Photometric and Polarimetric Interpretation of Blazar AO 0235+164 Behaviour

نویسندگان

چکیده

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

4-year optical-infrared photometric and polarimetric behaviors of a gamma- ray blazar 3C 454.3

We have performed a multi-color photo-polarimetric monitoring of 45 optical-bright blazars since 2007. 3C 454.3, which is one of the brightest blazars in the gamma-ray sky, is one of targets of its project. We have made photo-polarimetric monitorings since July 2007. The object showed violent variation in its flux and polarization. In particular, four large-amplitude outbursts in 2007, 2008, 20...

متن کامل

The Future of Photometric, Spectrophotometric and Polarimetric Standardization

The use of polarimetric techniques is nowadays widespread among solar and stellar astronomers. However, notwithstanding the recommandations that have often been made about the publication of polarimetric results in the astronomical literature, we are still far from having a standard protocol on which to conform. In this paper we review the basic definitions and the physical significance of the ...

متن کامل

The Future of Photometric, Spectrophotometric and Polarimetric Standardization

Free of any atmospheric contamination, the Hubble Space Telescope provides the best available spectrophotometry from the far-UV to the near-IR for stars as faint as V ∼ 16. The HST CALSPEC standard star network is based on three standard candles: the hot, pure hydrogen white dwarf (WD) stars G191B2B, GD153, and GD71, which have Hubeny NLTE model flux calculations that require the atomic physics...

متن کامل

The Future of Photometric, Spectrophotometric and Polarimetric Standardization

The 5-year project Supernova Legacy Survey (SNLS) delivers ∼ 100 Type-Ia supernovae (SNe Ia) per year, in the redshift range 0.3 < z < 1.0, with well-sampled griz lightcurves. The SNLS Collaboration uses the 1 deg Megacam imager (36 2048×4612 thinned CCDs) mounted on the 3.6-m CanadaFrance-Hawaii Telescope (CFHT) to observe four fields around the sky, in four filters. The primary goal of the pr...

متن کامل

The Future of Photometric, Spectrophotometric and Polarimetric Standardization

In the last few years our knowledge of the physics of massive stars has improved tremendously. However, further investigations are still needed, especially regarding accurate calibrations of their fundamental parameters. To this end, we have constructed a comprehensive grid of NLTE model atmospheres and corresponding synthetic spectra in the massive star domain. The grid covers the complete B t...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Atoms

سال: 2017

ISSN: 2218-2004

DOI: 10.3390/atoms5040039