J/A+A/546/A72     Light curves of Flora region asteroids   (Kryszczynska+, 2012)

Do Slivan States exist in the Flora family? I. Photometric survey of the Flora region. Kryszczynska A., Colas F., Polinska M., Hirsch R., Ivanova V., Apostolovska G., Bilkina B., Velichko F.P., Kwiatkowski T., Kankiewicz P., Vachier F., Umlenski V., Michalowski T., Marciniak A., Maury A., Kaminski K., Fagas M., Dimitrov W., Borczyk W., Sobkowiak K., Lecacheux J., Behrend R., Klotz A., Bernasconi L., Crippa R., Manzini F., Poncy R., Antonini P., Oszkiewicz D., Santana-Ros T. <Astron. Astrophys. 546, A72 (2012)> =2012A&A...546A..72K 2012A&A...546A..72K
ADC_Keywords: Solar system ; Minor planets ; Photometry, CCD Keywords: techniques: photometric - minor planets: asteroids: general Abstract: Recent studies have uncovered evidence that the statistical properties of asteroids' physical parameters are a fundamental source of information on the physics of their collisions and evolution. The analysis of the spin rates and spin vector distributions helps us to understand the role of various known and new effects. The alignment of spin vectors and the correlation of spin rates are for the first time observed for ten members of the Koronis family. These unexpected non-random orientations of the spin axes and correlations of the spin rates, now known as Slivan states are interpreted in terms of a YORP effect and spin-orbit resonances. To study non-gravitational-effects, there appears to be a need for new observational campaigns devoted to determining the physical parameters of the asteroid families. We analysed the photometric observations of the asteroids, which are the most efficient method of studying asteroid physical parameters. Description: The files contain asteroid brightness, aspect data and observing information for corresponding date. These files were used for obtaining synodic period rotation. Individual lightcurves within a files are identified with a light curve number, all lightcurves are relative. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table.dat 74 552 Aspect data and observing information lc/* . 55 Individual light curves -------------------------------------------------------------------------------- See also: B/astorb : Orbits of Minor Planets (Bowell+ 2012) J/A+A/465/331 : Asteroid brightness and geometry (Durech+, 2007) Byte-by-byte Description of file: table.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- Ast Designation of the asteroid 6- 15 A10 "YYYY/MM/DD" Obs.date Date of observation 17- 26 F10.2 d JD Julian date of observation(1) 28- 33 F6.4 AU r Asteroid-Sun distance (1) 35- 40 F6.4 AU Delta Asteroid-Earth distance Δ (1) 42- 46 F5.2 deg alpha Solar phase angle α (1) 48- 53 F6.2 deg ELon Ecliptic longitude (1) 55- 60 F6.2 deg ELat Ecliptic latitude (1) 62 A1 --- F [CBVRIL] Filter: clear (C), Bessel BVRI or L (at Pic du Midi) 64- 71 A8 --- Obs Observatory (2) 73- 74 I2 --- LCN Light curve number -------------------------------------------------------------------------------- Note (1): Coordinates given for the middle of the observation Note (2): Observatories and codes, as follows: Bed = (132) Bedoin Observatory, France Bor = (187) Borowiec, Poland Bor PST = (187) Poznan Spectroscopic Telescope, Borowiec, Poland HH = (E14) Hunters Hill Observatory, Australia Kie = (B02) Kielce Observatory, Poland Kha = (101) Kharkov, Ukraine Le Cres = (177) Le Cres Observatory, France LE = (A14) Les Engarouines, France NOT = (950) Nordic Optical Telescope, La Palma, Spain OHP = (511) Observatoire de Haute Provence, France Pic = (586) Pic du Midi, France PdD = Pico dos Dias, Brazil Poz = (47) Poznan Observatory, Poland Roz = (71) NAO Rozhen, Bulgaria Roz 2m = (71) NAO Rozhen, Bulgaria SAAO = (A60) South African Astronomical Observatory, Republic of South Africa SAdS = (A12) Stazione Astronomica di Sozzago, Italy SPA = (I10) San Pedro de Atacama, Chile -------------------------------------------------------------------------------- Byte-by-byte Description of file: lc/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 F15.7 d JD JD epoch (1) 18- 24 F7.3 --- br Relative brightness 26- 27 I2 --- LCN Light curve number -------------------------------------------------------------------------------- Note (1): not corrected for the light travel time -------------------------------------------------------------------------------- Acknowledgements: Agnieszka Kryszczynska, agn(at)amu.edu.pl
(End) A. Kryszczynska [Astron. Obs. Inst.], P. Vannier [CDS] 30-Jul-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line