассказать постараюсь. Только не сегодня ночью.ЗЫ. Полистайте тему "Журнал наблюдений покрытий звёзд астероидами" - много полезной информации.
Предлагаю свой бланк.
Расскажите и представьте пожалуйста бланк- отчет о наблюдении покрытии звезды луной.
Цитата: ГК от 24 Апр 2010 [06:21:01]т.к. многие ЛА наблюдают на нулевой высоте.Это что же, многие ЛА живут на берегу моря? Я думал, что на Восточноевропейской равнине преобладают высоты 100-250м.
т.к. многие ЛА наблюдают на нулевой высоте.
через недели открывается сезон серебристых облаков, но из-за отсутствия русскоязычного ресурса 9/10 сезонной информации снова имеет шанс не выйти за пределы Астрофорума.
Предлагаю свой бланк наблюдений переменных звёзд, предназначенный для последующей отправки в AAVSO:
Подозрение на открытие (кометы, Новые и Сверхновые звёзды):Общие инструкции по проверке и оформлению отчёта: Information You Should Include In A Discovery ReportСверхновые звёзды:Проверка подозрительного объекта: SNChecker.Список недавно открытых: List of Recent Supernovae.Добавлена форма отправки данных по Сверхновым (спасибо А.Иванову): Reporting SN Measures
http://www.astronomerstelegram.org/ -- не работает.
Electronic Telegram No. 2629Central Bureau for Astronomical TelegramsINTERNATIONAL ASTRONOMICAL UNIONCBAT Director: Daniel W. E. Green; Hoffman Lab 209; Harvard University; 20 Oxford St.; Cambridge, MA 02138; U.S.A.e-mail: cbatiau@eps.harvard.edu (alternate cbat@iau.org)URL http://www.cbat.eps.harvard.edu/index.htmlPrepared using the Tamkin Foundation Computer NetworkTRANSIENT OBJECTS CONFIRMATION PAGE The Central Bureau has established a "Transient Objects Confirmation Page"(TOCP), activated on 2011 January 1, to replace the former "Unconfirmed-Objects" webpage (http://www.cbat.eps.harvard.edu/unconf/cbat_unconf.html) thatthe CBAT has run quite successfully since 2003, and which was updated manuallyby CBAT staff members. In contrast, this new webpage is designed to be updatedautomatically both by astronomers worldwide who are registered (via the CBAT)to do so and (when necessary) manually by CBAT staff. The TOCP addresses a strong desire in the astronomical community forimmediate posting of interesting new transient objects, to solicit confirmingobservations (and thus to provide a place to post confirming observations, andto help prevent potentially unnecessary observations at multiple observatories).The TOCP is designed for use with stationary, extra-solar-system objects only.Data will be postable to the TOCP directly only by registered users, who canaccess RSS feeds and/or receive e-mails of new postings. There is nosubscription charge for access (or posting) to the TOCP. The website URL forthe new TOCP is http://www.cbat.eps.harvard.edu/unconf/tocp.html. Once itemsare posted on the TOCP, they will be available as RSS feeds -- as has been thecase since 2009 for CBETs and IAUCs. The discovery reports posted on the TOCPwill be sent automatically in standard XML format to the VOEvent system. The Central Bureau assigns formal IAU designations to various objects,both within and outside the solar system. For decades now, the CBAT hasassigned year-and-letter supernova designations to objects that are observedto be near extragalactic galaxies on two or more nights, even withoutspectroscopic confirmation -- while the formal GCVS designation of Milky-Waynovae is not given until such objects are spectroscopically confirmed. Withthe introduction of the TOCP, the Central Bureau will move immediately towardthe Milky-Way-nova model of designating supernovae, in which final year-and-letter designation will not be issued until spectroscopic confirmation ismade for any given object. For novae, supernovae, and other "new" variables,the TOCP will automatically assign provisional designations based on position,of the form TCP Jhhmmssss+ddmmsss (giving R.A. to 0s.01 and Decl. to 0".1 withno decimal points), where a three-letter prefix will be used to denote type ofobject (PSN = possible supernova; PNV = possible nova; TCP = unknown type ofvariable). Additional information is given at the following website URL:http://www.cbat.eps.harvard.edu/unconf/tocp_help.html. Once spectroscopicconfirmation is reported, a final designation will be announced by the CentralBureau both via the TOCP and via CBET or IAUC, and a cross-reference list (ofprovisional vs. final designations) is being maintained to aid users at URLhttp://www.cbat.eps.harvard.edu/unconf/tocp.html. In order to post a discovery or follow-up observation to the TOCP, a usermust be registered with the Central Bureau. The CBAT is starting with aworking list of several dozen registered users, compiled from contributors whohave sent multiple discovery or follow-up reports to the Central Bureau in thepast year. Additional registrants can contact the Bureau to be added to thelist, by sending an e-mail request to cbatiau@eps.harvard.edu. All can accessthe TOCP RSS feed at http://www.cbat.eps.harvard.edu/unconf/tocp.xml (requeststo receive TOCP postings by e-mail should be sent also as an e-mail request tocbatiau@eps.harvard.edu; this will not be done automatically unless a requestis made to do so a specific registrant). Of course, the TOCP and its RSSfeeds will be freely available to both registrants and non-registrants. There will be two types of formats for reporting observations: adiscovery-observation format and a follow-up-observation format. The discoveryformat requires that certain data be provided in order for automatic posting,whereas the follow-up format is a "comment" format with more flexibility.There are two automatic ways in which registered astronomers can add theirobservations to this webpage in a standard format: (1) by sending data viae-mail to cbattcp@eps.harvard.edu in a strict column-by-column format(described at the TOCP webpage) or (2) by filling out a form at the TOCPwebsite. There are automatic computer checks to determine whetherinformation is provided in proper columns; follow the instructions carefullyto ensure proper posting. Follow-up observations should be reported usingthe provisional positional designation posted at the TOCP for a given object.While the contributed TOCP discovery lines have a specific column-by-columnformat, the contributed follow-up-data lines are "free form" beyond column42 (i.e., after the proper inclusion of the provisional positionaldesignation and the UT date). To post one or more lines to the TOCP in ane-mail message, the sender must type either "TOCP discovery observation" or"TOCP follow-up observation" on the subject line for proper posting.Alternatively, reports sent outside of these two standard procedures (e.g.,to cbatiau@eps.harvard.edu) will be reviewed, and posted (sometimesnecessarily with a delay) on the TOCP, by the CBAT staff -- as has alwaysbeen the case in the past; numerous discovery reports from the last coupleof weeks have been so posted by the CBAT staff on the TOCP during finaltesting of the website mechanics. Note that all contributors to this TOCP should also send a separate e-mailwith details in textual form to cbatiau@eps.harvard.edu, as such details willbe used in any announcement CBET or IAUC later. Announcement of extra-solar-system transients on CBETs and IAUCs will generally be reserved for objectswith spectroscopic confirmation (and thus the site where "final" designationsare given, as is the case now) or for brighter objects that are being heavilyobserved. The CBAT will only occasionally publish reports on CBETs or IAUCs ofobjects discovered and observed on a single night only without spectroscopicconfirmation. Sometimes reports are received of such objects that containobservations on only a single night (or sometimes more than one night), needingconfirmation before formal announcement and designation on IAUCs or CBETs --but where the observer does not want his/her observation(s) posted prior toconfirmation; as in the past, such reports can be sent to the CBAT at e-mailaddress cbatiau@eps.harvard.edu -- which is also the e-mail address to use fornon-TOCP reports in textual form. The TOCP was created following extensive discussions with observers,both professional and amateur. It will necessarily evolve over time toaddress additional needs of the astronomical community. Users who experienceproblems with posting on the TOCP should (after verifying that theycarefully followed instructions at the TOCP webpages) contact the Bureauwith details.NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2011 CBAT2011 January 10 (CBET 2629) Daniel W. E. Green
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Тема: Результаты наблюдений: как оформлять, куда сообщать (Прочитано 17304 раз)
