activity
19932024
most citedObscured and unobscured active galactic nuclei in the Spitzer Space Telescope First Look Survey

692 citations · 8.7k across the 131 of their papers we have counts for

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49 papers · 1 filter

astro-ph2008★ 19 cited

Powerful H Emission and Star Formation on the Interacting Galaxy System Arp 143: Observations with Spitzer and GALEX

P. Beirão, P. N. Appleton, B. R. Brandl +3

We present new mid-infrared (m) and ultraviolet (1539 -- 2316 Å) observations of the interacting galaxy system Arp 143 (NGC 2444/2445) from the Spitzer Space Telescope and…

astro-ph2008★ 9 cited

The hidden HI-massive LIRG HIZOA J0836-43: Inside-out galaxy formation

M. E. Cluver, T. H. Jarrett, P. N. Appleton +6

HIZOA J0836-43 is an extreme gas-rich (=7.5$\times10^{10} M_{\sun}$) disk galaxy which lies hidden behind the strongly obscuring Vela region of the Milky Way. Utilizin…

astro-ph2008★ 26 cited

Molecular gas and dust in Arp 94: The formation of a recycled galaxy in an interacting system

U. Lisenfeld, C. G. Mundell, E. Schinnerer +2

We present new results for the molecular gas, dust emission and the ionized gas in J1023+1952, an HI rich intergalactic star-forming tidal dwarf galaxy candidate. It is located at…

astro-ph2008★ 8 cited

The Molecular Hydrogen Explorer H2EX

F. Boulanger, J. P. Maillard, P. Appleton +12

The Molecular Hydrogen Explorer, H2EX, was proposed in response to the ESA 2015 - 2025 Cosmic Vision Call as a medium class space mission with NASA and CSA participations. The miss…

astro-ph2008★ 44 cited

Stochastic `Beads on a String' in the Accretion Tail of Arp 285

B. J. Smith, C. Struck, M. Hancock +6

We present Spitzer infrared, GALEX UV, and SDSS and SARA optical images of the peculiar interacting galaxy pair Arp 285 (NGC 2856/4), and compare with a new numerical model of the…

astro-ph2007★ 50 cited

Spatially Resolved Spitzer-IRS Spectroscopy of the Central Region of M82

P. Beirão, B. R. Brandl, P. N. Appleton +6

We present high spatial resolution (~ 35 parsec) 5-38 um spectra of the central region of M82, taken with the Spitzer Infrared Spectrograph. From these spectra we determined the fl…