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PSR_J1412+7922 | 213.2305 | 79.36966 | 118.318972 | 37.018141 | 60,279.448611 | 60,279.985023 | 5,505,032,101 | -1 | 213.23279 | 79.36775 | 4,792 | 7,000 | 51 | VALIDATED | 60,290.445208 | 60,473 | 5,505 | We propose monitoring campaigns for five radio-quiet X-ray-only pulsars (PSR J0058-7218, J0537-6910, J1412+7922, J1811-1925, and J1849-0001), all of which can only be done with NICER observations. These data allow computation of an accurate phase-connected timing model for each pulsar, which enable LIGO/Virgo/KAGRA to ... | MAGNETARS AND ROTATION-POWERED PULSARS | 2 | HO | WYNN | 5 | NOR | MONITORING X-RAY PULSARS FOR GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2365 | 79.36968 | 118.317704 | 37.017693 | 60,140.565741 | 60,140.572222 | 6,020,290,201 | -1 | 213.232854 | 79.367806 | 281 | 0 | 51 | VALIDATED | 60,152.515278 | 60,154 | 6,020 | Observations dedicated to the Magnetar science working group | MAGNETAR | 2 | GENDREAU | KEITH C. | 6 | NOR | MAGNETAR WORKING GROUP | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2436 | 79.36971 | 118.316207 | 37.017157 | 58,174.135417 | 58,174.910382 | 1,020,290,126 | -1 | 213.232854 | 79.367806 | 1,040 | 20,000 | 52 | VALIDATED | 58,178.72456 | 58,188 | 1,020 | Observations dedicated to the Magnetar science working group | MAGNETAR | 2 | GENDREAU | KEITH C. | 1 | NOR | MAGNETAR WORKING GROUP | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2322 | 79.36977 | 118.318663 | 37.017918 | 60,340.055694 | 60,340.583333 | 5,505,032,302 | -1 | 213.23279 | 79.36775 | 0 | 7,000 | 41 | VALIDATED | 60,354.828623 | 60,534 | 5,505 | We propose monitoring campaigns for five radio-quiet X-ray-only pulsars (PSR J0058-7218, J0537-6910, J1412+7922, J1811-1925, and J1849-0001), all of which can only be done with NICER observations. These data allow computation of an accurate phase-connected timing model for each pulsar, which enable LIGO/Virgo/KAGRA to ... | MAGNETARS AND ROTATION-POWERED PULSARS | 2 | HO | WYNN | 5 | NOR | MONITORING X-RAY PULSARS FOR GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2081 | 79.36987 | 118.323844 | 37.01955 | 59,384.030093 | 59,384.62963 | 3,536,030,804 | -1 | 213.23279 | 79.36775 | 12,994 | 8,000 | 52 | VALIDATED | 59,394.655185 | 59,578 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2265 | 79.36998 | 118.319979 | 37.018133 | 60,052.428241 | 60,052.89456 | 5,505,031,311 | -1 | 213.23279 | 79.36775 | 1,609 | 7,000 | 51 | VALIDATED | 60,069.895741 | 60,246 | 5,505 | We propose monitoring campaigns for five radio-quiet X-ray-only pulsars (PSR J0058-7218, J0537-6910, J1412+7922, J1811-1925, and J1849-0001), all of which can only be done with NICER observations. These data allow computation of an accurate phase-connected timing model for each pulsar, which enable LIGO/Virgo/KAGRA to ... | MAGNETARS AND ROTATION-POWERED PULSARS | 2 | HO | WYNN | 5 | NOR | MONITORING X-RAY PULSARS FOR GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2369 | 79.37008 | 118.317813 | 37.017296 | 59,033.599074 | 59,033.865671 | 3,536,030,214 | -1 | 213.23279 | 79.36775 | 1,275 | 8,000 | 52 | VALIDATED | 59,037.660845 | 59,227 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
S5_0532+82 | 85.91455 | 82.6403 | 130.6879 | 24.771465 | 60,759.049225 | 60,759.956481 | 8,200,750,105 | -1 | 85.911862 | 82.64132 | 0 | 0 | 50 | VALIDATED | 60,772.481921 | 60,773 | 8,200 | Target of Opportunities sponsored by the Principal Investigator | DIR | 9 | GENDREAU | KEITH C. | 8 | DDT_TOO | Director Target of Operations | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2395 | 79.37011 | 118.317274 | 37.017082 | 59,114.941435 | 59,114.948137 | 3,536,030,309 | -1 | 213.23279 | 79.36775 | 350 | 8,000 | 51 | VALIDATED | 59,118.708507 | 59,308 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2438 | 79.37017 | 118.316388 | 37.016719 | 59,844.537269 | 59,844.543356 | 5,505,030,715 | -1 | 213.23279 | 79.36775 | 431 | 7,000 | 52 | VALIDATED | 59,855.118993 | 60,038 | 5,505 | We propose monitoring campaigns for five radio-quiet X-ray-only pulsars (PSR J0058-7218, J0537-6910, J1412+7922, J1811-1925, and J1849-0001), all of which can only be done with NICER observations. These data allow computation of an accurate phase-connected timing model for each pulsar, which enable LIGO/Virgo/KAGRA to ... | MAGNETARS AND ROTATION-POWERED PULSARS | 2 | HO | WYNN | 5 | NOR | MONITORING X-RAY PULSARS FOR GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2313 | 79.37021 | 118.319069 | 37.017577 | 58,518.501157 | 58,518.894433 | 1,020,290,265 | -1 | 213.232854 | 79.367806 | 32 | 0 | 52 | VALIDATED | 58,522.982014 | 58,532 | 1,020 | Observations dedicated to the Magnetar science working group | MAGNETAR | 2 | GENDREAU | KEITH C. | 1 | NOR | MAGNETAR WORKING GROUP | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.231 | 79.37029 | 118.319171 | 37.017525 | 59,325.505787 | 59,325.512211 | 3,536,030,705 | -1 | 213.23279 | 79.36775 | 429 | 8,000 | 52 | VALIDATED | 59,335.722778 | 59,519 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.21 | 79.37032 | 118.323658 | 37.018999 | 59,245.953935 | 59,245.961736 | 3,536,030,511 | -1 | 213.23279 | 79.36775 | 0 | 8,000 | 51 | VALIDATED | 59,250.835359 | 59,439 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.231 | 79.37032 | 118.319186 | 37.017497 | 60,341.4739 | 60,341.740509 | 5,505,032,303 | -1 | 213.23279 | 79.36775 | 683 | 7,000 | 41 | VALIDATED | 60,355.00294 | 60,535 | 5,505 | We propose monitoring campaigns for five radio-quiet X-ray-only pulsars (PSR J0058-7218, J0537-6910, J1412+7922, J1811-1925, and J1849-0001), all of which can only be done with NICER observations. These data allow computation of an accurate phase-connected timing model for each pulsar, which enable LIGO/Virgo/KAGRA to ... | MAGNETARS AND ROTATION-POWERED PULSARS | 2 | HO | WYNN | 5 | NOR | MONITORING X-RAY PULSARS FOR GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2379 | 79.37036 | 118.317736 | 37.016966 | 60,795.303704 | 60,795.309884 | 8,020,290,223 | -1 | 213.232854 | 79.367806 | 0 | 0 | 0 | VALIDATED | 60,804.806852 | 60,809 | 8,020 | Observations dedicated to the Magnetar science working group | MAGNETAR | 2 | GENDREAU | KEITH C. | 8 | NOR | MAGNETAR WORKING GROUP | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2377 | 79.37038 | 118.317789 | 37.016962 | 60,829.088438 | 60,829.997269 | 8,020,290,227 | -1 | 213.232854 | 79.367806 | 0 | 0 | 34 | VALIDATED | 60,840.882222 | 60,843 | 8,020 | Observations dedicated to the Magnetar science working group | MAGNETAR | 2 | GENDREAU | KEITH C. | 8 | NOR | MAGNETAR WORKING GROUP | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.246 | 79.37051 | 118.316085 | 37.016248 | 59,116.875243 | 59,116.884306 | 3,536,030,311 | -1 | 213.23279 | 79.36775 | 637 | 8,000 | 51 | VALIDATED | 59,120.716597 | 59,310 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2317 | 79.37053 | 118.319139 | 37.017254 | 58,170.016204 | 58,170.932546 | 1,020,290,122 | -1 | 213.232854 | 79.367806 | 6,154 | 20,000 | 52 | VALIDATED | 58,182.962998 | 58,184 | 1,020 | Observations dedicated to the Magnetar science working group | MAGNETAR | 2 | GENDREAU | KEITH C. | 1 | NOR | MAGNETAR WORKING GROUP | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2458 | 79.37059 | 118.316166 | 37.016189 | 59,845.053241 | 59,845.059109 | 5,505,030,716 | -1 | 213.23279 | 79.36775 | 404 | 7,000 | 52 | VALIDATED | 59,855.147593 | 60,039 | 5,505 | We propose monitoring campaigns for five radio-quiet X-ray-only pulsars (PSR J0058-7218, J0537-6910, J1412+7922, J1811-1925, and J1849-0001), all of which can only be done with NICER observations. These data allow computation of an accurate phase-connected timing model for each pulsar, which enable LIGO/Virgo/KAGRA to ... | MAGNETARS AND ROTATION-POWERED PULSARS | 2 | HO | WYNN | 5 | NOR | MONITORING X-RAY PULSARS FOR GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2343 | 79.37063 | 118.318634 | 37.016975 | 59,034.054398 | 59,034.386447 | 3,536,030,215 | -1 | 213.23279 | 79.36775 | 4,381 | 8,000 | 52 | VALIDATED | 59,038.625255 | 59,228 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2339 | 79.37068 | 118.318743 | 37.016958 | 59,904.76088 | 59,904.962002 | 5,505,030,911 | -1 | 213.23279 | 79.36775 | 1,241 | 7,000 | 52 | VALIDATED | 59,914.783287 | 60,098 | 5,505 | We propose monitoring campaigns for five radio-quiet X-ray-only pulsars (PSR J0058-7218, J0537-6910, J1412+7922, J1811-1925, and J1849-0001), all of which can only be done with NICER observations. These data allow computation of an accurate phase-connected timing model for each pulsar, which enable LIGO/Virgo/KAGRA to ... | MAGNETARS AND ROTATION-POWERED PULSARS | 2 | HO | WYNN | 5 | NOR | MONITORING X-RAY PULSARS FOR GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2374 | 79.37073 | 118.318023 | 37.016661 | 59,031.790278 | 59,031.80044 | 3,536,030,212 | -1 | 213.23279 | 79.36775 | 748 | 8,000 | 52 | VALIDATED | 59,035.682662 | 59,225 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2446 | 79.37086 | 118.316553 | 37.016026 | 60,076.165741 | 60,076.168229 | 5,505,031,504 | -1 | 213.23279 | 79.36775 | 151 | 7,000 | 51 | VALIDATED | 60,088.212963 | 60,270 | 5,505 | We propose monitoring campaigns for five radio-quiet X-ray-only pulsars (PSR J0058-7218, J0537-6910, J1412+7922, J1811-1925, and J1849-0001), all of which can only be done with NICER observations. These data allow computation of an accurate phase-connected timing model for each pulsar, which enable LIGO/Virgo/KAGRA to ... | MAGNETARS AND ROTATION-POWERED PULSARS | 2 | HO | WYNN | 5 | NOR | MONITORING X-RAY PULSARS FOR GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2444 | 79.37087 | 118.3166 | 37.016031 | 59,254.278241 | 59,254.281586 | 3,536,030,518 | -1 | 213.23279 | 79.36775 | 157 | 8,000 | 52 | VALIDATED | 59,268.675255 | 59,448 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2368 | 79.37093 | 118.318248 | 37.01652 | 58,017.372859 | 58,017.942789 | 1,020,290,105 | -1 | 213.232854 | 79.367806 | 2,521 | 20,000 | 52 | VALIDATED | 58,182.91 | 58,181 | 1,020 | Observations dedicated to the Magnetar science working group | MAGNETAR | 2 | GENDREAU | KEITH C. | 1 | NOR | MAGNETAR WORKING GROUP | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2061 | 79.37094 | 118.324789 | 37.018707 | 58,735.150463 | 58,735.606458 | 2,579,020,313 | -1 | 213.23279 | 79.36775 | 275 | 8,000 | 52 | VALIDATED | 58,739.626933 | 58,929 | 2,579 | We propose to perform monitoring campaigns for pulsars PSR J0537-6910, J1412+7922, J1813-1749, J1849-0001, and J2229+6114, four of which can only be done via X-ray observations. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform searches o... | X-RAY PULSARS AND NEUTRON STARS | 2 | HO | WYNN | 2 | NOR | MONITORING PULSARS TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2348 | 79.37116 | 118.318785 | 37.016451 | 58,016.138426 | 58,016.72228 | 1,020,290,104 | -1 | 213.232854 | 79.367806 | 1,256 | 20,000 | 52 | VALIDATED | 58,182.908356 | 58,181 | 1,020 | Observations dedicated to the Magnetar science working group | MAGNETAR | 2 | GENDREAU | KEITH C. | 1 | NOR | MAGNETAR WORKING GROUP | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.244 | 79.37118 | 118.316836 | 37.015774 | 58,453.797454 | 58,453.936678 | 1,020,290,244 | -1 | 213.232854 | 79.367806 | 2,042 | 0 | 52 | VALIDATED | 58,457.693924 | 58,467 | 1,020 | Observations dedicated to the Magnetar science working group | MAGNETAR | 2 | GENDREAU | KEITH C. | 1 | NOR | MAGNETAR WORKING GROUP | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2147 | 79.3712 | 118.323084 | 37.017852 | 58,741.454861 | 58,741.45875 | 2,579,020,316 | -1 | 213.23279 | 79.36775 | 243 | 8,000 | 52 | VALIDATED | 58,746.743125 | 58,935 | 2,579 | We propose to perform monitoring campaigns for pulsars PSR J0537-6910, J1412+7922, J1813-1749, J1849-0001, and J2229+6114, four of which can only be done via X-ray observations. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform searches o... | X-RAY PULSARS AND NEUTRON STARS | 2 | HO | WYNN | 2 | NOR | MONITORING PULSARS TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2517 | 79.3712 | 118.315207 | 37.015204 | 60,218.399769 | 60,218.403009 | 6,020,290,214 | -1 | 213.232854 | 79.367806 | 15 | 0 | 50 | VALIDATED | 60,230.618345 | 60,232 | 6,020 | Observations dedicated to the Magnetar science working group | MAGNETAR | 2 | GENDREAU | KEITH C. | 6 | NOR | MAGNETAR WORKING GROUP | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2324 | 79.37125 | 118.31934 | 37.01654 | 58,015.302778 | 58,015.692546 | 1,020,290,103 | -1 | 213.232854 | 79.367806 | 726 | 20,000 | 52 | VALIDATED | 58,182.906759 | 58,181 | 1,020 | Observations dedicated to the Magnetar science working group | MAGNETAR | 2 | GENDREAU | KEITH C. | 1 | NOR | MAGNETAR WORKING GROUP | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2415 | 79.37125 | 118.317403 | 37.015888 | 58,959.743519 | 58,959.746782 | 3,536,030,109 | -1 | 213.23279 | 79.36775 | 175 | 8,000 | 52 | VALIDATED | 58,963.826157 | 59,153 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
S5_0532+82 | 85.91947 | 82.6405 | 130.687935 | 24.772125 | 60,758.016655 | 60,758.989352 | 8,200,750,104 | -1 | 85.911862 | 82.64132 | 0 | 0 | 50 | VALIDATED | 60,769.811574 | 60,772 | 8,200 | Target of Opportunities sponsored by the Principal Investigator | DIR | 9 | GENDREAU | KEITH C. | 8 | DDT_TOO | Director Target of Operations | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2462 | 79.37153 | 118.316538 | 37.015294 | 60,698.443171 | 60,698.839549 | 7,508,031,118 | -1 | 213.23279 | 79.36775 | 0 | 7,000 | 41 | VALIDATED | 60,710.277975 | 60,712 | 7,508 | We propose monitoring observations of four radio-quiet X-ray-only pulsars (and PSR B0540-69), each of which can only be done using NICER, with total Cycle 6 exposure times of 208 ks for PSR J0058-7218, 26 ks for PSR B0540-69, 84 ks for PSR J1412+7922, 90 ks for PSR J1811-1925, and 50 ks for PSR J1849-0001. These data a... | MAGNETARS AND ROTATION-POWERED PULSARS | 2 | HO | WYNN | 7 | NOR | MONITORING X-RAY PULSARS FOR THEIR GRAVITATIONAL WAVES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2326 | 79.37167 | 118.319501 | 37.016138 | 59,176.163194 | 59,176.487025 | 3,536,030,417 | -1 | 213.23279 | 79.36775 | 687 | 8,000 | 51 | VALIDATED | 59,181.719502 | 59,370 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2366 | 79.37174 | 118.318684 | 37.015788 | 58,815.266898 | 58,815.852072 | 2,579,020,422 | -1 | 213.23279 | 79.36775 | 3,035 | 8,000 | 52 | VALIDATED | 58,821.916701 | 59,009 | 2,579 | We propose to perform monitoring campaigns for pulsars PSR J0537-6910, J1412+7922, J1813-1749, J1849-0001, and J2229+6114, four of which can only be done via X-ray observations. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform searches o... | X-RAY PULSARS AND NEUTRON STARS | 2 | HO | WYNN | 2 | NOR | MONITORING PULSARS TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2384 | 79.37177 | 118.318315 | 37.015631 | 59,252.344213 | 59,252.614595 | 3,536,030,517 | -1 | 213.23279 | 79.36775 | 548 | 8,000 | 52 | VALIDATED | 59,255.937222 | 59,446 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2609 | 79.37185 | 118.313565 | 37.013946 | 58,882.910486 | 58,882.919688 | 2,579,020,604 | -1 | 213.23279 | 79.36775 | 0 | 8,000 | 52 | VALIDATED | 58,886.793102 | 59,076 | 2,579 | We propose to perform monitoring campaigns for pulsars PSR J0537-6910, J1412+7922, J1813-1749, J1849-0001, and J2229+6114, four of which can only be done via X-ray observations. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform searches o... | X-RAY PULSARS AND NEUTRON STARS | 2 | HO | WYNN | 2 | NOR | MONITORING PULSARS TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2377 | 79.37188 | 118.318518 | 37.01558 | 59,542.562269 | 59,542.580197 | 3,536,031,027 | -1 | 213.23279 | 79.36775 | 1,458 | 8,000 | 52 | VALIDATED | 59,552.810625 | 59,736 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
S5_0532+82 | 85.91983 | 82.64069 | 130.687756 | 24.772234 | 60,757.049491 | 60,757.957407 | 8,200,750,103 | -1 | 85.911862 | 82.64132 | 0 | 0 | 50 | VALIDATED | 60,767.88934 | 60,771 | 8,200 | Target of Opportunities sponsored by the Principal Investigator | DIR | 9 | GENDREAU | KEITH C. | 8 | DDT_TOO | Director Target of Operations | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2489 | 79.372 | 118.316192 | 37.014667 | 59,249.313194 | 59,249.317095 | 3,536,030,515 | -1 | 213.23279 | 79.36775 | 34 | 8,000 | 52 | VALIDATED | 59,255.261655 | 59,443 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.224 | 79.37201 | 118.321497 | 37.01644 | 58,968.015046 | 58,968.150926 | 3,536,030,112 | -1 | 213.23279 | 79.36775 | 1,044 | 8,000 | 52 | VALIDATED | 58,973.705231 | 59,162 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2211 | 79.37207 | 118.322144 | 37.016593 | 60,339.47537 | 60,339.999306 | 5,505,032,301 | -1 | 213.23279 | 79.36775 | 0 | 7,000 | 41 | VALIDATED | 60,352.465081 | 60,533 | 5,505 | We propose monitoring campaigns for five radio-quiet X-ray-only pulsars (PSR J0058-7218, J0537-6910, J1412+7922, J1811-1925, and J1849-0001), all of which can only be done with NICER observations. These data allow computation of an accurate phase-connected timing model for each pulsar, which enable LIGO/Virgo/KAGRA to ... | MAGNETARS AND ROTATION-POWERED PULSARS | 2 | HO | WYNN | 5 | NOR | MONITORING X-RAY PULSARS FOR GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.223 | 79.37209 | 118.321749 | 37.016438 | 58,525.71853 | 58,525.729375 | 1,020,290,270 | -1 | 213.232854 | 79.367806 | 598 | 0 | 52 | VALIDATED | 58,535.674641 | 58,539 | 1,020 | Observations dedicated to the Magnetar science working group | MAGNETAR | 2 | GENDREAU | KEITH C. | 1 | NOR | MAGNETAR WORKING GROUP | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2309 | 79.37215 | 118.320097 | 37.015818 | 60,057.336806 | 60,057.536319 | 5,505,031,313 | -1 | 213.23279 | 79.36775 | 685 | 7,000 | 51 | VALIDATED | 60,067.102176 | 60,251 | 5,505 | We propose monitoring campaigns for five radio-quiet X-ray-only pulsars (PSR J0058-7218, J0537-6910, J1412+7922, J1811-1925, and J1849-0001), all of which can only be done with NICER observations. These data allow computation of an accurate phase-connected timing model for each pulsar, which enable LIGO/Virgo/KAGRA to ... | MAGNETARS AND ROTATION-POWERED PULSARS | 2 | HO | WYNN | 5 | NOR | MONITORING X-RAY PULSARS FOR GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2364 | 79.37251 | 118.319101 | 37.015092 | 59,332.808102 | 59,332.81588 | 3,536,030,707 | -1 | 213.23279 | 79.36775 | 276 | 8,000 | 52 | VALIDATED | 59,344.658495 | 59,526 | 3,536 | We propose monitoring campaigns for five pulsars (PSR J0537-6910, J1101-6101, J1412+7922, J1849-0001, and J2229+6114), four of which can only be done via X-ray observations using NICER. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform se... | ROTATION-POWERED NEUTRON STARS | 2 | HO | WYNN | 3 | NOR | PULSAR MONITORING TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
PSR_J1412+7922 | 213.2235 | 79.37286 | 118.322017 | 37.015693 | 58,739.136343 | 58,739.474525 | 2,579,020,315 | -1 | 213.23279 | 79.36775 | 3,438 | 8,000 | 52 | VALIDATED | 58,742.666146 | 58,933 | 2,579 | We propose to perform monitoring campaigns for pulsars PSR J0537-6910, J1412+7922, J1813-1749, J1849-0001, and J2229+6114, four of which can only be done via X-ray observations. These data will allow us to compute accurate phase-connected timing models for each pulsar, which will enable LIGO/Virgo to perform searches o... | X-RAY PULSARS AND NEUTRON STARS | 2 | HO | WYNN | 2 | NOR | MONITORING PULSARS TO ENABLE GRAVITATIONAL WAVE SEARCHES | 10,000,000,000,000,000 |
3C_390.3 | 280.5383 | 79.77109 | 111.437554 | 27.073779 | 60,791.226157 | 60,791.363194 | 8,653,030,102 | -1 | 280.53746 | 79.771424 | 1,463 | 0 | 50 | VALIDATED | 60,802.92831 | 60,805 | 8,653 | Nearby powerful AGN provide critical insights into the growth of black holes and their impact on host galaxies. The Swift-BAT survey offers the largest, most complete sample of local (z<0.1) powerful AGN. Major HST SNAP programs (>500 orbits) are observing 191 nearby Seyfert 1 AGN from this sample across UV (225W) and ... | ACTIVE GALAXIES AND QUASARS | 2 | KOSS | MICHAEL | 8 | NOR | RESOLVING THE AGN BOLOMETRIC EMISSION WITH NICER AND HST | 10,000,000,000,000,000 |
3C_390.3 | 280.5381 | 79.77112 | 111.437585 | 27.073816 | 60,790.961574 | 60,790.972454 | 8,653,030,101 | -1 | 280.53746 | 79.771424 | 746 | 0 | 50 | VALIDATED | 60,800.90169 | 60,804 | 8,653 | Nearby powerful AGN provide critical insights into the growth of black holes and their impact on host galaxies. The Swift-BAT survey offers the largest, most complete sample of local (z<0.1) powerful AGN. Major HST SNAP programs (>500 orbits) are observing 191 nearby Seyfert 1 AGN from this sample across UV (225W) and ... | ACTIVE GALAXIES AND QUASARS | 2 | KOSS | MICHAEL | 8 | NOR | RESOLVING THE AGN BOLOMETRIC EMISSION WITH NICER AND HST | 10,000,000,000,000,000 |
U_Cep | 15.62295 | 81.871 | 123.345058 | 19.00812 | 57,941.884722 | 57,941.889132 | 12,070,112 | -1 | 15.57 | 81.875 | 260 | 0 | 52 | VALIDATED | 58,180.090231 | 58,181 | 12 | Observations of sky background targets for NICER calibration | CAL | 1 | GENDREAU | KEITH C. | 0 | CAL | CALIBRATION BACKGROUND | 10,000,000,000,000,000 |
U_Cep | 15.62111 | 81.87173 | 123.344749 | 19.008837 | 57,944.201389 | 57,944.848264 | 12,070,115 | -1 | 15.57 | 81.875 | 869 | 0 | 52 | VALIDATED | 58,180.094225 | 58,181 | 12 | Observations of sky background targets for NICER calibration | CAL | 1 | GENDREAU | KEITH C. | 0 | CAL | CALIBRATION BACKGROUND | 10,000,000,000,000,000 |
U_Cep | 15.61355 | 81.87194 | 123.343609 | 19.008999 | 57,943.171528 | 57,943.754525 | 12,070,114 | -1 | 15.57 | 81.875 | 966 | 0 | 52 | VALIDATED | 58,180.092697 | 58,181 | 12 | Observations of sky background targets for NICER calibration | CAL | 1 | GENDREAU | KEITH C. | 0 | CAL | CALIBRATION BACKGROUND | 10,000,000,000,000,000 |
U_Cep | 15.57415 | 81.87221 | 123.33771 | 19.009018 | 58,017.231713 | 58,017.236806 | 1,012,070,131 | -1 | 15.57 | 81.875 | 337 | 67,500 | 52 | VALIDATED | 58,181.123947 | 58,181 | 1,012 | Observations of sky background targets for NICER calibration | CAL | 1 | GENDREAU | KEITH C. | 1 | CAL | CALIBRATION BACKGROUND | 10,000,000,000,000,000 |
U_Cep | 15.61855 | 81.87227 | 123.34434 | 19.00936 | 57,942.013889 | 57,942.017616 | 12,070,113 | -1 | 15.57 | 81.875 | 245 | 0 | 52 | VALIDATED | 58,180.091551 | 58,181 | 12 | Observations of sky background targets for NICER calibration | CAL | 1 | GENDREAU | KEITH C. | 0 | CAL | CALIBRATION BACKGROUND | 10,000,000,000,000,000 |
U_Cep | 15.55872 | 81.87273 | 123.335381 | 19.009441 | 57,957.048704 | 57,957.956586 | 1,012,070,105 | -1 | 15.57 | 81.875 | 7,879 | 67,500 | 52 | VALIDATED | 58,181.070833 | 58,181 | 1,012 | Observations of sky background targets for NICER calibration | CAL | 1 | GENDREAU | KEITH C. | 1 | CAL | CALIBRATION BACKGROUND | 10,000,000,000,000,000 |
U_Cep | 15.58243 | 81.87283 | 123.338918 | 19.00969 | 58,023.093056 | 58,023.733044 | 1,012,070,137 | -1 | 15.57 | 81.875 | 3,432 | 67,500 | 52 | VALIDATED | 58,181.143542 | 58,181 | 1,012 | Observations of sky background targets for NICER calibration | CAL | 1 | GENDREAU | KEITH C. | 1 | CAL | CALIBRATION BACKGROUND | 10,000,000,000,000,000 |
U_Cep | 15.56299 | 81.87356 | 123.33598 | 19.010297 | 57,956.16544 | 57,956.87794 | 1,012,070,104 | -1 | 15.57 | 81.875 | 4,703 | 67,500 | 52 | VALIDATED | 58,181.068912 | 58,181 | 1,012 | Observations of sky background targets for NICER calibration | CAL | 1 | GENDREAU | KEITH C. | 1 | CAL | CALIBRATION BACKGROUND | 10,000,000,000,000,000 |
U_Cep | 15.57035 | 81.8736 | 123.337077 | 19.010383 | 57,954.09478 | 57,954.991944 | 1,012,070,102 | -1 | 15.57 | 81.875 | 1,062 | 67,500 | 52 | VALIDATED | 58,181.067106 | 58,181 | 1,012 | Observations of sky background targets for NICER calibration | CAL | 1 | GENDREAU | KEITH C. | 1 | CAL | CALIBRATION BACKGROUND | 10,000,000,000,000,000 |
U_Cep | 15.56859 | 81.87366 | 123.336812 | 19.010432 | 57,955.124537 | 57,955.127836 | 1,012,070,103 | -1 | 15.57 | 81.875 | 153 | 67,500 | 52 | VALIDATED | 58,181.068021 | 58,181 | 1,012 | Observations of sky background targets for NICER calibration | CAL | 1 | GENDREAU | KEITH C. | 1 | CAL | CALIBRATION BACKGROUND | 10,000,000,000,000,000 |
U_Cep | 15.56986 | 81.87383 | 123.336993 | 19.01061 | 58,022.123264 | 58,022.718449 | 1,012,070,136 | -1 | 15.57 | 81.875 | 5,671 | 67,500 | 52 | VALIDATED | 58,181.140266 | 58,181 | 1,012 | Observations of sky background targets for NICER calibration | CAL | 1 | GENDREAU | KEITH C. | 1 | CAL | CALIBRATION BACKGROUND | 10,000,000,000,000,000 |
S5_0532+82 | 85.91104 | 82.64079 | 130.687222 | 24.771214 | 60,764.013588 | 60,764.987037 | 8,200,750,110 | -1 | 85.911862 | 82.64132 | 0 | 0 | 50 | VALIDATED | 60,774.919745 | 60,778 | 8,200 | Target of Opportunities sponsored by the Principal Investigator | DIR | 9 | GENDREAU | KEITH C. | 8 | DDT_TOO | Director Target of Operations | 10,000,000,000,000,000 |
S5_0532+82 | 85.9157 | 82.64092 | 130.687316 | 24.771818 | 60,756.017523 | 60,756.989329 | 8,200,750,102 | -1 | 85.911862 | 82.64132 | 0 | 0 | 50 | VALIDATED | 60,767.787778 | 60,770 | 8,200 | Target of Opportunities sponsored by the Principal Investigator | DIR | 9 | GENDREAU | KEITH C. | 8 | DDT_TOO | Director Target of Operations | 10,000,000,000,000,000 |
S5_0532+82 | 85.93692 | 82.64095 | 130.688325 | 24.774377 | 60,755.630741 | 60,755.956921 | 8,200,750,101 | -1 | 85.911862 | 82.64132 | 0 | 0 | 50 | VALIDATED | 60,766.159537 | 60,769 | 8,200 | Target of Opportunities sponsored by the Principal Investigator | DIR | 9 | GENDREAU | KEITH C. | 8 | DDT_TOO | Director Target of Operations | 10,000,000,000,000,000 |
S5_0532+82 | 85.91191 | 82.64098 | 130.687068 | 24.771384 | 60,763.04647 | 60,763.955324 | 8,200,750,109 | -1 | 85.911862 | 82.64132 | 0 | 0 | 50 | VALIDATED | 60,774.814375 | 60,777 | 8,200 | Target of Opportunities sponsored by the Principal Investigator | DIR | 9 | GENDREAU | KEITH C. | 8 | DDT_TOO | Director Target of Operations | 10,000,000,000,000,000 |
S5_0532+82 | 85.90981 | 82.64101 | 130.686934 | 24.771142 | 58,666.501806 | 58,666.853241 | 2,200,750,101 | -1 | 85.911862 | 82.64132 | 1,083 | 0 | 50 | VALIDATED | 58,670.618866 | 58,680 | 2,200 | Target of Opportunities sponsored by the Principal Investigator | DIR | 9 | GENDREAU | KEITH C. | 2 | DDT_TOO | Director Target of Operations | 10,000,000,000,000,000 |
S5_0532+82 | 85.90904 | 82.64126 | 130.686638 | 24.771137 | 58,667.477778 | 58,667.497454 | 2,200,750,102 | -1 | 85.911862 | 82.64132 | 73 | 0 | 50 | VALIDATED | 58,671.619838 | 58,681 | 2,200 | Target of Opportunities sponsored by the Principal Investigator | DIR | 9 | GENDREAU | KEITH C. | 2 | DDT_TOO | Director Target of Operations | 10,000,000,000,000,000 |
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