USAP-DC

{"dp_type": "Project", "free_text": "Neutrino"}

[{"awards": "2219065 Hood, John", "bounds_geometry": "POINT(0 -90)", "dataset_titles": null, "datasets": null, "date_created": "Mon, 19 Dec 2022 00:00:00 GMT", "description": "\\Millimeter-wave (mm-wave) observations of active galactic nucleus (AGN) variability have the potential to shed light on some of the key questions of AGN physics, such as the origin of blazar gamma-ray emission and the possible connection of AGN to the high-energy neutrinos detected by IceCube. While continuous, high-cadence monitoring of AGN is now common at gamma-ray, optical, and radio frequencies, AGN monitoring in the mm band has mostly been restricted to short campaigns on targeted sources. Cosmic Microwave Background (CMB) telescopes are now providing an option for daily monitoring of these objects within limited fields of view. I propose to use the South Pole Telescope (SPT), which was designed to observe the CMB at arcminute and larger angular scales, to monitor AGN, and then to expand this monitoring program to other CMB experiments such as Advanced ACTPol and the upcoming Simons Observatory and CMB-S4 experiments. A pilot project using data from the SPTpol camera on the SPT has enabled the monitoring of tens of mm-bright AGN on timescales from years to days at high signal to noise (S/N \u003e 10 in a 36-hour coadd). A study focused on the blazar PKS 2326-502, which has extensive, day-timescale monitoring data in gamma-ray, optical, and now mm-wave data between 2013 and 2016 shows intriguing evidence of correlated variability between SPTpol (150 GHz), SMARTS (O/IR) and Fermi (gamma-rays) observations. I propose to carry out such multi-wavelength correlation studies on a large statistical sample of mm-wave-bright AGN, enabled by the repurposing of existing and future CMB data. This large sample (covering nearly 70 % of the sky) will also be key to investigating hints of correlations between mm-bright blazar flares and high-energy neutrinos. I further propose to build a public-facing server that will provide the mm lightcurves I construct from CMB data to the wider community.", "east": 0.0, "geometry": "POINT(0 -90)", "instruments": null, "is_usap_dc": true, "keywords": "SOLAR ENERGETIC PARTICLE FLUX; South Pole Station", "locations": "South Pole Station", "north": -90.0, "nsf_funding_programs": "Post Doc/Travel", "paleo_time": null, "persons": "Hood, John", "platforms": null, "repositories": null, "science_programs": null, "south": -90.0, "title": "OPP-PRF: Millimeter-wave Blazar Monitoring With Cosmic Microwave Background Experiments: A New Tool for Probing Blazar Physics", "uid": "p0010399", "west": 0.0}, {"awards": "1852617 Carlstrom, John", "bounds_geometry": "POINT(0 -90)", "dataset_titles": null, "datasets": null, "date_created": "Tue, 11 May 2021 00:00:00 GMT", "description": "The South Pole Telescope Operations and Data Products award supports the maintenance and operation of the 10-meter South Pole Tele- scope (SPT) equipped with the current third-generation instrument, SPT-3G. The proposed operations plan includes five years of survey observations to obtain ultra-deep measurements of a 1500 square degree field with SPT-3G, as well as the production and public archiving of essential data products from the survey. The data products from SPT-3G as well as the previous SPTpol survey will be released to the public at regular and timely intervals over the project period. The operations also support SPT\u2019s critical role in the Event Horizon Telescope (EHT), a global array of telescopes to image the event horizon around the black hole at the center of our Galaxy.\r\n\r\nThe SPT-3G instrument, first deployed in the 2016-17 Austral summer, is a major upgrade in capabilities over previous generations of SPT cameras, with over 16,000 detectors configured for polarization-sensitive observations in three frequency bands. The SPT-3G maps of the temperature, polarization, and lensing potential of the CMB will have an unprecedented combination of depth, resolution and sky coverage (1500 square degrees). This unique data set will enable broad and impactful science, from sensitive constraints on inflationary models to the formation and evolution of galaxies.\r\n\r\nWorking in collaboration with the BICEP/Keck team, we will use the high-resolution SPT-3G data to remove the gravitational lensing signal from BICEP Array maps to enable a deep search for primordial gravitational waves (PGW). The full SPT-3G data set funded by this proposal will allow delensing of BICEP Array data that could improve constraints on PGW by more than a factor of two. \r\nThe SPT-3G temperature and polarization power spectrum measurements will play a central role in probing the nature of current tensions among cosmological parameter estimations from different data sets and determining if their explanation requires physics beyond the standard cosmological model (LCDM). One of the most well-motivated extensions to LCDM in light of these tensions is the existence of new light particles in the early Universe: SPT-3G will improve sensitivity to such particles by at least a factor of two over current CMB experiments.\r\n\r\nSPT-3G data will be used to constrain the properties of dark energy from its effect on the growth of structure through both CMB lensing and the abundance of galaxy clusters. These two observables will also be used to place nearly independent constraints on the sum of the neutrino masses. The unique catalogs of high-redshift galaxy clusters and early star-forming galaxies produced by SPT-3G will be used to understand cluster formation and trace massive galaxy evolution from the epoch of reionization to the peak of star formation.\r\n\r\nPublic data products will include temperature and polarization maps in all three SPT-3G frequency bands, CMB angular power spectra, gravitational lensing maps and power spectra, a catalog of distant massive galaxy clusters, and catalogs of mm-wave-bright galaxies.\r\n\r\nThis project is designed to provide calibrated, uniform, and publicly archived data products that will enable scientific breakthroughs in multiple areas. The public SPT data products will impact the larger community by enabling a broad range of studies that address some of the most compelling questions in cosmology and astrophysics. The sharing of the spirit of scientific inquiry will be extended beyond the research community through a well-established education network at all levels of the education continuum, from early childhood through graduate school. Summer Schools on CMB Instrumentation will be taught by the Co-I\u2019s and senior personnel on this proposal. For our proposed First Discoveries program, we will partner with The University of Chicago\u2019s Neighborhood Schools Program to work with students and teachers in less-advantaged classrooms to foster scientific reasoning through inquiry-based learning.", "east": 0.0, "geometry": "POINT(0 -90)", "instruments": "SOLAR/SPACE OBSERVING INSTRUMENTS \u003e RADIO WAVE DETECTORS \u003e RADIO TELESCOPES", "is_usap_dc": true, "keywords": "USAP-DC; AMD; Adelie Penguin; THERMAL INFRARED; South Pole Station; Amd/Us; OBSERVATORIES", "locations": "South Pole Station", "north": -90.0, "nsf_funding_programs": "Antarctic Science and Technology; Polar Special Initiatives; Antarctic Astrophysics and Geospace Sciences", "paleo_time": null, "persons": "Carlstrom, John; Holzapfel, William; Benson, Bradford", "platforms": "LAND-BASED PLATFORMS \u003e PERMANENT LAND SITES \u003e OBSERVATORIES", "repositories": null, "science_programs": null, "south": -90.0, "title": "South Pole Telescope Operations and Data Products", "uid": "p0010176", "west": 0.0}, {"awards": "2042807 Halzen, Francis; 0937462 Halzen, Francis; 1600823 Halzen, Francis; 0639286 Halzen, Francis", "bounds_geometry": "POINT(-180 -90)", "dataset_titles": "Amanda 7 Year Data Set; IceCube data releases", "datasets": [{"dataset_uid": "200374", "doi": "", "keywords": null, "people": null, "repository": "IceCube", "science_program": null, "title": "IceCube data releases", "url": "https://icecube.wisc.edu/science/data-releases/"}, {"dataset_uid": "601438", "doi": "10.15784/601438", "keywords": "Amanda-ii; Antarctica; Neutrino; Neutrino Candidate Events; Neutrino Telescope; South Pole", "people": "Halzen, Francis; Riedel, Benedikt", "repository": "USAP-DC", "science_program": "IceCube", "title": "Amanda 7 Year Data Set", "url": "https://www.usap-dc.org/view/dataset/601438"}], "date_created": "Wed, 07 Apr 2021 00:00:00 GMT", "description": "This award funds the continued management and operations (M\u0026O) of the IceCube Neutrino Observatory (ICNO) located at the South Pole Station. The core team of researchers and engineers maintain the existing ICNO infrastructure at the South Pole and home institution, guaranteeing an uninterrupted stream of scientifically unique, high-quality data. The M\u0026O activities are built upon eight highly successful years of managing the overall ICNO operations after the start of science operations in 2008. Construction of ICNO was supported by NSF\u0027s Major Research Equipment and Facilities Construction (MREFC) account and was completed on schedule and within budget in 2010. Effective coordination of efforts by the core M\u0026O personnel and efforts by personnel within the IceCube Collaboration has yielded significant increases in the performance of this cubic-kilometer detector over time. The scientific output from the IceCube Collaboration during the past five years has been outstanding. \u003cbr/\u003e\u003cbr/\u003eThe broader impacts of the ICNO/M\u0026O activities are strong, involving postdoctoral, graduate, and (in some cases) undergraduate students in the day-today operation \u0026 calibration of the neutrino detector. The extraordinary physics results recently produced by ICNO and its extraordinary location at South Pole have a high potential to excite the imagination of high school children and the public in general at a national and international level.\u003cbr/\u003e\u003cbr/\u003eThe current ICNO/M\u0026O effort produces better energy and angular resolution information about detected neutrino events, has more efficient data filters and more accurate detector simulations, and enables continuous software development for systems that are needed to acquire and analyze data. This has produced data acquisition and data management systems with high robustness, traceability, and maintainability. The current ICNO/M\u0026O effort includes: (1) resources for both distributed and centrally managed activities, and (2) additional accountability mechanisms for \"in-kind\" and institutional contributions. Both are necessary to ensure that the detector maintains its capability to produce quality scientific data at the level required to achieve the detector\u0027s scientific discovery objectives. Recent ICNO discoveries of cosmic high-energy neutrinos (some reaching energies close to and over 2.5 PeV) and oscillating atmospheric neutrinos in a previously unexplored energy range from 10 to 60 GeV became possible because of the \"state-of-the-art\" detector configuration, excellently supported infrastructure, and cutting-edge science analyses. The ICNO has set limits on Dark Matter annihilations, made precision measurements of the angular distribution of cosmic ray muons, and characterized in detail physical properties of the Antarctic 2.5-km thick ice sheet at South Pole. The discovery of high-energy cosmic neutrinos by IceCube with a flux at the level anticipated for those associated with high-energy gamma- and cosmic-ray accelerators brightens the prospect for identifying the sources of the highest energy particles.", "east": -180.0, "geometry": "POINT(-180 -90)", "instruments": "IN SITU/LABORATORY INSTRUMENTS \u003e PHOTON/OPTICAL DETECTORS \u003e ICECUBE", "is_usap_dc": true, "keywords": "USA/NSF; South Pole; OBSERVATORIES; Amd/Us; AMD; GLACIERS/ICE SHEETS; Icecube; Neutrino; USAP-DC", "locations": "South Pole", "north": -90.0, "nsf_funding_programs": "Antarctic Astrophysics and Geospace Sciences; Antarctic Astrophysics and Geospace Sciences; Antarctic Astrophysics and Geospace Sciences; Antarctic Astrophysics and Geospace Sciences", "paleo_time": null, "persons": "Halzen, Francis; Karle, Albrecht", "platforms": "LAND-BASED PLATFORMS \u003e PERMANENT LAND SITES \u003e OBSERVATORIES", "repo": "IceCube", "repositories": "IceCube; USAP-DC", "science_programs": "IceCube", "south": -90.0, "title": "Management and Operations of the IceCube Neutrino Observatory 2021-2026", "uid": "p0010168", "west": -180.0}, {"awards": "0838838 Evenson, Paul", "bounds_geometry": "POLYGON((-180 -56.02,-160.73 -56.02,-141.46 -56.02,-122.19 -56.02,-102.92 -56.02,-83.65 -56.02,-64.38 -56.02,-45.11 -56.02,-25.84 -56.02,-6.57 -56.02,12.7 -56.02,12.7 -58.203,12.7 -60.386,12.7 -62.569,12.7 -64.752,12.7 -66.935,12.7 -69.118,12.7 -71.301,12.7 -73.484,12.7 -75.667,12.7 -77.85,-6.57 -77.85,-25.84 -77.85,-45.11 -77.85,-64.38 -77.85,-83.65 -77.85,-102.92 -77.85,-122.19 -77.85,-141.46 -77.85,-160.73 -77.85,180 -77.85,178.589 -77.85,177.178 -77.85,175.767 -77.85,174.356 -77.85,172.945 -77.85,171.534 -77.85,170.123 -77.85,168.712 -77.85,167.301 -77.85,165.89 -77.85,165.89 -75.667,165.89 -73.484,165.89 -71.301,165.89 -69.118,165.89 -66.935,165.89 -64.752,165.89 -62.569,165.89 -60.386,165.89 -58.203,165.89 -56.02,167.301 -56.02,168.712 -56.02,170.123 -56.02,171.534 -56.02,172.945 -56.02,174.356 -56.02,175.767 -56.02,177.178 -56.02,178.589 -56.02,-180 -56.02))", "dataset_titles": "Measurement of Cosmic Ray Response Functions for an Ice Cherenkov Detector", "datasets": [{"dataset_uid": "600098", "doi": "10.15784/600098", "keywords": "Antarctica; Atmosphere; Cosmic Ray; Cosmos; Icecube; Oden; Southern Ocean", "people": "Clem, John; Tilav, Serap; Bieber, John; Evenson, Paul", "repository": "USAP-DC", "science_program": null, "title": "Measurement of Cosmic Ray Response Functions for an Ice Cherenkov Detector", "url": "https://www.usap-dc.org/view/dataset/600098"}], "date_created": "Sat, 26 Jun 2010 00:00:00 GMT", "description": "This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5). The proposal seeks funding to determine a complete set of cosmic ray response functions for the ice Cherenkov detector used by the surface air shower IceTop array that is part of the IceCube Neutrino Observatory at the South Pole. This would be accomplished by means of a global latitude survey conducted with a detector (identical to the IceTop sensors) built in a freezer van, which will be installed on the Swedish icebreaker Oden. The cosmic rays shower data will be recorded on the Oden voyage from Sweden to McMurdo and return during the 2009-2010 austral summer season. The potential use of Oden for scientific research has been announced in the NSF Antarctic Science solicitation NSF 08-535. Continued reliance on students provides a broader impact to this proposed research and firmly grounds this effort in its educational mission.", "east": 12.7, "geometry": "POINT(-90.705 -66.935)", "instruments": null, "is_usap_dc": true, "keywords": "Not provided", "locations": null, "north": -56.02, "nsf_funding_programs": "Antarctic Astrophysics and Geospace Sciences", "paleo_time": null, "persons": "Evenson, Paul; Bieber, John; Clem, John; Tilav, Serap", "platforms": "Not provided", "repo": "USAP-DC", "repositories": "USAP-DC", "science_programs": "IceCube", "south": -77.85, "title": "Collaborative Research: Measurement of Cosmic Ray Response Functions for an Ice Cherenkov Detector", "uid": "p0000516", "west": 165.89}]

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