Further Evidence that Quasar X-Ray Emitting Regions Are Compact: X-Ray and Optical Microlensing in the Lensed Quasar Q J0158-4325

التفاصيل البيبلوغرافية
العنوان: Further Evidence that Quasar X-Ray Emitting Regions Are Compact: X-Ray and Optical Microlensing in the Lensed Quasar Q J0158-4325
المؤلفون: Morgan, Christopher W., Hainline, Laura J., Chen, Bin, Tewes, Malte, Kochanek, Christopher S., Dai, Xinyu, Kozlowski, Szymon, Blackburne, Jeffrey A., Mosquera, Ana M., Chartas, George, Courbin, Frederic, Meylan, Georges
سنة النشر: 2012
المجموعة: Astrophysics
مصطلحات موضوعية: Astrophysics - Cosmology and Nongalactic Astrophysics
الوصف: We present four new seasons of optical monitoring data and six epochs of X-ray photometry for the doubly-imaged lensed quasar Q J0158-4325. The high-amplitude, short-period microlensing variability for which this system is known has historically precluded a time delay measurement by conventional methods. We attempt to circumvent this limitation by application of a Monte Carlo microlensing analysis technique, but we are only able to prove that the delay must have the expected sign (image A leads image B). Despite our failure to robustly measure the time delay, we successfully model the microlensing at optical and X-ray wavelengths to find a half light radius for soft X-ray emission log(r_{1/2,X,soft}/cm) = 14.3^{+0.4}_{-0.5}, an upper limit on the half-light radius for hard X-ray emission log(r_{1/2,X,hard}/cm) <= 14.6 and a refined estimate of the inclination-corrected scale radius of the optical R-band (rest frame 3100 Angstrom) continuum emission region of log(r_s/cm) = 15.6+-0.3.
Comment: 9 pages, 6 figures, submitted to ApJ
نوع الوثيقة: Working Paper
DOI: 10.1088/0004-637X/756/1/52
URL الوصول: http://arxiv.org/abs/1205.4727
رقم الأكسشن: edsarx.1205.4727
قاعدة البيانات: arXiv
الوصف
DOI:10.1088/0004-637X/756/1/52