Zobrazeno 1 - 10
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pro vyhledávání: '"Vandehei A"'
Two recent studies explicitly recommend labeling defective classes in releases using the affected versions (AV) available in issue trackers. The aim our study is threefold: 1) to measure the proportion of defects for which the realistic method is usa
Externí odkaz:
http://arxiv.org/abs/2011.05531
Autor:
Vandehei, Amy D.1 (AUTHOR) avandehei50@gmail.com, Perry, Anthony R.1 (AUTHOR)
Publikováno v:
Journal of Social Psychology. 2023, Vol. 163 Issue 3, p324-334. 11p. 1 Chart, 1 Graph.
Autor:
Nelson, C. A., Drake, A. J., Cook, K. H., Bennett, D. P., Popowski, P., Dalal, N., Nikolaev, S., Alcock, C., Axelrod, T. S., Becker, A. C., Freeman, K. C., Geha, M., Griest, K., Keller, S. C., Lehner, M. J., Marshall, S. L., Minniti, D., Pratt, M. R., Quinn, P. J., Stubbs, C. W., Sutherland, W., Tomaney, A. B., Vandehei, T., Welch, D.
We present Hubble Space Telescope (HST) WFPC2 photometry of 13 microlensed source stars from the 5.7 year Large Magellanic Cloud (LMC) survey conducted by the MACHO Project. The microlensing source stars are identified by deriving accurate centroids
Externí odkaz:
http://arxiv.org/abs/0902.2213
Autor:
Thomas, C. L., Griest, K., Popowski, P., Cook, K. H., Drake, A. J., Minniti, D., Alcock, C., Allsman, R. A., Alves, D. R., Axelrod, T. S., Becker, A. C., Bennett, D. P., Freeman, K. C., Geha, M., Lehner, M. J., Marshall, S. L., Myer, D. G., Nelson, C. A., Peterson, B. A., Quinn, P. J., Stubbs, C. W., Sutherland, W., Vandehei, T., Welch, D. L.
Publikováno v:
Astrophys.J. 631 (2005) 906-934
We present a catalog of 450 high signal-to-noise microlensing events observed by the MACHO collaboration between 1993 and 1999. The events are distributed throughout our fields and, as expected, they show clear concentration toward the Galactic cente
Externí odkaz:
http://arxiv.org/abs/astro-ph/0410341
Autor:
Popowski, P., Griest, K., Thomas, C. L., Cook, K. H., Bennett, D. P., Becker, A. C., Alves, D. R., Minniti, D., Drake, A. J., Alcock, C., Allsman, R. A., Axelrod, T. S., Freeman, K. C., Geha, M., Lehner, M. J., Marshall, S. L., Nelson, C. A., Peterson, B. A., Quinn, P. J., Stubbs, C. W., Sutherland, W., Vandehei, T., Welch, D.
Publikováno v:
Astrophys.J. 631 (2005) 879-905
Using 7 years of MACHO survey data, we present a new determination of the optical depth to microlensing towards the Galactic bulge. We select the sample of 62 microlensing events (60 unique) on clump giant sources and perform a detailed efficiency an
Externí odkaz:
http://arxiv.org/abs/astro-ph/0410319
Autor:
Alcock, C., Alves, D. R., Axelrod, T. S., Becker, A. C., Bennett, D. P., Clement, C. M., Cook, K. H., Drake, A. J., Freeman, K. C., Geha, M., Griest, K., Lehner, M. J., Marshall, S. L., Minniti, D., Muzzin, A., Nelson, C. A., Peterson, B. A., Popowski, P., Quinn, P. J., Rodgers, A. W., Rowe, J. F., Sutherland, W., Vandehei, T., Welch, D. L.
Fourier coefficents have been derived for the $V$ and $R$ light curves of 785 overtone RR Lyrae variables in 16 MACHO fields near the bar of the LMC. The $\phi_{31}$ and $R_{21}$ coefficients have been compared with those of the first overtone RR Lyr
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310281
Autor:
Alcock, C., Alves, D. R., Becker, A., Bennett, D., Cook, K. H., Drake, A., Freeman, K., Geha, M., Griest, K., Kovács, G., Lehner, M., Marshall, S., Minniti, D., Nelson, C., Peterson, B., Popowski, P., Pratt, M., Quinn, P., Rodgers, A., Stubbs, C., Sutherland, W., Vandehei, T., Welch, D. L.
Publikováno v:
Astrophys.J.598:597-609,2003
We have frequency analyzed 6391 variables classified earlier as fundamental mode RR Lyrae (RR0) stars in the MACHO database on the Large Magellanic Cloud (LMC). The overwhelming majority of these variables have been proved to be indeed RR0 stars, whe
Externí odkaz:
http://arxiv.org/abs/astro-ph/0308019
Autor:
Popowski, P., Nelson, C. A., Bennett, D. P., Drake, A. J., Vandehei, T., Griest, K., Cook, K. H., Alcock, C., Allsman, R. A., Alves, D. R., Axelrod, T. S., Becker, A. C., Freeman, K. C., Geha, M., Lehner, M. J., Marshall, S. L., Minniti, D., Peterson, B. A., Quinn, P. J., Stubbs, C. W., Sutherland, W., Welch, D.
We describe a few recent microlensing results from the MACHO Collaboration. The aim of the MACHO Project was the identification and quantitative description of dark and luminous matter in the Milky Way using microlensing toward the Magellanic Clouds
Externí odkaz:
http://arxiv.org/abs/astro-ph/0304464
Autor:
Geha, M., Alcock, C., Allsman, R. A., Alves, D. R., Axelrod, T. S., Becker, A. C., Bennett, D. P., Cook, K. H., Drake, A. J., Freeman, K. C., Griest, K., Keller, S. C., Lehner, M. J., Marshall, S. L., Minniti, D., Nelson, C. A., Peterson, B. A., Popowski, P., Pratt, M. R., Quinn, P. J., Stubbs, C. W., Sutherland, W., Tomaney, A. B., Vandehei, T., Welch, D. L.
Publikováno v:
Astron.J. 125 (2003) 1
We present 47 spectroscopically-confirmed quasars discovered behind the Magellanic Clouds identified via photometric variability in the MACHO database. Thirty-eight quasars lie behind the Large Magellanic Cloud and nine behind the Small Magellanic Cl
Externí odkaz:
http://arxiv.org/abs/astro-ph/0209513
We present an abundance analysis of six main sequence turnoff, subgiant, and giant branch stars toward the Galactic bulge that were observed with Keck/HIRES during microlensing events. This is an early look at the first detailed chemical analysis of
Externí odkaz:
http://arxiv.org/abs/astro-ph/0209196