800 citations · 7k across the 64 of their papers we have counts for
64 papers
Gravitational lensing reveals extreme dust-obscured star formation in quasar host galaxies
H. R. Stacey, J. P. McKean, N. C. Robertson +8
We have observed 104 gravitationally-lensed quasars at with Herschel/SPIRE, the largest such sample ever studied. By targeting gravitational lenses, we probe intrinsic f…
High-J CO Versus Far-Infrared Relations in Normal and Starburst Galaxies
Daizhong Liu, Yu Gao, Kate Isaak +4
We present correlations between 9 CO transition ( to ) and beam-matched far-infrared (Far-IR) luminosities () among 167 local galaxies, using {\…
The Herschel Comprehensive (U)LIRG Emission Survey (HerCULES): CO Ladders, fine structure lines, and neutral gas cooling
M. J. F. Rosenberg, P. P. van der Werf, S. Aalto +27
(Ultra) Luminous Infrared Galaxies ((U)LIRGs) are objects characterized by their extreme infrared (8-1000 m) luminosities (L and L…
Warm Molecular Gas in Luminous Infrared Galaxies
N. Lu, Y. Zhao, C. K. Xu +18
We present our initial results on the CO rotational spectral line energy distribution (SLED) of the to 1 transitions from up to from Herschel SPIRE spectroscop…
Molecular gas heating mechanisms, and star formation feedback in merger/s tarbursts: NGC 6240 and Arp 193 as case studies
Padelis P. Papadopoulos, Zhi-Yu Zhang, E. M. Xilouris +6
We used the SPIRE/FTS instrument aboard the Herschel Space Observatory (HSO) to obtain the Spectral Line Energy Distributions (SLEDs) of CO from J=4-3 to J=13-12 of Arp 193 and NGC…
The applicability of FIR fine-structure lines as Star Formation Rate tracers over wide ranges of metallicities and galaxy types
Ilse De Looze, Diane Cormier, Vianney Lebouteiller +19
We analyze the applicability of far-infrared fine-structure lines [CII] 158 micron, [OI] 63 micron and [OIII] 88 micron to reliably trace the star formation rate (SFR) in a sample…