Changes between Version 309 and Version 310 of AstroTechTalk

Timestamp:

27 Oct 2017, 09:51:31 (7 years ago)

Author:

Vianak Naranjo

Comment:

--

AstroTechTalk

@@ -30 +30 @@
 || 13.10.2017 || -- || No talk (MPIA Science Day) ||
 || 20.10.2017 (10hrs, HdA) || || ||
-|| '''27.10.2017[[BR]](10hrs, HdA)''' || '''Nicolas Baroan (NIT)''' || '''Novel Scientific high dynamic range SWIR camera: technology, capabilities and application in astronomy'''[[BR]][[BR]]High Dynamic Range is being widely adopted in different markets, like automotive, Industrial machine vision, defense…[[BR]][[BR]]Scientific cameras, usually driven by low light performances and extended Wavelength spectral response, is now considered also as a potential “consumer” of these emerging extended dynamic range devices.[[BR]][[BR]]Developed with its patented High Dynamic Range Pixel structure and with the LPA expertise in optronics ( i.e. : Laboratoire Pierre Aigrain – Ecole Nationale Supérieure ), NIT and LPA will present the first scientific Short Wave Infrared High dynamic Range camera.[[BR]][[BR]]The deep cooled camera performances and features will be illustrated through an interesting astronomy application case made at the “Pic du Midy” Observatory at the top of the French Pyrenees.[[BR]][[BR]]A comparison with a state of the art cooled !InGaAs camera, in similar conditions, will briefly be described.[[BR]][[BR]]Presentation: English[[BR]]Slides: English[[BR]]Questions: English ||
+|| '''27.10.2017[[BR]](10:30hrs, HdA)''' || '''Nicolas Baroan (NIT)''' || '''Novel Scientific high dynamic range SWIR camera: technology, capabilities and application in astronomy'''[[BR]][[BR]]High Dynamic Range is being widely adopted in different markets, like automotive, Industrial machine vision, defense…[[BR]][[BR]]Scientific cameras, usually driven by low light performances and extended Wavelength spectral response, is now considered also as a potential “consumer” of these emerging extended dynamic range devices.[[BR]][[BR]]Developed with its patented High Dynamic Range Pixel structure and with the LPA expertise in optronics ( i.e. : Laboratoire Pierre Aigrain – Ecole Nationale Supérieure ), NIT and LPA will present the first scientific Short Wave Infrared High dynamic Range camera.[[BR]][[BR]]The deep cooled camera performances and features will be illustrated through an interesting astronomy application case made at the “Pic du Midy” Observatory at the top of the French Pyrenees.[[BR]][[BR]]A comparison with a state of the art cooled !InGaAs camera, in similar conditions, will briefly be described.[[BR]][[BR]]Presentation: English[[BR]]Slides: English[[BR]]Questions: English ||
 || 03.11.2017[[BR]](10hrs, HdA) || || ||
 || '''10.11.2017[[BR]](11hrs, MPIA lecture hall)''' || '''Wolfgang Gaessler''' || '''4MOST - An Update'''[[BR]][[BR]]The 4MOST project upgrades the 4m VISTA  telescope on Paranal to a spectroscopic facility. Two low resolution  spectrographs (R ~ 5000) and one high resolution spectrograph (R ~  20000) are fed with light from 2400 fibers. [[BR]][[BR]]In the first 10  years of operation, 4MOST will serve 11 surveys of the responsible  consortium. In addition, whole community surveys are planned to observe  nearly everything on sky (except for exoplanets): individual stars in  the Milky Way galaxy and in the Magellanic Clouds, AGN, supernovae and  their hosts, quasars, LRGs, ELGs, and galaxy clusters. [[BR]][[BR]]Wolfgang Gaessler will give a project update and will explain interesting technical features in more detail.[[BR]][[BR]]Presentation: German[[BR]][https://svn.mpia.de/trac/gulli/att/raw-attachment/wiki/AlteVortraege2017S2/2017-11-03_4MOSTUpdate.pdf Slides: English][[BR]]Questions: German, English ||