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The R.A.P. Project (Reviews of Astro-Ph)

Metody nablyudenii

astro-ph/0207074 Rayleigh Laser Guide Star Systems: Application to UnISIS
Authors: L.A. Thompson, S.W. Teare
Comments: 42 pages, 10 figures, accepted for publication in the September issue of PASP

Kak izvestno, atmosfera ochen' meshaet zemnym nablyudatelyam v optike i IK. Mozhno zapuskat' teleskopy v kosmos, no eto dorogo (hotya, "v kosmose dollar vesit men'she" B. Pachin'skii). Na Zemle stroyat sistemy s adaptivnoi optikoi (ob etom byla otlichnaya stat'ya D. Vibe v nedavnem "Zvezdochete".

Dlya otslezhivaniya sostoyaniya atmosfery primenyayut lazery (sozdanie t.n. "lazernoi zvezdy"). Ob etom i idet rech' v stat'e Tompsona i dr.


obzor! astro-ph/0208170 The Roles of Small Telescopes in a Virtual Observatory Environment
Authors: S.G. Djorgovski
Comments: PDF file, 10 pages including 2 figures. An invited paper, to appear in: "The Future of Small Telescopes", ed. T. Oswalt, Kluwer, in press

Chto mogut delat' malen'kie teleskopy v epohu bol'shih teleskopov? Eto, kstati skazat', dovol'no aktual'nyi vopros dlya nashei strany. V stat'e daetsya obzor celei i metodov togo, chto nazyvaetsya Virtual'noi observatoriei. Sovremennye informacionnye tehnologii pozvolyayut ochen' effektivno ispol'zovat' set' iz mnozhestva nebol'shih teleskopov, razbrosannyh po vsemu miru. V pervuyu ochered' rech' idet ob obzorah i nepreryvnyh nablyudeniyah (ponyatno, chto dnem-to smotret' nel'zya, a 5-6 teleskopov na raznyh dolgotah mogut pozvolit' provodit' monitoring 24 chasa v sutki, konechno na sluchai plohoi pogody neobhodimo dublirovat' instrumenty, raznosya ih i po shirote i t.d.).

Zamechu, chto eto pravil'no provodit' special'nye konferencii, posvyashennye ispol'zovaniya malen'kih teleskopov.



astro-ph/0208177 WhiteDwarf.org - Establishing a permanent endowment for the Whole Earth Telescope
Authors: Travis S. Metcalfe
Comments: 5 pages, to appear in proceedings of the 6th Whole Earth Telescope workshop

Opisyvaetsya lyubopytnaya organizaciya, ch'e nazvanie lichno u menya vyzyvaet associacii s knigami Shekli: White Dwarf Research Corporation. Eto nekommercheskaya organizaciya, zanimayushayasya issledovaniem belyh karlikov. Predpolagaetsya, chto instituty takogo tipa, blagodarya bolee prostoi strukture, mogut ochen' effektivno ispol'zovat' sredstva.


astro-ph/0209338 The Joint astrophysical Plasmadynamic EXperiment (J-PEX): A high-resolution rocket spectrometer
Authors: M.A. Barstow et al.
Comments: 11 pages, including 9 figure and 2 tables. To be published in Proc SPIE, vol 4854

Opisyvayutsya rezul'taty raboty novogo ul'trafioletovogo spektrografa, ispytannogo v raketnom zapuske. Instrument imeet ryad osobennostei, interesnyh specialistam.


obzor astro-ph/0209468 Ground Based VLBI Facilities -- the European and Global VLBI NetworkAuthors: M.A. Garrett
Comments: 11 pages, 5 figures, lecture presented at the NATA ASI VLBI School, Oct 2001. To be published in "The Role of VLBI in Astrophysics, Astrometry and Geodesy", ed. F. Mantovani. See www.evlbi.org for more information

Sushestvuet neskol'ko krupnyh sistem interferometrov so sverhdlinnoi bazoi (VLBI): VN, VLBA, CMVA i APT/LBA. V stat'e podrobno obsuzhdayutsya evropeiskie sistemy (kotorye mogut rbotat' kak smostoyatel'no, tak i v sostave global'nyh sistem).


obzor astro-ph/0210044 The Challenge to Large Optical Telescopes from X-ray Astronomy
Authors: Ann E. Hornschemeier
Comments: 15 pages, 6 figures, Invited review for SPIE conference "Science with 6-10 m Class Telescopes"

Obsuzhdaetsya vzaimodeistvie opticheskih i rentgenovskih nablyudenii. Dlya poiska opticheskih "dvoinikov" bol'shinstva slabyh rentgenovskih istochnikov, nablyudayushihsya na N'yutone i Chandre, nuzhna vsya mosh' 10-metrovyh teleskopov. Novoe pokolenie rentgenovskih intsrumentov brosit novyi vyzov optike. K etomu nado gotovit'sya zaranee...


astro-ph/0210238 The ROTSE-III Robotic Telescope System
Authors: C. W. Akerlof et al.
Comments: 19 pages, including 4 figures. To be published in PASP in January, 2003. PASP Number IP02-110

Nablyudeniya opticheskoi vspyshki gamma-vspleska GRB990123 s pomosh'yu sistemy ROTSE bylo bol'shim dostizheniem. S teh por prodolzhayutsya popytki povtorit' etot rezul'tat. Odnako, poka nikakih uspehov net. Potomu prodolzhayut razvivat' mat.chast'. V stat'e opisyvaetsya sistema ROTSE-III. Avtory nadeyatsya, chto ih opyt okazhetsya poleznym dlya sozdatelei analogichnyh sistem, kotorye seichas nachinayut poyavlyat'sya vo vsem mire.

astro-ph/0210627 Radiant meteornogo potoka Leonida v 2001 g. (The radiant of the Leonids meteor storm in 2001)
Authors: Ken'ichi Torii (RIKEN), Mitsuhiro Kohama (RIKEN), Toshifumi Yanagisawa (NAL), Kouji Ohnishi (Nagano NCT, NAOJ)
Commets: 5 pages, 4 figures. Submitted to PASJ

Novaya professional'naya tehnika i metodika registracii meteornyh potokov. Izobrazheniya meteorov poluchalis' s pomosh'yu dvuh fotokamer s CCD-matricami. Linii, poluchennye na izobrazheniyah, ekstrapolirovalis' do ih peresecheniya. Poluchennye koordinaty radianta potoka - (pryamoe voshozhdenie = 154o.35, sklonenie = 21o.55 v epohe J2000) - horosho sovpadayut s teoreticheskimi predskazaniyami.

Pozhaluista, pokazhite etu stat'yu astronomam-lyubitelyam!


astro-ph/0211001 Vremennaya astrometriya na Dzhordell Benke (Jodrell Bank Timing Astrometry)
Authors: G. Hobbs (ATNF), A.G. Lyne (JBO), M. Kramer (JBO)
Commets: 4 pages, 3 figures, to appear in proceedings of the conference "Ra Pulsars" held in Chania, Crete, Sept 2002

Na 76-metrovom radioteleskope im.Lovella observatorii Dzhordell Benk regulyarno provodyatsya nablyudeniya bolee chem 500 radiopul'sarov. Bolee chem dlya 300 pul'sarov ryady nablyudenii dlyatsya bolee 6 let (samyi dolgii - 34 goda). Po eti dannym modno opredelit' period pul'sara i ego izmenenie, a takzhe ego polozhenie na nebe s ochen' vysokoi tochnost'yu. V stat'e izlozhena tehnika obrabotki taiminga pul'sarov (momentov prihoda impul'sov k nablyudatelyu) Predlozhen novyi podhod, pozvolyayushii po vremennoi informacii pouchit' sobstvennye dvizheniya pul'sarov. Etim metodom vpervye opredeleny znacheniya sobstvennyh dvizhenii dlya 111 pul'sarov (no sami eti znacheniya v stat'e ne privedeny).


astro-ph/0211121 Klassifikaciya krivyh bleska v bol'shih obzorah (Lightcurve Classification in Massive Variability Surveys)
Authors: Vasily Belokurov, N. Wyn Evans, Yann Le Du
Comments: 14 pages, 8 figures, submitted to MNRAS

Interesnaya rabota. Avtory pytayutsya primenit' prostye neironnye seti dlya analiza mnozhestva krivyh bleska, poluchaemyh v bol'shih obzorah (naprimer, obzorah po poisku mikrolinzirovaniya).


astro-ph/0212144 Massovye poiski peremennosti i monitoring v eksperimentah OGLE i ASAS (Massive Variability Search and Monitoring by OGLE and ASAS)
Authors: Bohdan Paczynski
Commets: 4 pages, latex, to appear in: owards an International Virtual Observatory'', June 2002, Garching bei Muenchen (Germany), eds. Gorski M. et al, ESO conference series

Kratko opisyvayutsya dva proekta: OGLE (Optical Gravitational Lensing Experiment) i ASAS (All Sky Automated Survey). Oba proekta dayut ogromnoe kolichestvo informacii. Obsuzhdaetsya, kak etot massiv dannyh mozhet byt' ispol'zovan Virtual'noi observatoriei.


astro-ph/0301100 Sovremennye neopredelennosti pri ispol'zovanii Cefeid kak indikatorov rasstoyaniya (Current Uncertainties in the Use of Cepheids as Distance Indicators)
Authors: Michael Feast
Commets: 26 pages, no figs, to appear in "Stellar Candles for the Extragalactic Distance Scale" Lecture Notes in Physics (Springer) ed. D. Alloin and W. Gieren

Avtor podrobno rassmatrivaet metodiku nalibrovki svetimosti cefeid v nashei Galaktike i ucheta ih mezhzvezdnogo pokrasneniya. Eti izmereniya, sovmestno s izmereniyami cefeid v galaktike NGC4258 pokazyvayut, chto tochnost' etoi kalibrovki ne huzhe 0.1m, po krainei mere dlya cefeid s solnechnym himsostavom. Razlichie v himicheskom sostave vnosit primerno takuyu zhe oshibku. Dlya togo, chtoby uvelichit' tochnost' predskazanniya svetimosti cefeid neobhodimy obshirnye raboty po izucheniyu ih metallichnosti, uchet nelineinosti v zavisimostyah period-svetimost' i period-cvet, a takzhe tochnoe opredelenie v kakoi mode proishodyat ih pul'sacii - na osnovnoi chastote ili na pervom obertone.


astro-ph/0301128 Okolozemnye nablyudeniya s pomosh'yu raznesennyh teleskopov (Near-Earth Observations by Spread Telescopes)
Authors: I.A.Maslov et al.
Commets: submitted to Astronomical and Astrophysical Transactions, 7 pages

Predlozhena sistema iz neskol'kih nebol'shih opticheskih teleskopah dlya obzora neba s cel'yu issledovaniya nebol'shih meteornyh tel i issledovaniya mezhplanetnoi sredy.


astro-ph/0301413 VLBI imaging of the RS CVn binary star system HR 5110
Authors: R.R.Ransom et al.
Commets: 22 pages, 4 figures

S pomosh'yu VLBI tehniki udalos' postroit' izobrazhenie dvoinoi zvezdy tipa RS CVn: HR 5110 (=BH CVn; HD118216). Nablyudeniya velis' na chastote 8.4 Ggc.


astro-ph/0301465 Samyi bol'shoi i glubokii obzor VLBI na nastoyashii moment (The Deepest & Widest VLBI Survey yet: VLBA+GBT 1.4 GHz observations in Bootes)
Authors: M.A. Garrett et al.
Commets: 6 pages, 2 figures. To appear in the proceedings of the conference "Radio Galaxies: Past, present and future", Leiden, 11-15 Nov 2002, eds. M. Jarvis et al.Paper with improved figures at http://www.jive.nl/~mag/leiden.ps.gz

VLBI - Very Large Baseline Interferometry. Radionablyudeniya so sverhdlinnoi bazoi. Obychno VLBI obzorami ne zanimaetsya - nablyudayutsya izbrannye istochniki (chashe vsego - aktivnye galaktiki) v raznyh chastyah neba. Svyazano eto s malym polem zreniya (sotni millisekund dugi). V stat'e opisyvaetsya pervaya ser'eznaya popytka preodolet' eti trudnosti za schet primeneniya tehnologii nablyudenii s korotkoi bazoi, no s sohraneniem vseh dostoinstv VLBI.


astro-ph/0301583 Strategiya obzorov neba, maksimiziruyushaya kolichestvo otkryvaemyh tranzientov (Tile or Stare? Cadence and Sky Monitoring Observing Strategies that Maximize the Number of Discovered Transients)
Authors: Robert J. Nemiroff
Commets: 28 pages, 4 figures. Accepted to Astronomical Journal. Mission specific correspondence welcome (to nemiroff@mtu.edu)

Kak iskat' tranzientnye (t.e. vspyhivayushie) istochniki? Smotret' v odnu tochku? Metodichno osmatrivat' nebo? Sluchainym (ili ne sluchainym?) obrazm smotret' to tuda, to tuda? Avtor rassmatrivaet razlichnye vozmozhnosti s cel'yu vyrabotki naibolee razumnoi strategii.


obzor hep-ex/0302008 Gamma-polyarimetriya (Gamma-ray Polarimetry)
Authors: Hiroyasu Tajima (SLAC)
Commets: 6 pages, 9 figures. Contributed to International Workshop on Vertex Detectors, Kailua-Kona, Hawaii USA, November 3-8, 2002

Opisyvayutsya dvuh-storonnie kremnievye strip-detektory i proektiruemyi s ih ispol'zovaniem nauchnyi sputnik SMCT (Semiconductor Multiple-Compton Telescope), Kotoryi budet rabotat' v diapazone energii 0.1-20 MeV.


astro-ph/0302522 Fundamental'noe opredelenie 'radial'noi skorosti' (The fundamental definition of 'radial velocity')
Authors: Lennart Lindegren and Dainis Dravins (Lund Observatory, Sweden)
Commets: 19 pages, 1 figure. Accepted for publication in Astronomy & Astrophysics

Pri tochnosti izmereniya radial'nyh skorostei zvezd i drugih udalennyh ob'ektov poryadka 1 m/s razlichie mezhdu "astrometricheskoi radial'noi skorost'yu" i "spektroskopicheskoi skorost'yu" stanovyatsya sushestvennymi. Obe eti koncepcii opredeleny v poslednih rezolyuciyah IAU (Mezhdunarodnogo Astronomicheskogo Soyuza) i obsuzhdayutsya v dannoi stat'e.


astro-ph/0302523 Vnegalakticheskaya astronomiya s VLTI: novoe okno vo Vselennuyu (Extragalactic Astronomy with the VLTI: a new window on the Universe)
Authors: Alessandro Marconi, Roberto Maiolino and Romain G. Petrov
Commets: invited contribution, to appear in the proceedings of the JENAM 2002

Stat'ya posvyashena priboram dlya opticheskih interferometricheskih nablyudenii na VLTI (Very Large Telescope-Interferometer) v Chili, kotorye pozvolyayut issledovat' umerenno slabye vnegalakticheskie ob'ekty s ochen' vysokim uglovym razresheniem.


miniobzor astro-ph/0303342 Astrometriya s VLBI (VLBI Astrometry)
Authors: Norbert Bartel
Commets: Latex, 6 pages, 8 figures; Invited Review Talk at the DeLA2002 - Astrometry in Latin America'' Conference, Araraquara - Sao Paulo, 2 - 5 September 2002, to be published in ADeLA Publications Series, Vol. 1, 2003

Sovsem korotkaya zametka, kotoruyu vsem rekomenduem prochitat'. Rech' idet o vysokotochnyh nablyudeniyah s pomosh'yu interferometrov so sverhdlinnoi bazoi. Otnositel'nye koordinaty istochnikov pri takih nablyudeniyah opredelyayutsya s tochnost'yu poryadka desyatka mikrosekund dugi!!!

astro-ph/0303445 Opredelenie kosmologicheskih rasstoyanii s VLTI (Distances on Cosmological Scales with VLTI)
Authors: Margarita Karovska, Martin Elvis and Massimo Marengo
Commets: 6 pages, 2 postscript figures, to appear in the proceedings of the JENAM 2002 Workshop WS-VLTI "The Very Large Telescope Interferometer: Challenges for the Future", Editors: P.J.V. Garcia, A. Glindemann, Th. Henning, F. Malbet, Ap&SS, Kluwer, in press

Predlagaetsya novyi metod interferometricheskogo opredeleniya rasstoyanii do kvazarov. Novizna zaklyuchaetsya v ispol'zovanii novogo "standartnogo metra": oblastei shirokih emissionnyh linii. VLTI po ocenkam avtorov vpolne mozhet spravit'sya s takoi zadachei.

Zametim, chto deistvitel'no "standartnaya lineika" luchshe "standartnoi svechi", t.k. menee podverzhena sistematike. Problema v tom, chtoby lineika deistvitel'no byla standartnoi.

obzor astro-ph/0303507 Optimal'nye tehniki dlya 2-mernoi spektroskopii ili kak vychitat' fon v 21 veke (Optimal Techniques in Two-dimensional Spectroscopy: Background Subtraction for the 21st Century)
Authors: Daniel D. Kelson (Carnegie Observatories)
Commets: 26 pages, 15 figures, accepted for publication in PASP, Figures wi full resolution available at http://www.ociw.edu/~kelson.

2-mernaya spektroskopiya - eto kogda na odnoi PZS-matrice fiksiruyutsya spektry ot mnogih ob'ektov v pole zreniya pribora ili ot bol'shogo chisla tochek izobrazheniya. Pri takoi tehnike izmerenii nachinayut igrat' rol' melkomasshtabnye neodnorodnosti i iskazheniya v matrice i v dispergiruyushem elemente + shum + kosmicheskie luchi + ... Podrobnee ob etom - v obzore. Po moemu on budet interesen ne tol'ko astronomam.


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