Astronomy:Optical Gravitational Lensing Experiment

From HandWiki
Short description: Long-term variability sky survey
Optical Gravitational Lensing Experiment
[edit on Wikidata]

The Optical Gravitational Lensing Experiment (OGLE) is a Polish astronomical project based at the University of Warsaw that runs a long-term variability sky survey (1992–present). The main goals are the detection and classification of variable stars (pulsating and eclipsing), discovery of microlensing events, dwarf novae, and studies of the structure of the Galaxy and the Magellanic Clouds. Since the project began in 1992, it has discovered a multitude of extrasolar planets, together with the first planet discovered using the transit method (OGLE-TR-56b) and gravitational microlensing. The project has been led by professor Andrzej Udalski since its inception.

Description

OGLE-IV Galactic Bulge fields with cadence, from OGLE-IV sky coverage.

The main targets of the experiment are the Magellanic Clouds and the Galactic Bulge, because of the large number of intervening stars that can be used for microlensing during a stellar transit. Most of the observations have been made at the Las Campanas Observatory in Chile . Cooperating institutions include Princeton University and the Carnegie Institution.

The project is now in its fourth phase. The first phase, OGLE-I (1992–1995) used the 1.0-metre (3 ft 3 in) Swope telescope and a single-chip CCD sensor. For OGLE-II (1996–2000), a 1.3-metre (4 ft 3 in) telescope dedicated to the project (the Warsaw telescope) was constructed at Las Campanas Observatory. It was equipped with a single 2048×2048 pixel sensor with a field of view 0.237 degrees wide.[1]

OGLE-III (2001–2009) expanded the camera to a mosaic of eight 2048×4096 pixel CCDs, and was able to search for gravitational microlensing events and transiting planets in four fields: the Galactic Bulge, the constellation Carina,[2] and toward both Magellanic Clouds. As a byproduct of the constant monitoring of hundreds of millions of stars, the largest catalogs of variable stars were constructed, and the first exoplanets discovered using the microlensing technique were detected.

In 2010, following engineering work in 2009, the fourth and current phase, OGLE-IV, was started using a 32-chip mosaic CCD camera which fills the Warsaw telescope's 1.5° field of view.[3] The main goal for this phase is to increase the number of planetary detections using microlensing, enabled by the new camera.

Recently the OGLE team, in cooperation with scientists mostly from the US, New Zealand and Japan, proved that small, Earth-like planets can exist at a significant distance from stars around which they revolve despite there being other stars near them.[4][5]

In January 2022 in collaboration with Microlensing Observations in Astrophysics (MOA) they reported in a preprint the first rogue black hole.[6][7][8][9] While there have been other candidates[10] this is the most solid detection so far as their technique allowed to measure not only the amplification of light but also its deflection by the BH from the microlensing data.

Planets discovered

At least seventeen planets have so far been discovered by the OGLE project. Eight of the planets were discovered by the transit method and six by the gravitational microlensing method.

Planets are shown in the order of discovery. Planets in multiple-planet systems are highlighted in yellow. The list below may not be complete.

Star Constellation Right
ascension 		Declination App.
mag. 		Distance (ly) Spectral
type 		Planet Mass
(MJ) 		Radius (RJ) Orbital
period
(d) 		a
(AU) 		ecc. incl.
(°) 		Discovery
year
OGLE-TR-10[11][12] Sagittarius  17h 51m 28s −29° 52′ 34″ 15.78 5000 G2V OGLE-TR-10 b 0.63 1.26 3.10129 0.04162 0 84.5 2002
OGLE-TR-111 Carina  10h 53m 01s −61° 24′ 20″ 16.96 5000 G OGLE-TR-111 b 0.53 1.0 4.01610 0.047 0 88.1 2002
OGLE-TR-132 Carina  10h 50m 34s −61° 57′ 25″ 15.72 7110 F OGLE-TR-132 b 1.14 1.18 1.689868 0.0306 0 85 2003
OGLE-TR-56 Sagittarius  17h 56m 35s −29° 32′ 21″ 16.56 4892 G OGLE-TR-56 b 1.29 1.30 1.211909 0.0225 0 78.8 2003
OGLE-TR-113 Carina  10h 52m 24s −61° 26′ 48″ 16.08 1800 K OGLE-TR-113 b 1.32 1.09 1.4324757 0.0229 0 89.4 2004
OGLE-2003-BLG-235L
/MOA-2003-BLG-53L		 Sagittarius  18h 05m 16s −28° 53′ 42″ 19000 K OGLE-2003-BLG-235Lb 2.6 4.3 2004
OGLE-2005-BLG-071L Scorpius  17h 50m 09s −34° 40′ 23″ 19.5 9500 M OGLE-2005-BLG-071Lb 3.5 3600 3.6 2005
OGLE-2005-BLG-169L Sagittarius  18h 06m 05s –30° 43′ 57″ 19.4 8800 M? OGLE-2005-BLG-169Lb 0.041 0.345 2006
OGLE-2005-BLG-390L Sagittarius  17h 54m 19s −30° 22′ 38″ 21500 M? OGLE-2005-BLG-390Lb 0.018 2006
OGLE-TR-211 Carina  10h 40m 15s −62° 27′ 20″ 5300 F OGLE-TR-211 b 1.03 1.36 3.67724 0.051 0 ≥87.2 2007
OGLE-TR-182 Carina  11h 09m 19s −61° 05′ 43″ 16.84 12700 G OGLE-TR-182 b 1.01 1.13 3.9791 0.051 0 85.7 2007
OGLE2-TR-L9 Carina  11h 07m 55s −61° 08′ 46″ 2935 F3 OGLE2-TR-L9 b 4.5 1.61 2.4855335 0.0308 2008
OGLE-2006-BLG-109L Sagittarius  17h 52m 35s −30° 05′ 16″ 4900 M0V? OGLE-2006-BLG-109Lb 0.71 1825 2.3 2008
OGLE-2006-BLG-109Lc 0.27 5100 4.8 0.11 59 2008
OGLE-2012-BLG-0026L  17h 34m 19s −27° 08′ 34″ 4080 OGLE-2012-BLG-0026Lb 0.11 3.82 2012
OGLE-2012-BLG-0026Lc 0.68 4.63 2012
OGLE-2011-BLG-0251  17h 38m 14s −27° 08′ 10″ 8232 M OGLE-2011-BLG-0251 b 0.53 2.72 or 1.5 2013
OGLE-2007-BLG-349(AB) 8000 OGLE-2007-BLG-349(AB)b 0.25 2.9 2016
OGLE-2016-BLG-1190L Sagittarius  17h 58m 53s −27° 36′ 49″ 22000 G OGLE-2016-BLG-1190Lb 13.38 1223.6 2.17 0.42 41.2 2017
OGLE-2016-BLG-1195L OGLE-2016-BLG-1195Lb 0.0045 2017
OGLE-2013-BLG-0132L 13000 OGLE-2013-BLG-0132Lb 0.29 2017
OGLE-2013-BLG-1721L 21000 OGLE-2013-BLG-1721Lb 0.64 2.6 2017
OGLE-2016-BLG-0263L 21000 OGLE-2016-BLG-0263Lb 4.10 5.4 2017
OGLE-2018-BLG-0799L 2900 OGLE-2018-BLG-0799Lb 0.22 1.75 2018
N/A OGLE-2019-BLG-0551b 0.0242 2020
OGLE-2019-BLG-0960L OGLE-2019-BLG-0960Lb 0.0071 2021
Artist's impression of the planet OGLE-2005-BLG-390Lb discovered by the OGLE Team

Notes: For events detected by the gravitational microlensing method, year stands for OGLE season, BLG means that an event detected is in the Galactic BuLGe, and the following 3-digit number is an ordinal number of microlensing event in that season. For events detected by the transit method TR stands for TRansit and the following 3-digit number is an ordinal number of transit event.

See also


References

  1. ↑ Udalski, A.; Kubiak, M.; Szymański, M. (1997). "Optical Gravitational Lensing Experiment. OGLE-2 – the Second Phase of the OGLE Project". Acta Astronomica 47 (3): 319–344. Bibcode: 1997AcA....47..319U. http://acta.astrouw.edu.pl/Vol47/n3/pap_47_3_1.pdf. 
  2. ↑ Udalski, Andrzej (2003). "The Optical Gravitational Lensing Experiment. Real Time Data Analysis Systems in the OGLE-III Survey". Acta Astronomica 53 (4): 291–306. Bibcode: 2003AcA....53..291U. http://acta.astrouw.edu.pl/Vol53/n4/pap_53_4_1.pdf. 
  3. ↑ Udalski, A.; Szymański, M. K.; Szymański, G. (2015). "OGLE-IV: Fourth Phase of the Optical Gravitational Lensing Experiment". Acta Astronomica 65 (1): 1–38. Bibcode: 2015AcA....65....1U. http://acta.astrouw.edu.pl/Vol65/n1/pdf/pap_65_1_1.pdf. 
  4. ↑ "Laureaci FNP odkryli zimną Ziemię" (in pl). Foundation for Polish Science (FNP). 7 July 2014. https://www.fnp.org.pl/laureaci-fnp-odkryli-zimna-ziemie/. 
  5. ↑ Gould, A. (4 July 2014). "A terrestrial planet in a ~1-AU orbit around one member of a ~15-AU binary". Science 345 (6192): 46–49. doi:10.1126/science.1251527. PMID 24994642. Bibcode: 2014Sci...345...46G. 
  6. ↑ Sahu, Kailash C.; Anderson, Jay; Casertano, Stefano; Bond, Howard E.; Udalski, Andrzej; Dominik, Martin; Calamida, Annalisa; Bellini, Andrea et al. (2022-05-25). "An Isolated Stellar-mass Black Hole Detected through Astrometric Microlensing". The Astrophysical Journal 933: 83. doi:10.3847/1538-4357/ac739e. Bibcode: 2022ApJ...933...83S. 
  7. ↑ Lam, Casey Y.; Lu, Jessica R.; Udalski, Andrzej; Bond, Ian; Bennett, David P.; Skowron, Jan; Mroz, Przemek; Poleski, Radek et al. (2022-05-31). "An Isolated Mass-gap Black Hole or Neutron Star Detected with Astrometric Microlensing". The Astrophysical Journal Letters 933: L23. doi:10.3847/2041-8213/ac7442. Bibcode: 2022ApJ...933L..23L. 
  8. ↑ Gianopoulos, Andrea (2022-06-07). "Hubble Determines Mass of Isolated Black Hole Roaming Milky Way". http://www.nasa.gov/feature/goddard/2022/hubble-determines-mass-of-isolated-black-hole-roaming-our-milky-way-galaxy. 
  9. ↑ O'Callaghan, Jonathan. "Astronomers Find First Ever Rogue Black Hole Adrift in the Milky Way" (in en). https://www.scientificamerican.com/article/astronomers-find-first-ever-rogue-black-hole-adrift-in-the-milky-way/. 
  10. ↑ Bennett, D. P.; Becker, A. C.; Quinn, J. L.; Tomaney, A. B.; Alcock, C.; Allsman, R. A.; Alves, D. R.; Axelrod, T. S. et al. (2002-11-10). "Gravitational Microlensing Events Due to Stellar‐Mass Black Holes" (in en). The Astrophysical Journal 579 (2): 639–659. doi:10.1086/342225. ISSN 0004-637X. Bibcode: 2002ApJ...579..639B. https://iopscience.iop.org/article/10.1086/342225. 
  11. ↑ Udalski, A. et al. (2002). "The Optical Gravitational Lensing Experiment. Search for Planetary and Low-Luminosity Object Transits in the Galactic Disk. Results of 2001 Campaign". Acta Astronomica 52 (1): 1–37. Bibcode: 2002AcA....52....1U. http://acta.astrouw.edu.pl/Vol52/n1/a_52_1_1.html. 
  12. ↑ Konacki, Maciej et al. (2005). "A Transiting Extrasolar Giant Planet around the Star OGLE-TR-10". The Astrophysical Journal 624 (1): 372–377. doi:10.1086/429127. Bibcode: 2005ApJ...624..372K. 

External links



Retrieved from "https://handwiki.org/wiki/index.php?title=Astronomy:Optical_Gravitational_Lensing_Experiment&oldid=3341802"