El documento resume la situación del sector eléctrico boliviano, incluyendo datos sobre la oferta y demanda de electricidad, la generación hidroeléctrica y termoeléctrica, los grandes consumidores, la distribución y transmisión. Proporciona estadísticas sobre el crecimiento anual de la potencia instalada, la potencia instalada en el sistema interconectado nacional y sistemas aislados, la generación bruta por fuente, y el consumo de energía por las principales empresas distribuidoras.
Report on methods of primary data.bimal.doc.xBimal Yadav
This document discusses various methods for collecting primary data for research purposes. It describes questionnaires, interviews, focus groups, observation, case studies, diaries, critical incidents, and portfolios as the main methods. For each method, it provides details on what they are, their advantages and disadvantages, and examples of how they are used to gather original data from respondents, observe behaviors, or document experiences.
Sour Lake Elementary's 2006-2009 Star Chart compares the school's technology readiness across five categories: Teaching and Learning, Educator Preparation and Development, Leadership, Administration, and Instructional Support, Infrastructure for Technology, and Goals for the Future. The chart shows downward trends in Teaching and Learning and Educator Preparation that Sour Lake aims to reverse, continued advancement in Infrastructure for Technology, and a goal of progress in Leadership, Administration, and Instructional Support.
The Blue River Valley school district is proposing a 1:1 technology initiative to provide every student from kindergarten through 12th grade with their own computing device. Younger students would receive Kindle Fires or similar tablets, while older students would receive 2GoPC convertible tablets. The goals of the initiative are to prepare students for 21st century work environments, create a more relevant and motivating learning environment, and improve the quality of student work through personalized instruction. The timeline shows a committee forming in fall 2011, a pilot program launching in spring 2013, and full implementation in fall 2013 when all BRV students would receive their own devices.
Este documento propõe estratégias para minimizar a indisciplina em uma escola. Algumas estratégias-chave incluem: 1) preparar os professores para lidar com questões disciplinares e relacionais; 2) estabelecer regras claras no início do ano letivo; 3) manter a motivação dos alunos para evitar comportamentos indesejados.
El documento resume la situación del sector eléctrico boliviano, incluyendo datos sobre la oferta y demanda de electricidad, la generación hidroeléctrica y termoeléctrica, los grandes consumidores, la distribución y transmisión. Proporciona estadísticas sobre el crecimiento anual de la potencia instalada, la potencia instalada en el sistema interconectado nacional y sistemas aislados, la generación bruta por fuente, y el consumo de energía por las principales empresas distribuidoras.
Report on methods of primary data.bimal.doc.xBimal Yadav
This document discusses various methods for collecting primary data for research purposes. It describes questionnaires, interviews, focus groups, observation, case studies, diaries, critical incidents, and portfolios as the main methods. For each method, it provides details on what they are, their advantages and disadvantages, and examples of how they are used to gather original data from respondents, observe behaviors, or document experiences.
Sour Lake Elementary's 2006-2009 Star Chart compares the school's technology readiness across five categories: Teaching and Learning, Educator Preparation and Development, Leadership, Administration, and Instructional Support, Infrastructure for Technology, and Goals for the Future. The chart shows downward trends in Teaching and Learning and Educator Preparation that Sour Lake aims to reverse, continued advancement in Infrastructure for Technology, and a goal of progress in Leadership, Administration, and Instructional Support.
The Blue River Valley school district is proposing a 1:1 technology initiative to provide every student from kindergarten through 12th grade with their own computing device. Younger students would receive Kindle Fires or similar tablets, while older students would receive 2GoPC convertible tablets. The goals of the initiative are to prepare students for 21st century work environments, create a more relevant and motivating learning environment, and improve the quality of student work through personalized instruction. The timeline shows a committee forming in fall 2011, a pilot program launching in spring 2013, and full implementation in fall 2013 when all BRV students would receive their own devices.
Este documento propõe estratégias para minimizar a indisciplina em uma escola. Algumas estratégias-chave incluem: 1) preparar os professores para lidar com questões disciplinares e relacionais; 2) estabelecer regras claras no início do ano letivo; 3) manter a motivação dos alunos para evitar comportamentos indesejados.
El documento describe varios problemas con las colaciones en la universidad, incluyendo precios altos que generan ganancias de más del 200% para los dueños de quioscos, poca variedad de alimentos y opciones sanas, espacios reducidos para comer, y dificultades para calentar la comida o comer con amigos.
La escuela tiene juegos en buen estado, buena vialidad y seguridad. Los niños participan en un periódico mural y la escuela mantiene buena higiene con botes de basura ordenados.
The document discusses position vs time graphs and velocity vs time graphs. It explains that position is graphed on the y-axis and time on the x-axis for position graphs. Velocity can be determined from the slope of the position graph. Velocity graphs show velocity directly on the y-axis rather than as a slope. Both graph types can provide information about an object's speed and whether it is slowing down, speeding up or stopping.
This document proposes a live dashboard to visualize stock market data and sentiment in an engaging way, similar to a sports game. Key elements include focusing on winning and losing streaks, live coverage in a visually attractive format, and splitting times to show the current score. Users could get alerts on stock performance through a Twitter feed or emails/texts. The dashboard would also feature lists of top winners and losers, analyst and investor gut feelings on buying or selling, and allowing users to track if their stocks are going up or down.
This document discusses the volunteer activities of an individual with a background in electronics technology and IT infrastructure. It summarizes his involvement leading Cub Scouts and coordinating science activities for Vacation Bible School for children ages 3 to 12. It also details a STEM workshop he developed for Scouts ages 14 and older focused on Arduino projects, where participants experimented with circuits controlling LEDs, switches, joysticks, speakers, and photo-resistors.
Aplicaciones en la planificación estratégica del System Thinking Juan Martin Garcia
El System Thinking es un conjunto de procedimientos que van desde la forma de identificación correcta de los elementos de una sistema (que podamos apreciar su aumento o disminución) a la forma en la que se exponen las conclusiones (en ocasiones mediante arquetipos sistémicos). Tomando que un problema existe cuando la realidad actual o futura es diferente de la forma que ha de tener según nuestro deseos, existen muchas formas de abordar el problema, en concreto podemos usar el System Thinking a encontrar una forma eficaz de lograr nuestro objetivo.
Este documento proporciona una introducción a la criptografía para principiantes. Explica brevemente los tipos de criptografía simétrica y asimétrica, así como otras herramientas criptográficas como certificados digitales e infraestructura de claves públicas. También resume los problemas de seguridad que la criptografía ayuda a resolver, como privacidad, integridad y autenticación. El objetivo general es explicar conceptos criptográficos básicos de manera sencilla.
Which transient when? - A utility function for transient follow-up schedulingTim Staley
Next-generation astronomical facilities such as the LSST and the SKA will be game-changers, allowing us to observe the entire southern sky and track changing sources in near real-time. Keeping up with their alert-streams represents a significant challenge - how do we make the most of our limited telescope resources to follow up 100000 sources per night?
The biggest problem here is classification - we want to find the really interesting transients and spend our time watching those. However, classification based on the initial survey data can only get you so far - we'll need to use robotic follow-up telescopes for rapid-response observations, to give us more information on the most promising targets. To get the most science done, we need to be smart about scheduling that follow-up.
We're exploring use of active learning algorithms (AKA Bayesian Decision Theory) to solve this problem, building a framework that allows for iterative refinement of a probabilistic classification state. Because there are no algorithms that fit this problem 'out-of-the-box', we've built our own analysis framework using the emcee and PyMultiNest packages to power the underlying Bayesian inference. I'll give an overview of how our proposed system fits into the wider context of an automated astronomy ecosystem, then give a gentle introduction to Bayesian Decision Theory and how it can be applied to this problem.
How to build a TraP: An image-plane transient-discovery toolTim Staley
There are three main points summarized:
1. There are many interesting slow radio transients that could be detected through imaging surveys like accretion flares, orphan gamma-ray bursts, and flare stars.
2. Radio surveys are increasing in sensitivity and field of view by orders of magnitude with instruments like LOFAR, enabling the detection of more rare transient events.
3. TraP is a transient detection pipeline that works by extracting sources from radio images, matching to known sources, identifying new bright sources, analyzing light curves, and making the results accessible through a user-friendly web interface.
From gamma-ray to radio: Multi-wavelength follow-up in the first five minutesTim Staley
This document summarizes recent work on fast radio follow-up of transient sources and multi-wavelength classification. It discusses three key areas: 1) examples of fast radio follow-up of gamma-ray bursts and stellar flares, 2) using radio and optical measurements to classify transients, and 3) the need to automate "transient triage" to efficiently prioritize follow-up observations across different facilities. The presenter argues that distributing information about new transients via VOEvents can help the community automate real-time classification and prioritization of targets.
Tunable algorithms for transient follow-upTim Staley
This document discusses an approach for optimizing follow-up observations of astronomical transients using Bayesian decision theory. The approach uses transient lightcurve models, telescope noise models, and prior information to calculate the information content of potential future observations. Observations are prioritized based on their expected information content to efficiently classify transients. The presenter outlines the necessary components for a software system to implement this approach, including lightcurve generation, data fitting, calculating confusion matrices, and an observation scheduler. Future work involves integrating these components and testing the system in realistic simulations.
A brief introduction to version control systemsTim Staley
This is a lunchtime talk I gave to the Southampton astronomy department. The aim was to make them aware of version control systems and when they might need to use them.
Training your astronomy robots to work as a teamTim Staley
I present a case that the astronomy community is missing a part of the puzzle for the next era of automated big-survey astronomy: we currently have very little published work on target prioritization and optimized observation scheduling. I discuss the sociological issues surrounding the sort of open collaboration needed to make optimal use of globally distributed observatories, and show some preliminary work on generally-applicable classification methods.
An invited talk given to an audience interested in using lucky imaging for microlensing studies. I tried to give an overview of where the challenges lie in getting good science data using lucky imaging techniques.
Lucky imaging - Life in the visible after HSTTim Staley
This document discusses using lucky imaging techniques to improve spatial resolution in astronomy. Standard lucky imaging can select the best frames from thousands taken at high speed to achieve near-diffraction limited resolution on ground-based telescopes. When combined with adaptive optics, lucky imaging can further improve resolution and help expand the sky coverage of AO. Potential applications include exoplanet imaging, resolving close binary stars, and probing binarity in globular cluster cores.
El documento describe varios problemas con las colaciones en la universidad, incluyendo precios altos que generan ganancias de más del 200% para los dueños de quioscos, poca variedad de alimentos y opciones sanas, espacios reducidos para comer, y dificultades para calentar la comida o comer con amigos.
La escuela tiene juegos en buen estado, buena vialidad y seguridad. Los niños participan en un periódico mural y la escuela mantiene buena higiene con botes de basura ordenados.
The document discusses position vs time graphs and velocity vs time graphs. It explains that position is graphed on the y-axis and time on the x-axis for position graphs. Velocity can be determined from the slope of the position graph. Velocity graphs show velocity directly on the y-axis rather than as a slope. Both graph types can provide information about an object's speed and whether it is slowing down, speeding up or stopping.
This document proposes a live dashboard to visualize stock market data and sentiment in an engaging way, similar to a sports game. Key elements include focusing on winning and losing streaks, live coverage in a visually attractive format, and splitting times to show the current score. Users could get alerts on stock performance through a Twitter feed or emails/texts. The dashboard would also feature lists of top winners and losers, analyst and investor gut feelings on buying or selling, and allowing users to track if their stocks are going up or down.
This document discusses the volunteer activities of an individual with a background in electronics technology and IT infrastructure. It summarizes his involvement leading Cub Scouts and coordinating science activities for Vacation Bible School for children ages 3 to 12. It also details a STEM workshop he developed for Scouts ages 14 and older focused on Arduino projects, where participants experimented with circuits controlling LEDs, switches, joysticks, speakers, and photo-resistors.
Aplicaciones en la planificación estratégica del System Thinking Juan Martin Garcia
El System Thinking es un conjunto de procedimientos que van desde la forma de identificación correcta de los elementos de una sistema (que podamos apreciar su aumento o disminución) a la forma en la que se exponen las conclusiones (en ocasiones mediante arquetipos sistémicos). Tomando que un problema existe cuando la realidad actual o futura es diferente de la forma que ha de tener según nuestro deseos, existen muchas formas de abordar el problema, en concreto podemos usar el System Thinking a encontrar una forma eficaz de lograr nuestro objetivo.
Este documento proporciona una introducción a la criptografía para principiantes. Explica brevemente los tipos de criptografía simétrica y asimétrica, así como otras herramientas criptográficas como certificados digitales e infraestructura de claves públicas. También resume los problemas de seguridad que la criptografía ayuda a resolver, como privacidad, integridad y autenticación. El objetivo general es explicar conceptos criptográficos básicos de manera sencilla.
Which transient when? - A utility function for transient follow-up schedulingTim Staley
Next-generation astronomical facilities such as the LSST and the SKA will be game-changers, allowing us to observe the entire southern sky and track changing sources in near real-time. Keeping up with their alert-streams represents a significant challenge - how do we make the most of our limited telescope resources to follow up 100000 sources per night?
The biggest problem here is classification - we want to find the really interesting transients and spend our time watching those. However, classification based on the initial survey data can only get you so far - we'll need to use robotic follow-up telescopes for rapid-response observations, to give us more information on the most promising targets. To get the most science done, we need to be smart about scheduling that follow-up.
We're exploring use of active learning algorithms (AKA Bayesian Decision Theory) to solve this problem, building a framework that allows for iterative refinement of a probabilistic classification state. Because there are no algorithms that fit this problem 'out-of-the-box', we've built our own analysis framework using the emcee and PyMultiNest packages to power the underlying Bayesian inference. I'll give an overview of how our proposed system fits into the wider context of an automated astronomy ecosystem, then give a gentle introduction to Bayesian Decision Theory and how it can be applied to this problem.
How to build a TraP: An image-plane transient-discovery toolTim Staley
There are three main points summarized:
1. There are many interesting slow radio transients that could be detected through imaging surveys like accretion flares, orphan gamma-ray bursts, and flare stars.
2. Radio surveys are increasing in sensitivity and field of view by orders of magnitude with instruments like LOFAR, enabling the detection of more rare transient events.
3. TraP is a transient detection pipeline that works by extracting sources from radio images, matching to known sources, identifying new bright sources, analyzing light curves, and making the results accessible through a user-friendly web interface.
From gamma-ray to radio: Multi-wavelength follow-up in the first five minutesTim Staley
This document summarizes recent work on fast radio follow-up of transient sources and multi-wavelength classification. It discusses three key areas: 1) examples of fast radio follow-up of gamma-ray bursts and stellar flares, 2) using radio and optical measurements to classify transients, and 3) the need to automate "transient triage" to efficiently prioritize follow-up observations across different facilities. The presenter argues that distributing information about new transients via VOEvents can help the community automate real-time classification and prioritization of targets.
Tunable algorithms for transient follow-upTim Staley
This document discusses an approach for optimizing follow-up observations of astronomical transients using Bayesian decision theory. The approach uses transient lightcurve models, telescope noise models, and prior information to calculate the information content of potential future observations. Observations are prioritized based on their expected information content to efficiently classify transients. The presenter outlines the necessary components for a software system to implement this approach, including lightcurve generation, data fitting, calculating confusion matrices, and an observation scheduler. Future work involves integrating these components and testing the system in realistic simulations.
A brief introduction to version control systemsTim Staley
This is a lunchtime talk I gave to the Southampton astronomy department. The aim was to make them aware of version control systems and when they might need to use them.
Training your astronomy robots to work as a teamTim Staley
I present a case that the astronomy community is missing a part of the puzzle for the next era of automated big-survey astronomy: we currently have very little published work on target prioritization and optimized observation scheduling. I discuss the sociological issues surrounding the sort of open collaboration needed to make optimal use of globally distributed observatories, and show some preliminary work on generally-applicable classification methods.
An invited talk given to an audience interested in using lucky imaging for microlensing studies. I tried to give an overview of where the challenges lie in getting good science data using lucky imaging techniques.
Lucky imaging - Life in the visible after HSTTim Staley
This document discusses using lucky imaging techniques to improve spatial resolution in astronomy. Standard lucky imaging can select the best frames from thousands taken at high speed to achieve near-diffraction limited resolution on ground-based telescopes. When combined with adaptive optics, lucky imaging can further improve resolution and help expand the sky coverage of AO. Potential applications include exoplanet imaging, resolving close binary stars, and probing binarity in globular cluster cores.
The technology uses reclaimed CO₂ as the dyeing medium in a closed loop process. When pressurized, CO₂ becomes supercritical (SC-CO₂). In this state CO₂ has a very high solvent power, allowing the dye to dissolve easily.
(June 12, 2024) Webinar: Development of PET theranostics targeting the molecu...Scintica Instrumentation
Targeting Hsp90 and its pathogen Orthologs with Tethered Inhibitors as a Diagnostic and Therapeutic Strategy for cancer and infectious diseases with Dr. Timothy Haystead.
When I was asked to give a companion lecture in support of ‘The Philosophy of Science’ (https://shorturl.at/4pUXz) I decided not to walk through the detail of the many methodologies in order of use. Instead, I chose to employ a long standing, and ongoing, scientific development as an exemplar. And so, I chose the ever evolving story of Thermodynamics as a scientific investigation at its best.
Conducted over a period of >200 years, Thermodynamics R&D, and application, benefitted from the highest levels of professionalism, collaboration, and technical thoroughness. New layers of application, methodology, and practice were made possible by the progressive advance of technology. In turn, this has seen measurement and modelling accuracy continually improved at a micro and macro level.
Perhaps most importantly, Thermodynamics rapidly became a primary tool in the advance of applied science/engineering/technology, spanning micro-tech, to aerospace and cosmology. I can think of no better a story to illustrate the breadth of scientific methodologies and applications at their best.
Sexuality - Issues, Attitude and Behaviour - Applied Social Psychology - Psyc...PsychoTech Services
A proprietary approach developed by bringing together the best of learning theories from Psychology, design principles from the world of visualization, and pedagogical methods from over a decade of training experience, that enables you to: Learn better, faster!
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...Sérgio Sacani
Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters
represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions
among stars.
Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate
the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars.
The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun.
Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically,
the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec.
Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within
and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation
were carried out using the ACIS-Extract software.
Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a
photon flux threshold of approximately 2 × 10−8 photons cm−2
s
−1
. The X-ray sources exhibit a highly concentrated spatial distribution,
with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known
massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.
PPT on Direct Seeded Rice presented at the three-day 'Training and Validation Workshop on Modules of Climate Smart Agriculture (CSA) Technologies in South Asia' workshop on April 22, 2024.
Authoring a personal GPT for your research and practice: How we created the Q...Leonel Morgado
Thematic analysis in qualitative research is a time-consuming and systematic task, typically done using teams. Team members must ground their activities on common understandings of the major concepts underlying the thematic analysis, and define criteria for its development. However, conceptual misunderstandings, equivocations, and lack of adherence to criteria are challenges to the quality and speed of this process. Given the distributed and uncertain nature of this process, we wondered if the tasks in thematic analysis could be supported by readily available artificial intelligence chatbots. Our early efforts point to potential benefits: not just saving time in the coding process but better adherence to criteria and grounding, by increasing triangulation between humans and artificial intelligence. This tutorial will provide a description and demonstration of the process we followed, as two academic researchers, to develop a custom ChatGPT to assist with qualitative coding in the thematic data analysis process of immersive learning accounts in a survey of the academic literature: QUAL-E Immersive Learning Thematic Analysis Helper. In the hands-on time, participants will try out QUAL-E and develop their ideas for their own qualitative coding ChatGPT. Participants that have the paid ChatGPT Plus subscription can create a draft of their assistants. The organizers will provide course materials and slide deck that participants will be able to utilize to continue development of their custom GPT. The paid subscription to ChatGPT Plus is not required to participate in this workshop, just for trying out personal GPTs during it.
ESR spectroscopy in liquid food and beverages.pptxPRIYANKA PATEL
With increasing population, people need to rely on packaged food stuffs. Packaging of food materials requires the preservation of food. There are various methods for the treatment of food to preserve them and irradiation treatment of food is one of them. It is the most common and the most harmless method for the food preservation as it does not alter the necessary micronutrients of food materials. Although irradiated food doesn’t cause any harm to the human health but still the quality assessment of food is required to provide consumers with necessary information about the food. ESR spectroscopy is the most sophisticated way to investigate the quality of the food and the free radicals induced during the processing of the food. ESR spin trapping technique is useful for the detection of highly unstable radicals in the food. The antioxidant capability of liquid food and beverages in mainly performed by spin trapping technique.
The cost of acquiring information by natural selectionCarl Bergstrom
This is a short talk that I gave at the Banff International Research Station workshop on Modeling and Theory in Population Biology. The idea is to try to understand how the burden of natural selection relates to the amount of information that selection puts into the genome.
It's based on the first part of this research paper:
The cost of information acquisition by natural selection
Ryan Seamus McGee, Olivia Kosterlitz, Artem Kaznatcheev, Benjamin Kerr, Carl T. Bergstrom
bioRxiv 2022.07.02.498577; doi: https://doi.org/10.1101/2022.07.02.498577
The debris of the ‘last major merger’ is dynamically youngSérgio Sacani
The Milky Way’s (MW) inner stellar halo contains an [Fe/H]-rich component with highly eccentric orbits, often referred to as the
‘last major merger.’ Hypotheses for the origin of this component include Gaia-Sausage/Enceladus (GSE), where the progenitor
collided with the MW proto-disc 8–11 Gyr ago, and the Virgo Radial Merger (VRM), where the progenitor collided with the
MW disc within the last 3 Gyr. These two scenarios make different predictions about observable structure in local phase space,
because the morphology of debris depends on how long it has had to phase mix. The recently identified phase-space folds in Gaia
DR3 have positive caustic velocities, making them fundamentally different than the phase-mixed chevrons found in simulations
at late times. Roughly 20 per cent of the stars in the prograde local stellar halo are associated with the observed caustics. Based
on a simple phase-mixing model, the observed number of caustics are consistent with a merger that occurred 1–2 Gyr ago.
We also compare the observed phase-space distribution to FIRE-2 Latte simulations of GSE-like mergers, using a quantitative
measurement of phase mixing (2D causticality). The observed local phase-space distribution best matches the simulated data
1–2 Gyr after collision, and certainly not later than 3 Gyr. This is further evidence that the progenitor of the ‘last major merger’
did not collide with the MW proto-disc at early times, as is thought for the GSE, but instead collided with the MW disc within
the last few Gyr, consistent with the body of work surrounding the VRM.
The debris of the ‘last major merger’ is dynamically young
Fast radio follow-up
1. Fast radio followup
Tim Staley
University of Southampton
TKP Meeting, December 2012
WWW: 4pisky.org , timstaley.co.uk
2. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
OUTLINE
5 MINUTE TOUR OF GRBS
SWIFT-AMI UPDATE
WHAT’S NEXT
3. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
OUTLINE
5 MINUTE TOUR OF GRBS
SWIFT-AMI UPDATE
WHAT’S NEXT
4. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
GRB PROGENITORS
L. Rezzolla et al 2011
5. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
GRBS: RELATIVISTIC FIREBALLS
M. Rees and P. Meszaros, 1992; W. Zhang and S.
Woosley, 2004.
6. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
SYNCHROTRON AFTERGLOW
Gou, Fox & Meszaros 2007
7. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
SYNCHROTRON AFTERGLOW
Chandra and Frail, 2012.
8. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
TRANSITION: REVERSE SHOCK
Z. Lucas Uhm , Bing Zhang, 2012
9. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
REVERSE SHOCK
Z. Lucas Uhm , Bing Zhang, 2012
10. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
RS+FS COMBINED
GRB110205A (Cucchiara et. al 2011)
11. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
RS IN THE RADIO (‘FLARES’)
(S. Kulkarni et. al 1999)
12. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
RS IN THE RADIO (‘FLARES’)
GRB051221A (Soderberg 2006)
13. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
MANUAL RADIO FOLLOW UP OF
GRBS
Data from Chanda and Frail, 2012. ∼ 8GHz.
14. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
PRIOR RADIO OBSERVATIONS
(Excluding Dave Green et al. 1995)
15. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
WHY IS THIS INTERESTING?
Reverse shocks and radio flares (or lack thereof)
inform us on:
Magnetization of GRB jets,
Lorentz factor of ejecta,
Nature of ejecta (Baryonic vs Poynting flux
dominated).
16. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
MEANWHILE...
‘Dark’ GRBs (Rol 2005; Zauderer 2012).
Re-injection events (Soderberg 2006;
Cucchiara 2011)
Unknown phenomena (Bannister 2012).
17. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
REBRIGHTENING
GRB110213A (Cucchiara 2011)
18. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
OUTLINE
5 MINUTE TOUR OF GRBS
SWIFT-AMI UPDATE
WHAT’S NEXT
19. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
AMI-LA (UK)
20. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
AMI-LA (UK)
Arcminute Microkelvin Imager —
Large Array
15 GHz central frequency, 4.5 GHz
bandwidth
5.5 arcmin primary beam (FoV)
30 arcsec synthesised beam (PSF FWHM)
≈ 0.1mJy noise level, 1 hr image
21. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
THE SYSTEM
4 Pi Sky
SWIFT
BAT
GCN Comet
pysovo
AMI
Data
reduction
TraP
(Staley et al 2012)
22. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
THE SYSTEM
4 Pi Sky
SWIFT
BAT
GCN Comet
pysovo
AMI
Data
reduction
TraP
BAT:
13-30
sec
GCN:
~2 sec
GCN ->
AMI:
~5 sec Slew:
4 min
(Staley et al 2012)
23. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
FASTER RESPONSE TIMES
24. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
FASTER RESPONSE TIMES
25. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
OUTLINE
5 MINUTE TOUR OF GRBS
SWIFT-AMI UPDATE
WHAT’S NEXT
26. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
NETWORKING
[Transient] astronomy
currently follows the “second
grade soccer system” -
everyone chases the same ball.
27. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
NETWORKING
4 Pi Sky
SWIFT
BAT
GCN Comet
pysovo
AMI
Data
reduction
TraP
LOFAR-
UK
FERMI
Southern
hemisphere
?
???
Comet
28. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
OPTICAL FOLLOWUP: LT AND PT5M
29. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
OPTICAL FOLLOWUP: LT AND PT5M
(LA PALMA)
30. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
QUESTIONS
Classification
Teo, Adam, Gosia.
Prioritization and scheduling
Well framed as an ‘Intelligent Agents’ /
computer science project.
Collaborating with Southampton IA group
(Amr Hussein).
31. 5 MINUTE TOUR OF GRBS SWIFT-AMI UPDATE WHAT’S NEXT
SUMMARY
Swift-AMI ‘proof of concept’ has piqued
the interest from the GRB community.
‘Plumbing’ works fine.
Reduction process continues to evolve.
Follow-up prioritization and scheduling
system now in design phase.