Sentences with phrase «spectroscopy survey»

One of NASA's proposed missions, known as the Fast INfrared Exoplanet Spectroscopy Survey Explorer (FINESSE), could greatly improve our understanding of extrasolar worlds.

My research focuses on characterizing the atmospheres of transiting exoplanets as part of ACCESS: the Arizona - CfA - Católica Exoplanet Spectroscopy Survey.

He participates in the HATSouth survey, a global network of automated wide - field telescopes dedicated to discovering transiting exoplanets, and is the PUC principal investigator of ACCESS, the Arizona - CfA - Católica Exoplanet Spectroscopy Survey, which will provide the first homogeneous database of ground - based exoplanetary transmission spectra in the optical using the IMACS instrument in Chile.

As part of the ACCESS team (Arizona - CfA - Catolica Exoplanet Spectroscopy Survey), I study the atmospheres of transiting exoplanets through transmission spectroscopy.

She is an expert on exoplanet atmospheres studies and the CfA Principal Investigator of ACCESS, the Arizona - CfA - Catolica Exoplanet Spectroscopy Survey.

Swain is principal investigator of the Fast Infrared Exoplanet Spectroscopy Survey Explorer (Finesse), a proposed 30 - inch space telescope that would probe more than 200 planets around nearby stars to learn about their atmospheres and how they formed.

The third contender, the Fast Infrared Exoplanet Spectroscopy Survey Explorer (FINESSE), aims to probe the origins and makeup of the atmospheres around exoplanets.

Not exact matches

These surveys combined spectroscopy with visible and near - infrared imaging by Hubble's Wide Field Camera 3 and Advanced Camera for Ssurveys combined spectroscopy with visible and near - infrared imaging by Hubble's Wide Field Camera 3 and Advanced Camera for SurveysSurveys.

Its specialty will be time - domain spectroscopy — useful for observing accretion by galactic black holes, surveys of distant supernovae and even searches for extrasolar planets.

The Tarantula Survey is an ambitious ESO Large Programme that has obtained multi-epoch spectroscopy of over 1,000 massive stars in the 30 Doradus region of the Large Magellanic Cloud.

My research interest is the detection of prebiotic molecules in space via rotational spectroscopy, and my prior research includes a spectral survey of Orion - Kl, as well as searching for molecules in Sagittarius B2 (N).

Multi-epoch optical spectroscopy of R139 was obtained as part of the VLT - FLAMES Tarantula Survey, revealing a double - lined system.

We combined photometry, medium / high - resolution spectroscopy, adaptive optics / speckle imaging and archival survey images to rule out any false positive detection scenarios, validate the planet, and further characterize the system.

Near - IR spectroscopy of... ▽ More We have searched ~ 8200 sq. degs for high proper motion (~ 0.5 - 2.7» / year) T dwarfs by combining first - epoch data from the Pan-STARRS1 (PS1) 3 - Pi Survey, the 2MASS All - Sky Point Source Catalog, and the WISE Preliminary Data Release.

Here we combine K2 photometry with spectroscopy, adaptive optics imaging, and archival survey images to analyze two small planets orbiting the nearby, field age, M dwarfs K2 - 26 (EPIC 202083828) and K2 - 9.

Ecliptic fields will be observed for approximately 75 - days enabling a unique exoplanet survey which fills the gaps in duration and sensitivity between the Kepler and TESS missions, and offers pre-launch exoplanet target identification for JWST transit spectroscopy.

The initial transit signal was identified in KELT - North survey data, and the planetary nature of the occulter was established using a combination of follow - up photometry, high - resolution imaging, high - resolution spectroscopy, and precise radial velocity measurements.

We identified the initial transit signal in the KELT - North survey data and established the planetary nature of the companion through precise follow - up photometry, high - resolution spectroscopy, precise radial velocity measurements, and high - resolution adaptive optics imaging.

Shectman led the Las Campanas Redshift Survey (LCRS), the first galaxy redshift survey to use fiber - optic spectroscopy to measure the distances to hundreds of galaxies in each expSurvey (LCRS), the first galaxy redshift survey to use fiber - optic spectroscopy to measure the distances to hundreds of galaxies in each expsurvey to use fiber - optic spectroscopy to measure the distances to hundreds of galaxies in each exposure.

From low - resolution optical and near - IR spectroscopy we classified the primary and the companion as an M7.5 +... ▽ More In a search for common proper motion companions using the VISTA Hemisphere Survey and 2MASS catalogs we have identified a very red (J - Ks = 2.47 mag) late - L dwarf companion of a previously unrecognized M dwarf VHS J125601.92 - 125723.9, located at a projected angular separation of 8.06» + / -0.03».

Data obtained for this project includes a deep Chandra survey of the Galactic Bulge; deep, high resolution IR imaging from VLT / ISAAC, CTIO / ISPI, and the UKIDSS Galactic Plane Survey (GPS); and IR spectroscopy from VLT / ISAAC and IRTF /survey of the Galactic Bulge; deep, high resolution IR imaging from VLT / ISAAC, CTIO / ISPI, and the UKIDSS Galactic Plane Survey (GPS); and IR spectroscopy from VLT / ISAAC and IRTF /Survey (GPS); and IR spectroscopy from VLT / ISAAC and IRTF / SpeX.

Initial data came from the TRENDS (TaRgetting bENchmark - objects with Doppler Spectroscopy) high - contrast imaging survey that uses adaptive optics and related technologies to target older, faint objects orbiting nearby stars, and precise measurements were made at the W. M. Keck Observatory on the summit of Mauna Kea, Hawaii.

The scope and flexibility of SDSS - V will be unique among extant and future spectroscopic surveys: it is all - sky, with matched survey infrastructures in both hemispheres; it provides near - IR and optical multi-object fiber spectroscopy that is rapidly reconfigurable to serve high target densities, targets of opportunity, and time - domain monitoring; and it provides optical, ultra-wide-field integral field spectroscopy.

The instruments also have the capability for imaging and spectroscopy in the wavelength range 2 - 180 micron in the pointed observation mode, occasionally inserted into the continuous survey operation.

The combination of radial velocity and imaging follow - up was represented by the California Planet Survey Targeting Benchmark - objects with Doppler Spectroscopy (CPS / TRENDS), a consortium of US - based universities and researchers.