PATHWAY TO THE GALACTIC DISTRIBUTION OF PLANETS: COMBINED SPITZER AND GROUND-BASED MICROLENS PARALLAX MEASUREMENTS OF 21 SINGLE-LENS EVENTS

CALCHI NOVATI, Sebastiano; Gould, A.; Udalski, A.; Menzies, J. W.; Bond, I. A.; Shvartzvald, Y.; Street, R. A.; Hundertmark, M.; Beichman, C. A.; Yee, J. C.; Carey, S.; Poleski, R.; Skowron, J.; Kozłowski, S.; Mróz, P.; Pietrukowicz, P.; Pietrzyński, G.; Szymański, M. K.; Soszyński, I.; Ulaczyk, K.; Wyrzykowski, Ł.; Albrow, M.; Beaulieu, J. P.; Caldwell, J. A. R.; Cassan, A.; Coutures, C.; Danielski, C.; Prester, D. Dominis; Donatowicz, J.; Lončarić, K.; Mcdougall, A.; Morales, J. C.; Ranc, C.; Zhu, W.; Abe, F.; Barry, R. K.; Bennett, D. P.; Bhattacharya, A.; Fukunaga, D.; Inayama, K.; Koshimoto, N.; Namba, S.; Sumi, T.; Suzuki, D.; Tristram, P. J.; Wakiyama, Y.; Yonehara, A.; Maoz, D.; Kaspi, S.; Friedmann, M.; Bachelet, E.; Jaimes, R. Figuera; Bramich, D. M.; Tsapras, Y.; Horne, K.; Snodgrass, C.; Wambsganss, J.; Steele, I. A.; Kains, N.; Bozza, Valerio; Dominik, M.; Jørgensen, U. G.; Alsubai, K. A.; Ciceri, S.; D'Ago, Giuseppe; Haugbølle, T.; Hessman, F. V.; Hinse, T. C.; Juncher, D.; Korhonen, H.; Mancini, Luigi; Popovas, A.; Rabus, M.; Rahvar, S.; Scarpetta, Gaetano; Schmidt, R. W.; Skottfelt, J.; Southworth, J.; Starkey, D.; Surdej, J.; Wertz, O.; Zarucki, M.; Gaudi, B. S.; Pogge, R. W.; Depoy, D. L.

doi:10.1088/0004-637X/804/1/20

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We present microlens parallax measurements for 21 (apparently) isolated lenses observed toward the Galactic bulge that were imaged simultaneously from Earth and Spitzer, which was ~1 AU west of Earth in projection. We combine these measurements with a kinematic model of the Galaxy to derive distance estimates for each lens, with error bars that are small compared to the Sun's galactocentric distance. The ensemble therefore yields a well-defined cumulative distribution of lens distances. In principle, it is possible to compare this distribution against a set of planets detected in the same experiment in order to measure the Galactic distribution of planets. Since these Spitzer observations yielded only one planet, this is not yet possible in practice. However, it will become possible as larger samples are accumulated.

Titolo:	PATHWAY TO THE GALACTIC DISTRIBUTION OF PLANETS: COMBINED SPITZER AND GROUND-BASED MICROLENS PARALLAX MEASUREMENTS OF 21 SINGLE-LENS EVENTS
Autori:	CALCHI NOVATI, Sebastiano Gould, A. Udalski, A. Menzies, J. W. Bond, I. A. Shvartzvald, Y. Street, R. A. Hundertmark, M. Beichman, C. A. Yee, J. C. Carey, S. Poleski, R. Skowron, J. Kozłowski, S. Mróz, P. Pietrukowicz, P. Pietrzyński, G. Szymański, M. K. Soszyński, I. Ulaczyk, K. Wyrzykowski, Ł. Albrow, M. Beaulieu, J. P. Caldwell, J. A. R. Cassan, A. Coutures, C. Danielski, C. Prester, D. Dominis Donatowicz, J. Lončarić, K. Mcdougall, A. Morales, J. C. Ranc, C. Zhu, W. Abe, F. Barry, R. K. Bennett, D. P. Bhattacharya, A. Fukunaga, D. Inayama, K. Koshimoto, N. Namba, S. Sumi, T. Suzuki, D. Tristram, P. J. Wakiyama, Y. Yonehara, A. Maoz, D. Kaspi, S. Friedmann, M. Bachelet, E. Jaimes, R. Figuera Bramich, D. M. Tsapras, Y. Horne, K. Snodgrass, C. Wambsganss, J. Steele, I. A. Kains, N. BOZZA, Valerio Dominik, M. Jørgensen, U. G. Alsubai, K. A. Ciceri, S. D'AGO, GIUSEPPE Haugbølle, T. Hessman, F. V. Hinse, T. C. Juncher, D. Korhonen, H. MANCINI, Luigi Popovas, A. Rabus, M. Rahvar, S. SCARPETTA, Gaetano Schmidt, R. W. Skottfelt, J. Southworth, J. Starkey, D. Surdej, J. Wertz, O. Zarucki, M. Gaudi, B. S. Pogge, R. W. Depoy, D. L. mostra contributor esterni nascondi contributor esterni
Data di pubblicazione:	2015
Rivista:	THE ASTROPHYSICAL JOURNAL
Abstract:	We present microlens parallax measurements for 21 (apparently) isolated lenses observed toward the Galactic bulge that were imaged simultaneously from Earth and Spitzer, which was ~1 AU west of Earth in projection. We combine these measurements with a kinematic model of the Galaxy to derive distance estimates for each lens, with error bars that are small compared to the Sun's galactocentric distance. The ensemble therefore yields a well-defined cumulative distribution of lens distances. In principle, it is possible to compare this distribution against a set of planets detected in the same experiment in order to measure the Galactic distribution of planets. Since these Spitzer observations yielded only one planet, this is not yet possible in practice. However, it will become possible as larger samples are accumulated.
Handle:	http://hdl.handle.net/11386/4644690
Appare nelle tipologie:	1.1.1 Articolo su rivista con DOI

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