Extremely Large Telescope: publications

Identification of old tidal dwarfs near early-type galaxies from deep imaging and HI observations

(2014)

Authors:

Pierre-Alain Duc, Sanjaya Paudel, Richard M McDermid, Jean-Charles Cuillandre, Paolo Serra, Frédéric Bournaud, Michele Cappellari, Eric Emsellem

Salpeter normalization of the Stellar Initial Mass Function for massive galaxies at z~1

(2014)

Authors:

Shravan Shetty, Michele Cappellari

WTS-2 b: a hot Jupiter orbiting near its tidal destruction radius around a K-dwarf

(2014)

Authors:

JL Birkby, M Cappetta, P Cruz, J Koppenhoefer, O Ivanyuk, AJ Mustill, ST Hodgkin, DJ Pinfield, B Sipőcz, G Kovács, R Saglia, Y Pavlenko, D Barrado, A Bayo, D Campbell, S Catalan, L Fossati, M-C Gálvez-Ortiz, M Kenworthy, J Lillo-Box EL Martín, D Mislis, EJW de Mooij, SV Nefs, IAG Snellen, H Stoev, J Zendejas, C del Burgo, J Barnes, N Goulding, CA Haswell, M Kuznetsov, N Lodieu, F Murgas, E Palle, E Solano, P Steele, R Tata

The Atlas3D project - XXVI. HI discs in real and simulated fast and slow rotators

(2014)

Authors:

Paolo Serra, Ludwig Oser, Davor Krajnovic, Thorsten Naab, Tom Oosterloo, Raffaella Morganti, Michele Cappellari, Eric Emsellem, Lisa M Young, Leo Blitz, Timothy A Davis, Pierre-Alain Duc, Michaela Hirschmann, Anne-Marie Weijmans, Katherine Alatalo, Estelle Bayet, Maxime Bois, Frederic Bournaud, Martin Bureau, Roger L Davies, PT de Zeeuw, Sadegh Khochfar, Harald Kuntschner, Pierre-Yves Lablanche, Richard M McDermid, Marc Sarzi, Nicholas Scott

Herschel Observations of Far-Infrared Cooling Lines in intermediate Redshift (Ultra)-luminous Infrared Galaxies

ArXiv 1401.23 (2014)

Authors:

D Rigopoulou, R Hopwood, GE Magdis, N Thatte, BM Swinyard, D Farrah, J-S Huang, A Alonso-Herrero, JJ Bock, D Clements, A Cooray, MJ Griffin, S Oliver, C Pearson, D Riechers, D Scott, A Smith, M Vaccari, I Valtchanov, L Wang

Abstract:

We report the first results from a spectroscopic survey of the [CII] 158um line from a sample of intermediate redshift (0.210^11.5 Lsun), using the SPIRE-Fourier Transform Spectrometer (FTS) on board the Herschel Space Observatory. This is the first survey of [CII] emission, an important tracer of star-formation, at a redshift range where the star-formation rate density of the Universe increases rapidly. We detect strong [CII] 158um line emission from over 80% of the sample. We find that the [CII] line is luminous, in the range (0.8-4)x10^(-3) of the far-infrared continuum luminosity of our sources, and appears to arise from photodissociation regions on the surface of molecular clouds. The L[CII]/LIR ratio in our intermediate redshift (U)LIRGs is on average ~10 times larger than that of local ULIRGs. Furthermore, we find that the L[CII]/LIR and L[CII]/LCO(1-0) ratios in our sample are similar to those of local normal galaxies and high-z star-forming galaxies. ULIRGs at z~0.5 show many similarities to the properties of local normal and high-z star forming galaxies. Our findings strongly suggest that rapid evolution in the properties of the star forming regions of luminous infrared galaxies is likely to have occurred in the last 5 billion years.

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