output
20052026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2009Show all

13 papers · 1 filter

astro-ph.CO2009★ 47 cited

Non-parametric modeling of the intra-cluster gas using APEX-SZ bolometer imaging data

K. Basu, Y. -Y. Zhang, M. W. Sommer +23

We demonstrate the usability of mm-wavelength imaging data obtained from the APEX-SZ bolometer array to derive the radial temperature profile of the hot intra-cluster gas out to ra…

astro-ph.CO2009★ 26 cited

ASTE CO(3-2) Mapping toward the Whole Optical Disk of M 83: Properties of Inter-arm GMAs

Kazuyuki Muraoka, Kotaro Kohno, Tomoka Tosaki +9

We present a new on-the-fly (OTF) mapping of CO(J=3-2) line emission with the Atacama Submillimeter Telescope Experiment (ASTE) toward the 8' x 8' (or 10.5 x 10.5 kpc at the distan…

astro-ph.SR2009★ 76 cited

Disk and Envelope Structure in Class 0 Protostars: I. The Resolved Massive Disk in Serpens FIRS 1

Melissa L. Enoch, Stuartt Corder, Michael M. Dunham +1

We present the first results of a program to characterize the disk and envelope structure of typical Class 0 protostars in nearby low-mass star forming regions. We use Spitzer IRS…

astro-ph.GA2009★ 32 cited

Young Stars and Protostellar Cores near NGC 2023

B. Mookerjea, G. Sandell, T. H. Jarrett +1

We investigate the young (proto)stellar population in NGC 2023 and the L 1630 molecular cloud bordering the HII region IC 434, using Spitzer IRAC and MIPS archive data, JCMT SCUBA…

astro-ph.CO2009★ 99 cited

The AzTEC/SMA Interferometric Imaging Survey of Submillimeter-Selected High-Redshift Galaxies

J. D. Younger, G. G. Fazio, J. -S. Huang +14

We present results from a continuing interferometric survey of high-redshift submillimeter galaxies with the Submillimeter Array, including high-resolution (beam size ~2 arcsec) im…

astro-ph.CO2009★ 54 cited

Is cold gas fuelling the radio galaxy NGC 315?

R. Morganti, A. B. Peck, T. A. Oosterloo +5

We present WSRT, VLA and VLBI observations of the HI absorption in the radio galaxy NGC 315. The main result is that two HI absorbing systems are detected against the central regio…