- 追加された行はこの色です。
- 削除された行はこの色です。
*IoA Seminar 2014 / 2014年度・東京大学・天文学教育研究センター・談話会 [#na2aa933]
#contents
**次回以降の談話会 [#tbf77961]
*** 第261回: 2015/3/5 (Thu) 15:30-16:30 [#y0c6ad97]
*** 第259回: 2015/2/16 (Mon) 14:00-15:00 [#y0c6ad97]
*** Speaker: Leonardo Vanzi (Pontificia Universidad Catolica de Chile) [#w10e627c]
*** Speaker: Kevin Bundy (IPMU, U.Tokyo) [#k4e7336c]
*** Title: Astronomical Instrumentation Made in Chile [#wac46e13]
*** Title: MaNGA: Mapping Nearby Galaxies at APO An IFU Survey of 10,000 Galaxies [#tea1557b]
Since the recognition of Chile as an Astronomical paradise about 50 years ago,
Chilean Astronomy has grown inflactionary to the proportion of being today
one of the most productive areas of science in Chile, represented by a well developed
community at the level of the most developed countries. Today we are facing
a second phase in this growth with a program aimed at the development in Chile
of instrumentation for astronomy. This task is being especially challenging
because of the limiting boundary conditions of a developing country.
In this talk I will present the efforts carried out in this direction at the Center of
Astro Engineering UC, the first scientific results obtained with astronomical instruments
made in Chile and the exciting challenges that we are preparing for the future.
I will discuss the design and execution of a new survey to obtain resolved spectroscopy
for 10,000 nearby galaxies called MaNGA (Mapping Nearby Galaxies at Apache Point Observatory).
One of three core programs in the 6-year SDSS-IV project that began on July 1st, 2014,
MaNGA will deploy 17 fiber-bundle IFUs across the Sloan 2.5m Telescope's 3 degree field-of-view,
targeting a mass-selected sample with a median redshift of 0.03, typical spatial resolution of 1-2 kpc,
and a per-fiber signal-to-noise ratio of 4-8 in the outskirts of target galaxies. For each galaxy
in the sample, MaNGA will provide maps and measured gradients of the composition
and dynamics of both stars and gas. I will present early results using a prototype instrument
that highlight MaNGA's potential to shed light on the ionization and chemical enrichment of gas
in galaxies, spatial patterns in their star formation histories, and the internal makeup of
stellar populations. MaNGA's unprecedented data set will not only provide powerful new
insight on galaxy formation and evolution but will serve as a valuable benchmark for future
high-z observations from large telescopes as well as JWST.
*** 第260回: 2015/2/19 (Thu) 15:30-16:30 [#je0027ac]
*** Speaker: Wiphu Rujopakarn (IPMU, U.Tokyo) [#i2ec0ab7]
*** Title: Resolving the Obscured Cosmic Accretion History and Modes of Galaxy Assembly [#u0de23c7]
Dust obscuration has hidden at least half of the cosmic accretion
activity and concealed the most intense sites of star formation during
the peak epoch for both processes in galaxy evolution at 1 < z < 3.
Centimetric radio interferometry is the only means of identifying the
AGNs and tracing star-forming activities at sub-arcsecond resolution,
in an extinction-independent manner. I will discuss the use of radio
survey to study star formation and AGN at 1 < z < 3, focusing on the
early results from two ultra-deep 4-8 GHz Jansky VLA (JVLA) radio
observations at 0.3" resolution in the UDS and HUDF fields. The goals
of these surveys are to combine the radio data with the existing
panchromatic observations to produce a complete census of AGN and to
spatially resolve the star-forming galaxies. The ongoing survey in the
HUDF, in particular, will reach 0.3 microJy/beam RMS and will provide
the definitive radio dataset for spatially-resolved, ultra-deep,
broadband extragalactic studies until the SKA era.
** 趣旨 [#v1d3180b]
東京大学・天文学教育研究センターでは2003年4月から, [[院生コロキウム:http://www.ioa.s.u-tokyo.ac.jp/colloquium/wiki/]]に引き続き, 談話会を開いています.
第一線で活躍されている研究者の方々を講師にお招きし, 最先端の研究成果をお話しいただきます.
講師の方には, 大学院生の参加者のことも考慮し, レビュー的な側面も含めた上で, ご自身の研究紹介をお願いしています.
**日時 [#q477aa18]
-木曜日
-15:30-16:30
**場所 [#t599f0e2]
-天文センター講義室
**標準タイムテーブル [#i15c8b29]
|13:30-14:30|[[院生コロキウム:http://www.ioa.s.u-tokyo.ac.jp/colloquium/wiki/]]|講義室|
|15:30-16:30|談話会|講義室|
|16:30-|お茶の時間|講義室横のお茶部屋~講師の方を交えて~|
**世話人 [#zd16b7cd]
-河野孝太郎: kkohno_at_ioa.s.u-tokyo.ac.jp (_at_を@に置き換えてください)
-田辺俊彦: ttanabe_at_ioa.s.u-tokyo.ac.jp (_at_を@に置き換えてください)
-石井峻: sishii_at_ioa.s.u-tokyo.ac.jp (_at_を@に置き換えてください)
**予定 [#j8e660b8]
|BGCOLOR(cyan):#|BGCOLOR(cyan):日付|BGCOLOR(cyan):講演者 (所属)|BGCOLOR(cyan):タイトル|
|258|2015/1/29(Thu)|Giuseppe Bono (University of Rome Tor Vergata)|The E-ELT project and stellar populations|
|259|2015/2/16(Mon) 14:00 - 15:00|Kevin Bundy (IPMU, U.Tokyo)|MaNGA: Mapping Nearby Galaxies at APO An IFU Survey of 10,000 Galaxies|
|260|2015/2/19(Thu)|Wiphu Rujopakarn (IPMU, U.Tokyo)|Resolving the Obscured Cosmic Accretion History and Modes of Galaxy Assembly|
|261|2015/3/5(Thu)|Leonardo Vanzi (Pontificia Universidad Catolica de Chile)|(TBD)|
|261|2015/3/5(Thu)|Leonardo Vanzi (Pontificia Universidad Catolica de Chile)|Astronomical Instrumentation Made in Chile|
**終了した談話会(2014年度) [#qc092a5c]
詳細はこちら: [[平成26 (2014) 年度談話会]]
|BGCOLOR(cyan):#|BGCOLOR(cyan):日付|BGCOLOR(cyan):講演者 (所属)|BGCOLOR(cyan):タイトル|
|243|2014/04/17(Thu)|田中雅臣(NAOJ)|重力波天文学時代の突発天体観測|
|244|2014/04/24(Thu)|石井峻(東大天文センター)|南極天文学開拓のための可搬型サブミリ波望遠鏡の開発|
|245|2014/05/8(Thu)|藤井通子 (NAOJ)|N体シミュレーションで探る星団の形成と進化|
|246|2014/05/12(Mon) 16:00-17:00※曜日・開始時刻注意|Francois Petrelis(Laboratoire de Physique Statistique, Ecole Normale Superieure)|Reversals and Dynamics of the magnetic field generated by dynamo instability|
|247|2014/05/15(Thu)|細川隆史 (東大)|The first stars: their diversity and beyond|
|248|2014/06/19(Thu)|大澤亮 (東大 IoA)|星周環境における PAH とそのスペクトルの進化|
|249|2014/06/26(Thu)|中島王彦 (NAOJ)|星形成銀河の星間物質の電離状態|
|250|2014/07/03(Thu)|廿日出文洋 (NAOJ)|Two gamma-ray bursts from dusty regions with little molecular gas|
|251|2014/07/17(Thu)|福島登志夫 (NAOJ)|Analytical computation of generalized Fermi-Dirac integrals by truncated Sommerfeld expansions|
|252|2014/08/21(Thu)|但木謙一 (NAOJ)|最盛期の銀河形成を解剖する|
|253|2014/10/8(Wed) 13:35 - 14:00 |Prof. Hideo Kimura (U.Tokyo, Graduate School of Arts and Sciences)|Native Andean and Amazonian Astronomy|
| |2014/10/8(Wed) 14:00 - 14:30 |Ana María Barón (Environmental Consultant)|Archaeology and cultural heritage in the context of ALMA and TAO project|
|254|2014/10/16(Thu)|James Chibueze (Chile Observatory, NAOJ)|The Puzzle of Massive Star Formation: A Multi-wavelength Approach|
|255|2014/10/23(Thu)|Mark Hammonds (U.Tokyo)|Decomposition of the 3 micron feature in AKARI grism spectra|
|256|2014/11/20(Thu)|Ronin Wu (U.Tokyo)|Spatially resolved physical conditions in M83, revealed by the Herschel SPIRE FTS|
|257|2014/12/04(Thu)|川口俊宏 (国立天文台・天文データセンター)|銀河衝突に伴う巨大ブラックホールの進化|
|258|2015/1/29(Thu)|Giuseppe Bono (University of Rome Tor Vergata)|The E-ELT project and stellar populations|
|259|2015/2/16(Mon) 14:00 - 15:00|Kevin Bundy (IPMU, U.Tokyo)|MaNGA: Mapping Nearby Galaxies at APO An IFU Survey of 10,000 Galaxies|
|260|2015/2/19(Thu)|Wiphu Rujopakarn (IPMU, U.Tokyo)|Resolving the Obscured Cosmic Accretion History and Modes of Galaxy Assembly|
**これまでの談話会 [#p38c7eef]
-[[平成26 (2014) 年度談話会]]
-[[平成25 (2013) 年度談話会]]
-[[平成24 (2012) 年度談話会]]
-[[平成23 (2011) 年度談話会]]
-[[平成22 (2010) 年度談話会:http://www.ioa.s.u-tokyo.ac.jp/danwakai//past/danwakai_H22.html]]
-[[平成21 (2009) 年度談話会:http://www.ioa.s.u-tokyo.ac.jp/danwakai//past/danwakai_H21.html]]
-[[平成20 (2008) 年度談話会:http://www.ioa.s.u-tokyo.ac.jp/danwakai//past/danwakai_H20.html]]
-[[平成19 (2007) 年度談話会:http://www.ioa.s.u-tokyo.ac.jp/danwakai//past/danwakai_H19.html]]
-[[平成18 (2006) 年度談話会:http://www.ioa.s.u-tokyo.ac.jp/danwakai//past/danwakai_H18.html]]
-[[平成17 (2005) 年度談話会:http://www.ioa.s.u-tokyo.ac.jp/danwakai//past/danwakai_H17.html]]
-[[平成16 (2004) 年度談話会:http://www.ioa.s.u-tokyo.ac.jp/danwakai//past/danwakai_H16.html]]
-[[平成15 (2003) 年度談話会:http://www.ioa.s.u-tokyo.ac.jp/danwakai//past/danwakai_H15.html]]
![[PukiWiki]](image/pukiwiki.png "[PukiWiki]")
