Lead Software Developer at University of Toronto

Lead Software Developer
Job Number: 1800046

To apply: https://utoronto.taleo.net/careersection/10000/jobdetail.ftl?job=1800046&tz=GMT-05%3A00

University of Toronto
Faculty / Division: Faculty of Arts and Science
Department: Dunlap Institute for Astronomy and Astrophysics
Campus: St. George (downtown Toronto)

Description:
Under the direction of the Director, Dunlap Institute and in close collaboration with the Development Manager at the University of Alberta, the incumbent is responsible for acting as the lead software developer for a major scientific nationwide project funded by the Canada Foundation for Innovation (CFI) to convert the enormous raw data streams from next-generation radio telescopes into sophisticated digital databases that astronomers can use to make new discoveries. Key responsibilities include: coordinating and overseeing software development activities between six Canadian universities and other partners; developing uniform codebase through a central repository; and ensuring that all components are interoperable and meet scientific and technical specifications. The incumbent also coordinates, prioritises and oversees the project’s software milestones, feature requests and bug reports; participates in the project’s management committee; and facilitates multi-site collaboration.

Qualifications:
Minimum Qualifications:
Education:
§  Bachelor’s Degree in Computer Science, Engineering or an equivalent combination of education and experience. Master’s Degree preferred.

Experience:
§  Minimum five (5) years of recent and related experience in software development and software project management.
§  Experience in Linux systems administration.
§  Experience in Unix or Apple OSX.
§  Experience with database design and maintenance.
§  Experience in interpreting raw data streams from radio telescopes or similar data.
§  Experience in high performance computing, especially involving massively parallel applications.
§  Experience in scalable computing (e.g. hadoop / mapreduce), containerisation (e,g, docker) and Cloud computing (e.g. AWS, openstack).
§  Strong debugging/bug-tracking/code review/documentation experience.

Skills:
§  Advanced programming skills in C++ .
§  Advanced skills in Python and/or Julia.
§  Excellent project management skills.
§  Advanced skills in git or similar version control systems.

Other:
§  Superior problem solving and analytical ability.
§  Demonstrated ability to work well as a team member and independently.
§  Demonstrated sensitivity to organizational priorities with the ability to multi-task.
§  Demonstrated ability to work in a high-pressure environment.
§  Ability to articulate and explain technical issues to non-technical users in a clear and precise manner.

Travel: None
Notes: Please note that this is a two-year term position with the possibility of renewal.

Employee Group: United Steelworkers (USW)
Appointment Type: Grant – Term
Schedule: Full-time
Pay Scale Group and Hiring Rate: USW Pay Band 16 — $83,966 with an annual step progression to a maximum of $107,378. Pay scale and job class assignment is subject to determination pursuant to the Job Evaluation/Pay Equity Maintenance Protocol.
Job Field: Information Technology
Job Posting: Feb 1, 2018
Job Closing: Feb 11, 2018

Directeur ou directrice – Planétarium Ville de Montréal

Postulation

Salaire: Salaire minimal : 111 766 $ Maximal normal : 139 713 $ Maximum mérite : 167 659 $
Classe FM10

Catégorie d’emploi: Directeur(trice) – cadre de direction Organisation: Service Espace pour la vie
Durée: Emploi permanent
Période d’inscription: Du 3 au 26 janvier 2018 Catégorie d’emploi

Directeur(trice) – cadre de direction

Description

Espace pour la vie réunit sur un même site le Biodôme, l’Insectarium, le Jardin botanique et le Planétarium Rio Tinto Alcan, les quatre musées en sciences de la nature de Montréal. Ensemble, ces institutions prestigieuses forment le plus grand complexe muséal en son genre au Canada; un important pôle de biodiversité actif et ouvert sur le monde, en milieu urbain. Avec plus de deux millions de visiteurs chaque année, dont 600 000 jeunes, Espace pour la vie est aussi l’un des principaux pôles d’attraction de la métropole.

Espace pour la vie tire sa force de la complémentarité de ses quatre institutions, qui partagent une même vision : repenser la relation entre l’humain et la nature. Ensemble, elles initient un mouvement rassembleur, audacieux, créatif et urbain qui dépasse les frontières des institutions; un engagement envers la biodiversité.

Par ses actions de diffusion, de conservation, de recherche et d’éducation, le Planétarium Rio Tinto Alcan contribue à la réalisation de cette mission, plus spécifiquement au niveau de l’astronomie. Pendant plus de 45 ans, le Planétarium de Montréal a partagé sa passion du ciel et des étoiles avec ses visiteurs, petits et grands. Aujourd’hui, le Planétarium Rio Tinto Alcan propose une expérience totalement renouvelée de l’astronomie. Dans son bâtiment au design audacieux, inauguré en 2013, le Planétarium Rio Tinto Alcan intègre les critères les plus élevés du développement durable. Il utilise des technologies de pointe pour faire vivre une expérience inédite de l’Univers à travers deux spectacles complémentaires, l’un poétique et l’autre scientifique. Cette approche novatrice et unique de l’astronomie, conjuguant science, art et émotion fait du Planétarium un véritable précurseur dans son domaine.

Relevant du directeur d’Espace pour la vie, vous gérez les activités d’une équipe composée de 25 personnes, sous la direction du Planétarium Rio Tinto Alcan. Vous collaborez également à la gestion des dossiers transversaux de la direction d’Espace pour la vie.

Défis du poste

À titre de directeur(trice) du Planétarium, vous aurez à gérer et développer la production des programmes scientifiques de haut niveau. De plus, vous contribuerez à réaliser la mission d’Espace pour la vie en collaboration avec les quatre (4) autres directeurs.

Vos principales responsabilités sont les suivantes :

  • Proposer les orientations, objectifs, programmes et budgets nécessaires aux activités du Planétarium Rio Tinto Alcan, notamment les activités relatives au développement et à la diffusion de programmes éducatifs;
  • Participer, en tant que membre du comité de direction, à l’élaboration des orientations, stratégies et objectifs d’Espace pour la vie;
  • Agir comme chargé de projet pour les mandats transversaux du Service qu’il se voit confier;
  • Déterminer, en étroite collaboration avec les unités du Service les objectifs et les actions à prioriser pour mettre en valeur les collections et les contenus scientifiques.
  • Déterminer en étroite collaboration avec les divisions Marketing et Communications,Commercialisation, Service à la clientèle et Services techniques, les actions à prioriser pour réaliser les activités et atteindre les objectifs spécifiques du Planétarium, dans une perspective d’amélioration continue et d’expérience client;
  • Gérer, conjointement avec le directeur de l’Exploitation et le directeur du Biodôme, la qualité et l’intégration des processus-client pour l’ensemble du site (Biodôme et Planétarium);
  • Établir et développer des liens de collaboration, d’échange et de partage d’expertise avec des organismes, institutions ou partenaires de différents milieux (universitaire, muséologique, scientifique, culturel, communautaire, médiatique, environnemental, économique, etc.) dans le respect des principes du développement durable et de l’éthique pour la biosphère;
  • Diriger ou siéger, selon le cas, à divers comités de gestion, à des tables de concertation regroupant des représentants de la Ville ou d’organismes externes, ministères ou universités dans le cadre des mandats qui lui sont confiés.
  • Représenter occasionnellement l’institution auprès des instances publiques, privées et des médias en tant que porte-parole du Planétarium et d’Espace pour la vie;
  • Favoriser et supporter les occasions afin de soumettre la candidature du Planétarium pour l’obtention de subventions, de commandites ou la tenue d’événements spéciaux;
  • Favoriser le rayonnement du Planétarium et d’Espace pour la vie aux niveaux régional, national et international par diverses activités telles que la publication d’articles, la présentation de conférences, la participation à des colloques et à des congrès, etc.ExigencesScolarité

    Posséder un diplôme universitaire de premier cycle (baccalauréat) en astronomie, en administration ou tout autre domaine jugé pertinent.

    Expérience

    Détenir une vaste expérience correspondant aux défis et responsabilités du poste identifiés sur le présent affichage dont un minimum de cinq (5) années en gestion d’équipe pluridisciplinaire et en gestion de projets et avoir à son actif des réalisations significatives en lien avec le poste. L’expérience doit avoir été acquise dans des postes et des milieux de travail d’envergure similaire.

    Aout

    Détenir un diplôme universitaire de deuxième cycle.

    Compétences – Profil des compétences génériques de gestion de la Ville de Montréal

  • Posséder une vision stratégique et un sens politique.
  • Démontrer une très bonne capacité d’influence et de prise de décision.
  • Posséder des habiletés de mobilisation d’équipes diversifiées.
  • Démontrer de grandes habiletés de gestion des opérations.
  • Faire preuve d’une bonne capacité d’adaptation et se distinguer par son approche- client.
  •   Avoir des aptitudes pour la communication interpersonnelle.

Remarques

La Ville de Montréal remercie à l’avance toutes les personnes ayant manifesté leur intérêt. Elle se réserve toutefois le droit de limiter le nombre personnes à rencontrer en entrevue et ne communiquera qu’avec celles dont la candidature est retenue.

Le processus d’évaluation compte deux étapes éliminatoires distinctes. La première étape concerne les exigences spécifiques au poste à combler. La seconde étape concerne les compétences génériques de gestion pour le niveau de gestion du poste à pourvoir.

Lieu de travail : 480, Avenue Pierre-de-Coubertin, Montréal Pour postuler
L’inscription en ligne est obligatoire

Vous pouvez accéder au portail Internet de la Ville de Montréal, section « Carrières » à l’adresse suivante : www.ville.montreal.qc.ca/emploi et cliquer sur le bouton « Consulter les offres d’emploi ».

Notez qu’une foire aux questions (FAQ) y est disponible. Vous pourrez y trouver des réponses aux questions d’ordre technique ou sur les processus de dotation.

Pour toute autre question à laquelle la FAQ n’aurait pas répondu, vous pouvez vous adresser à la boîte courriel Dotation@ville.montreal.qc.ca en spécifiant le numéro de l’affichage dans l’objet de votre courriel.

Accès à l’égalité en emploi

La Ville de Montréal applique un programme d’accès à l’égalité en emploi et invite les femmes, les autochtones, les minorités visibles, les minorités ethniques et les personnes handicapées à soumettre leur candidature.

Veuillez nous faire part de tout handicap qui nécessiterait des arrangements spéciaux adaptés à votre situation advenant que vous soyez invité(e) à un processus d’évaluation. Soyez assuré(e) que nous traiterons cette information en toute confidentialité.

Pour plus de renseignements, veuillez consulter :

https://simenligne.ville.montreal.qc.ca:443/OA_HTML/OA.jsp?OAFunc=IRC_VIS_VAC_DISP LAY&p_svid=149625&p_spid=4938116

2017 U of T Summer Undergraduate Research Program in Astronomy & Astrophysics

The annual Summer Undergraduate Research Program (SURP) in Astronomy & Astrophysics at the University of Toronto is a unique opportunity for undergraduate students in Astronomy, Physics and Engineering to prepare for a career in scientific research.

Over the 16-week program, students will:

• Experience what a career in research is like by independently conducting a project related to on-going astronomical research at U of T
• Collaborate with U of T astronomers
• Enhance their computing skills
• Improve their research writing and communication skills
• Learn about research being conducted at U of T
• Have an opportunity to participate in U of T public outreach activities

Students will be funded by the program and will work with astronomers from the Dunlap Institute, the Department of Astronomy & Astrophysics (DAA), or the Canadian Institute for Theoretical Astrophysics (CITA), depending on the student’s research interest, choice of supervisor, or choice of research project.

It is a unique opportunity to work within a group comprising three units with complementary expertise in observational research, astronomical instrumentation (Dunlap), and theoretical astrophysics (CITA).

Students will receive a $10,000 CAD stipend.

The program runs from 7 May to 24 August, 2018.

The deadline for applications is 26 January 2018.

For full details and to apply, visit:

www.dunlap.utoronto.ca/SURP
www.cita.utoronto.ca/SURP

www.dunlap.utoronto.ca
www.astro.utoronto.ca
www.cita.utoronto.ca

Faculty Vacancy Brandon University Department of Physics and Astronomy

Brandon University is a leader in providing high quality education in arts, sciences, education, music, and health studies. Based in southwestern Manitoba, Brandon University also offers pre-professional and Masters programs, as well as innovative and award-winning outreach programs in a personalized learning environment.

Applications are invited for a one-year term position at the rank of Assistant Professor in the Department of Physics and Astronomy at Brandon University. Applications are solicited from all fields of Physics and
Astronomy.

Brandon University is a predominantly undergraduate institution, and while department members are all active researchers, the focus is on successful and innovative teaching of our students, who thrive in the small-class and personalized learning environment that Brandon University provides. A successful track record of teaching will therefore be an important consideration. The Department offers 3-year, 4-year, and 4-year Honours undergraduate degree programs in Physics.

Qualifications: A minimum of the M.Sc. degree is required for this position, with preference given to those
with an earned Ph.D. or doctoral candidates.

Responsibilities: The assignment of courses will be partly determined based on the abilities of the successful candidate.

Application Deadline: February 16, 2018

Start Date: August 1, 2018, or upon availability of successful candidate.

Salary: Commensurate with qualifications and experience

Applications should be sent via e-mail in a single pdf file of reasonable size, and include letter of application, vitae, statement of teaching philosophy, citizenship or Canadian immigration status, as well as the names and e-mail addresses of three referees to:

Dean of Science, Brandon University, Brandon, MB, R7A 6A9 E-mail: science@brandonu.ca

For more information on this position and Brandon University please see http://www.brandonu.ca or contact the Department Chair, Dr. Todd Fugleberg ( fuglebergt@brandonu.ca ).

We thank all applicants for their interest in applying for this position and advise that only candidates selected for interviews will be contacted. Short listed candidates will be expected to provide copies of credentials at time of interview.

Brandon University is committed to equity, welcomes diversity, and hires on the basis of merit. All qualified individuals who may contribute to the diversification of the University, especially women, persons with disabilities, Indigenous persons, racialized persons, and persons of all sexual orientations and genders are encouraged to apply. Canadian citizens and permanent residents are given priority. Evidence of citizenship must be provided. To ensure this employment opportunity is accessible to all interested individuals, please advise of any accessibility needs by contacting the Human Resources office at (204)727-9782 or hr@brandonu.ca.

Call for nominations for the Chair of the Murchison Widefield Array Executive Board

Applications close on Friday 1 December 3PM AEST

The Murchison Widefield Array (MWA) is now seeking expressions of interest for the position of Chair of the Executive Board.

The Murchison Widefield Array

The MWA is a low-frequency radio telescope operating between 70 and 300 MHz. It is located at the Murchison Radio-astronomy Observatory (MRO) in Western Australia, about 350km northeast of Geraldton, Western Australia. The MWA is a pre-cursor to the Square Kilometre Array (SKA). The instrument is operated by a consortium of 21 institutions from Australia, Canada, China, Japan, New Zealand and the United States led by Curtin University in Australia. The MWA Collaboration currently comprises some 230 individual scientists and engineers and spans a range of scientific and technical research programs in low frequency radio astronomy.

Further details of the project can be found at www.mwatelescope.org

Governance

The MWA is governed by an Executive Board comprised of an independent Chair and 10 Board members drawn from the MWA member countries (4 from Australia, 2 from China, 1 each from Canada, Japan, New Zealand and the United States). The role of the Board is to oversee policy and provide strategic direction for the Collaboration. The Board, and in particular the Chair, have a close working relationship with the MWA Director, Program Manager, Principal Scientist and Principal Engineer.

Role of Chair of the Board

The Board is seeking a Chair to facilitate the operation of the MWA Collaboration for 2018. The appointment is for one year, with the possibility of annual renewal. Ideally the appointment will commence in January 2018, though flexibility in the start date might be required. As per the new MWA Phase II agreement, which is pending ratification, the Chair can either be drawn from the elected representatives of the Board, or as an independent Chair appointed externally from a member country.

The role of the Chair encompasses the following:

. Providing high-level strategic guidance for the project, including leadership on the implementation or revision of collaboration policies.
. Ensuring the smooth functioning of the MWA Collaboration by working with national consortia in MWA member countries on their institutional membership, internal policies and future engagement with the project.
. Negotiating the MWA membership terms for new and renewing MWA members as the project continues to expand.
. Arranging and chairing meetings of the Board. These include two full-day face-to-face meetings in June and December, as well as 1-hour teleconferences on a monthly basis. The Chair is required to attend the face-to-face meetings in person. The locations of these meetings will be in MWA member countries.
. The role is approximately a 0.1 FTE time commitment, though the workload is variable and requires some flexibility. The position is not remunerated and has historically been filled largely by individuals whose current employer consider such positions as part of their workload.

Eligibility Requirements:
. Familiarity with international astronomical collaborations is essential.
. The Chair must possess the ability to work with a culturally diverse collaboration of geographically distributed individuals.
. The Chair must reside in one of the MWA member countries: Australia, Canada, China, Japan, New Zealand or the United States.
. The Chair must not be an employee of Curtin University, but there are no other restrictions on employment status.
. The MWA is a culturally diverse collaboration and the Board strongly encourages applications from minorities and women.

Nominations Process

Expressions of Interest and a brief CV outlining relevant experience (no more than 3 pages) should be sent to the current Chair, Melanie Johnston-Hollitt (Melanie@PeripetySci.com), by 3PM AEST December 1, 2017. Late applications will not be accepted.

Questions regarding any aspect of the role may also be directed to the current Board Chair.

Postdoc position in Time Domain Astrophysics at Purdue University

The Department of Physics and Astronomy at Purdue University invites applications for a postdoctoral position to collaborate with Prof. Dan Milisavljevic on research topics connected with Time Domain Astrophysics.

The successful applicant will lead and be engaged in multiple active projects investigating the explosion mechanisms, progenitor stars, compact object remnants, and environmental impacts of core-collapse supernovae. Desirable skills include: familiarity with general techniques of UV/optical/IR imaging and spectroscopy; experience analyzing data from an array of space- and ground-based observatories (including HST, Chandra, VLA, Gemini, Magellan); expertise in data science or data visualization; and/or a background in theoretical simulations.

Purdue University has a strong astrophysics group and presently maintains partnerships with several major facilities including the Large Synoptic Survey Telescope, the WIYN 3.5m telescope, VERITAS, and XENON1T. Purdue University is also a world leader in high performance scientific computing and data storage facilities.

The position is for two years, renewable for a third year upon mutual agreement. The negotiable starting date is September 1, 2018. Candidates must have a Ph.D. in astronomy, physics, or equivalent, by the date of appointment. Salary is highly competitive, and candidates will be eligible for health benefits including major medical, vision, and life insurance. Purdue University’s benefit package is summarized at: www.purdue.edu/hr/Benefits/. The Faculty and Staff Handbook, which is updated annually, is also available online at http://www.purdue.edu/faculty_staff_handbook/.​

All materials and inquiries should be sent by email to dmilisav@purdue.edu. The application package must be submitted as a PDF and include a cover letter, CV, list of publications, and a statement explaining research interests and qualifications. Three letters of support should also accompany each application and be submitted directly by references with the applicant’s full name in the header.

Review of applications will begin immediately after the deadline and will continue until the position is filled. For full consideration, all application materials should be received no later than December 15, 2017.

Purdue University provides ample support and resources for career development, and is an EEO/AA employer fully committed to achieving a diverse workforce. All individuals, including minorities, women, individuals with disabilities, and veterans are encouraged to apply.​

URL of posting:

http://www.physics.purdue.edu/about/positions/postdoc_time_domain_astrophysics.html

TolTEC postdoc position at INAOE

INSTITUTO NACIONAL DE ASTROFÍSICA, ÓPTICA Y ELECTRÓNICA DEPARTMENT OF ASTROPHYSICS
Postdoctoral Research Assistant
(1 appointment, fixed term)
MXN$ ~280000 per annum (USD ~15000), tax free
The Department of Astrophysics at Instituto Nacional de Astrofísica, Óptica y Electrónica (INAOE, www.inaoep.mx) invites applications for a postdoctoral research assistant position in the area of millimeter astronomy to work on the CONACyT project led by Dr. Itziar Aretxaga entitled “Deep panoramic surveys at 1.1/1.4/2.1mm with the new polarimetric camera TolTEC”.

INAOE is the leading Mexican partner in the operation of the Large Millimeter Telescope (LMT, www.lmtgtm.org), now in scientific operation. TolTEC (http://toltec.astro.umass.edu/), the new imaging camera of the LMT is currently under development and is expected to be deployed to the telescope at the end of 2018.
A large fraction of the research undertaken by the assistant is expected to be based on data acquired with this facility. The candidate is expected to contribute in the planning of the public surveys approved and to contribute to the development of the analysis pipeline, as part of an international team of researchers from INAOE and other Mexican institutions, the universities of Massachusetts-Amherst, Michigan, Northwestern, Arizona State, Wisconsin and Cardiff and NIST. The public surveys of the LMT will include a set of embedded areas of the galactic and extragalactic sky to unprecedented depths and angular resolution (http://toltec.astro.umass.edu/science.php).
The appointment is for 1 year commencing from January 2018, renewable to 1 extra year contingent on performance, and is based at INAOE, Tonantzintla, Pue., Mexico.
The successful candidate should have a PhD awarded within the previous 5 years in a relevant area of astronomy or astrophysics, and should have a demonstrated capacity for independent work. Desirable skills include proficiency in development of scientific coding preferably in C++ and python and experience with Data Mining and statistics, scientific interest in star formation, galaxy evolution or large scale structure of the Universe.
Applications must be written in English, and be emailed as PDF files to itziar@inaoep.mx
before December 1st, and include:
- Cover letter addressed to Dr. Itziar Aretxaga
- Curriculum vitae, including current address, nationality, age, and date of PhD
- Description (max. 10 pages) of research interests
- Complete publication list, with a maximum of 5 papers particularly relevant to the application highlighted
- Full contact details of 3 professional references, and arrange for letters to be sent to the same address before the deadline.

Postdoc Positions in Galaxy Formation and Evolution with JWST

We invite applications for two postdoctoral positions to work with the 200-hour James Webb Space Telescope Guaranteed Time Observer extragalactic program of the JWST NIRISS Instrument Science Team. This campaign targets lensing clusters with multiple JWST instruments to study a range of topics in galaxy evolution. We expect that one position will be located at Saint Mary’s University in Halifax, Canada, and the other at Herzberg Astronomy and Astrophysics, National Research Council, in Victoria, Canada.

The JWST Near-IR Imager and Slitless Spectrograph (NIRISS) provides R~150 slitless grism spectroscopy over 1 to 2.5 microns for every object in a 2.2×2.2 sq arcmin field of view. Soon after JWST launch in early 2019 our NIRISS team will devote 200 hours of guaranteed observing time to the CANUCS program, whose primary component is NIRISS spatially-resolved spectroscopy of thousands of galaxies in fields lensed by massive intermediate-redshift galaxy clusters. This will produce maps of key physical quantities such as stellar populations, ionized gas, metallicity, dust, etc. This slitless spectroscopy program will be supported by extensive imaging and multi-slit spectroscopy with JWST’s NIRCam and NIRSpec instruments, and by existing multi-wavelength datasets. Key science possible with these data will range from studies of galaxies in the Epoch of Reionization, to those at the peak of cosmic star formation at z~1-3, to galaxy populations in massive z~0.5 clusters. For a brie
f description of the CANUCS GTO program, see: http://bit.ly/2yYA9PX

The postdoctoral fellows will first contribute to the development of a comprehensive data simulation and reduction pipeline and will be subsequently involved in the scientific analysis of this exceptional dataset. There will be significant scope for defining and leading scientific investigations within this program. The fellows will also have time for independent research and will be able to apply for Canadian time on ALMA, CFHT, Gemini, Astrosat, JCMT, and JWST.

The appointments are expected to start in or around September 2018 and are expected to be for three years, subject to satisfactory performance. Experience with the analysis of optical/IR extragalactic data is essential, while experience with IR spectroscopy and/or data pipeline development will be considered an asset. Applicants should submit a CV, a statement of research interests and accomplishments, and arrange for three letters of reference to be sent separately to the email address below. The application material should ideally include a description of the scientific investigation(s) that the applicant would be interested in performing using the JWST GTO dataset.

The review of applications will begin on 15 December 2017. All materials should be sent electronically to JWST-GTO@ap.smu.ca and addressed to Drs. Marcin Sawicki and Chris Willott. Any inquiries about these positions may also be sent to the same address.

Research Associate (Limited Term) – Radio Polarimetry in University of Toronto

Job Number: 1701829

Description: The Dunlap Institute for Astronomy and Astrophysics at the University of Toronto invites applications for a Research Associate in Radio Polarimetry (Limited Term). The appointment is for three years, with the possibility of renewal, subject to funding. The anticipated start date is September 1, 2018.

The responsibilities will be as follows:

• 75%: the production of science-ready data products from new radio polarization surveys using the Very Large Array Sky Survey (VLASS), the Canadian Hydrogen Intensity Mapping Experiment (CHIME) and the Australian Square Kilometre Array Pathfinder (ASKAP), supervised by Prof Gaensler and in collaboration with the rest of the VLASS, CHIME and ASKAP teams.
• 25%: self-directed research in Galactic or extragalactic radio astronomy, in consultation with Prof Gaensler.

In all these activities, there is the expectation that the appointee will supervise the work of undergraduate and graduate students.

The Dunlap Institute pursues groundbreaking astronomical research across the electromagnetic spectrum, through innovative approaches to instrumentation, data-driven science and observations, alongside a substantive commitment to outreach and training. The Dunlap Institute is co-located with and has strong ties to the University’s Department of Astronomy and Astrophysics (DAA) and to the Canadian Institute for Theoretical Astrophysics (CITA). These three units together host over 130 staff and students in astronomy, who conduct a diverse research program across instrumentation, observations, computation and theory.

The Dunlap Institute is located on a beautiful 19th century campus in the heart of one of the world’s great cities. Rated as having one of the highest standards of living in the world, Toronto offers a huge range of indoor and outdoor pursuits, outstanding food and music, and a vibrant and diverse cultural community.

Qualifications: Education

PhD or equivalent certification in astrophysics, astronomy or physics

Required Experience

• Experience in radio polarization processing
• Advanced skills in radio interferometry, radio polarimetry, radio astronomy pipelines, and survey science
• A record of lead-author publications on Galactic or extragalactic radio astronomy in high-impact scientific journals
• Demonstrated excellence in scientific writing and scientific communication
• Demonstrated ability to work with students
• Demonstrated ability to work effectively with a team

Preferred Experience

• At least one year of relevant postdoctoral experience
• Some understanding of radio astronomical instrumentation and polarization calibration.

Travel: Extended

Notes: Applicants should apply online at the link below and include a covering letter, curriculum vitae, list of publications, and the e-mail addresses of three referees by December 1, 2017. Questions regarding this position should be directed to Prof. Bryan Gaensler at bgaensler@dunlap.utoronto.ca.

The University of Toronto is strongly committed to diversity within its community and especially welcomes applications from racialized persons/persons of colour, women, Indigenous/Aboriginal People of North America, persons with disabilities, LGBTQ persons, and others who may contribute to the further diversification of ideas.

All qualified individuals are encouraged to apply; however, Canadians and permanent residents will be given priority.

Employee Group: Research Associate, Limited Term
Appointment Type: Grant – Term
Schedule: Full-time
Pay Scale Group and Hiring Rate: R01 — Research Associates (Limited Term): $42,264 – $79,245
Job Field: Research Associate (Limited Term)
Job Closing: Dec 1, 2017

To apply: https://utoronto.taleo.net/careersection/10000/jobdetail.ftl?job=1701829

Two Postdocs in Extragalactic Astrophysics and Data Science at U. Manitoba

Deadline: Dec 31, 2017
Contact: Prof. Christopher O’Dea, University of Manitoba, odeac@umanitoba.ca

The Faculty of Science at the University of Manitoba has two (2) open post-doctoral positions in extragalactic multi-wavelength astrophysics with emphasis on active galactic nuclei and clusters of galaxies, and requiring skills and experience in either data science and/or data visualization. The candidates will be part of a multidisciplinary team of researchers from the University of Manitoba analyzing the data from the Very Large Array Sky Survey (VLASS) and collaborating with experts at the Universities of Toronto and Alberta, covering the domains of astrophysics, data science and scientific visualization. The positions will be 50% astrophysics research and 50% computer science.

The astrophysics research will consist of reduction and analysis of multi-wavelength (e.g., Chandra X-ray, Gemini and HST optical/infrared, ALMA and VLA radio) observations of Active Galactic Nuclei (AGN) and Clusters of Galaxies with emphasis on the interaction of the AGN with its environment. This will be in collaboration with Profs. Stefi Baum and Chris O’Dea and will involve working with several undergraduate and graduate students. Successful candidates will be expected to publish research results in the refereed journal literature.
The computer science component of the position is a joint project between research groups in Computer Science (Profs. Pourang Irani and Neil Bruce) and Astronomy (Profs. Chris O’Dea, Stefi Baum, Samar Safi-Harb, Jayanne English, and Dr. Gilles Ferrand). The science data products that will emerge from the Square Kilometre Array (SKA) will not be in a final state optimized for data analysis, and the data volumes will be so large that direct delivery to users will not be feasible. The SKA project therefore envisages an international collaborative alliance of inter-operating centres. A Canadian SKA Regional Centre would need to provide services
such as archiving, processing, user support and pipeline development. We are part of a large collaboration of Canadian Universities supported by a Canada Foundation for Innovation (CFI) grant to develop a pilot virtual regional centre for radio astronomy, using data from VLASS, the Canadian Hydrogen Intensity Mapping Experiment (CHIME), and the Australian Square Kilometre Array Pathfinder (ASKAP).
Candidates must have a PhD degree or equivalent in astrophysics with skills in computational and/or data sciences and software development; or, demonstrate the ability to acquire skills in these areas. Programming competence and fluency in written and spoken English are required. Experience in radio astronomy and/or multi-wavelength data analysis is highly desired.

Analysis tasks may include creation of a catalog of VLASS continuum data products, development of algorithms for multi-band data matching and source classification, and development of perception-based visualization schemes for large, multi-waveband data and products of data mining tools. The candidates will merge expertise from the fields of astrophysics with that of visual analytics, to combine human interaction via visual representations with machine learning, including dimensionality reduction and clustering. The candidate may also explore promising emerging technologies such as virtual and augmented reality.
We offer:
* Full-time employment at University of Manitoba with a negotiable starting date but ideally April 1, 2018 or soon after for a period of 3 years.
* A competitive salary $40,000 to $60,000 CAD per year (with benefits) depending on qualifications and seniority.
* A budget allowing the postdoctoral fellow to hire and supervise co-op students, and travel to related scientific conferences.
* We invite applications from those who can support and enhance our diversity, including women, Indigenous peoples, other visible minorities, and those committed to a diverse environment. Application materials, including letters of reference, will be handled in accordance with the “Freedom of Information and Protection of Privacy Act”. Please note that curricula vitae may be provided to participating members of the search process.
*Applications will be accepted until Dec 31, 2017