Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet
In order to exhume the buried signatures of “missing planetary caustics” in Korea Microlensing Telescope Network (KMTNet) data, we conducted a systematic anomaly search of the residuals from point-source point-lens fits, based on a modified version of the KMTNet EventFinder algorithm. This search re...
Gespeichert in:
| Veröffentlicht in: | The Astronomical journal 2021-10, Vol.162 (4), p.163 |
|---|---|
| Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext bestellen |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | 4 |
| container_start_page | 163 |
| container_title | The Astronomical journal |
| container_volume | 162 |
| creator | Zang, Weicheng Hwang, Kyu-Ha Udalski, Andrzej Wang, Tianshu Zhu, Wei Sumi, Takahiro Yee, Jennifer C. Gould, Andrew Mao, Shude Zhang, Xiangyu Albrow, Michael D. Chung, Sun-Ju Han, Cheongho Jung, Youn Kil Ryu, Yoon-Hyun Shin, In-Gu Shvartzvald, Yossi Cha, Sang-Mok Kim, Dong-Jin Kim, Hyoun-Woo Kim, Seung-Lee Lee, Chung-Uk Lee, Dong-Joo Lee, Yongseok Park, Byeong-Gon Pogge, Richard W. Mróz, Przemek Skowron, Jan Poleski, Radoslaw Szymański, Michał K. Soszyński, Igor Pietrukowicz, Paweł Kozłowski, Szymon Ulaczyk, Krzysztof Rybicki, Krzysztof A. Iwanek, Patryk Wrona, Marcin Gromadzki, Mariusz Bond, Ian A. Abe, Fumio Barry, Richard Bennett, David P. Bhattacharya, Aparna Donachie, Martin Fujii, Hirosane Fukui, Akihiko Hirao, Yuki Itow, Yoshitaka Kirikawa, Rintaro Kondo, Iona Koshimoto, Naoki Li, Man Cheung Alex Matsubara, Yutaka Muraki, Yasushi Miyazaki, Shota Olmschenk, Greg Ranc, Clément Rattenbury, Nicholas J. Satoh, Yuki Shoji, Hikaru Ishitani Silva, Stela Suzuki, Daisuke Tanaka, Yuzuru Tristram, Paul J. Yamawaki, Tsubasa Yonehara, Atsunori Beichman, Charles A. Bryden, Geoffery Calchi Novati, Sebastiano Carey, Sean Gaudi, B. Scott Henderson, Calen B. Johnson, Samson |
| description | In order to exhume the buried signatures of “missing planetary caustics” in Korea Microlensing Telescope Network (KMTNet) data, we conducted a systematic anomaly search of the residuals from point-source point-lens fits, based on a modified version of the KMTNet EventFinder algorithm. This search revealed the lowest-mass-ratio planetary caustic to date in the microlensing event OGLE-2019-BLG-1053, for which the planetary signal had not been noticed before. The planetary system has a planet–host mass ratio of
q
= (1.25 ± 0.13) × 10
−5
. A Bayesian analysis yielded estimates of the mass of the host star,
M
host
=
0.61
−
0.24
+
0.29
M
⊙
, the mass of its planet,
M
planet
=
2.48
−
0.98
+
1.19
M
⊕
, the projected planet–host separation,
a
⊥
=
3.4
−
0.5
+
0.5
au, and the lens distance,
D
L
=
6.8
−
0.9
+
0.6
kpc. The discovery of this very-low-mass-ratio planet illustrates the utility of our method and opens a new window for a large and homogeneous sample to study the microlensing planet–host mass ratio function down to
q
∼ 10
−5
. |
| doi_str_mv | 10.3847/1538-3881/ac12d4 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_iop_journals_10_3847_1538_3881_ac12d4</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2577067947</sourcerecordid><originalsourceid>FETCH-LOGICAL-c444t-6ebb086b3a03e91a34911bd1b6f22fc72e4140b2691b2502656f6af9b55c3d863</originalsourceid><addsrcrecordid>eNp1kM9PwjAYhhujiYjePTbxyqC_1x2BIBKnmIDn2nZdGIEN23Lgv3dkRE-evuTL87558wDwiNGQSpaOMKcyoVLikbaYFOwK9H5f16CHEGKJIFzcgrsQtghhLBHrga_VKUS317Gy8PVt_e4i_Njp2kXtT3BcN3u9O8GV095uhnAxhMt5PksIwlkyyecJRpzmZgA1nBx95Qq4dt67EH2ld5eee3BT6l1wD5fbB5_Ps_X0JcmX88V0nCeWMRYT4YxBUhiqEXUZ1pRlGJsCG1ESUtqUOIYZMkRk2BCOiOCiFLrMDOeWFlLQPnjqepsQKxVsFZ3d2KaunY2KUMwzKskfdfDN97FdqrbN0dftMEV4miKRZixtKdRR1jcheFeqg6_2rRGFkTrbVme16qxWdbbbyKCLVM3hr_Nf_AdDYnuJ</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2577067947</pqid></control><display><type>article</type><title>Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet</title><source>IOP Publishing Free Content</source><creator>Zang, Weicheng ; Hwang, Kyu-Ha ; Udalski, Andrzej ; Wang, Tianshu ; Zhu, Wei ; Sumi, Takahiro ; Yee, Jennifer C. ; Gould, Andrew ; Mao, Shude ; Zhang, Xiangyu ; Albrow, Michael D. ; Chung, Sun-Ju ; Han, Cheongho ; Jung, Youn Kil ; Ryu, Yoon-Hyun ; Shin, In-Gu ; Shvartzvald, Yossi ; Cha, Sang-Mok ; Kim, Dong-Jin ; Kim, Hyoun-Woo ; Kim, Seung-Lee ; Lee, Chung-Uk ; Lee, Dong-Joo ; Lee, Yongseok ; Park, Byeong-Gon ; Pogge, Richard W. ; Mróz, Przemek ; Skowron, Jan ; Poleski, Radoslaw ; Szymański, Michał K. ; Soszyński, Igor ; Pietrukowicz, Paweł ; Kozłowski, Szymon ; Ulaczyk, Krzysztof ; Rybicki, Krzysztof A. ; Iwanek, Patryk ; Wrona, Marcin ; Gromadzki, Mariusz ; Bond, Ian A. ; Abe, Fumio ; Barry, Richard ; Bennett, David P. ; Bhattacharya, Aparna ; Donachie, Martin ; Fujii, Hirosane ; Fukui, Akihiko ; Hirao, Yuki ; Itow, Yoshitaka ; Kirikawa, Rintaro ; Kondo, Iona ; Koshimoto, Naoki ; Li, Man Cheung Alex ; Matsubara, Yutaka ; Muraki, Yasushi ; Miyazaki, Shota ; Olmschenk, Greg ; Ranc, Clément ; Rattenbury, Nicholas J. ; Satoh, Yuki ; Shoji, Hikaru ; Ishitani Silva, Stela ; Suzuki, Daisuke ; Tanaka, Yuzuru ; Tristram, Paul J. ; Yamawaki, Tsubasa ; Yonehara, Atsunori ; Beichman, Charles A. ; Bryden, Geoffery ; Calchi Novati, Sebastiano ; Carey, Sean ; Gaudi, B. Scott ; Henderson, Calen B. ; Johnson, Samson</creator><creatorcontrib>Zang, Weicheng ; Hwang, Kyu-Ha ; Udalski, Andrzej ; Wang, Tianshu ; Zhu, Wei ; Sumi, Takahiro ; Yee, Jennifer C. ; Gould, Andrew ; Mao, Shude ; Zhang, Xiangyu ; Albrow, Michael D. ; Chung, Sun-Ju ; Han, Cheongho ; Jung, Youn Kil ; Ryu, Yoon-Hyun ; Shin, In-Gu ; Shvartzvald, Yossi ; Cha, Sang-Mok ; Kim, Dong-Jin ; Kim, Hyoun-Woo ; Kim, Seung-Lee ; Lee, Chung-Uk ; Lee, Dong-Joo ; Lee, Yongseok ; Park, Byeong-Gon ; Pogge, Richard W. ; Mróz, Przemek ; Skowron, Jan ; Poleski, Radoslaw ; Szymański, Michał K. ; Soszyński, Igor ; Pietrukowicz, Paweł ; Kozłowski, Szymon ; Ulaczyk, Krzysztof ; Rybicki, Krzysztof A. ; Iwanek, Patryk ; Wrona, Marcin ; Gromadzki, Mariusz ; Bond, Ian A. ; Abe, Fumio ; Barry, Richard ; Bennett, David P. ; Bhattacharya, Aparna ; Donachie, Martin ; Fujii, Hirosane ; Fukui, Akihiko ; Hirao, Yuki ; Itow, Yoshitaka ; Kirikawa, Rintaro ; Kondo, Iona ; Koshimoto, Naoki ; Li, Man Cheung Alex ; Matsubara, Yutaka ; Muraki, Yasushi ; Miyazaki, Shota ; Olmschenk, Greg ; Ranc, Clément ; Rattenbury, Nicholas J. ; Satoh, Yuki ; Shoji, Hikaru ; Ishitani Silva, Stela ; Suzuki, Daisuke ; Tanaka, Yuzuru ; Tristram, Paul J. ; Yamawaki, Tsubasa ; Yonehara, Atsunori ; Beichman, Charles A. ; Bryden, Geoffery ; Calchi Novati, Sebastiano ; Carey, Sean ; Gaudi, B. Scott ; Henderson, Calen B. ; Johnson, Samson ; The Spitzer Team ; The OGLE Collaboration ; Leading Authors ; The MOA Collaboration ; The KMTNet Collaboration</creatorcontrib><description>In order to exhume the buried signatures of “missing planetary caustics” in Korea Microlensing Telescope Network (KMTNet) data, we conducted a systematic anomaly search of the residuals from point-source point-lens fits, based on a modified version of the KMTNet EventFinder algorithm. This search revealed the lowest-mass-ratio planetary caustic to date in the microlensing event OGLE-2019-BLG-1053, for which the planetary signal had not been noticed before. The planetary system has a planet–host mass ratio of
q
= (1.25 ± 0.13) × 10
−5
. A Bayesian analysis yielded estimates of the mass of the host star,
M
host
=
0.61
−
0.24
+
0.29
M
⊙
, the mass of its planet,
M
planet
=
2.48
−
0.98
+
1.19
M
⊕
, the projected planet–host separation,
a
⊥
=
3.4
−
0.5
+
0.5
au, and the lens distance,
D
L
=
6.8
−
0.9
+
0.6
kpc. The discovery of this very-low-mass-ratio planet illustrates the utility of our method and opens a new window for a large and homogeneous sample to study the microlensing planet–host mass ratio function down to
q
∼ 10
−5
.</description><identifier>ISSN: 0004-6256</identifier><identifier>ISSN: 1538-3881</identifier><identifier>EISSN: 1538-3881</identifier><identifier>DOI: 10.3847/1538-3881/ac12d4</identifier><language>eng</language><publisher>Madison: The American Astronomical Society</publisher><subject>ALGORITHMS ; Astronomy ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; Bayesian analysis ; Exoplanet detection methods ; Gravitational microlensing exoplanet detection ; Lenses ; Microlenses ; OTHER INSTRUMENTATION ; Planetary systems ; PLANETS ; POINT SOURCES ; Searching ; SIGNALS ; STARS ; TELESCOPES ; Terrestrial environments ; Terrestrial planets</subject><ispartof>The Astronomical journal, 2021-10, Vol.162 (4), p.163</ispartof><rights>2021. The American Astronomical Society. All rights reserved.</rights><rights>Copyright IOP Publishing Oct 2021</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c444t-6ebb086b3a03e91a34911bd1b6f22fc72e4140b2691b2502656f6af9b55c3d863</citedby><cites>FETCH-LOGICAL-c444t-6ebb086b3a03e91a34911bd1b6f22fc72e4140b2691b2502656f6af9b55c3d863</cites><orcidid>0000-0002-4035-5012 ; 0000-0003-4084-880X ; 0000-0002-4909-5763 ; 0000-0002-7669-1069 ; 0000-0001-7016-1692 ; 0000-0001-9818-1513 ; 0000-0003-4776-8618 ; 0000-0001-6364-408X ; 0000-0002-0548-8995 ; 0000-0003-3316-4012 ; 0000-0002-9245-6368 ; 0000-0003-1435-3053 ; 0000-0003-0395-9869 ; 0000-0001-5207-5619 ; 0000-0003-1525-5041 ; 0000-0001-8263-1006 ; 0000-0002-3401-1029 ; 0000-0003-0043-3925 ; 0000-0002-1650-1518 ; 0000-0001-8317-2788 ; 0000-0002-2641-9964 ; 0000-0001-9397-4768 ; 0000-0001-8877-9060 ; 0000-0001-6000-3463 ; 0000-0001-8043-8413 ; 0000-0003-2388-4534 ; 0000-0002-6982-7722 ; 0000-0001-9823-2907 ; 0000-0002-9241-4117 ; 0000-0001-5966-837X ; 0000-0001-5069-319X ; 0000-0002-0314-6000 ; 0000-0002-6212-7221 ; 0000-0001-9481-7123 ; 0000-0002-5843-9433 ; 0000-0003-4027-4711 ; 0000-0003-4916-0892 ; 0000-0001-6285-4528 ; 0000-0002-2339-5899 ; 0000-0003-2302-9562 ; 0000-0003-0562-5643 ; 0000-0002-4355-9838 ; 0000-0002-3051-274X ; 0000-0002-8198-1968 ; 0000-0001-8472-2219 ; 0000-0002-7777-0842 ; 0000-0002-0221-6871 ; 0000-0003-1978-2092 ; 0000-0002-2335-1730</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/1538-3881/ac12d4/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>230,314,776,780,881,27901,27902,38845,38867,53815,53842</link.rule.ids><linktorsrc>$$Uhttps://iopscience.iop.org/article/10.3847/1538-3881/ac12d4$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttps://www.osti.gov/biblio/23159382$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Zang, Weicheng</creatorcontrib><creatorcontrib>Hwang, Kyu-Ha</creatorcontrib><creatorcontrib>Udalski, Andrzej</creatorcontrib><creatorcontrib>Wang, Tianshu</creatorcontrib><creatorcontrib>Zhu, Wei</creatorcontrib><creatorcontrib>Sumi, Takahiro</creatorcontrib><creatorcontrib>Yee, Jennifer C.</creatorcontrib><creatorcontrib>Gould, Andrew</creatorcontrib><creatorcontrib>Mao, Shude</creatorcontrib><creatorcontrib>Zhang, Xiangyu</creatorcontrib><creatorcontrib>Albrow, Michael D.</creatorcontrib><creatorcontrib>Chung, Sun-Ju</creatorcontrib><creatorcontrib>Han, Cheongho</creatorcontrib><creatorcontrib>Jung, Youn Kil</creatorcontrib><creatorcontrib>Ryu, Yoon-Hyun</creatorcontrib><creatorcontrib>Shin, In-Gu</creatorcontrib><creatorcontrib>Shvartzvald, Yossi</creatorcontrib><creatorcontrib>Cha, Sang-Mok</creatorcontrib><creatorcontrib>Kim, Dong-Jin</creatorcontrib><creatorcontrib>Kim, Hyoun-Woo</creatorcontrib><creatorcontrib>Kim, Seung-Lee</creatorcontrib><creatorcontrib>Lee, Chung-Uk</creatorcontrib><creatorcontrib>Lee, Dong-Joo</creatorcontrib><creatorcontrib>Lee, Yongseok</creatorcontrib><creatorcontrib>Park, Byeong-Gon</creatorcontrib><creatorcontrib>Pogge, Richard W.</creatorcontrib><creatorcontrib>Mróz, Przemek</creatorcontrib><creatorcontrib>Skowron, Jan</creatorcontrib><creatorcontrib>Poleski, Radoslaw</creatorcontrib><creatorcontrib>Szymański, Michał K.</creatorcontrib><creatorcontrib>Soszyński, Igor</creatorcontrib><creatorcontrib>Pietrukowicz, Paweł</creatorcontrib><creatorcontrib>Kozłowski, Szymon</creatorcontrib><creatorcontrib>Ulaczyk, Krzysztof</creatorcontrib><creatorcontrib>Rybicki, Krzysztof A.</creatorcontrib><creatorcontrib>Iwanek, Patryk</creatorcontrib><creatorcontrib>Wrona, Marcin</creatorcontrib><creatorcontrib>Gromadzki, Mariusz</creatorcontrib><creatorcontrib>Bond, Ian A.</creatorcontrib><creatorcontrib>Abe, Fumio</creatorcontrib><creatorcontrib>Barry, Richard</creatorcontrib><creatorcontrib>Bennett, David P.</creatorcontrib><creatorcontrib>Bhattacharya, Aparna</creatorcontrib><creatorcontrib>Donachie, Martin</creatorcontrib><creatorcontrib>Fujii, Hirosane</creatorcontrib><creatorcontrib>Fukui, Akihiko</creatorcontrib><creatorcontrib>Hirao, Yuki</creatorcontrib><creatorcontrib>Itow, Yoshitaka</creatorcontrib><creatorcontrib>Kirikawa, Rintaro</creatorcontrib><creatorcontrib>Kondo, Iona</creatorcontrib><creatorcontrib>Koshimoto, Naoki</creatorcontrib><creatorcontrib>Li, Man Cheung Alex</creatorcontrib><creatorcontrib>Matsubara, Yutaka</creatorcontrib><creatorcontrib>Muraki, Yasushi</creatorcontrib><creatorcontrib>Miyazaki, Shota</creatorcontrib><creatorcontrib>Olmschenk, Greg</creatorcontrib><creatorcontrib>Ranc, Clément</creatorcontrib><creatorcontrib>Rattenbury, Nicholas J.</creatorcontrib><creatorcontrib>Satoh, Yuki</creatorcontrib><creatorcontrib>Shoji, Hikaru</creatorcontrib><creatorcontrib>Ishitani Silva, Stela</creatorcontrib><creatorcontrib>Suzuki, Daisuke</creatorcontrib><creatorcontrib>Tanaka, Yuzuru</creatorcontrib><creatorcontrib>Tristram, Paul J.</creatorcontrib><creatorcontrib>Yamawaki, Tsubasa</creatorcontrib><creatorcontrib>Yonehara, Atsunori</creatorcontrib><creatorcontrib>Beichman, Charles A.</creatorcontrib><creatorcontrib>Bryden, Geoffery</creatorcontrib><creatorcontrib>Calchi Novati, Sebastiano</creatorcontrib><creatorcontrib>Carey, Sean</creatorcontrib><creatorcontrib>Gaudi, B. Scott</creatorcontrib><creatorcontrib>Henderson, Calen B.</creatorcontrib><creatorcontrib>Johnson, Samson</creatorcontrib><creatorcontrib>The Spitzer Team</creatorcontrib><creatorcontrib>The OGLE Collaboration</creatorcontrib><creatorcontrib>Leading Authors</creatorcontrib><creatorcontrib>The MOA Collaboration</creatorcontrib><creatorcontrib>The KMTNet Collaboration</creatorcontrib><title>Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet</title><title>The Astronomical journal</title><addtitle>AJ</addtitle><addtitle>Astron. J</addtitle><description>In order to exhume the buried signatures of “missing planetary caustics” in Korea Microlensing Telescope Network (KMTNet) data, we conducted a systematic anomaly search of the residuals from point-source point-lens fits, based on a modified version of the KMTNet EventFinder algorithm. This search revealed the lowest-mass-ratio planetary caustic to date in the microlensing event OGLE-2019-BLG-1053, for which the planetary signal had not been noticed before. The planetary system has a planet–host mass ratio of
q
= (1.25 ± 0.13) × 10
−5
. A Bayesian analysis yielded estimates of the mass of the host star,
M
host
=
0.61
−
0.24
+
0.29
M
⊙
, the mass of its planet,
M
planet
=
2.48
−
0.98
+
1.19
M
⊕
, the projected planet–host separation,
a
⊥
=
3.4
−
0.5
+
0.5
au, and the lens distance,
D
L
=
6.8
−
0.9
+
0.6
kpc. The discovery of this very-low-mass-ratio planet illustrates the utility of our method and opens a new window for a large and homogeneous sample to study the microlensing planet–host mass ratio function down to
q
∼ 10
−5
.</description><subject>ALGORITHMS</subject><subject>Astronomy</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>Bayesian analysis</subject><subject>Exoplanet detection methods</subject><subject>Gravitational microlensing exoplanet detection</subject><subject>Lenses</subject><subject>Microlenses</subject><subject>OTHER INSTRUMENTATION</subject><subject>Planetary systems</subject><subject>PLANETS</subject><subject>POINT SOURCES</subject><subject>Searching</subject><subject>SIGNALS</subject><subject>STARS</subject><subject>TELESCOPES</subject><subject>Terrestrial environments</subject><subject>Terrestrial planets</subject><issn>0004-6256</issn><issn>1538-3881</issn><issn>1538-3881</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNp1kM9PwjAYhhujiYjePTbxyqC_1x2BIBKnmIDn2nZdGIEN23Lgv3dkRE-evuTL87558wDwiNGQSpaOMKcyoVLikbaYFOwK9H5f16CHEGKJIFzcgrsQtghhLBHrga_VKUS317Gy8PVt_e4i_Njp2kXtT3BcN3u9O8GV095uhnAxhMt5PksIwlkyyecJRpzmZgA1nBx95Qq4dt67EH2ld5eee3BT6l1wD5fbB5_Ps_X0JcmX88V0nCeWMRYT4YxBUhiqEXUZ1pRlGJsCG1ESUtqUOIYZMkRk2BCOiOCiFLrMDOeWFlLQPnjqepsQKxVsFZ3d2KaunY2KUMwzKskfdfDN97FdqrbN0dftMEV4miKRZixtKdRR1jcheFeqg6_2rRGFkTrbVme16qxWdbbbyKCLVM3hr_Nf_AdDYnuJ</recordid><startdate>20211001</startdate><enddate>20211001</enddate><creator>Zang, Weicheng</creator><creator>Hwang, Kyu-Ha</creator><creator>Udalski, Andrzej</creator><creator>Wang, Tianshu</creator><creator>Zhu, Wei</creator><creator>Sumi, Takahiro</creator><creator>Yee, Jennifer C.</creator><creator>Gould, Andrew</creator><creator>Mao, Shude</creator><creator>Zhang, Xiangyu</creator><creator>Albrow, Michael D.</creator><creator>Chung, Sun-Ju</creator><creator>Han, Cheongho</creator><creator>Jung, Youn Kil</creator><creator>Ryu, Yoon-Hyun</creator><creator>Shin, In-Gu</creator><creator>Shvartzvald, Yossi</creator><creator>Cha, Sang-Mok</creator><creator>Kim, Dong-Jin</creator><creator>Kim, Hyoun-Woo</creator><creator>Kim, Seung-Lee</creator><creator>Lee, Chung-Uk</creator><creator>Lee, Dong-Joo</creator><creator>Lee, Yongseok</creator><creator>Park, Byeong-Gon</creator><creator>Pogge, Richard W.</creator><creator>Mróz, Przemek</creator><creator>Skowron, Jan</creator><creator>Poleski, Radoslaw</creator><creator>Szymański, Michał K.</creator><creator>Soszyński, Igor</creator><creator>Pietrukowicz, Paweł</creator><creator>Kozłowski, Szymon</creator><creator>Ulaczyk, Krzysztof</creator><creator>Rybicki, Krzysztof A.</creator><creator>Iwanek, Patryk</creator><creator>Wrona, Marcin</creator><creator>Gromadzki, Mariusz</creator><creator>Bond, Ian A.</creator><creator>Abe, Fumio</creator><creator>Barry, Richard</creator><creator>Bennett, David P.</creator><creator>Bhattacharya, Aparna</creator><creator>Donachie, Martin</creator><creator>Fujii, Hirosane</creator><creator>Fukui, Akihiko</creator><creator>Hirao, Yuki</creator><creator>Itow, Yoshitaka</creator><creator>Kirikawa, Rintaro</creator><creator>Kondo, Iona</creator><creator>Koshimoto, Naoki</creator><creator>Li, Man Cheung Alex</creator><creator>Matsubara, Yutaka</creator><creator>Muraki, Yasushi</creator><creator>Miyazaki, Shota</creator><creator>Olmschenk, Greg</creator><creator>Ranc, Clément</creator><creator>Rattenbury, Nicholas J.</creator><creator>Satoh, Yuki</creator><creator>Shoji, Hikaru</creator><creator>Ishitani Silva, Stela</creator><creator>Suzuki, Daisuke</creator><creator>Tanaka, Yuzuru</creator><creator>Tristram, Paul J.</creator><creator>Yamawaki, Tsubasa</creator><creator>Yonehara, Atsunori</creator><creator>Beichman, Charles A.</creator><creator>Bryden, Geoffery</creator><creator>Calchi Novati, Sebastiano</creator><creator>Carey, Sean</creator><creator>Gaudi, B. Scott</creator><creator>Henderson, Calen B.</creator><creator>Johnson, Samson</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0002-4035-5012</orcidid><orcidid>https://orcid.org/0000-0003-4084-880X</orcidid><orcidid>https://orcid.org/0000-0002-4909-5763</orcidid><orcidid>https://orcid.org/0000-0002-7669-1069</orcidid><orcidid>https://orcid.org/0000-0001-7016-1692</orcidid><orcidid>https://orcid.org/0000-0001-9818-1513</orcidid><orcidid>https://orcid.org/0000-0003-4776-8618</orcidid><orcidid>https://orcid.org/0000-0001-6364-408X</orcidid><orcidid>https://orcid.org/0000-0002-0548-8995</orcidid><orcidid>https://orcid.org/0000-0003-3316-4012</orcidid><orcidid>https://orcid.org/0000-0002-9245-6368</orcidid><orcidid>https://orcid.org/0000-0003-1435-3053</orcidid><orcidid>https://orcid.org/0000-0003-0395-9869</orcidid><orcidid>https://orcid.org/0000-0001-5207-5619</orcidid><orcidid>https://orcid.org/0000-0003-1525-5041</orcidid><orcidid>https://orcid.org/0000-0001-8263-1006</orcidid><orcidid>https://orcid.org/0000-0002-3401-1029</orcidid><orcidid>https://orcid.org/0000-0003-0043-3925</orcidid><orcidid>https://orcid.org/0000-0002-1650-1518</orcidid><orcidid>https://orcid.org/0000-0001-8317-2788</orcidid><orcidid>https://orcid.org/0000-0002-2641-9964</orcidid><orcidid>https://orcid.org/0000-0001-9397-4768</orcidid><orcidid>https://orcid.org/0000-0001-8877-9060</orcidid><orcidid>https://orcid.org/0000-0001-6000-3463</orcidid><orcidid>https://orcid.org/0000-0001-8043-8413</orcidid><orcidid>https://orcid.org/0000-0003-2388-4534</orcidid><orcidid>https://orcid.org/0000-0002-6982-7722</orcidid><orcidid>https://orcid.org/0000-0001-9823-2907</orcidid><orcidid>https://orcid.org/0000-0002-9241-4117</orcidid><orcidid>https://orcid.org/0000-0001-5966-837X</orcidid><orcidid>https://orcid.org/0000-0001-5069-319X</orcidid><orcidid>https://orcid.org/0000-0002-0314-6000</orcidid><orcidid>https://orcid.org/0000-0002-6212-7221</orcidid><orcidid>https://orcid.org/0000-0001-9481-7123</orcidid><orcidid>https://orcid.org/0000-0002-5843-9433</orcidid><orcidid>https://orcid.org/0000-0003-4027-4711</orcidid><orcidid>https://orcid.org/0000-0003-4916-0892</orcidid><orcidid>https://orcid.org/0000-0001-6285-4528</orcidid><orcidid>https://orcid.org/0000-0002-2339-5899</orcidid><orcidid>https://orcid.org/0000-0003-2302-9562</orcidid><orcidid>https://orcid.org/0000-0003-0562-5643</orcidid><orcidid>https://orcid.org/0000-0002-4355-9838</orcidid><orcidid>https://orcid.org/0000-0002-3051-274X</orcidid><orcidid>https://orcid.org/0000-0002-8198-1968</orcidid><orcidid>https://orcid.org/0000-0001-8472-2219</orcidid><orcidid>https://orcid.org/0000-0002-7777-0842</orcidid><orcidid>https://orcid.org/0000-0002-0221-6871</orcidid><orcidid>https://orcid.org/0000-0003-1978-2092</orcidid><orcidid>https://orcid.org/0000-0002-2335-1730</orcidid></search><sort><creationdate>20211001</creationdate><title>Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet</title><author>Zang, Weicheng ; Hwang, Kyu-Ha ; Udalski, Andrzej ; Wang, Tianshu ; Zhu, Wei ; Sumi, Takahiro ; Yee, Jennifer C. ; Gould, Andrew ; Mao, Shude ; Zhang, Xiangyu ; Albrow, Michael D. ; Chung, Sun-Ju ; Han, Cheongho ; Jung, Youn Kil ; Ryu, Yoon-Hyun ; Shin, In-Gu ; Shvartzvald, Yossi ; Cha, Sang-Mok ; Kim, Dong-Jin ; Kim, Hyoun-Woo ; Kim, Seung-Lee ; Lee, Chung-Uk ; Lee, Dong-Joo ; Lee, Yongseok ; Park, Byeong-Gon ; Pogge, Richard W. ; Mróz, Przemek ; Skowron, Jan ; Poleski, Radoslaw ; Szymański, Michał K. ; Soszyński, Igor ; Pietrukowicz, Paweł ; Kozłowski, Szymon ; Ulaczyk, Krzysztof ; Rybicki, Krzysztof A. ; Iwanek, Patryk ; Wrona, Marcin ; Gromadzki, Mariusz ; Bond, Ian A. ; Abe, Fumio ; Barry, Richard ; Bennett, David P. ; Bhattacharya, Aparna ; Donachie, Martin ; Fujii, Hirosane ; Fukui, Akihiko ; Hirao, Yuki ; Itow, Yoshitaka ; Kirikawa, Rintaro ; Kondo, Iona ; Koshimoto, Naoki ; Li, Man Cheung Alex ; Matsubara, Yutaka ; Muraki, Yasushi ; Miyazaki, Shota ; Olmschenk, Greg ; Ranc, Clément ; Rattenbury, Nicholas J. ; Satoh, Yuki ; Shoji, Hikaru ; Ishitani Silva, Stela ; Suzuki, Daisuke ; Tanaka, Yuzuru ; Tristram, Paul J. ; Yamawaki, Tsubasa ; Yonehara, Atsunori ; Beichman, Charles A. ; Bryden, Geoffery ; Calchi Novati, Sebastiano ; Carey, Sean ; Gaudi, B. Scott ; Henderson, Calen B. ; Johnson, Samson</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c444t-6ebb086b3a03e91a34911bd1b6f22fc72e4140b2691b2502656f6af9b55c3d863</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>ALGORITHMS</topic><topic>Astronomy</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>Bayesian analysis</topic><topic>Exoplanet detection methods</topic><topic>Gravitational microlensing exoplanet detection</topic><topic>Lenses</topic><topic>Microlenses</topic><topic>OTHER INSTRUMENTATION</topic><topic>Planetary systems</topic><topic>PLANETS</topic><topic>POINT SOURCES</topic><topic>Searching</topic><topic>SIGNALS</topic><topic>STARS</topic><topic>TELESCOPES</topic><topic>Terrestrial environments</topic><topic>Terrestrial planets</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zang, Weicheng</creatorcontrib><creatorcontrib>Hwang, Kyu-Ha</creatorcontrib><creatorcontrib>Udalski, Andrzej</creatorcontrib><creatorcontrib>Wang, Tianshu</creatorcontrib><creatorcontrib>Zhu, Wei</creatorcontrib><creatorcontrib>Sumi, Takahiro</creatorcontrib><creatorcontrib>Yee, Jennifer C.</creatorcontrib><creatorcontrib>Gould, Andrew</creatorcontrib><creatorcontrib>Mao, Shude</creatorcontrib><creatorcontrib>Zhang, Xiangyu</creatorcontrib><creatorcontrib>Albrow, Michael D.</creatorcontrib><creatorcontrib>Chung, Sun-Ju</creatorcontrib><creatorcontrib>Han, Cheongho</creatorcontrib><creatorcontrib>Jung, Youn Kil</creatorcontrib><creatorcontrib>Ryu, Yoon-Hyun</creatorcontrib><creatorcontrib>Shin, In-Gu</creatorcontrib><creatorcontrib>Shvartzvald, Yossi</creatorcontrib><creatorcontrib>Cha, Sang-Mok</creatorcontrib><creatorcontrib>Kim, Dong-Jin</creatorcontrib><creatorcontrib>Kim, Hyoun-Woo</creatorcontrib><creatorcontrib>Kim, Seung-Lee</creatorcontrib><creatorcontrib>Lee, Chung-Uk</creatorcontrib><creatorcontrib>Lee, Dong-Joo</creatorcontrib><creatorcontrib>Lee, Yongseok</creatorcontrib><creatorcontrib>Park, Byeong-Gon</creatorcontrib><creatorcontrib>Pogge, Richard W.</creatorcontrib><creatorcontrib>Mróz, Przemek</creatorcontrib><creatorcontrib>Skowron, Jan</creatorcontrib><creatorcontrib>Poleski, Radoslaw</creatorcontrib><creatorcontrib>Szymański, Michał K.</creatorcontrib><creatorcontrib>Soszyński, Igor</creatorcontrib><creatorcontrib>Pietrukowicz, Paweł</creatorcontrib><creatorcontrib>Kozłowski, Szymon</creatorcontrib><creatorcontrib>Ulaczyk, Krzysztof</creatorcontrib><creatorcontrib>Rybicki, Krzysztof A.</creatorcontrib><creatorcontrib>Iwanek, Patryk</creatorcontrib><creatorcontrib>Wrona, Marcin</creatorcontrib><creatorcontrib>Gromadzki, Mariusz</creatorcontrib><creatorcontrib>Bond, Ian A.</creatorcontrib><creatorcontrib>Abe, Fumio</creatorcontrib><creatorcontrib>Barry, Richard</creatorcontrib><creatorcontrib>Bennett, David P.</creatorcontrib><creatorcontrib>Bhattacharya, Aparna</creatorcontrib><creatorcontrib>Donachie, Martin</creatorcontrib><creatorcontrib>Fujii, Hirosane</creatorcontrib><creatorcontrib>Fukui, Akihiko</creatorcontrib><creatorcontrib>Hirao, Yuki</creatorcontrib><creatorcontrib>Itow, Yoshitaka</creatorcontrib><creatorcontrib>Kirikawa, Rintaro</creatorcontrib><creatorcontrib>Kondo, Iona</creatorcontrib><creatorcontrib>Koshimoto, Naoki</creatorcontrib><creatorcontrib>Li, Man Cheung Alex</creatorcontrib><creatorcontrib>Matsubara, Yutaka</creatorcontrib><creatorcontrib>Muraki, Yasushi</creatorcontrib><creatorcontrib>Miyazaki, Shota</creatorcontrib><creatorcontrib>Olmschenk, Greg</creatorcontrib><creatorcontrib>Ranc, Clément</creatorcontrib><creatorcontrib>Rattenbury, Nicholas J.</creatorcontrib><creatorcontrib>Satoh, Yuki</creatorcontrib><creatorcontrib>Shoji, Hikaru</creatorcontrib><creatorcontrib>Ishitani Silva, Stela</creatorcontrib><creatorcontrib>Suzuki, Daisuke</creatorcontrib><creatorcontrib>Tanaka, Yuzuru</creatorcontrib><creatorcontrib>Tristram, Paul J.</creatorcontrib><creatorcontrib>Yamawaki, Tsubasa</creatorcontrib><creatorcontrib>Yonehara, Atsunori</creatorcontrib><creatorcontrib>Beichman, Charles A.</creatorcontrib><creatorcontrib>Bryden, Geoffery</creatorcontrib><creatorcontrib>Calchi Novati, Sebastiano</creatorcontrib><creatorcontrib>Carey, Sean</creatorcontrib><creatorcontrib>Gaudi, B. Scott</creatorcontrib><creatorcontrib>Henderson, Calen B.</creatorcontrib><creatorcontrib>Johnson, Samson</creatorcontrib><creatorcontrib>The Spitzer Team</creatorcontrib><creatorcontrib>The OGLE Collaboration</creatorcontrib><creatorcontrib>Leading Authors</creatorcontrib><creatorcontrib>The MOA Collaboration</creatorcontrib><creatorcontrib>The KMTNet Collaboration</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>The Astronomical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Zang, Weicheng</au><au>Hwang, Kyu-Ha</au><au>Udalski, Andrzej</au><au>Wang, Tianshu</au><au>Zhu, Wei</au><au>Sumi, Takahiro</au><au>Yee, Jennifer C.</au><au>Gould, Andrew</au><au>Mao, Shude</au><au>Zhang, Xiangyu</au><au>Albrow, Michael D.</au><au>Chung, Sun-Ju</au><au>Han, Cheongho</au><au>Jung, Youn Kil</au><au>Ryu, Yoon-Hyun</au><au>Shin, In-Gu</au><au>Shvartzvald, Yossi</au><au>Cha, Sang-Mok</au><au>Kim, Dong-Jin</au><au>Kim, Hyoun-Woo</au><au>Kim, Seung-Lee</au><au>Lee, Chung-Uk</au><au>Lee, Dong-Joo</au><au>Lee, Yongseok</au><au>Park, Byeong-Gon</au><au>Pogge, Richard W.</au><au>Mróz, Przemek</au><au>Skowron, Jan</au><au>Poleski, Radoslaw</au><au>Szymański, Michał K.</au><au>Soszyński, Igor</au><au>Pietrukowicz, Paweł</au><au>Kozłowski, Szymon</au><au>Ulaczyk, Krzysztof</au><au>Rybicki, Krzysztof A.</au><au>Iwanek, Patryk</au><au>Wrona, Marcin</au><au>Gromadzki, Mariusz</au><au>Bond, Ian A.</au><au>Abe, Fumio</au><au>Barry, Richard</au><au>Bennett, David P.</au><au>Bhattacharya, Aparna</au><au>Donachie, Martin</au><au>Fujii, Hirosane</au><au>Fukui, Akihiko</au><au>Hirao, Yuki</au><au>Itow, Yoshitaka</au><au>Kirikawa, Rintaro</au><au>Kondo, Iona</au><au>Koshimoto, Naoki</au><au>Li, Man Cheung Alex</au><au>Matsubara, Yutaka</au><au>Muraki, Yasushi</au><au>Miyazaki, Shota</au><au>Olmschenk, Greg</au><au>Ranc, Clément</au><au>Rattenbury, Nicholas J.</au><au>Satoh, Yuki</au><au>Shoji, Hikaru</au><au>Ishitani Silva, Stela</au><au>Suzuki, Daisuke</au><au>Tanaka, Yuzuru</au><au>Tristram, Paul J.</au><au>Yamawaki, Tsubasa</au><au>Yonehara, Atsunori</au><au>Beichman, Charles A.</au><au>Bryden, Geoffery</au><au>Calchi Novati, Sebastiano</au><au>Carey, Sean</au><au>Gaudi, B. Scott</au><au>Henderson, Calen B.</au><au>Johnson, Samson</au><aucorp>The Spitzer Team</aucorp><aucorp>The OGLE Collaboration</aucorp><aucorp>Leading Authors</aucorp><aucorp>The MOA Collaboration</aucorp><aucorp>The KMTNet Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet</atitle><jtitle>The Astronomical journal</jtitle><stitle>AJ</stitle><addtitle>Astron. J</addtitle><date>2021-10-01</date><risdate>2021</risdate><volume>162</volume><issue>4</issue><spage>163</spage><pages>163-</pages><issn>0004-6256</issn><issn>1538-3881</issn><eissn>1538-3881</eissn><abstract>In order to exhume the buried signatures of “missing planetary caustics” in Korea Microlensing Telescope Network (KMTNet) data, we conducted a systematic anomaly search of the residuals from point-source point-lens fits, based on a modified version of the KMTNet EventFinder algorithm. This search revealed the lowest-mass-ratio planetary caustic to date in the microlensing event OGLE-2019-BLG-1053, for which the planetary signal had not been noticed before. The planetary system has a planet–host mass ratio of
q
= (1.25 ± 0.13) × 10
−5
. A Bayesian analysis yielded estimates of the mass of the host star,
M
host
=
0.61
−
0.24
+
0.29
M
⊙
, the mass of its planet,
M
planet
=
2.48
−
0.98
+
1.19
M
⊕
, the projected planet–host separation,
a
⊥
=
3.4
−
0.5
+
0.5
au, and the lens distance,
D
L
=
6.8
−
0.9
+
0.6
kpc. The discovery of this very-low-mass-ratio planet illustrates the utility of our method and opens a new window for a large and homogeneous sample to study the microlensing planet–host mass ratio function down to
q
∼ 10
−5
.</abstract><cop>Madison</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-3881/ac12d4</doi><tpages>18</tpages><orcidid>https://orcid.org/0000-0002-4035-5012</orcidid><orcidid>https://orcid.org/0000-0003-4084-880X</orcidid><orcidid>https://orcid.org/0000-0002-4909-5763</orcidid><orcidid>https://orcid.org/0000-0002-7669-1069</orcidid><orcidid>https://orcid.org/0000-0001-7016-1692</orcidid><orcidid>https://orcid.org/0000-0001-9818-1513</orcidid><orcidid>https://orcid.org/0000-0003-4776-8618</orcidid><orcidid>https://orcid.org/0000-0001-6364-408X</orcidid><orcidid>https://orcid.org/0000-0002-0548-8995</orcidid><orcidid>https://orcid.org/0000-0003-3316-4012</orcidid><orcidid>https://orcid.org/0000-0002-9245-6368</orcidid><orcidid>https://orcid.org/0000-0003-1435-3053</orcidid><orcidid>https://orcid.org/0000-0003-0395-9869</orcidid><orcidid>https://orcid.org/0000-0001-5207-5619</orcidid><orcidid>https://orcid.org/0000-0003-1525-5041</orcidid><orcidid>https://orcid.org/0000-0001-8263-1006</orcidid><orcidid>https://orcid.org/0000-0002-3401-1029</orcidid><orcidid>https://orcid.org/0000-0003-0043-3925</orcidid><orcidid>https://orcid.org/0000-0002-1650-1518</orcidid><orcidid>https://orcid.org/0000-0001-8317-2788</orcidid><orcidid>https://orcid.org/0000-0002-2641-9964</orcidid><orcidid>https://orcid.org/0000-0001-9397-4768</orcidid><orcidid>https://orcid.org/0000-0001-8877-9060</orcidid><orcidid>https://orcid.org/0000-0001-6000-3463</orcidid><orcidid>https://orcid.org/0000-0001-8043-8413</orcidid><orcidid>https://orcid.org/0000-0003-2388-4534</orcidid><orcidid>https://orcid.org/0000-0002-6982-7722</orcidid><orcidid>https://orcid.org/0000-0001-9823-2907</orcidid><orcidid>https://orcid.org/0000-0002-9241-4117</orcidid><orcidid>https://orcid.org/0000-0001-5966-837X</orcidid><orcidid>https://orcid.org/0000-0001-5069-319X</orcidid><orcidid>https://orcid.org/0000-0002-0314-6000</orcidid><orcidid>https://orcid.org/0000-0002-6212-7221</orcidid><orcidid>https://orcid.org/0000-0001-9481-7123</orcidid><orcidid>https://orcid.org/0000-0002-5843-9433</orcidid><orcidid>https://orcid.org/0000-0003-4027-4711</orcidid><orcidid>https://orcid.org/0000-0003-4916-0892</orcidid><orcidid>https://orcid.org/0000-0001-6285-4528</orcidid><orcidid>https://orcid.org/0000-0002-2339-5899</orcidid><orcidid>https://orcid.org/0000-0003-2302-9562</orcidid><orcidid>https://orcid.org/0000-0003-0562-5643</orcidid><orcidid>https://orcid.org/0000-0002-4355-9838</orcidid><orcidid>https://orcid.org/0000-0002-3051-274X</orcidid><orcidid>https://orcid.org/0000-0002-8198-1968</orcidid><orcidid>https://orcid.org/0000-0001-8472-2219</orcidid><orcidid>https://orcid.org/0000-0002-7777-0842</orcidid><orcidid>https://orcid.org/0000-0002-0221-6871</orcidid><orcidid>https://orcid.org/0000-0003-1978-2092</orcidid><orcidid>https://orcid.org/0000-0002-2335-1730</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | ISSN: 0004-6256 |
| ispartof | The Astronomical journal, 2021-10, Vol.162 (4), p.163 |
| issn | 0004-6256 1538-3881 1538-3881 |
| language | eng |
| recordid | cdi_iop_journals_10_3847_1538_3881_ac12d4 |
| source | IOP Publishing Free Content |
| subjects | ALGORITHMS Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Bayesian analysis Exoplanet detection methods Gravitational microlensing exoplanet detection Lenses Microlenses OTHER INSTRUMENTATION Planetary systems PLANETS POINT SOURCES Searching SIGNALS STARS TELESCOPES Terrestrial environments Terrestrial planets |
| title | Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-04T20%3A36%3A02IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Systematic%20KMTNet%20Planetary%20Anomaly%20Search.%20I.%20OGLE-2019-BLG-1053Lb,%20a%20Buried%20Terrestrial%20Planet&rft.jtitle=The%20Astronomical%20journal&rft.au=Zang,%20Weicheng&rft.aucorp=The%20Spitzer%20Team&rft.date=2021-10-01&rft.volume=162&rft.issue=4&rft.spage=163&rft.pages=163-&rft.issn=0004-6256&rft.eissn=1538-3881&rft_id=info:doi/10.3847/1538-3881/ac12d4&rft_dat=%3Cproquest_O3W%3E2577067947%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2577067947&rft_id=info:pmid/&rfr_iscdi=true |