output
19922026
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

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199 papers · 1 filter

astro-ph2008★ 3 cited

The shaping effect of collimated fast outflows in the Egg nebula

Dinh-V-Trung, Jeremy Lim

We present high angular resolution observations of the HCN J=5--4 line from the Egg nebula, which is the archetype of protoplanetary nebulae. We find that the HCN emi…

astro-ph2008★ 38 cited

Molecular Superbubbles and Outflows from Starburst Galaxy NGC 2146

An-Li Tsai, Satoki Matsushita, Kouichiro Nakanishi +7

We present results from a deep (1 sigma = 5.7 mJy beam^{-1} per 20.8 km s^{-1} velocity channel) ^{12}CO(1-0) interferometric observation of the central 60" region of the nearby ed…

astro-ph2008★ 38 cited

Submillimeter narrow emission lines from the inner envelope of IRC+10216

Nimesh A. Patel, Ken H. Young, Sandra Brünken +8

A spectral-line survey of IRC+10216 in the 345 GHz band has been undertaken with the Submillimeter Array. Although not yet completed, it has already yielded a fairly large sample o…

astro-ph2008★ 14 cited

Tests of AMiBA Data Integrity

Hiroaki Nishioka, Fu-Cheng Wang, Jiun-Huei Proty Wu +26

We describe methods used to validate data from the Y.T. Lee Array for Microwave Background Anisotropy (AMiBA), an interferometric array designed to measure the Sunyaev-Zel'dovich e…

astro-ph2008★ 59 cited

SMA CO(J=6-5) and 435 micron interferometric imaging of the nuclear region of Arp 220

Satoki Matsushita, Daisuke Iono, Glen R. Petitpas +11

We have used the Submillimeter Array (SMA) to make the first interferometric observations (beam size ~1") of the 12CO J=6-5 line and 435 micron (690 GHz) continuum emission toward…

astro-ph2008★ 17 cited

Galaxy Clusters at 0.9<z<1.7 in the AKARI NEP deep field

Tomotsugu Goto, Hitoshi Hanami, Myungshin Im +11

There is a huge gap between properties of red-sequence selected massive galaxy clusters at z<1 and Lyman-break selected proto-clusters at z>3. It is important to understand when an…