output
19912026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2013 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2013★ 67 cited

A survey for transients and variables with the Murchison Widefield Array 32-tile prototype at 154 MHz

M. E. Bell, T. Murphy, D. L. Kaplan +55

We present a search for transient and variable radio sources at 154 MHz with the Murchison Widefield Array 32-tile prototype. Fifty-one images were obtained that cover a field of v…

astro-ph.GA2013★ 55 cited

W40 region in the Gould Belt : An embedded cluster and H II region at the junction of filaments

K. K. Mallick, M. S. N. Kumar, D. K. Ojha +3

We present a multiwavelength study of W40 star-forming region using IR observations in UKIRT JHK bands, Spitzer IRAC bands & Herschel PACS bands; 2.12 micron H2 narrow-band imaging…

astro-ph.GA2013★ 18 cited

Molecular line and continuum study of the W40 cloud

L. Pirogov, D. K. Ojha, M. Thomasson +2

The dense cloud associated with W40, one of the nearby H II regions, has been studied in millimeter-wave molecular lines and in 1.2 mm continuum. Besides, 1280 MHz and 610 MHz inte…

astro-ph.GA2013★ 1 cited

O~{\small VI} absorption in the Milky Way along the Large Magellanic Cloud lines of sight

Rathin Sarma, Amit Pathak, Ananta C. Pradhan +2

We have used \textit{Far Ultraviolet Spectroscopic Explorer (FUSE)} observations of the Large Magellanic Cloud (LMC) to determine the O {\small VI} column densities in the Milky Wa…

astro-ph.GA2013

Gas and Dust in the Magellanic Clouds

Ananta C. Pradhan

The far-ultraviolet (FUV) diffuse emission is predominantly due to scattering of starlight from interstellar dust grains which shows a large regional variation depending on the rel…

astro-ph.GA2013★ 9 cited

Large-scale mapping of the massive star-forming region RCW38 in the [CII] and PAH emission

H. Kaneda, T. Nakagawa, S. K. Ghosh +10

We investigate the large-scale structure of the interstellar medium (ISM) around the massive star cluster RCW38 in the [CII] 158 um line and polycyclic aromatic hydrocarbon (PAH) e…