Homework 1
BD+28-4211-oke.dta ,
hw1_fil.dta ,
sdsu-qe.dta ,
window.dta
|
Due: 15/11/2015 |
Homework 2
...... (Solution)
|
Due: 29/11/2015 |
Midterm I:
Choose one of the TFOSC long slit spectra,
obtain normalized flux and identify all spectral lines.
Calculate equivalent widths of the HAlpha line
and the others.
(Use sample data provided *) |
Due: 13/12/2015 |
Lecture notes High Energy Astrophysics by Altan Baykal |
ROTSE workshop 2002 |
Learning Center for X-Ray Telescopes and Detectors
All High Energy Missions (Alphabetical)
Recent X and Gamma Ray Observatories
(operational and ready to go) |
E. Kalemci / NASA |
Homework 3
A series of CCD images for GRB 020813 is given.
Apply standart fotometric reduction and identify
the afterglow. You will need to co-add frames.
Use PSF fotometry to determine instrumental magnitude.
Also determine the brightness using USNO standart stars.
(Use sample data provided *) |
Due: 27/12/2015 |
Exercise
( A ROSAT application )
absnh.f ,
datain.f,
drma.f ,
drm1.dta ,
drm2.dta ,
drm3.dta ,
effar.dta ,
drmch.dta ,
boron.dta |
... |
Midterm II:
40-50 minute Talks
On current missions; Instruments, Science and Impacts
Cigdem Gamsizkan | SWIFT - Gamma-Ray Burst Mission |
Danjela Cerri | FERMI (GLAST) - Gamma-ray Space Telescope |
Armin Nabizadeh | AGILE - Astrorivelatore Gamma a Immagini LEggero |
Nasrin Talebpour Sheshivan | SDO - Solar Dynamics Observatory |
| Due: 23,24/12/2015 - 6,7/01/2016 |
Final:
| Due: 20/01/2016 |