output
20002025
most citedThe Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters

629 citations

Showing 2009Show all

6 papers · 1 filter

math.MG2009★ 3 cited

An interval version of separation by semispaces in max-min convexity

Viorel Nitica, Sergei Sergeev

We study separation of a closed box from a max-min convex set by max-min semispace. This can be regarded as an interval extension of known separation results. We give a constructiv…

astro-ph.HE2009★ 5 cited

X-ray and UV observations of nova V598 Puppis between 147 and 255 days after outburst

K. L. Page, J. P. Osborne, A. M. Read +6

Aims: The launch of Swift has allowed many more novae to be observed regularly over the X-ray band. Such X-ray observations of novae can reveal ejecta shocks and the nuclear burnin…

astro-ph.HE2009★ 62 cited

Swift observations of the X-ray and UV evolution of V2491 Cyg (Nova Cyg 2008 No. 2)

K. L. Page, J. P. Osborne, P. A. Evans +8

We present extensive, high-density Swift observations of V2491 Cyg (Nova Cyg 2008 No. 2). Observing the X-ray emission from only one day after the nova discovery, the source is fol…

astro-ph.SR2009★ 30 cited

No Transition Disk? Infrared Excess, PAH, H2, and X-rays from the Weak-Lined T Tauri Star DoAr 21

Eric L. N. Jensen, David H. Cohen, Marc Gagné

We present new high-resolution mid-infrared imaging, high-resolution optical spectroscopy, and Chandra grating X-ray spectroscopy of the weak-lined T Tauri star DoAr 21. DoAr 21 (a…

astro-ph.CO2009★ 93 cited

The Atacama Cosmology Telescope (ACT): Beam Profiles and First SZ Cluster Maps

A. D. Hincks, V. Acquaviva, P. Ade +69

The Atacama Cosmology Telescope (ACT) is currently observing the cosmic microwave background with arcminute resolution at 148 GHz, 218 GHz, and 277 GHz. In this paper, we present A…

astro-ph.HE2009★ 37 cited

Swift X-ray and UV monitoring of the Classical Nova V458 Vul (Nova Vul 2007)

J. -U. Ness, J. J. Drake, A. P. Beardmore +18

We describe the highly variable X-ray and UV emission of V458 Vul (Nova Vul 2007), observed by Swift between 1 and 422 days after outburst. Initially bright only in the UV, V458 Vu…