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The HATNet Exoplanet SurveyThe HATNet Exoplanet Survey
http://www.hatnet.org/
The HATNet Exoplanet Survey
http://www.hatnet.org/
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HATNet Project
Waqas Bhatti
4 I●●●ane
Pri●●●ton , NJ, 08544
US
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HATNet Project
Waqas Bhatti
4 I●●●ane
Pri●●●ton , NJ, 08544
US
View this contact
HATNet Project
Waqas Bhatti
4 I●●●ane
Pri●●●ton , NJ, 08544
US
View this contact
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The HATNet Exoplanet Survey | hatnet.org Reviews
https://hatnet.org
The HATNet Exoplanet Survey
hatnet.org
HATNet / Follow-up Data
https://www.hatnet.org/planets/followup-data.html
The HATNet Exoplanet Survey. The HATNet Exoplanet Survey has discovered 58 planets as of June 2016. The table below lists these planets, their orbital periods, masses, and radii, and provides links to follow-up lightcurves and radial velocity data. Each data file is a tar.gz archive, and contains a README file describing its contents. Click on any table column header below to sort by that column. Download all follow-up lightcurve data. Download all follow-up radial velocity data. HAT-P-10 b = WASP-11b.
HATNet / Planet Lightcurves
https://www.hatnet.org/planets/discovery-hatlcs.html
The HATNet Exoplanet Survey. The HATNet Exoplanet Survey has discovered 58 planets as of June 2016. The table below lists these planets, their orbital periods, masses, and radii, and provides links to HATNet lightcurves from which they were discovered. A description. Of the lightcurve file format is provided at the end of the page. Click on any table column header below to sort by that column. Download all HATNet lightcurves. HAT-P-10 b = WASP-11b. Available to read these files (you will need Numpy.
HATNet / Operations
https://www.hatnet.org/operations.html
The HATNet Exoplanet Survey. We detect exoplanets by monitoring large parts of the sky and attempting to determine if the light from a star periodically dims for a short time. This short dip in the light received may be caused by a small planetary-sized object moving in its orbit in front of the star as seen from our vantage point on Earth. This is a so-called exoplanet. Over the past twenty years. HATNet telescopes are located at the Fred Lawrence Whipple Observatory. HATNet telescopes at FLWO operating...
HATNet / Planets
https://www.hatnet.org/planets
The HATNet Exoplanet Survey. The HATNet Exoplanet Survey has discovered 58 planets as of June 2016. The table below lists these planets, along with links to papers describing their discovery, as well as some of their fundamental properties. HATNet discovery lightcurves. For each planet are available. In most cases, data. From follow-up photometric and spectroscopic campaigns are also provided. Click on any table column header to sort by that column. HAT-P-10 b = WASP-11b.
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Expert Opinions | PALE RED DOT
https://palereddot.org/category/expert-opinions
Category Archives: Expert Opinions. Opportunities and Obstacles for Life on Proxima b. August 28, 2016. By Prof. Rory Barnes, University of Washington. The discovery of Proxima b is the biggest exoplanet discovery since the discovery of exoplanets. The planet is not much bigger than Earth and resides in the “habitable zone” of the Sun’s nearest stellar neighbor. This planet may represent humanity’s best chance to search for life among the stars. But is Proxima b habitable? So what to make of Proxima b?
Terrestrial Planets over the Next Decade | PALE RED DOT
https://palereddot.org/terrestrial-planets-over-the-next-decade
Terrestrial Planets over the Next Decade. March 26, 2016. By Don Pollaco, Warwick University, UK. There can be no doubt that NASA’s Kepler mission. Has been a resounding success. In particular, much of what we know about rocky planets has come from this mission. After saying that, ground-based radial velocity surveys had already indicated the existence of super-Earths—a class of planet not found in our solar system (ignoring Planet 9! The commonality of multi-planet systems. Almost as impressive has been...
HAT LC Server
https://hatsurveys.org/lightcurves
Enter coordinates, 2MASS ID, or HAT ID. The HAT Lightcurve Server. Welcome to the HAT Surveys'. Lightcurve and data server. This project is currently in the alpha-test phase. And not all functionality has been implemented yet. You can run a quick search by putting an object's coordinates, its 2MASS ID, or its HAT object ID into the search box at the top of the page. You can also use the full search service. Or browse the available datasets. Finally, we have an API. Available for use in your scripts.
BCS Astro
http://www.bcsastro.com/index.html
Welcome to BCS Astro! We are proud of our selection of top quality astronomy mount equipment and would be happy to answer any questions that you may have. Our selection includes telescope and astrophotography mounts of various sizes and technical specifications, as well as other accompanying equipment. You can get more information about each product and then securely order online. Through the Products page. Quality telescope and astrophotography mount. We are proud of our selection of top quality astrono...
Kepler K2 Light Curves reduced by the HAT team
http://k2.hatsurveys.org/archive/K2.0
Kepler K2 Light Curves reduced by the HAT team. K2 HAT Light Curves. Read the data release notes. Download all full lightcurves for this campaign. Download all best aperture lightcurves for this campaign. Object summary table in CSV format. Description of the light curve file format. Python module to read light curves. No light curves yet. No light curves yet. No light curves yet. No light curves yet. No light curves yet. No light curves yet. No light curves yet. No light curves yet. No light curves yet.
Kepler K2 Light Curves reduced by the HAT team
http://k2.hatsurveys.org/docs/about.html
Kepler K2 Light Curves reduced by the HAT team. K2 HAT Light Curves. The K2 HAT Light Curve project is led by Melinda Soares-Furtado, graduate student in the Department of Astrophysical Sciences at Princeton University. People associated with the project are listed below:. Melinda Soares-Furtado —. Joel D. Hartman. Gáspár Á. Bakos. Chelsea X. Huang. If you're having trouble with this website, the light curve data, or if something around here is broken, please email Waqas Bhatti at.
Kepler K2 Light Curves reduced by the HAT team
http://k2.hatsurveys.org/archive/K2.0/release-notes.html
Kepler K2 Light Curves reduced by the HAT team. K2 HAT Light Curves. This reduction was carried out using image-subtraction photometry and tools developed for the HAT Surveys. The details of the process are available in Huang et al. 2015. For the general K2 data extraction pipeline, and in Soares-Furtado et al. 2017. And image-subtraction photometry (ISM) carried out by our team. We performed time-series ISM on stitched images. We make available light curves for 3960 objects in and near the M 35/NGC 2158...
Kepler K2 Light Curves reduced by the HAT team
http://k2.hatsurveys.org/archive/K2.1
Kepler K2 Light Curves reduced by the HAT team. K2 HAT Light Curves. Download all full lightcurves for this campaign. Download all best aperture lightcurves for this campaign. Object summary table in CSV format. Description of the light curve file format. Python module to read light curves. 2015, The Trustees of Princeton University. HATNet and HATSouth are supported by NASA and NSF. The K2 HAT light curves project. Astrophysical Sciences at Princeton University.
exoplanetarchive.ipac.caltech.edu
Bulk Data Download
http://exoplanetarchive.ipac.caltech.edu/bulk_data_download
Interactive Tables Search and File Upload. Interactive Table Search and File Upload. Transit and Ephemeris Service. Predicted Observables for Exoplanets (POE). Confirmed Planets Plotting Tool. Application Programming Interface (API). User Guides and Help Desk. Subscribe to email updates. Downloading Data in Bulk. The NASA Exoplanet Archive serves a variety of spectra, time series and other exoplanet related data, and has generated a set of wget scripts to enable users to download these data in bulk.
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The HATNet Exoplanet Survey
The HATNet Exoplanet Survey. HATNet telescopes at Fred Lawrence Whipple Observatory, Mount Hopkins, Arizona. Photo credit: Gaspar Bakos. The Hungarian-made Automated Telescope Network ( HATNet. Exoplanet Survey is a geographically distributed network of 7 small telescopes optimized for detecting transiting exoplanets. Since first light in 2003, we have discovered 61 exoplanets. 2018, The Trustees of Princeton University. HATNet is supported by NASA grants NNG04GN74G and NNX13AJ15G.
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