{"projectId":94691,"project":{"projectId":94691,"title":"Nanotechnology based X-ray Detectors for Space Observations","startDate":"2018-07-27","startYear":2018,"startMonth":7,"endDate":"2019-02-15","endYear":2019,"endMonth":2,"programId":73,"program":{"ableToSelect":false,"acronym":"SBIR/STTR","isActive":true,"description":"<p>The NASA SBIR and STTR programs fund the research, development, and demonstration of innovative technologies that fulfill NASA needs as described in the annual Solicitations and have significant potential for successful commercialization. If you are a small business concern (SBC) with 500 or fewer employees or a non-profit RI such as a university or a research laboratory with ties to an SBC, then NASA encourages you to learn more about the SBIR and STTR programs as a potential source of seed funding for the development of your innovations.</p><p><strong>The SBIR and STTR programs have 3 phases</strong>:</p><ul><li><strong>Phase I</strong> is the opportunity to establish the scientific, technical, and commercial feasibility of the proposed innovation in fulfillment of NASA needs.</li><li><strong>Phase II</strong> is focused on the development, demonstration and delivery of the proposed innovation.</li></ul><p>The SBIR and STTR Phase I contracts last for 6 months with a maximum funding of $125,000, and Phase II contracts last for 24 months with a maximum funding of $750,000 - $1.5 million.</p><ul><li><strong>Phase III</strong> is the commercialization of innovative technologies, products, and services resulting from either a Phase I or Phase II contract. Phase III contracts are funded from sources other than the SBIR and STTR programs and may be awarded without further competition.</li></ul><p><strong>Opportunity for Continued Technology Development Post-Phase II</strong>:</p><p>The NASA SBIR/STTR Program currently has in place two initiatives for supporting its small business partners past the basic Phase I and Phase II elements of the program that emphasize opportunities for commercialization. Specifically, the NASA SBIR/STTR Program has the Phase II Enhancement (Phase II-E) and Phase II eXpanded (Phase II-X) contract options.&nbsp;</p><p><strong>Please review the links below to obtain more information on the SBIR/STTR programs.</strong></p><ul><li><strong><a target=\"_blank\" href=\"http://sbir.gsfc.nasa.gov/sites/default/files/ParticipationGuide.pdf\">Participation Guide</a></strong></li></ul><p>Provides an overview of the SBIR and STTR programs as implemented by NASA</p><ul><li><strong><a href=\"http://sbir.gsfc.nasa.gov/solicitations\">Program Solicitations</a></strong></li></ul><p>Provides access to the annual SBIR/STTR Solicitations containing detailed information on the program eligibility requirements, proposal instructions and research topics and subtopics</p><ul><li><strong><a href=\"http://sbir.gsfc.nasa.gov/prg_sched_anncmnt\">Schedule and Awards</a></strong></li></ul><p>Schedule and links for the SBIR/STTR solicitations and selection announcements</p><ul><li><strong><a href=\"http://sbir.gsfc.nasa.gov/content/additional-sources-assistance\">Sources of Assistance</a></strong></li></ul><p>Federal and non-Federal sources of assistance for small business</p><ul><li><strong><a href=\"http://sbir.gsfc.nasa.gov/abstract_archives\">Awarded Abstracts</a></strong></li></ul><p>Search our complete archive of awarded project abstracts to learn about what NASA has funded</p><ul><li><strong><a href=\"http://sbir.gsfc.nasa.gov/content/frequently-asked-questions\">Frequently Asked Questions</a></strong></li></ul><p>&nbsp;Still have questions? Visit the program FAQs</p>","parentProgram":{"ableToSelect":false,"isActive":true,"description":"Catalyst is a portfolio of early stage programs that specialize in different innovation constituencies and mechanisms to push the state of the art in aerospace technology development","programId":92327,"responsibleMd":{"canUserEdit":false,"locationEdit":false,"organizationRolePretty":"","organizationTypePretty":""},"title":"Catalyst","manageGaps":false,"acronymOrTitle":"Catalyst"},"parentProgramId":92327,"programId":73,"responsibleMd":{"organizationId":4875,"organizationName":"Space Technology Mission Directorate","acronym":"STMD","organizationType":"NASA_Mission_Directorate","canUserEdit":false,"locationEdit":false,"organizationRolePretty":"","organizationTypePretty":"NASA Mission Directorate"},"responsibleMdOffice":4875,"stockImageFileId":36648,"title":"Small Business Innovation Research/Small Business Tech Transfer","manageGaps":false,"acronymOrTitle":"SBIR/STTR"},"description":"X-Ray detector technologies that possess improved number of readout pixels, lower power, faster readout rates, greater quantum efficiency, and enhanced energy resolution are critical to space exploration and scientific research missions. This proposal identifies a transformative new approach for X-ray detection using ion-sensitive nanomaterials. Recent work has shown that certain nanomaterials are extremely sensitive to ionized gas molecules, which enables them to detect even individual ions. These sensors can be utilized as a core element within an ionizable gas-filled volume that responds strongly to X-Rays. This project proposes to develop self-standing X-Ray detector elements with higher quantum gain with reduced power consumption compared to conventional X-Ray detectors, without sacrificing readout speed and miniaturizability. This development will be carried out by an optimization of the ion-sensing core nanomaterial, the sensing geometry, and the ionizable front-end gas volume architecture. These optimized materials and architectures will be combined with low-power fast readout electronics at the back-end to form self-standing X-Ray detector elements. This project will combine the state-of-the-art in materials science, physics, detector technology, and electrical engineering to address an issue of enormous scientific importance and technical value. The successful development of such a detector element will enable the project to move into phase II, where prototype solar X-ray detectors with small independent pixels (< 250 µm) and fast read-out (>10,000 count/s/pixel) over an energy range from < 5 keV to 300 keV will be developed. This technology will have the reach to influence a number of NASA missions beyond Solar observation, such as deep-space imaging and navigation. It will also have a huge potential for commercial applications in industrial testing and process control, medical diagnostics, and advanced scientific research in materials science and beyond.","benefits":"The proposed work will eliminate high-voltage requirements and reduce power consumption, reduce payload, and enable nanometer size pixels. Combined, these advancements will enable: High-density arrays for X-ray astrophysics (imaging and spectroscopy) Low keV sensors for solar flare monitoring XNAV for Pulsars for autonomous navigation<br /> <br />Sensitive, small form-factor, low-power, and low-cost X-ray detectors have a tremendous amount of commercial applications: Imaging applications in medical, industrial, and defense sectors Fundamental research around X-rays analysis of material science, and space","releaseStatus":"Released","status":"Completed","viewCount":527,"destinationType":["Outside_the_Solar_System"],"trlBegin":4,"trlCurrent":6,"trlEnd":6,"lastUpdated":"01/22/26","favorited":false,"detailedFunding":false,"projectContacts":[{"contactId":3251221,"canUserEdit":false,"firstName":"Joanne","lastName":"Hill-kittle","fullName":"Joanne Hill-kittle","fullNameInverted":"Hill-kittle, Joanne","email":"joanne.e.hill@nasa.gov","receiveEmail":"Subscribed_Contact","projectContactRole":"Project_Manager","projectContactId":548879,"projectId":94691,"programContactRolePretty":"","projectContactRolePretty":"Project Manager"},{"contactId":96269,"canUserEdit":false,"firstName":"Daniel","lastName":"Esposito","fullName":"Daniel M Esposito","fullNameInverted":"Esposito, Daniel M","middleInitial":"M","email":"dan@guardiontech.com","receiveEmail":"Subscribed_User","projectContactRole":"Principal_Investigator","projectContactId":548880,"projectId":94691,"programContactRolePretty":"","projectContactRolePretty":"Principal Investigator"}],"programContacts":[{"contactId":206378,"canUserEdit":false,"firstName":"Jason","lastName":"Kessler","fullName":"Jason L Kessler","fullNameInverted":"Kessler, Jason L","middleInitial":"L","email":"jason.l.kessler@nasa.gov","receiveEmail":"Subscribed_User","programContactRole":"Program_Director","programContactId":143,"programId":73,"programContactRolePretty":"Program Director","projectContactRolePretty":""},{"contactId":62051,"canUserEdit":false,"firstName":"Carlos","lastName":"Torrez","fullName":"Carlos Torrez","fullNameInverted":"Torrez, Carlos","email":"carlos.torrez@nasa.gov","receiveEmail":"Subscribed_User","programContactRole":"Program_Manager","programContactId":194,"programId":73,"programContactRolePretty":"Program Manager","projectContactRolePretty":""}],"leadOrganization":{"organizationId":2613,"organizationName":"Guardion, Inc.","organizationType":"Industry","city":"Boston","stateTerritoryId":30,"stateTerritory":{"abbreviation":"MA","country":{"abbreviation":"US","countryId":236,"name":"United States"},"countryId":236,"name":"Massachusetts","stateTerritoryId":30,"isTerritory":false},"country":{"abbreviation":"US","countryId":236,"name":"United States"},"countryId":236,"zipCode":"02210-2377","dunsNumber":"081018714","uei":"V31JYMV2LJS7","cageCode":"812X8","congressionalDistrict":"Massachusetts 06","projectId":94691,"projectOrganizationId":576830,"organizationRole":"Lead_Organization","canUserEdit":false,"locationEdit":false,"organizationRolePretty":"Lead Organization","organizationTypePretty":"Industry"},"otherOrganizations":[{"organizationId":2613,"organizationName":"Guardion, Inc.","organizationType":"Industry","city":"Boston","stateTerritoryId":30,"stateTerritory":{"abbreviation":"MA","country":{"abbreviation":"US","countryId":236,"name":"United States"},"countryId":236,"name":"Massachusetts","stateTerritoryId":30,"isTerritory":false},"country":{"abbreviation":"US","countryId":236,"name":"United States"},"countryId":236,"zipCode":"02210-2377","dunsNumber":"081018714","uei":"V31JYMV2LJS7","cageCode":"812X8","congressionalDistrict":"Massachusetts 06","projectId":94691,"projectOrganizationId":576830,"organizationRole":"Lead_Organization","canUserEdit":false,"locationEdit":false,"organizationRolePretty":"Lead Organization","organizationTypePretty":"Industry"},{"organizationId":4947,"organizationName":"Goddard Space Flight Center","acronym":"GSFC","organizationType":"NASA_Center","city":"Greenbelt","stateTerritoryId":3,"stateTerritory":{"abbreviation":"MD","country":{"abbreviation":"US","countryId":236,"name":"United States"},"countryId":236,"name":"Maryland","stateTerritoryId":3,"isTerritory":false},"country":{"abbreviation":"US","countryId":236,"name":"United States"},"countryId":236,"zipCode":"20771","projectId":94691,"projectOrganizationId":576831,"organizationRole":"Supporting_Organization","canUserEdit":false,"locationEdit":false,"organizationRolePretty":"Supporting Organization","organizationTypePretty":"NASA Center"}],"primaryTx":{"taxonomyNodeId":11217,"taxonomyRootId":8817,"parentNodeId":11216,"code":"TX08.1.1","title":"Detectors and Focal Planes","description":"Detectors, focal planes, and readout integrated circuits (ROICs) provide large-format array technologies that require high quantum efficiency (QE); low noise, high resolution, uniform, and stable response; low power and cost; and high reliability. These technologies include low-noise, high-speed, low-power, and radiation hardened ROIC electronics; superconducting sensors; spectral detectors; polarization-sensitive detectors; radiation-hardened detectors; and micro-Kelvin and sub-Kelvin high sensitivity detectors that cover the spectrum from submillimeter wave (Far-IR) to X-ray.","exampleTechnologies":"Backshort Undergrid bolometer arrays, Mercury Cadmium Telluride and Strained Superlattice Arrays, charge coupled devices, sidecar readout integrated circuits, radiometric calibration and abnormality correction algorithms (e.g. non-uniformity)","level":3,"hasChildren":false,"selected":false,"isPrimary":true,"hasInteriorContent":true},"primaryTxTree":[[{"taxonomyNodeId":11215,"taxonomyRootId":8817,"code":"TX08","title":"Sensors and Instruments","level":1,"hasChildren":true,"selected":false,"hasInteriorContent":true},{"taxonomyNodeId":11216,"taxonomyRootId":8817,"parentNodeId":11215,"code":"TX08.1","title":"Remote Sensing Instruments and Sensors","description":"Remote sensing instruments and sensors include components, sensors, and instruments that are sensitive to electromagnetic radiation; particles (charged, neutral, dust); electromagnetic fields, both direct current (DC) and alternating current (AC); acoustic energy; seismic energy; and whatever physical phenomenology the science requires. These instruments and sensors can be active or passive devices, depending on the measurement regime and detection technology.","level":2,"hasChildren":true,"selected":false,"hasInteriorContent":true},{"taxonomyNodeId":11217,"taxonomyRootId":8817,"parentNodeId":11216,"code":"TX08.1.1","title":"Detectors and Focal Planes","description":"Detectors, focal planes, and readout integrated circuits (ROICs) provide large-format array technologies that require high quantum efficiency (QE); low noise, high resolution, uniform, and stable response; low power and cost; and high reliability. These technologies include low-noise, high-speed, low-power, and radiation hardened ROIC electronics; superconducting sensors; spectral detectors; polarization-sensitive detectors; radiation-hardened detectors; and micro-Kelvin and sub-Kelvin high sensitivity detectors that cover the spectrum from submillimeter wave (Far-IR) to X-ray.","exampleTechnologies":"Backshort Undergrid bolometer arrays, Mercury Cadmium Telluride and Strained Superlattice Arrays, charge coupled devices, sidecar readout integrated circuits, radiometric calibration and abnormality correction algorithms (e.g. non-uniformity)","level":3,"hasChildren":false,"selected":true,"hasInteriorContent":true}]],"technologyOutcomes":[{"technologyOutcomeId":98216,"projectId":94691,"project":{"projectId":94691,"title":"Nanotechnology based X-ray Detectors for Space Observations","startDate":"2018-07-27","startYear":2018,"startMonth":7,"endDate":"2019-02-15","endYear":2019,"endMonth":2,"programId":73,"program":{"ableToSelect":false,"acronym":"SBIR/STTR","isActive":true,"description":"<p>The NASA SBIR and STTR programs fund the research, development, and demonstration of innovative technologies that fulfill NASA needs as described in the annual Solicitations and have significant potential for successful commercialization. If you are a small business concern (SBC) with 500 or fewer employees or a non-profit RI such as a university or a research laboratory with ties to an SBC, then NASA encourages you to learn more about the SBIR and STTR programs as a potential source of seed funding for the development of your innovations.</p><p><strong>The SBIR and STTR programs have 3 phases</strong>:</p><ul><li><strong>Phase I</strong> is the opportunity to establish the scientific, technical, and commercial feasibility of the proposed innovation in fulfillment of NASA needs.</li><li><strong>Phase II</strong> is focused on the development, demonstration and delivery of the proposed innovation.</li></ul><p>The SBIR and STTR Phase I contracts last for 6 months with a maximum funding of $125,000, and Phase II contracts last for 24 months with a maximum funding of $750,000 - $1.5 million.</p><ul><li><strong>Phase III</strong> is the commercialization of innovative technologies, products, and services resulting from either a Phase I or Phase II contract. Phase III contracts are funded from sources other than the SBIR and STTR programs and may be awarded without further competition.</li></ul><p><strong>Opportunity for Continued Technology Development Post-Phase II</strong>:</p><p>The NASA SBIR/STTR Program currently has in place two initiatives for supporting its small business partners past the basic Phase I and Phase II elements of the program that emphasize opportunities for commercialization. Specifically, the NASA SBIR/STTR Program has the Phase II Enhancement (Phase II-E) and Phase II eXpanded (Phase II-X) contract options.&nbsp;</p><p><strong>Please review the links below to obtain more information on the SBIR/STTR programs.</strong></p><ul><li><strong><a target=\"_blank\" href=\"http://sbir.gsfc.nasa.gov/sites/default/files/ParticipationGuide.pdf\">Participation Guide</a></strong></li></ul><p>Provides an overview of the SBIR and STTR programs as implemented by NASA</p><ul><li><strong><a href=\"http://sbir.gsfc.nasa.gov/solicitations\">Program Solicitations</a></strong></li></ul><p>Provides access to the annual SBIR/STTR Solicitations containing detailed information on the program eligibility requirements, proposal instructions and research topics and subtopics</p><ul><li><strong><a href=\"http://sbir.gsfc.nasa.gov/prg_sched_anncmnt\">Schedule and Awards</a></strong></li></ul><p>Schedule and links for the SBIR/STTR solicitations and selection announcements</p><ul><li><strong><a href=\"http://sbir.gsfc.nasa.gov/content/additional-sources-assistance\">Sources of Assistance</a></strong></li></ul><p>Federal and non-Federal sources of assistance for small business</p><ul><li><strong><a href=\"http://sbir.gsfc.nasa.gov/abstract_archives\">Awarded Abstracts</a></strong></li></ul><p>Search our complete archive of awarded project abstracts to learn about what NASA has funded</p><ul><li><strong><a href=\"http://sbir.gsfc.nasa.gov/content/frequently-asked-questions\">Frequently Asked Questions</a></strong></li></ul><p>&nbsp;Still have questions? Visit the program FAQs</p>","parentProgram":{"ableToSelect":false,"isActive":true,"description":"Catalyst is a portfolio of early stage programs that specialize in different innovation constituencies and mechanisms to push the state of the art in aerospace technology development","programId":92327,"responsibleMd":{"canUserEdit":false,"locationEdit":false,"organizationRolePretty":"","organizationTypePretty":""},"title":"Catalyst","manageGaps":false,"acronymOrTitle":"Catalyst"},"parentProgramId":92327,"programId":73,"responsibleMd":{"organizationId":4875,"organizationName":"Space Technology Mission Directorate","acronym":"STMD","organizationType":"NASA_Mission_Directorate","canUserEdit":false,"locationEdit":false,"organizationRolePretty":"","organizationTypePretty":"NASA Mission Directorate"},"responsibleMdOffice":4875,"stockImageFileId":36648,"title":"Small Business Innovation Research/Small Business Tech Transfer","manageGaps":false,"acronymOrTitle":"SBIR/STTR"},"description":"X-Ray detector technologies that possess improved number of readout pixels, lower power, faster readout rates, greater quantum efficiency, and enhanced energy resolution are critical to space exploration and scientific research missions. This proposal identifies a transformative new approach for X-ray detection using ion-sensitive nanomaterials. Recent work has shown that certain nanomaterials are extremely sensitive to ionized gas molecules, which enables them to detect even individual ions. These sensors can be utilized as a core element within an ionizable gas-filled volume that responds strongly to X-Rays. This project proposes to develop self-standing X-Ray detector elements with higher quantum gain with reduced power consumption compared to conventional X-Ray detectors, without sacrificing readout speed and miniaturizability. This development will be carried out by an optimization of the ion-sensing core nanomaterial, the sensing geometry, and the ionizable front-end gas volume architecture. These optimized materials and architectures will be combined with low-power fast readout electronics at the back-end to form self-standing X-Ray detector elements. This project will combine the state-of-the-art in materials science, physics, detector technology, and electrical engineering to address an issue of enormous scientific importance and technical value. The successful development of such a detector element will enable the project to move into phase II, where prototype solar X-ray detectors with small independent pixels (< 250 µm) and fast read-out (>10,000 count/s/pixel) over an energy range from < 5 keV to 300 keV will be developed. This technology will have the reach to influence a number of NASA missions beyond Solar observation, such as deep-space imaging and navigation. It will also have a huge potential for commercial applications in industrial testing and process control, medical diagnostics, and advanced scientific research in materials science and beyond.","benefits":"The proposed work will eliminate high-voltage requirements and reduce power consumption, reduce payload, and enable nanometer size pixels. Combined, these advancements will enable: High-density arrays for X-ray astrophysics (imaging and spectroscopy) Low keV sensors for solar flare monitoring XNAV for Pulsars for autonomous navigation<br /> <br />Sensitive, small form-factor, low-power, and low-cost X-ray detectors have a tremendous amount of commercial applications: Imaging applications in medical, industrial, and defense sectors Fundamental research around X-rays analysis of material science, and space","releaseStatus":"Released","status":"Completed","destinationType":["Outside_the_Solar_System"],"trlBegin":4,"trlCurrent":6,"trlEnd":6,"favorited":false,"detailedFunding":false,"programContacts":[{"contactId":206378,"canUserEdit":false,"firstName":"Jason","lastName":"Kessler","fullName":"Jason L Kessler","fullNameInverted":"Kessler, Jason L","middleInitial":"L","email":"jason.l.kessler@nasa.gov","receiveEmail":"Subscribed_User","programContactRole":"Program_Director","programContactId":143,"programId":73,"programContactRolePretty":"Program Director","projectContactRolePretty":""},{"contactId":62051,"canUserEdit":false,"firstName":"Carlos","lastName":"Torrez","fullName":"Carlos Torrez","fullNameInverted":"Torrez, Carlos","email":"carlos.torrez@nasa.gov","receiveEmail":"Subscribed_User","programContactRole":"Program_Manager","programContactId":194,"programId":73,"programContactRolePretty":"Program Manager","projectContactRolePretty":""}],"endDateString":"Feb 2019","startDateString":"Jul 2018"},"technologyOutcomeDate":"2019-02-15","technologyOutcomePath":"Closed_Out","files":[{"title":"Final Summary Chart","file":{"fileExtension":"pdf","fileId":369956,"fileName":"1550264763646","fileSize":163843,"objectId":98216,"objectType":"technologyOutcomeFiles","presignedUpload":false,"fileSizeString":"160.0 KB"},"technologyOutcomeId":98216,"fileId":369956}],"infoText":"Closed out","infoTextExtra":"Project closed out","isIndirect":false,"infusionPretty":"","isBiDirectional":false,"technologyOutcomeDateString":"Feb 2019","technologyOutcomeDateFullString":"February 2019","technologyOutcomePartnerPretty":"","technologyOutcomePathPretty":"Closed Out","technologyOutcomeRationalePretty":""}],"primaryImage":{"file":{"fileExtension":"jpg","fileId":369954,"presignedUpload":false,"fileSizeString":"0 Byte"},"libraryItemId":369584,"description":"Final Summary Chart Image","projectId":94691,"publishedDateString":"","entryDateString":"","libraryItemTypePretty":"","modifiedDateString":""},"libraryItems":[{"file":{"fileExtension":"pdf","fileId":369952,"fileName":"1520629914497","fileSize":707306,"objectId":369582,"objectType":"libraryItemFiles","presignedUpload":false,"fileSizeString":"690.7 KB"},"files":[{"fileExtension":"pdf","fileId":369952,"fileName":"1520629914497","fileSize":707306,"objectId":369582,"objectType":"libraryItemFiles","presignedUpload":false,"fileSizeString":"690.7 KB"}],"libraryItemId":369582,"title":"Briefing Chart","libraryItemType":"Document","projectId":94691,"internalOnly":false,"publishedDateString":"","entryDateString":"01/22/25 01:10 AM","libraryItemTypePretty":"Document","modifiedDateString":"01/08/24 08:27 PM"},{"file":{"fileExtension":"jpg","fileId":369955,"fileName":"1520553716334","fileSize":612323,"objectId":369585,"objectType":"libraryItemFiles","presignedUpload":false,"fileSizeString":"598.0 KB"},"files":[{"fileExtension":"jpg","fileId":369955,"fileName":"1520553716334","fileSize":612323,"objectId":369585,"objectType":"libraryItemFiles","presignedUpload":false,"fileSizeString":"598.0 KB"}],"libraryItemId":369585,"title":"Briefing Chart Image","description":"Briefing Chart Image","libraryItemType":"Image","projectId":94691,"isPrimary":false,"internalOnly":false,"publishedDateString":"","entryDateString":"01/22/25 01:10 AM","libraryItemTypePretty":"Image","modifiedDateString":"01/08/24 08:27 PM"},{"file":{"fileExtension":"jpg","fileId":369954,"fileName":"1550264754100","fileSize":51222,"objectId":369584,"objectType":"libraryItemFiles","presignedUpload":false,"fileSizeString":"50.0 KB"},"files":[{"fileExtension":"jpg","fileId":369954,"fileName":"1550264754100","fileSize":51222,"objectId":369584,"objectType":"libraryItemFiles","presignedUpload":false,"fileSizeString":"50.0 KB"}],"libraryItemId":369584,"title":"Final Summary Chart Image","description":"Final Summary Chart Image","libraryItemType":"Image","projectId":94691,"isPrimary":true,"internalOnly":false,"publishedDateString":"","entryDateString":"01/22/25 01:10 AM","libraryItemTypePretty":"Image","modifiedDateString":"01/08/24 08:27 PM"}],"states":[{"abbreviation":"MD","country":{"abbreviation":"US","countryId":236,"name":"United States"},"countryId":236,"name":"Maryland","stateTerritoryId":3,"isTerritory":false},{"abbreviation":"MA","country":{"abbreviation":"US","countryId":236,"name":"United States"},"countryId":236,"name":"Massachusetts","stateTerritoryId":30,"isTerritory":false}],"endDateString":"Feb 2019","startDateString":"Jul 2018"}}