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The quest to discover exoplanets is one of the most important missions in astrophysics, and is widely performed using the transit method, which allows for the detection of exoplanets down to the size of Mercury. However, to confirm these…

The Transiting Exoplanet Survey Satellite (TESS) will be conducting a nearly all-sky photometric survey over two years, with a core mission goal to discover small transiting exoplanets orbiting nearby bright stars. It will obtain 30-minute…

As the NASA Transiting Exoplanet Survey Satellite (TESS) fulfills its primary mission it is executing an unprecedented all-sky survey with the potential to discover distant planets in our own solar system, as well as hundreds of…

地球与行星天体物理 · 物理学 2019-10-16 Matthew J. Holman , Matthew J. Payne , András Pál

We discuss the system requirements for obtaining millimagnitude photometric precision over a wide field using small aperture short focal length telescope systems, such as are being developed by a number of research groups to search for…

天体物理学 · 物理学 2011-05-05 G. Bakos , R. W. Noyes , G. Kovacs , K. Z. Stanek , D. D. Sasselov , Istvan Domsa

The CALorimetric Electron Telescope (CALET) is a high-energy astroparticle physics space experiment installed on the International Space Station (ISS), developed and operated by Japan in collaboration with Italy and the United States. The…

The processes that transform gas and dust in circumstellar disks into diverse exoplanets remain poorly understood. One key pathway is to study exoplanets as they form in their young ($\sim$few~Myr) natal disks. Extremely Large Telescopes…

NEAT is an astrometric mission proposed to ESA with the objectives of detecting Earth-like exoplanets in the habitable zone of nearby solar-type stars. In NEAT, one fundamental aspect is the capability to measure stellar centroids at the…

天体物理仪器与方法 · 物理学 2013-09-18 A. Crouzier , F. Malbet , O. Preis , F. Henault , P. Kern , G. Martin , P. Feautrier , c. Cara , P. Lagage , A. Leger , J. M. LeDuigou , M. Shao , R. Goullioud

We show that a space-based gravitational microlensing survey for terrestrial extra-solar planets is feasible in the near future, and could provide a nearly complete picture of the properties of planetary systems in our Galaxy. We present…

天体物理学 · 物理学 2009-10-31 David P. Bennett , Sun Hong Rhie

We present design considerations for a ground-based survey for transiting exoplanets around L and T dwarfs, spectral classes that have yet to be thoroughly probed for planets. We simulate photometry for L and T targets with a variety of…

地球与行星天体物理 · 物理学 2019-10-09 Patrick Tamburo , Philip S. Muirhead

The Near Earth Object Surveillance Satellite (NEOSSat) is a Canadian-led 15 cm Earth-orbiting telescope originally designed to detect asteroids near the Sun. Its design is however also suitable for the observation of exoplanetary transits…

地球与行星天体物理 · 物理学 2022-09-21 Chris Fox , Paul Wiegert

Ground-based exoplanet surveys such as SuperWASP, HATNet and KELT have discovered close to two hundred transiting extrasolar planets in the past several years. The strategy of these surveys is to look at a large field of view and measure…

天体物理仪器与方法 · 物理学 2016-03-23 M. Zhang , G. Á. Bakos , K. Penev , Z. Csubry , J. D. Hartman , W. Bhatti , M. de Val-Borro

The Deep Lens Survey (DLS) is a deep BVRz' imaging survey of seven 2x2 degree fields, with all data to be made public. The primary scientific driver is weak gravitational lensing, but the survey is also designed to enable a wide array of…

We present a conceptual design for a space based Galactic Exoplanet Survey Telescope (GEST) which will use the gravitational microlensing technique to detect extra solar planets with masses as low as that of Mars at all separations >~ 1 AU.…

天体物理学 · 物理学 2007-05-23 David P. Bennett , Sun Hong Rhie

In this paper we present simulated observations of galaxies at z=2 and z=3 to probe the capabilities of next-generation telescopes (E-ELT and JWST) to measure the structural and photometrical properties of high redshift galaxies. We carry…

星系天体物理 · 物理学 2016-08-31 M. Gullieuszik , R. Falomo , L. Greggio , M. Uslenghi , D. Fantinel

Two planetary mass objects in the far outer Solar System --- collectively referred to here as Planet X --- have recently been hypothesized to explain the orbital distribution of distant Kuiper Belt Objects. Neither planet is thought to be…

地球与行星天体物理 · 物理学 2018-06-14 David E. Trilling , Eric C. Bellm , Renu Malhotra

Extremely large telescopes (ELTs) are considered worldwide to be one of the highest priorities in ground-based astronomy. The European Southern Observatory (ESO) is developing an ELT that will have a 39 m main mirror and will be the largest…

天体物理仪器与方法 · 物理学 2023-12-08 Paolo Padovani , Michele Cirasuolo

CALET (CALorimetric Electron Telescope) is a high energy astroparticle physics experiment planned for a long exposure mission aboard the International Space Station (ISS) by the Japanese Aerospace Exploration Agency, in collaboration with…

天体物理仪器与方法 · 物理学 2015-12-29 Pier Simone Marrocchesi

The photometric data collected during 2001 season OGLE-III planetary/low luminosity object transit campaign were reanalyzed with the new transit search technique -- the BLS method by Kovacs, Zucker and Mazeh. In addition to all presented in…

天体物理学 · 物理学 2007-05-23 A. Udalski , K. Zebrun , M. Szymanski , M. Kubiak , I. Soszynski , O. Szewczyk , L. Wyrzykowski , G. Pietrzynski

Planetary transits of bright stars, V < 10, offer the best opportunity for detailed studies of extra-solar planets, such as are already being carried out for HD209458b. Since these stars are rare, they should be searched over the entire…

天体物理学 · 物理学 2007-05-23 Joshua Pepper , Andrew Gould , D. L. DePoy