The VST/OmegaCAM Photometric H-Alpha Survey (VPHAS+) is imaging the Southern Milky Way in visible light using the ESO VLT Survey Telescope (VST) in Chile.
http://www.vphasplus.org/
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VPHAS+: The VST/OmegaCam Photometric Hα Survey of the Southern Galactic Plane and Bulge | vphasplus.org Reviews
https://vphasplus.org
The VST/OmegaCAM Photometric H-Alpha Survey (VPHAS+) is imaging the Southern Milky Way in visible light using the ESO VLT Survey Telescope (VST) in Chile.
vphasplus.org
VPHAS+: Gallery
http://www.vphasplus.org/gallery.shtml
NGC 3293 and 3324. VPHAS is able to take advantage of the high-quality active optics of the VLT Survey Telescope (VST), which, along with the good atmospheric conditions at Paranal, allow images to be obtained which routinely benefit from sub-arcsecond seeing. This page offers a few examples of the imaging data. A crowded field towards Baade's Window. The open cluster NGC 6520. The Wolf-Rayet star WR 31a. Details in the Carina Nebula. The images below are constructed from overlapping survey exposures, ma...
VPHAS+: The Collaboration
http://www.vphasplus.org/people.shtml
Centre for Astrophysics Research, STRI. E-mail: j.drew at herts.ac.uk. Alphabetically, by institution ). Armagh Observatory, NI (UK). Steve Phillipps, Rhys Morris. ESTEC, Noordwijk (ESA/The Netherlands). Tim Naylor, Stuart Sale. Harvard-Smithsonian Center for Astrophysics (USA). Imperial College London (UK). Institute of Astronomy, Cambridge (UK). Eduardo Gonzalez-Solares, Mike Irwin, Nic Walton. Instituto de Astrofisica de Canarias (Spain). NASA Ames, California (USA). Nordic Optical Telescope (Spain).
VPHAS+: Science applications
http://www.vphasplus.org/science.shtml
Science using VPHAS data. Thanks to the Hα narrowband filter, VPHAS will reveal emission line objects of the following types:. Wolf-Rayet and other massive evolved emission line stars. Compact planetary nebulae and rapidly evolving post-AGB stars. Be stars of all types - including young Herbig stars. Clustered and field T Tau stars. A range of interacting binary stars: symbiotics, 'supersoft' compact binaries, WD/NS/BH accreting binaries. White dwarfs and hot subdwarfs, horizontal branch stars.
VPHAS+: Data
http://www.vphasplus.org/data.shtml
VPHAS is an ESO Public Survey. Hence all data will be released through ESO. Initial data products include reduced images and unstacked single-band source lists. There will be a succession of releases leading to the final goal of a well-validated point source catalogue of u/g/r/i/Hα photometry at an external (systematic) precision of 0.02 0.03 magnitudes on over 300 million objects. Third VPHAS data release (DR3). Second VPHAS data release (DR2). The VPHAS-DR2 Point Source Catalogue. While the following f...
VPHAS+: The Survey
http://www.vphasplus.org/survey.shtml
The image below shows the VPHAS survey footprint plotted in Galactic coordinates. All 2269 fields are shown in outline. Different colours are used to identify the observations obtained for each field by the end of August 2015. Proposed data acquisition strategy. For VST operational reasons the consortium was asked by ESO to split the data-taking, executing the blue/red filters in darker/brighter time. To meet this request, we submit separated u/g/r and Ha/r/i observing blocks to the queue, including ...
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Data products - latest data releases | Gaia-ESO Survey
https://www.gaia-eso.eu/data-products
Jump to main content. Data products - latest data releases. Data products - latest data releases. Internal CASU data archive: http:/ casu.ast.cam.ac.uk/gaiaeso/. Public data archive: http:/ ges.roe.ac.uk/. The first public release to the ESO and Edinburgh archives is available. Gaia-ESO Data Release 2. Reduced Gaia-ESO data release 2 spectra. We are pleased to let you know that the Gaia-ESO data release 2 is now online. Read more. Http:/ archive.eso.org/wdb/wdb/adp/phase3 spectral/form? Project ERC-2012-...
Data reduction | Gaia-ESO Survey
https://www.gaia-eso.eu/data-reduction/data-management
Jump to main content. An overview of the Gaia-ESO Survey data flow system. An overview of the Gaia-ESO Survey data flow process is presented in the Figure above. The tasks are distributed among 19 Working Groups. Page last updated: 13/03/2013. Gaia-ESO Survey Management Plan. Edinburgh public data archive. Semester protected target list at ESO. ESO Ambient Conditions Database. Gaia-ESO Survey Management Plan. WEBDA open cluster database. Gaia-ESO Survey is an ESO.
Latest news | Gaia-ESO Survey
https://www.gaia-eso.eu/news
Jump to main content. Public Data Release 2. We are pleased to let you know that the Gaia-ESO data release 2 is now online. Read more. Visualisations of Gaia-ESO [Mg/Fe] and age data superimposed on a model Galaxy are available for download. These use DR2 data, and are described in Stinson et al 2012. The visualisations are courtesy of Greg Stinson and Maria Bergemann, MPIA. Read more. Gaia and GES video. May 2014 Gaia-ESO Newsletter available. May 2014 Gaia-ESO Newsletter is available. Read more. Gaia-E...
Gaia-ESO visualisations | Gaia-ESO Survey
https://www.gaia-eso.eu/news/archive/gaia-eso-visualisations
Jump to main content. Download visualisations of Gaia-ESO [Mg/Fe] and age data superimposed on a model Galaxy. These use DR2 data, and are described in Stinson et al 2012. The visualisations are courtesy of Greg Stinson and Maria Bergemann, MPIA. Http:/ www.mpia.de/ stinson/maria/mgfe.mp4. Http:/ www.mpia.de/ stinson/maria/ages.mp4. Feel free to use them (with acknowledgement) widely. Page last updated: 29/05/2015. Edinburgh public data archive. Semester protected target list at ESO.
Latest observations | Gaia-ESO Survey
https://www.gaia-eso.eu/observations
Jump to main content. Total number of spectra observed up to date:. Number of open cluster spectra:. Number of Milky Way spectra:. Number of calibration spectra:. Number of sky background observations:. Nightly summaries in PDF format will be available for observing runs made after April 2012. 22 August, 2013. To 28 August, 2013. 24 July, 2013. To 30 July, 2013. 24 June, 2013. To 30 June, 2013. Giovanni Carraro and Clare Worley. 28 May, 2013. To 3 June, 2013. 22 March, 2013. To 27 March, 2013. Institute ...
The Gaia–ESO Large Public Spectroscopic Survey | Gaia-ESO Survey
https://www.gaia-eso.eu/publications/archive/gaia–eso-large-public-spectroscopic-survey
Jump to main content. The Gaia ESO Large Public Spectroscopic Survey. The Gaia ESO Large Public Spectroscopic Survey. Sofia Randich and Gerry Gilmore on behalf of the Gaia ESO Consortium. Publication / submission date:. Https:/ www.eso.org/sci/publications/messenger/. Published in December 2013 (No. 154) issue of The Messenger, pp.47-49. Download the article. Page last updated: 24/02/2014. Edinburgh public data archive. Semester protected target list at ESO. ESO Ambient Conditions Database.
Red Giants in the Gaia-ESO Survey (slides) | Gaia-ESO Survey
https://www.gaia-eso.eu/publications/archive/red-giants-gaia-eso-survey-slides
Jump to main content. Red Giants in the Gaia-ESO Survey (slides). Red Giants in the Gaia-ESO Survey (slides). Rodolfo Smiljanic and the Gaia-ESO Survey Consortium. Publication / submission date:. Slides of "Red Giants in the Gaia-ESO Survey" talk given by Rodolfo Smiljanic at Dig Sites of Stellar Archaeology: Giant Stars in the Milky Way workshop. Red Giants in the Gaia-ESO Survey slides. Page last updated: 19/11/2013. Edinburgh public data archive. Semester protected target list at ESO.
Gaia and GES video | Gaia-ESO Survey
https://www.gaia-eso.eu/news/archive/gaia-and-ges-video
Jump to main content. Gaia and GES video. Gaia and GES video. GES team at the Instituto de Astrofísica de Andalucía have produced a video popularizing Gaia and GES projects. The video is in Spanish with English subtitles. Page last updated: 18/03/2015. Edinburgh public data archive. Semester protected target list at ESO. ESO Ambient Conditions Database. Gaia-ESO Survey Management Plan. WEBDA open cluster database. 2013 Gaia-ESO Survey, Institute of Astronomy, University of Cambridge.
The Gaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars | Gaia-ESO Survey
https://www.gaia-eso.eu/publications/archive/gaia-eso-survey-analysis-high-resolution-uves-spectra-fgk-type-stars
Jump to main content. The Gaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars. The Gaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars. R Smiljanic et al. Publication / submission date:. Http:/ www.aanda.org/articles/aa/abs/2014/10/aa23937-14/aa23937-14.html. Link opens in new window) . The importance of this milestone for the Survey made the paper one of the 2014 research highlights of the journal. Link opens in new window). Institute of Astronomy,...
GES 2013: Gaia-ESO Survey First Science | Gaia-ESO Survey
https://www.gaia-eso.eu/events/archive/ges-2013-gaia-eso-survey-first-science
Jump to main content. GES 2013: Gaia-ESO Survey First Science. GES 2013: Gaia-ESO Survey First Science. Http:/ ges2013.sciencesconf.org/. The Gaia-ESO Survey (GES) will obtain spectra for 10. The GES science verification projects are grouped into broad categories listed below (see the GES science verification projects. On the internal Gaia-ESO Wiki for details):. Local Field Dwarfs (UVES parallels). Inner Galaxy (b 15deg). Inner Galaxy (b 15deg). Page last updated: 31/03/2013. WEBDA open cluster database.
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VPHAS+: The VST/OmegaCam Photometric Hα Survey of the Southern Galactic Plane and Bulge
The VST Photometric Hα Survey of the Southern Galactic Plane and Bulge (VPHAS ). Read the survey description ». VPHAS is imaging the Southern Milky Way in visible light (u, g, r, i, Hα) at 1 arcsecond resolution down to 20th magnitude. Image: ESO/S. Brunier. News: image gallery updated. View the gallery ». New images which demonstrate the quality of the VPHAS data, including observations towards Baade's Window, have been added to the gallery. Image: Baade's Window (VPHAS /G. Barentsen). VPHAS uses VST/Om...
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VPHAS+: The VST/OmegaCam Photometric Hα Survey of the Southern Galactic Plane and Bulge
The VST Photometric Hα Survey of the Southern Galactic Plane and Bulge (VPHAS ). Read the survey description ». VPHAS is imaging the Southern Milky Way in visible light (u, g, r, i, Hα) at 1 arcsecond resolution down to 20th magnitude. Image: ESO/S. Brunier. News: image gallery updated. View the gallery ». New images which demonstrate the quality of the VPHAS data, including observations towards Baade's Window, have been added to the gallery. Image: Baade's Window (VPHAS /G. Barentsen). VPHAS uses VST/Om...
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Welcome visitor you can Log In. Hình ảnh RBC 2013 Convention tại Seattle. Nổi bật trong ngày. Câu chuyện ông tiên ngày tết. Cứu lụt năm Thìn. Hồn Ma Trong Bệnh viện. Sinh viên dược khoa nấu bánh chưng tại sân trường. Nam Trung Tạp Ngâm. CE Dinner sponsored by VPhA-USA and Biovail. Thư mời 25 năm VPHA USA. Hình ảnh RBC 2013 Convention tại Seattle. Tin Mới Trong Tuần. SINH HOẠT SẮP ĐẾN. CE Dinner sponsored by VPhA-USA and Biovail. Thư mời 25 năm VPHA USA. Văn học nghệ thuật. Câu chuyện ông tiên ngày tết.
