Erratum: The first planet detected in the WTS: an inflated hot-Jupiter in a 3.35 d orbit around a late F star

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 444:4 (2014) 3150-3150

Authors:

M Cappetta, RP Saglia, JL Birkby, J Koppenhoefer, DJ Pinfield, ST Hodgkin, P Cruz, G Kovács, B Sipőcz, D Barrado, B Nefs, YV Pavlenko, L Fossati, C del Burgo, EL Martín, I Snellen, J Barnes, D Campbell, S Catalan, MC Gálvez-Ortiz, N Goulding, C Haswell, O Ivanyuk, H Jones, M Kuznetsov, N Lodieu, F Marocco, D Mislis, F Murgas, R Napiwotzki, E Palle, D Pollacco, L Sarro Baro, E Solano, P Steele, H Stoev, R Tata, J Zendejas

A far-infrared spectroscopic survey of intermediate redshift (ultra) luminous infrared galaxies

Astrophysical Journal IOP Publishing 796:1 (2014) 63-63

Authors:

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

Abstract:

We present Herschel far-IR photometry and spectroscopy as well as ground-based CO observations of an intermediate redshift (0.21 ≤ z ≤ 0.88) sample of Herschel-selected (ultra)-luminous infrared galaxies (L IR > 1011.5 L ☉). With these measurements, we trace the dust continuum, far-IR atomic line emission, in particular [C II] 157.7 μm, as well as the molecular gas of z ~ 0.3 luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) and perform a detailed investigation of the interstellar medium of the population. We find that the majority of Herschel-selected intermediate redshift (U)LIRGs have L C II /L FIR ratios that are a factor of about 10 higher than that of local ULIRGs and comparable to that of local normal and high-z star-forming galaxies. Using our sample to bridge local and high-z [C II] observations, we find that the majority of galaxies at all redshifts and all luminosities follow an L C II –L FIR relation with a slope of unity, from which local ULIRGs and high- z active-galactic-nucleus-dominated sources are clear outliers. We also confirm that the strong anti-correlation between the L C II /L FIR ratio and the far-IR color L 60/L 100 observed in the local universe holds over a broad range of redshifts and luminosities, in the sense that warmer sources exhibit lower L C II /L FIR at any epoch. Intermediate redshift ULIRGs are also characterized by large molecular gas reservoirs and by lower star formation efficiencies compared to that of local ULIRGs. The high L C II /L FIR ratios, the moderate star formation efficiencies (L IR/$L^{\prime }_{\rm CO}$ or L IR/$M_{\rm H_{\rm 2}}$), and the relatively low dust temperatures of our sample (which are also common characteristics of high-z star-forming galaxies with ULIRG-like luminosities) indicate that the evolution of the physical properties of (U)LIRGs between the present day and z > 1 is already significant by z ~ 0.3.

CoRoT-22 b: a validated 4.9 R⊕ exoplanet in 10-d orbit★†

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 444:3 (2014) 2783-2792

Authors:

C Moutou, JM Almenara, RF Díaz, R Alonso, M Deleuil, E Guenther, T Pasternacki, S Aigrain, A Baglin, P Barge, AS Bonomo, P Bordé, F Bouchy, J Cabrera, S Carpano, WD Cochran, Sz Csizmadia, HJ Deeg, R Dvorak, M Endl, A Erikson, S Ferraz-Mello, M Fridlund, D Gandolfi, T Guillot, A Hatzes, G Hébrard, C Lovis, H Lammer, PJ MacQueen, T Mazeh, A Ofir, M Ollivier, M Pätzold, H Rauer, D Rouan, A Santerne, J Schneider, B Tingley, G Wuchterl

The transit spectra of Earth and Jupiter

Icarus Elsevier 242 (2014) 172-187

Authors:

PGJ Irwin, JK Barstow, NE Bowles, LN Fletcher, S Aigrain, J-M Lee

HST hot-Jupiter transmission spectral survey: detection of potassium in WASP-31b along with a cloud deck and Rayleigh scattering

(2014)

Authors:

DK Sing, HR Wakeford, AP Showman, N Nikolov, JJ Fortney, AS Burrows, GE Ballester, D Deming, S Aigrain, J-M Désert, NP Gibson, GW Henry, H Knutson, A Lecavelier des Etangs, F Pont, A Vidal-Madjar, MW Williamson, PA Wilson