HAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P-53b: Three Transiting Hot Jupiters and a Transiting Hot Saturn From the HATNet Survey

We report the discovery and characterization of four transiting exoplanets by the HATNet survey. The planet HAT-P-50b has a mass of 1.35 M_J and a radius of 1.29 R_J, and orbits a bright (V = 11.8 mag) M = 1.27 M_sun, R = 1.70 R_sun star every P = 3.1220 days. The planet HAT-P-51b has a mass of 0.31 M_J and a radius of 1.29 R_J, and orbits a V = 13.4 mag, M = 0.98 M_sun, R = 1.04 R_sun star with a period of P = 4.2180 days. The planet HAT-P-52b has a mass of 0.82 M_J and a radius of 1.01 R_J, and orbits a V = 14.1 mag, M = 0.89 M_sun, R = 0.89 R_sun star with a period of P = 2.7536 days. The planet HAT-P-53b has a mass of 1.48 M_J and a radius of 1.32 R_J, and orbits a V = 13.7 mag, M = 1.09 M_sun, R = 1.21 R_sun star with a period of P = 1.9616 days. All four planets are consistent with having circular orbits and have masses and radii measured to better than 10% precision. The low stellar jitter and favorable R_P/R_star ratio for HAT-P-51 make it a promising target for measuring the Rossiter-McLaughlin effect for a Saturn-mass planet.Comment: Submitted to AJ. 20 pages, 9 figures, 5 tables. Data available at http://hatnet.org

Nouvelles recherches expérimentales sur le virus de la rhino-amygdalite contagieuse du chien I. Pouvoir pathogène expérimental

Goret Pierre, Brion Abel, Fontaine M., Fontaine M.-P., Pilet Charles, Girard Marc, Girard M. Nouvelles recherches expérimentales sur le virus de la rhino-amygdalite contagieuse du chien. I - Pouvoir pathogène expérimental. In: Bulletin de l'Académie Vétérinaire de France tome 112 n°10, 1959. pp. 625-634

Report on the CCT Supplementary Comparison S1 of Infrared Spectral Normal Emittance/Emissivity

open9openHanssen, L; Wilthan, B; Filtz, J -R; Hameury, J; Girard, F; Battuello, M; Ishii, J; Hollandt, J; Monte, CHanssen, L; Wilthan, B; Filtz, J. R; Hameury, J; Girard, Ferruccio; Battuello, Mauro; Ishii, J; Hollandt, J; Monte, C

Searching for young Jupiter analogs around AP Col: L-band high-contrast imaging of the closest pre-main sequence star

The nearby M-dwarf AP Col was recently identified by Riedel et al. 2011 as a pre-main sequence star (age 12 - 50 Myr) situated only 8.4 pc from the Sun. The combination of its youth, distance, and intrinsically low luminosity make it an ideal target to search for extrasolar planets using direct imaging. We report deep adaptive optics observations of AP Col taken with VLT/NACO and Keck/NIRC2 in the L-band. Using aggressive speckle suppression and background subtraction techniques, we are able to rule out companions with mass m >= 0.5 - 1M_Jup for projected separations a>4.5 AU, and m >= 2 M_Jup for projected separations as small as 3 AU, assuming an age of 40 Myr using the COND theoretical evolutionary models. Using a different set of models the mass limits increase by a factor of ~2. The observations presented here are the deepest mass-sensitivity limits yet achieved within 20 AU on a star with direct imaging. While Doppler radial velocity surveys have shown that Jovian bodies with close-in orbits are rare around M-dwarfs, gravitational microlensing studies predict that ~17% of these stars host massive planets with orbital separations of 1-10 AU. Sensitive high-contrast imaging observations, like those presented here, will help to validate results from complementary detection techniques by determining the frequency of gas giant planets on wide orbits around M-dwarfs.Comment: Accepted for publication in ApJ, 6 pages text ApJ style (incl. references), 4 figures, 1 tabl

The food of the larvae of the northern anchovy Engraulis mordax

ENGLISH: Hitherto the only investigation dealing with the food and feeding of the larvae of the northern anchovy, Engraulis mordax Girard, was that of Arthur (1956). His main consideration was, however, with the Pacific sardine, Sardinops caerulea (Girard), and his work on the anchovy can only be considered preliminary. The present investigation is a continuation of Arthur's work on the food of the larval northern anchovy. SPANISH:El único trabajo publicado hasta ahora que trata sobre el alimento y nutrición de las larvas de la anchoa norteña, Engraulis mordax Girard, es el de Arthur (1956); pero su objeto principal fué la sardina del Pacifico, Sardinops caendea (Girard), y el estudio dedicado a la anchoa solo puede considerarse como preliminar. La presente investigación es una continuación del estudio de Arthur sobre el alimento de las larvas de la anchoa norteña