We present rotation periods of four asteroids: 1660 Wood, 7173 Sepkoski, 12738 Satoshimiki, and (23233) 2000 WM72. The observations were undertaken using the SARA (Southeastern Association for Research in Astronomy) South telescope, located in Cerro Tololo Inter-American Observatory in Chile, from 2011 December to 2012 April. The following synodic periods were found: 1660 Wood, P = 6.8088 ± 0.0002 h; 7173 Sepkoski, P = 2.44 ± 0.02 h; 12738 Satoshimiki, P = 8.708 ± 0.001 h; and (23233) 2000 WM72, P = 3.732 ± 0.003 h
The Kepler mission is a powerful tool for the study of different types of astrophysical objects or e...
Synodic rotation periods and amplitudes are reported for 318 Magdalena, 455 Bruchsalia, 486 Cremona,...
Five solar system minor planets were measured photometrically between 2012 October and December usin...
Photometric observations of three main-belt asteroids were conducted in order to determine their syn...
From June 2011 through May 2012 May, photometric data for four asteroids were obtained using the Sou...
Collaborative photometric observations of two main-belt asteroids were conducted from five observato...
The main-belt asteroid 8077 Hoyle was observed on 13 nights over a span of 47 days in 2012 April-May...
The Palomar Transient Factory (PTF) is a synoptic survey designed to explore the transient and varia...
A global collaboration of observers from Australia, Europe, and North America found synodic rotation...
A new asteroid rotation period survey has been carried out by using the Palomar Transient Factory (P...
Photometric studies of asteroid 2501 Lohja were made between 2014 June 24 and 25 using the Southeast...
1 page.Coordinated broadband photometric measurements of the asteroid 665 Sabine were obtained in Au...
Understanding outer space is a longcraved aspiration of science. We are investigating the rotational...
An observing campaign was conducted among teams at the University of Maryland, College Park, and in...
Lightcurve analysis for (162421) 2000 ET70 was performed in collaboration with observers in Uruguay,...
The Kepler mission is a powerful tool for the study of different types of astrophysical objects or e...
Synodic rotation periods and amplitudes are reported for 318 Magdalena, 455 Bruchsalia, 486 Cremona,...
Five solar system minor planets were measured photometrically between 2012 October and December usin...
Photometric observations of three main-belt asteroids were conducted in order to determine their syn...
From June 2011 through May 2012 May, photometric data for four asteroids were obtained using the Sou...
Collaborative photometric observations of two main-belt asteroids were conducted from five observato...
The main-belt asteroid 8077 Hoyle was observed on 13 nights over a span of 47 days in 2012 April-May...
The Palomar Transient Factory (PTF) is a synoptic survey designed to explore the transient and varia...
A global collaboration of observers from Australia, Europe, and North America found synodic rotation...
A new asteroid rotation period survey has been carried out by using the Palomar Transient Factory (P...
Photometric studies of asteroid 2501 Lohja were made between 2014 June 24 and 25 using the Southeast...
1 page.Coordinated broadband photometric measurements of the asteroid 665 Sabine were obtained in Au...
Understanding outer space is a longcraved aspiration of science. We are investigating the rotational...
An observing campaign was conducted among teams at the University of Maryland, College Park, and in...
Lightcurve analysis for (162421) 2000 ET70 was performed in collaboration with observers in Uruguay,...
The Kepler mission is a powerful tool for the study of different types of astrophysical objects or e...
Synodic rotation periods and amplitudes are reported for 318 Magdalena, 455 Bruchsalia, 486 Cremona,...
Five solar system minor planets were measured photometrically between 2012 October and December usin...