output
19942026
most citedThe Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

5k citations

Showing 2010 · astro-ph.EPShow all

39 papers · 2 filters

astro-ph.EP2010★ 71 cited

Qatar-1b: a hot Jupiter orbiting a metal-rich K dwarf star

K. A. Alsubai, N. R. Parley, D. M. Bramich +18

We report the discovery and initial characterisation of Qatar-1b, a hot Jupiter orbiting a metal-rich K dwarf star, the first planet discovered by the Alsubai Project exoplanet tra…

astro-ph.EP2010★ 9 cited

The WASP-South search for transiting exoplanets

Coel Hellier, D. R. Anderson, A. Collier Cameron +9

Since 2006 WASP-South has been scanning the Southern sky for transiting exoplanets. Combined with Geneva Observatory radial velocities we have so far found over 30 transiting exopl…

astro-ph.EP2010★ 56 cited

WASP-34b: a near-grazing transiting sub-Jupiter-mass exoplanet in a hierarchical triple system

B. Smalley, D. R. Anderson, A. Collier Cameron +19

We report the discovery of WASP-34b, a sub-Jupiter-mass exoplanet transiting its 10.4-magnitude solar-type host star (1SWASP J110135.89-235138.4; TYC 6636-540-1) every 4.3177 days…

astro-ph.EP2010

Detection limits for close eclipsing and transiting sub-stellar and planetary companions to white dwarfs in the WASP survey

F. Faedi, R. G. West, M. R. Burleigh +2

We used photometric data from the WASP (Wide-Angle Search for Planets) survey to explore the possibility of detecting eclipses and transit signals of brown dwarfs, gas giants and t…

astro-ph.EP2010★ 341 cited

High C/O Ratio and Weak Thermal Inversion in the Very Hot Atmosphere of Exoplanet WASP-12b

Nikku Madhusudhan, Joseph Harrington, Kevin B. Stevenson +16

The carbon-to-oxygen ratio (C/O) in a planet provides critical information about its primordial origins and subsequent evolution. A primordial C/O greater than 0.8 causes a carbide…

astro-ph.EP2010★ 142 cited

WASP-41b: A transiting hot Jupiter planet orbiting a magnetically-active G8V star

P. F. L. Maxted, D. R. Anderson, A. Collier Cameron +13

We report the discovery of a transiting planet with an orbital period of 3.05d orbiting the star TYC 7247-587-1. The star, WASP-41, is a moderately bright G8V star (V=11.6) with a…

astro-ph.EP2010★ 63 cited

The spin-orbit angles of the transiting exoplanets WASP-1b, WASP-24b, WASP-38b and HAT-P-8b from Rossiter-McLaughlin observations

E. K. Simpson, D. Pollacco, A. Collier Cameron +18

We present observations of the Rossiter-McLaughlin effect for the transiting exoplanet systems WASP-1, WASP-24, WASP-38 and HAT-P-8, and deduce the orientations of the planetary or…

astro-ph.EP2010★ 61 cited

WASP-31b: a low-density planet transiting a metal-poor, late-F-type dwarf star

D. R. Anderson, A. Collier Cameron, C. Hellier +15

We report the discovery of the low-density, transiting giant planet WASP-31b. The planet is 0.48 Jupiter masses and 1.55 Jupiter radii. It is in a 3.4-day orbit around a metal-poor…

astro-ph.EP2010★ 111 cited

A collision in 2009 as the origin of the debris trail of asteroid P/2010 A2

Colin Snodgrass, Cecilia Tubiana, Jean-Baptiste Vincent +15

The peculiar object P/2010 A2 was discovered by the LINEAR near-Earth asteroid survey in January 2010 and given a cometary designation due to the presence of a trail of material, a…

astro-ph.EP2010★ 54 cited

WASP-38b: A Transiting Exoplanet in an Eccentric, 6.87d Period Orbit

S. C. C. Barros, F. Faedi, A. Collier Cameron +31

We report the discovery of WASP-38b, a long period transiting planet in an eccentric 6.871815 day orbit. The transit epoch is 2455335.92050 +/- 0.00074 (HJD) and the transit durati…

astro-ph.EP2010★ 29 cited

The Doppler Shadow of WASP-3b: A tomographic analysis of Rossiter-McLaughlin observations

G. R. M. Miller, A. Collier Cameron, E. K. Simpson +9

Hot-Jupiter planets must form at large separations from their host stars where the temperatures are cool enough for their cores to condense. They then migrate inwards to their curr…

astro-ph.EP2010★ 29 cited

WASP-32b: A transiting hot Jupiter planet orbiting a lithium-poor, solar-type star

P. F. L Maxted, D. R. Anderson, A. Collier Cameron +13

We report the discovery of a transiting planet orbiting the star TYC 2-1155-1. The star, WASP-32, is a moderately bright (V=11.3) solar-type star (Teff=6100 +- 100K, [Fe/H] = -0.13…

astro-ph.EP2010★ 53 cited

WASP-37b: a 1.8 MJ exoplanet transiting a metal-poor star

E. K. Simpson, F. Faedi, S. C. C. Barros +39

We report on the discovery of WASP-37b, a transiting hot Jupiter orbiting a mv = 12.7 G2-type dwarf, with a period of 3.577471 \pm 0.00001 d, transit epoch T0 = 2455338.6188 \pm 0.…

astro-ph.EP2010★ 55 cited

WASP-25b: a 0.6 M_J planet in the Southern hemisphere

B. Enoch, A. Collier Cameron, D. R. Anderson +18

We report the detection of a 0.6 M_J extrasolar planet by WASP-South, WASP-25b, transiting its solar-type host star every 3.76 days. A simultaneous analysis of the WASP, FTS and Eu…

astro-ph.EP2010★ 32 cited

Ground-based multisite observations of two transits of HD 80606b

A. Shporer, J. N. Winn, S. Dreizler +41

We present ground-based optical observations of the September 2009 and January 2010 transits of HD 80606b. Based on 3 partial light curves of the September 2009 event, we derive a…

astro-ph.EP2010★ 79 cited

WASP-29b: A Saturn-sized transiting exoplanet

Coel Hellier, D. R. Anderson, A. Collier Cameron +14

We report the discovery of a Saturn-sized planet transiting a V = 11.3, K4 dwarf star every 3.9 d. WASP-29b has a mass of 0.24+/-0.02 M_Jup and a radius of 0.79+/-0.05 R_Jup, makin…

astro-ph.EP2010★ 372 cited

The first WASP public data release

O. W. Butters, R. G. West, D. R. Anderson +17

The WASP (Wide Angle Search for Planets) project is an exoplanet transit survey that has been automatically taking wide field images since 2004. Two instruments, one in La Palma an…

astro-ph.EP2010★ 10 cited

Independent discovery and refined parameters of the transiting exoplanet HAT-P-14b

E. K. Simpson, S. C. C. Barros, D. J. A. Brown +30

We present SuperWASP observations of HAT-P-14b, a hot Jupiter discovered by Torres et al. The planet was found independently by the SuperWASP team and named WASP-27b after follow-u…

astro-ph.EP2010★ 77 cited

On the alignment of debris disks and their host stars' rotation axis -implications for spin-orbit misalignment in exoplanetary systems

C. A. Watson, S. P. Littlefair, C. Diamond +5

It has been widely thought that measuring the misalignment angle between the orbital plane of a transiting exoplanet and the spin of its host star was a good discriminator between…

astro-ph.EP2010★ 454 cited

Spin-orbit angle measurements for six southern transiting planets; New insights into the dynamical origins of hot Jupiters

Amaury H. M. J. Triaud, Andrew Collier Cameron, Didier Queloz +14

For transiting planets, the Rossiter-McLaughlin effect allows the measurement of the sky-projected angle beta between the stellar rotation axis and a planet's orbital axis. Using t…

astro-ph.EP2010★ 161 cited

WASP-8b: a retrograde transiting planet in a multiple system

Didier Queloz, David Anderson, Andrew Collier Cameron +11

We report the discovery of WASP-8, a transiting planet of 2.25+-0.08 M_Jup on a strongly inclined eccentric 8.15-day orbit, moving in a retrograde direction to the rotation of its…

astro-ph.EP2010★ 56 cited

Rotation periods of exoplanet host stars

Elaine Simpson, Sallie Baliunas, Greg Henry +1

The stellar rotation periods of ten exoplanet host stars have been determined using newly analysed Ca II H & K flux records from Mount Wilson Observatory and Stromgren b, y photome…

astro-ph.EP2010★ 61 cited

WASP-21b: a hot-Saturn exoplanet transiting a thick disc star

F. Bouchy, L. Hebb, I. Skillen +25

We report the discovery of WASP-21b, a new transiting exoplanet discovered by the Wide Angle Search for Planets (WASP) Consortium and established and characterized with the FIES, S…

astro-ph.EP2010★ 32 cited

Estimating the masses of extra-solar planets

C. A. Watson, S. P. Littlefair, A. Collier Cameron +2

All extra-solar planet masses that have been derived spectroscopically are lower limits since the inclination of the orbit to our line-of-sight is unknown except for transiting sys…