Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES) and Its Initial Results
Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES) has been utilizing the HST parallel orbits to do deep imaging along a large number of random sightlines since Cycle 17. The backbone data set of HIPPIES is from its four-band observations with WFC3, which are being obtained at a rate of ~ 40 fields/year. As its survey fields are disjoint and independent, the impact of "cosmic variance" is minimal. The details of HIPPIES will be presented, and some of its initial results will be discussed, which include: 1) the search for the most luminous Lyman-break galaxies (LBGs) at z>7.4 and the constraint on the brightest end of the luminosity function at these redshifts; 2) the study of very red galaxy population at intermediate redshifts, including a serendipitous discovery of a matured galaxy cluster cadidate at z ~ 2.1; 3) the search of cool Galactic dwarfs and the constraint on their scale height; and 4) the weak lensing experiment with the WFC3 data.
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Speaker:9:30am, August 01th, Tuesday
Time:Yan Gong (Max-Planck-Institute for Radio Astronomy)
Location:Middle conference room, 3rd floor
Speaker:9:30 am July 27th (Thursday)
Time:Junhao Liu (East Asian Observatory)
Location:Middle conference room, 3rd floor
Speaker:Wednesday, July 26th 3:00pm
Time:Dr. Pinghui Huang (黄平辉)
Location:Middle conference room, 3rd floor
Speaker:7月14日,星期五,上午10点
Time:闫大海(云南大学)
Location:1715
Speaker:3:00 pm July 13th (Thursday)
Time:Shuang Zhou (University of Nottingham)
Location:Lecture Hall, 3rd floor
Speaker:1:30 pm July 6th (Thursday)
Time:Prof. Wen-Ping Chen (National Central University)
Location:Lecture Hall, 3rd floor