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11月4日 Strongly lensed high redshift galaxies identified in Herschel wide surveys. Prospects for ALMA observations
2011年11月02日
报告题目:Strongly lensed high redshift galaxies identified in Herschel wide surveys. Prospects for ALMA observations
报 告 人:Prof. Alain Omont
   (Institut d'Astrophysique de Paris)
  Research Director at The Centre National de la Recherche Scientifique,France
  Former director of IAP and Observatoire de Grenoble
  Former member of National Committee of Scientific Programs of CNES
摘   要:The very few early known, strongly lensed high-z sub-mm sources (FIRAS10214, Cloverleaf, APM08279), played a very important role in the development of high-z submm/mm astronomy through pioneer detections of 0.85-1.2mm continuum and CO lines, and various high sensitivity studies allowed by their strong magnification. Herschel wide surveys, which will hopefully observe ~1000 deg², are discovering hundreds of similarly strongly lensed submm galaxies (e.g. Negrello et al. 2010). I will first review the current state of mm/submm follow-up of such Herschel lensed galaxies with IRAM and other facilities, for CO redshift determination, mapping mm continuum and CO lines with interferometers, measuring 1.2mm continuum flux density, etc. I will specially stress the case of the recent detection of H2O at IRAM/PdBI in two such sources at z=2.3 and 3.3 (Omont et al. 2011). These examples give an idea of the numerous studies allowed by strong lensing magnification and the enhanced capabilities of ALMA and IRAM/NOEMA, using this unique sample of hundreds of Herschel high-z lensed galaxies.
时   间:2011年11月4日(星期五)上午10:30
地   点:苏富特 三楼 会议室
欢迎大家参加,提前占座。
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