검색결과 : 9건
| No. | Article |
|---|---|
| 1 |
A distance to the Large Magellanic Cloud that is precise to one per cent Pietrzynski G, Graczyk D, Gallenne A, Gieren W, Thompson IB, Pilecki B, Karczmarek P, Gorski M, Suchomska K, Taormina M, Zgirski B, Wielgorski P, Kolaczkowski Z, Konorski P, Villanova S, Nardetto N, Kervella P, Bresolin F, Kudritzki RP, Storm J, Smolec R, Narloch W Nature, 567(7747), 200, 2019 |
| 2 |
Method for studying dark matter turns 25 Pietrzynski G Nature, 562(7727), 349, 2018 |
| 3 |
Extremely metal-poor stars from the cosmic dawn in the bulge of the Milky Way Howes LM, Casey AR, Asplund M, Keller SC, Yong D, Nataf DM, Poleski R, Lind K, Kobayashi C, Owen CI, Ness M, Bessell MS, Da Costa GS, Schmidt BP, Tisserand P, Udalski A, Szymanski MK, Soszynski I, Pietrzynski G, Ulaczyk K, Wyrzykowski L, Pietrukowicz P, Skowron J, Kozlowski S, Mroz P Nature, 527(7579), 484, 2015 |
| 4 |
A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source Motch C, Pakull MW, Soria R, Grise F, Pietrzynski G Nature, 514(7521), 198, 2014 |
| 5 |
A terrestrial planet in a similar to 1-AU orbit around one member of a similar to 15-AU binary Gould A, Udalski A, Shin IG, Porritt I, Skowron J, Han C, Yee JC, Kozlowski S, Choi JY, Poleski R, Wyrzykowski L, Ulaczyk K, Pietrukowicz P, Mroz P, Szymanski MK, Kubiak M, Soszynski I, Pietrzynski G, Gaudi BS, Christie GW, Drummond J, McCormick J, Natusch T, Ngan H, Tan TG, Albrow M, DePoy DL, Hwang KH, Jung YK, Lee CU, Park H, Pogge RW, Abe F, Bennett DP, Bond IA, Botzler CS, Freeman M, Fukui A, Fukunaga D, Itow Y, Koshimoto N, Larsen P, Ling CH, Masuda K, Matsubara Y, Muraki Y, Namba S, Ohnishi K, Philpott L, Rattenbury NJ, Saito T, Sullivan DJ, Sumi T, Suzuki D, Tristram PJ, Tsurumi N, Wada K, Yamai N, Yock PCM, Yonehara A, Shvartzvald Y, Maoz D, Kaspi S, Friedmann M Science, 345(6192), 46, 2014 |
| 6 |
An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent Pietrzynski G, Graczyk D, Gieren W, Thompson IB, Pilecki B, Udalski A, Soszynski I, Kozlowski S, Konorski P, Suchomska K, Bono G, Moroni PGP, Villanova S, Nardetto N, Bresolin F, Kudritzki RP, Storm J, Gallenne A, Smolec R, Minniti D, Kubiak M, Szymanski MK, Poleski R, Wyrzykowski L, Ulaczyk K, Pietrukowicz P, Gorski M, Karczmarek P Nature, 495(7439), 76, 2013 |
| 7 |
One or more bound planets per Milky Way star from microlensing observations Cassan A, Kubas D, Beaulieu JP, Dominik M, Horne K, Greenhill J, Wambsganss J, Menzies J, Williams A, Jorgensen UG, Udalski A, Bennett DP, Albrow MD, Batista V, Brillant S, Caldwell JAR, Cole A, Coutures C, Cook KH, Dieters S, Prester DD, Donatowicz J, Fouque P, Hill K, Kains N, Kane S, Marquette JB, Martin R, Pollard KR, Sahu KC, Vinter C, Warren D, Watson B, Zub M, Sumi T, Szymanski MK, Kubiak M, Poleski R, Soszynski I, Ulaczyk K, Pietrzynski G, Wyrzykowski L Nature, 481(7380), 167, 2012 |
| 8 |
RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system Pietrzynski G, Thompson IB, Gieren W, Graczyk D, Stepien K, Bono G, Moroni PGP, Pilecki B, Udalski A, Soszynski I, Preston GW, Nardetto N, McWilliam A, Roederer IU, Gorski M, Konorski P, Storm J Nature, 484(7392), 75, 2012 |
| 9 |
Unbound or distant planetary mass population detected by gravitational microlensing Sumi T, Kamiya K, Bennett DP, Bond IA, Abe F, Botzler CS, Fukui A, Furusawa K, Hearnshaw JB, Itow Y, Kilmartin PM, Korpela A, Lin W, Ling CH, Masuda K, Matsubara Y, Miyake N, Motomura M, Muraki Y, Nagaya M, Nakamura S, Ohnishi K, Okumura T, Perrott YC, Rattenbury N, Saito T, Sako T, Sullivan DJ, Sweatman WL, Tristram PJ, Yock PCM, Udalski A, Szymanski MK, Kubiak M, Pietrzynski G, Poleski R, Soszynski I, Wyrzykowski L, Ulaczyk K Nature, 473(7347), 349, 2011 |