CMB-S4 Jobs
Job Postings
 
Open opportunities for CMB-S4-related positions
This page is for advertising positions related to CMB research, e.g., postdocs, faculty, laboratory and technical positions. To post positions, send description and link to C. Reichardt.

 
Postdoctoral Fellow in Theoretical Cosmology/Astrophysics at UT Austin
Deadline: Dec 2, 2019
The Theory Group at The University of Texas at Austin invites applications for a postdoctoral position starting September 2020. The successful candidate will work in collaboration with Professor Kimberly Boddy (who is joining the faculty in the Fall of 2020) on projects relating to theoretical cosmology, astroparticle physics, and/or stochastic gravitational waves. The candidate will also benefit from interactions with other members of the theory group and with members in the Department of Astronomy. The appointment is for a two year term, extendable to a third year contingent on funding and satisfactory performance.Learn more

 
Illinois Survey Science Fellowship
Deadline: Dec 1, 2019
The National Center for Supercomputer Applications (NCSA) and the Departments of Astronomy and Physics at the University of Illinois at Urbana-Champaign invite applications from Ph.D. scientists for the Illinois Survey Science postdoctoral fellowship. This independent fellowship is for 3 years and offers a competitive salary, benefits, and research funds.

This fellowship offers an opportunity to carry out independent research and to be connected with the vibrant research programs in astrophysics at the University of Illinois. Existing research programs at Illinois include the Dark Energy Survey (DES), Large Synoptic Survey Telescope (LSST), SDSS-V, WFIRST, CMB-S4, and the South Pole Telescope (SPT), along with the development of future ground-based, balloon, and satellite projects. NCSA leads data management and processing for the DES project with support from the National Science Foundation, is a partner in the construction and commissioning of LSST and, will be the global central hub for LSST processing, archiving, and serving terabytes of data that will be collected each night of the decade-long survey. Illinois is also an institutional member of the SPT collaboration.Learn more

 
Postdoctoral Research Associate or Senior Research Associate in Cosmology at Cambridge
Deadline: Dec 6, 2019
We invite applications for a postdoctoral position in cosmology at the University of Cambridge. This ERC-funded position will be based at the Department of Applied Mathematics and Theoretical Physics and the Kavli Institute for Cosmology, Cambridge.

Candidates should be qualified to undertake research in the areas of CMB, large-scale structure, cosmological tests of fundamental physics, or other areas of cosmology. While the main selection criterion is research excellence and strong researchers in any area of cosmology will be seriously considered, candidates interested in collaborating with Dr Blake Sherwin to work on CMB gravitational lensing, CMB polarization, large-scale structure or combined probes (potentially within the ACT, POLARBEAR, Simons Observatory, and/or CMB-S4 collaborations) may be of particular interest.Learn more and apply

 
Harvard CMB Group Postdoctoral Fellowships
Review begins Dec 1, 2019
The Harvard CMB group invites applications for two Harvard Postdoctoral Fellow positions to pursue research related to cosmic microwave background measurements with the BICEP Array telescopes, the South Pole Observatory, and CMB Stage 4. The multi-institutional BICEP program produces extremely deep maps of polarization of the CMB at multiple frequencies from the South Pole, measuring gravitational lensing and galactic foregrounds and placing leading constraints on primordial gravitational waves. The BICEP Array project is upgrading the current program with new instrumentation to include over 30,000 detectors and five frequency bands, to be deployed and operated over the next five years. The program will continue to produce maps with groundbreaking sensitivity, while validating technologies and methodologies essential to Stage 3 and Stage 4 CMB science goals. A major focus is analysis of current and upcoming BICEP data, including joint analysis with data from the 10m South Pole Telescope and external datasets, to continue to improve lensing measurements, component separation, and constraints on primordial cosmology, as well as forecasting and design optimization for future efforts of the South Pole Observatory and CMB Stage 4.

Successful candidates will play a variety of leading roles spanning receiver and telescope design, deployment and operation, real time control code, optimization of data reduction and simulation on leading HPC infrastructure at Harvard and NERSC, and development of high-level analyses for survey combination and cosmological interpretation. Applicants should indicate which roles best match their experience and interest. Successful candidates will actively represent this research at conferences and take leading roles in preparation of results for publication. The postdoctoral fellow positions offer a highly competitive salary, an independent research fund and an allowance for relocation expense. The position will be renewed annually based on satisfactory performance, for an expected total length of three years. Joint appointments with collaborating institutions are possible and may be considered on a case by case basis.

 
Tenure-track position at the University of Wisconsin-Madison
For full consideration, apply by Dec 1, 2019
We welcome all theoretical physics applicants who can take advantage of the anticipated unprecedentedly large influx of disparate, complex cosmological data to advance the frontiers of computational/theoretical cosmology.Learn more

 
Postdoc on Ultra-sensitive Far-IR Bolometers at JPL
We are seeking a postdoctoral researcher to lead the demonstration of the world's most sensitive far-IR detectors. We are building transition-edge sensor (TES) arrays with per-pixel noise equivalent power of 10^-19 W/sqrt(Hz) in the JPL micro devices lab (MDL) in preparation for space-borne astrophysics missions including SPICA and the Origins Space Telescope. We are characterizing the prototype TES arrays electrically and optically in our dilution-cooled test facility using a frequency-domain multiplexing readout. The postdoc will work closely with our dynamic group of scientists, technologists and engineers in Pasadena, as well as our collaborators at SRON, Holland. Key people in the JPL detector group include Drs. Matt Kenyon, Pierre Echternach, and Roger O'Brient. For qualified and interested candidates, opportunities also exist for collaboration on ongoing and proposed ground-based and balloon-borne instruments targeting the early Universe. Experiments include SuperSpec (a millimeter-wave spectrometer on a chip slated for the large millimeter telescope targeting individual high-redshift galaxies ), TIME (a mm-wave tomographic intensity mapper targeting ionized carbon fro the Reionzation epoch), and TIM ((formerly STARFIRE), a proposed balloon-borne far-IR imaging spectrometer targeting the history of star formation when the Universe was half its current age). Dr. Matt Bradford will serve as the postdoctoral advisor. The appointee will carry out research in collaboration with the JPL advisor and others, resulting in publications in the open literature.Learn more

 
Postdoctoral position in cosmic microwave background research at MPA
Deadline: Dec 1, 2019
The intended research projects include, but are not limited to, the development and implementation of simulation and analysis tools for two CMB experiments and their early science exploitation:

- LiteBIRD (launch 2028), the CMB satellite mission selected by JAXA
- CCAT-prime (first light 2021), sub-mm telescope to measure polarisation of CMB and dust emission at high frequencies

Within these areas, we seek to fill one postdoctoral position intended for a promising young scientist who completed the PhD within the last six years. The successful candidate will work closely with Prof. Dr. Eiichiro Komatsu, the director of the department of Physical Cosmology at MPA.Learn more

 
CMB Analysis Postdoc at Columbia
Deadline: Dec 15, 2019
Columbia University invites applications for a Postdoctoral Research Scientist position in the Columbia Astrophysics Laboratory to perform research in Physical Cosmology. The successful candidate will join the cosmology group led by Professor Colin Hill in the Physics Department. They will be expected to contribute to ongoing cosmic microwave background (CMB) analysis work in the Atacama Cosmology Telescope and Simons Observatory collaborations. They will have the opportunity to collaborate on research in other areas of cosmology with faculty in CAL and the high-energy theory group.

Questions regarding this position can be addressed to Professor Hill at jch2200@columbia.edu.Learn more

 
Litebird Tenure track faculty position at Okayama U. -- Women only --
Deadline: Oct 31, 2019
The Department of Physics, Division of Mathematics and Physics, Graduate School of Natural Science and Technology, is seeking an applicant for a woman tenure track assistant professor position who has research interests in experiments for Cosmology or Astroparticle Physics, especially for the studies of the cosmic microwave background, or developments of related observation instruments and/or data analyses.

The successful candidate is expected to:
- conduct active, internationally recognized, and externally funded research programs, especially the LiteBIRD
project, with Prof. Hirokazu Ishino
- in charge of undergraduate and graduate level courses in Physics. - advise undergraduate and graduate student on their thesis projects.Learn more

 
Postdoctoral researchers in experimental cosmology at Argonne
The High Energy Physics Division at Argonne National Laboratory invites applications for postdoctoral research positions in the Experimental Cosmology group. Members of our group study the cosmic microwave background as participants in the South Pole Telescope (SPT, https://pole.uchicago.edu/) and CMB-S4 (https://cmb-s4.org/) collaborations. Successful applicants will have opportunities for cosmological analysis of data from the SPT-3G receiver as well as in technology development for CMB-S4. They will have access to multiple test and fabrication facilities at Argonne, the latter involving close collaboration with the Materials Science Division and the Center for Nanoscale Materials. Opportunities also exist to collaborate closely with the Cosmological Physics and Advanced Computing group as well as groups at Fermilab and the University of Chicago.Learn more (Job ID #407093)

 
Schramm Fellowship in Experimental Astrophysics at Fermilab
Deadline: 2019/11/01
The Schramm postdoctoral fellowship is intended to attract early-career researchers of extraordinary promise — from exceptional recent Ph.D. recipients to those with a proven research record from prior postdoctoral experience. The successful applicant will be expected to conduct original research on his/her choice of experimental activities within the Fermilab Cosmic Physics Center (CPC). Current experimental projects in the CPC cover a broad range of topics including the direct detection of dark matter (SuperCDMS, ADMX, SENSEI), investigating dark energy via astrophysical surveys (DES, DESI, LSST) and studying the cosmic microwave background (SPT-3G, CMB-S4). There are also opportunities to participate in the development of new projects targeting cosmic probes of fundamental physics and detector R&D. Members of the CPC interact regularly with scientific, engineering and technical departments throughout the laboratory.Learn more and apply

 
CMB Postdoctoral positions at KIPAC/Stanford/SLAC
In addition to these CMB-focused positions, there are a number of other astrophysics and cosmology postdoctoral fellowships at KIPAC that could be in the CMB.
Applications are invited for up to two postdoctoral positions at the Kavli Institute of Particle Astrophysics and Cosmology (KIPAC) at Stanford University and the SLAC National Accelerator Laboratory with a focus on Cosmic Microwave Background (CMB) surveys. The positions are intended to expand our work with the CMB experiments in which we participate, including BICEP/Keck Array, the South Pole Telescope (SPT), Simons Observatory, and CMB-S4.

We seek highly motivated candidates with a strong track record in data analysis, simulations and/or instrumentation development in observational cosmology or particle astrophysics, and expect them to work in one or more of the following areas: 1. Development and implementation of simulations and analyses of the CMB lensing signal, its cross correlation with optical datasets, and its removal in inflation searches. To this end, our groups actively work with datasets from SPT, DES and BICEP/Keck. 2. Development of dark matter searches using CMB lensing, temperature and polarization data, including searches for ultra-light axions. 3. Development of bolometric and calorimetric detector systems that cross cut CMB, X-ray and Quantum Information Science (QIS) applications with a focus on manipulation of superconducting resonators.Learn more

 
Postdoctoral Position in CMB Theory, Analysis, and/or Instrument Design at Stony Brook University
Deadline Dec. 15, 2019
We invite applications for a postdoctoral position in the field of theoretical/observational cosmology to be based in the Physics and Astronomy Department at Stony Brook University.

The successful applicant will work in collaboration with Prof. Neelima Sehgal and will interact with the rest of the physics and astrophysics community at Stony Brook University. The postdoctoral scholar will be expected to carry out research broadly related to probing fundamental physics with cosmological data. The postdoctoral scholar, if he/she chooses, may in particular work on CMB data analysis for AdvACT or the Simons Observatory, or on CMB theory or instrumentation concept development for CMB-HD.Learn more and apply

 
Cosmic Microwave Background Instrumentation for the LiteBIRD Satellite
Review begins Aug 15, 2019.
The University of California San Diego is searching for a postdoctoral scholar to work on cosmic microwave background (CMB) science, primarily instrumentation development for a future satellite mission. The LiteBIRD CMB satellite mission (http://litebird.jp/eng/) was recently selected by ISAS/JAXA as a large strategic mission to launch in the 2020s. UC San Diego's Center for Astrophysics and Space Sciences (http://cass.ucsd.edu) is contributing cryogenic detector and readout instrumentation to the satellite. Funding for development of this hardware is for two years, with the possibility of extension. The ideal candidate will have a Ph.D. in astronomy or physics and will be familiar with astronomical instrumentation.

The CMB program at UC San Diego (https://cosmology.ucsd.edu/projects.php) is also part of the leadership of the ground-based experiments POLARBEAR and the Simons Observatory. The successful candidate would have the opportunity to work on aspects of these project, and with the other faculty at UC San Diego working on experimental and theoretical issues in CMB science, including Brian Keating, Raphael Flauger, Daniel Green, and George Fuller.

If you are interested in the position, please contact Kam Arnold at arnold@ucsd.edu.Learn more

 
Postdoctoral Fellow in Cosmology at Harvard
Deadline: Dec 1, 2019
We invite applications for a postdoctoral position starting in the Fall of 2020 or before in the field of theoretical/numerical cosmology to be based at the Physics Department at Harvard University. The successful applicant will work in collaboration with Prof. Cora Dvorkin and will interact with the rest of the physics and astrophysics community at Harvard University.

The postdoctoral scholar will be expected to carry out research broadly related to testing fundamental physics with cosmological data. The duration of the postdoctoral appointment is up to three years, with renewable one-year terms.Learn more and apply

 
South Pole MAPO Machinist
The South Pole Machinist operates and maintains the MAPO machine shop, which is located in the Dark Sector Laboratory of the NSF Amundsen-Scott research station at the South Pole in Antarctica. The Machinist works as part of a team to provide on-site machinist services to scientists and engineers from several universities. A continuous stay at the South Pole, lasting approximately eleven months, is required. The position begins 1/15/20 and ends 11/30/20.Learn more and apply.

 
SPT-3G 2020 Winter-Over (two positions)
The 10-meter South Pole Telescope (SPT) Winter-over will be a member of a two-person crew located at the NSF Amundsen-Scott South Pole research station in Antarctica. The crew will be responsible for the hands-on maintenance and operation of the SPT. The crew will participate in the preliminary analysis of the astronomical data and is an integral part of the SPT collaboration. A continuous stay at the South Pole, lasting approximately eleven months, is required. The position begins in December 2019 and ends in November 2020.Learn more and apply.