Dunlap Institute 2017 Summer School

Dunlap Institute 2017 Summer School  

INTRODUCTION TO ASTRONOMICAL INSTRUMENTATION 

University of Toronto

Toronto, Ontario, Canada

23 – 28 July 2017

The annual Dunlap Institute Summer School includes both lecture and laboratory activities and is intended for students who have finished at least the 3rd year of an undergraduate program or are in the early years of a graduate program, and have a background in astronomy, physics, or engineering.

Students will:

• Learn basic principles of radio, infrared, optical and x-ray instrumentation
• Learn how detectors and spectrographs work
• Learn in lecture and hands-on laboratory sessions 
• Work with students from around the world
• Learn about a career in instrumentation
• Learn from international leaders in the field of astronomical instrumentation
• Attend a professional development/mentoring session 

Instructors include leading instrumentation and observational astronomers from the Dunlap Institute, U of T’s Department of Astronomy & Astrophysics, and from Canadian, U.S. and international institutions. Visit our website for a list of confirmed instructors as it is updated.

Registration fee: $500.00

Travel subsidies and registration fee waivers available.
Applications and travel subsidy deadline: 31 March 2017

For details and to apply: dunlap.utoronto.ca/summer-school

Dunlap Institute 2017 Summer School

Dunlap Institute 2017 Summer School

INTRODUCTION TO ASTRONOMICAL INSTRUMENTATION

University of Toronto

Toronto, Ontario, Canada

23 – 28 July 2017

The annual Dunlap Institute Summer School includes both lecture and laboratory activities and is intended for students who have finished at least the 3rd year of an undergraduate program or are in the early years of a graduate program, and have a background in astronomy, physics, or engineering.

Students will:

• Learn basic principles of radio, infrared, optical and x-ray instrumentation
• Learn how detectors and spectrographs work
• Learn in lecture and hands-on laboratory sessions
• Work with students from around the world
• Learn about a career in instrumentation
• Learn from international leaders in the field of astronomical instrumentation
• Attend a professional development/mentoring session

Instructors include leading instrumentation and observational astronomers from the Dunlap Institute, U of T’s Department of Astronomy & Astrophysics, and from Canadian, U.S. and international institutions. Visit our website for a list of confirmed instructors as it is updated.

Registration fee: $500.00

Travel subsidies and registration fee waivers available.
Applications and travel subsidy deadline: 31 March 2017

For details and to apply: dunlap.utoronto.ca/summer-school

ALMA Director

Name: ALMA Director Search Committee
Email address: almasearchcommittee@gmail.com
Affiliation: ALMA

ALMA Director
The Atacama Large Millimeter/submillimeter Array (ALMA) is the world’s preeminent facility for millimeter and submillimeter-wave astronomy with transformational capabilities to study the origin of galaxies, stars and planets. ALMA consists of 66 antennas located on the Chajnantor plateau, 5000 meters altitude in northern Chile, and equipped with receivers covering atmospheric windows between 30 and 950 GHz. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile.

ESO, NSF and NINS have each designated an Executive (ESO, AUI/NRAO and NAOJ, respectively), as their legal representatives, to carry out and manage tasks and responsibilities on their behalf. The Joint ALMA Observatory (JAO) in Chile, staffed by the Executives and headed by the ALMA Director, provides the unified management and leadership of ALMA operations and development. The ALMA Board, responsible for governance and oversight and consisting of members representing the parties, Executives and astronomy community, invites applications for the position of ALMA Director. The successful applicant will be expected to take up the post on 1 April 2018, when the current ALMA Director completes his term.

The responsibilities of the ALMA Director include:
• Direct the JAO, leading and managing operations in Chile, and working with and coordinating the Executives’ off-site operations activities
• Prepare and execute an annual budget and long-range plan
• Participate in the promotion of ALMA and its science program
• Report to, and implement the decisions of, the ALMA Board
• Chair the Director’s Council, consisting of representatives of the Executives
• Allocate observing time
• Develop and maintain the vision and overall direction of the ALMA development program

Required experience:
• Extensive management experience at a senior level with a proven record of scientific leadership
• Strong awareness of the major areas of research and future developments in astronomy, emphasizing millimeter and submillimeter wavelengths
• Ability to communicate the scientific vision of the ALMA project to the various funding agencies and to the scientific community
• Sensitivity to the diverse cultures of the partners, with demonstrated excellent negotiation and influencing skills to take account of stakeholder concerns and interests and to promote contact and collaboration with key international partners
• Ability to lead by influence rather than using direct line management authority
• Capable of leading, supervising, coordinating and evaluating staff from diverse cultural backgrounds, while promoting a good team spirit
• Demonstrated flexibility to adapt quickly and resourcefully to shifting priorities and requirements
• Excellent command of the English language is required; knowledge of Spanish is an asset.

The ALMA Director will be employed by either ESO or AUI/NRAO or NAOJ. Each of these organizations offers attractive remuneration packages including a competitive salary, comprehensive benefits, and financial support in relocating families. The duty station is Santiago, Chile, and frequent travel to the ALMA observatory sites, other locations within Chile, and internationally is required. The Director must be able to function at the altitudes of the observatory and support facility sites (5000-m and 3000-m respectively).

A search committee has been constituted by the ALMA Board to evaluate applications for the ALMA Director position, and to recommend a short list of candidates for Board consideration. Interested candidates should submit their curriculum vitae, a motivation letter, and the names of three references who may be contacted about the qualifications of the candidate, to the Chair of the search committee Dr. David Silva at almasearchcommittee@gmail.com. The same email address should be used for any questions related to the position.

ESO, AUI/NRAO, and NAOJ are Equal Opportunity Employers. The post is equally open to suitably qualified female and male applicants.

All materials submitted electronically by 31st March 2017 will receive full consideration.

Research Associate, Adaptive Optics NATIONAL RESEARCH COUNCIL of CANADA (NRC)

Herzberg Astronomy and Astrophysics, Dominion Astrophysical Observatory
5071 West Saanich Road
Victoria, BC V9E 2E7
CANADA
Fax : (613) 990-1286
Telephone: (613) 949-7685
E-mail enquiries: HRQuestionsRH_CG1@nrc-cnrc.gc.ca.

Related URLs: http://www.nrc-cnrc.gc.ca/careers/jobpost.nsf/PostbyCity_E

Further information on NRC Herzberg can be found at http://www.nrc-cnrc.gc.ca/eng/rd/nsi/index.html

Information on NRC Herzberg staff and their research interests is available at http://bit.ly/2aoT8tf

Proposed start date: Summer 2017

A Research Associate is required to work on adaptive optics (AO) research, as part of the National Research Council of Canada’s Herzberg Astronomy and Astrophysics Portfolio (HAA) Adaptive Optics (AO) Team. The HAA-AO Team is currently involved in a number of international projects, which include the Gemini Planet Image (GPI) and the Narrow Field Infra-Red AO System (NFIRAOS), the first light Multi-Conjugate AO (MCAO) system for the Thirty Meter Telescope (TMT). The GPI instrument is in operation but will soon require upgrades. The NFIRAOS project is in its final design phase. In addition, the AO Team is also engaged in an ambitious R&D program focussed on advanced wave-front sensing and wide-field AO.

To support these activities, the HAA-AO Team has developed an extensive laboratory infrastructure (AO Lab), which currently includes two optical benches. The first is an MCAO bench called Herzberg NFIRAOS Optical Simulator (HENOS). HENOS is a scaled down model of NFIRAOS and is used develop and validate the control algorithms, the calibration procedures, and the post-processing software that will be implemented in NFIRAOS. The HENOS bench includes simulated natural and laser guide stars, simulated atmospheric turbulence, two deformable mirrors, one Shack-Hartmann wave-front sensor (WFS), one pyramid WFS and a science camera. The second bench is dedicated to exploring novel wave-front sensing techniques, including pyramid WFSs and non-linear techniques such as phase diversity. Plans are also in the works to deploy a third bench dedicated to high-contrast imaging. The HAA-AO Team engages with graduate students (typically three to four at any given time) from the University of Victoria and elsewhere in Canada, who use the AO Lab to carry out their research projects.

The Research Associate will play a key role in using the AO Lab to carry out original AO research, developing its capabilities and coordinating the work of the graduate students. He/she will also be expected to support on-going projects such as NFIRAOS by providing critical AO-related analysis to help progress designs.

Applicants must have acquired their Ph.D. within the last five years or expect to obtain their degree before taking up the position. Applications should be made by 10 February 2017 via the process described at the URL provided.

NRC is an equal opportunity employer.

Vous pouvez obtenir ces renseignements en français au site web indiqué ci-haut.