relation between asteroids and rotational velocity
TRANSCRIPT
Confirming Asteroid TrendsWorking with the Palomar Transient Factory (PTF)
Chan-Kao “Rex” ChangDr. Wing-Huen IpNicholas Powers and Anthony Smith
Palomar Transient Factory (PTF)
Project at CalTech in California
Centered around one main telescope 48 arc-second 12 CCD chips – one is out of order
F.o.V is ~7 deg2 Resolution of 1 arc-second/pixel
The Process Download the data
Program to download data Outputs catalogs and images Only working with catalogs
Differentiate objects as either static or moving
Objects that do not move over the course of multiple catalogs are static
The Process continued Compare moving point sources to ephemerids
Position of objects at the time of recording vs. approximate position of objects in the database
Right Ascension and Declination (long and lat) Analyze light curves to determine rotation periods
Plot Diameter vs. Period of rotation (or freq) Diameter can be determined based on traits such as albedo – magnitude of solar reflection
Progress Read PTF data
Julian Dates Right Ascension Declination Magnitude
Sort Objects Moving Stationary
R.A.
Dec
R.A.
Dec
Progress Read MPC data
Organize Compare MPC with PTF Output files for each known object Plotted Light Curves Analyzed Period Data Determined Approximate Diameter
Masiero et. al. 2009 Graph Period vs. Diameter
Acknowledgements Office of International Programs, SUNY Oswego
Dr. Shashi M. Kanbur Dr. Wing-Huen Ip and Chan-Kao “Rex” Chang
National Central University Graduate institute of Astronomy, Jhongli, Taiwan
National Science Foundation's Office of International Science and Engineering award number 1065093
Office of International Programs, NCU
Picture Sources “A search for main-belt comets in the Palomar Transient Factory survey: I”. Extended-object analysis - Waszczak et al. 2013 (submitted to MNRAS)
“The Asteroid Lightcurve Database” Warner et al. 2009. Icarus, Volume 202, Issue 1, p. 134-146
“P48 Observers Information” California Institute of Technology. http://www.astro.caltech.edu/palomar/P48observers.html