PPT-Photometric Studies of Transiting

Exoplanets Norio Narita NAOJ Transit of Venus on June 5 2012 at Hawaii Outline Introduction of Transit Current Status of Studies of Transiting Exoplanets Further Studies of Transiting . and other items Transiting planets set the tone for the birth chart and astrologers assess all aspects of life from the freezeframe of the planetary patterns at that moment As those planets continue to make their orbits they affect the birth chart a In this chapter the characteristics of human vision and of the human eye and are summarized in particular as these characteristics relate to hum an eye sensitivity and photometric quantities 161 Light receptors of the human eye Figure 161 a shows a RV curve for KELT Bright transiting exoplanetsfrom the KELT SurveyKELTSouth in Sutherland, South Africa Discovery light curve for KELT2Ab Discovery of hot Jovian planets transiting bright (8 V 10) hos Outline. 1.) Step 1 – TV3 Calibration. 2.) Step 2 – SMOV4 (+ Cycle 17 Calibration). 3.) Step 3 – Final Calibration (present analysis). - More data. - New flat fields. - Astrodrizzle. - Precise calibration. A. . Pasewaldt. 1. , . K. . Willner. 2. , . J. . Oberst. 1,2. , . Frank . Scholten. 1. , . M. . Wählisch. 1. , . K.-D. . Matz. 1. , . T. . Roatsch. 1. , . H. . Hoffmann. 1. , . A. . Grechishev. 3. . RESEARCH. q. uality and quantity. Paul Dowling. Institute of Education. University of London. Photometric . redshifts. can be routinely obtained to accuracies of better than 0.1 in Deltaz/(1 +. z. ). The issue of dust extinction, however, is one that has still not been well quantified. In this paper the success of two template-fitting photometric . Studies for Transiting . Exoplanets. Norio Narita. National Astronomical Observatory of Japan. Outline. Introduction of Science of Transiting . Exoplanets. What’s New and What’s Going on Now?. Near Future Prospects. Synergy with Transiting Planets. Norio Narita (NAOJ. ). Thanks to IRD Transit Group. Members of . the . IRD Transit Group. Norio Narita . (Chief: NAOJ. ). Akihiko Fukui (NAOJ, Okayama Astrophysical . by Transit Observations. Norio Narita. National Astronomical Observatory of Japan. Outline. Introduction of transit photometry. Further studies for transiting planets. Future studies in this field. CS5670 : Computer Vision. Noah Snavely. A Single Image: Shape from Shading. Assume is 1 for now.. What can we measure from one image?. is the angle between N and L. Add assumptions:. Studies for Transiting . Exoplanets. Norio Narita. National Astronomical Observatory of Japan. Outline. Introduction of Science of Transiting . Exoplanets. What’s New and What’s Going on Now?. Near Future Prospects. Photometric stereo Radiance Pixels measure radiance This pixel Measures radiance along this ray Where do the rays come from? Rays from the light source “reflect” off a surface and reach camera Reflection: Surface absorbs light energy and radiates it back Announcements. Project 4 (stereo) released today, due Friday, April 1, at 8pm. To be done in groups of 2. Recap: . Lambertian (Diffuse) Reflectance. I . : observed image intensity. k. d. . : object albedo. „4.5. Light . sources. “. With the agreed objective to allow all light source technologies in all lamps (functions) the text of section 4.5.1. condenses significantly. 4.5. Light sources. 4.5.1. Restrictions on light sources .