44 results on '"Rabus M"'
Search Results
2. Near-infrared and optical emission of WASP-5 b
- Author
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Kovacs, G., primary, Dékány, I., additional, Karamiqucham, B., additional, Chen, G., additional, Zhou, G., additional, Rabus, M., additional, and Kovács, T., additional
- Published
- 2022
- Full Text
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3. A spectroscopic follow-up for Gaia19bld
- Author
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Bachelet, E., primary, Zieliński, P., additional, Gromadzki, M., additional, Gezer, I., additional, Rybicki, K., additional, Kruszyńska, K., additional, Ihanec, N., additional, Wyrzykowski, Ł., additional, Street, R. A., additional, Tsapras, Y., additional, Hundertmark, M., additional, Cassan, A., additional, Harbeck, D., additional, and Rabus, M., additional
- Published
- 2021
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4. TDCOSMO
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Millon, M., primary, Courbin, F., additional, Bonvin, V., additional, Buckley-Geer, E., additional, Fassnacht, C. D., additional, Frieman, J., additional, Marshall, P. J., additional, Suyu, S. H., additional, Treu, T., additional, Anguita, T., additional, Motta, V., additional, Agnello, A., additional, Chan, J. H. H., additional, Chao, D. C.-Y., additional, Chijani, M., additional, Gilman, D., additional, Gilmore, K., additional, Lemon, C., additional, Lucey, J. R., additional, Melo, A., additional, Paic, E., additional, Rojas, K., additional, Sluse, D., additional, Williams, P. R., additional, Hempel, A., additional, Kim, S., additional, Lachaume, R., additional, and Rabus, M., additional
- Published
- 2020
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5. The highly inflated giant planet WASP-174b
- Author
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Mancini, L., primary, Sarkis, P., additional, Henning, Th., additional, Bakos, G. Á., additional, Bayliss, D., additional, Bento, J., additional, Bhatti, W., additional, Brahm, R., additional, Csubry, Z., additional, Espinoza, N., additional, Hartman, J., additional, Jordán, A., additional, Penev, K., additional, Rabus, M., additional, Suc, V., additional, de Val-Borro, M., additional, Zhou, G., additional, Chen, G., additional, Damasso, M., additional, Southworth, J., additional, and Tan, T. G., additional
- Published
- 2020
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6. COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses XVI. Time delays for the quadruply imaged quasar DES J0408−5354 with high-cadence photometric monitoring
- Author
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Courbin, F, Bonvin, V, Buckley-Geer, E, Fassnacht, CD, Frieman, J, Lin, H, Marshall, PJ, Suyu, SH, Treu, T, Anguita, T, Motta, V, Meylan, G, Paic, E, Tewes, M, Agnello, A, Chao, DCY, Chijani, M, Gilman, D, Rojas, K, Williams, P, Hempel, A, Kim, S, Lachaume, R, Rabus, M, Abbott, TMC, Allam, S, Annis, J, Banerji, M, Bechtol, K, Benoit-Lévy, A, Brooks, D, Burke, DL, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, D'Andrea, CB, Da Costa, LN, Davis, C, Depoy, DL, Desai, S, Flaugher, B, Fosalba, P, García-Bellido, J, Gaztanaga, E, Goldstein, DA, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Honscheid, K, James, DJ, Kuehn, K, Kuhlmann, S, Kuropatkin, N, Lahav, O, Lima, M, Maia, MAG, March, M, Marshall, JL, McMahon, RG, Menanteau, F, Miquel, R, Nord, B, Plazas, AA, Sanchez, E, Scarpine, V, Schindler, R, Schubnell, M, Sevilla-Noarbe, I, Smith, M, Soares-Santos, M, Sobreira, F, Suchyta, E, Banerji, Manda [0000-0002-0639-5141], McMahon, Richard [0000-0001-8447-8869], and Apollo - University of Cambridge Repository
- Subjects
Astrophysics::Instrumentation and Methods for Astrophysics ,gravitational lensing: strong ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,cosmological parameters ,methods: data analysis ,Astrophysics::Galaxy Astrophysics - Abstract
© ESO, 2018. We present time-delay measurements for the new quadruple imaged quasar DES J04085354, the first quadruple imaged quasar found in the Dark Energy Survey (DES). Our result is made possible by implementing a new observational strategy using almost daily observations with the MPIA 2.2 m telescope at La Silla observatory and deep exposures reaching a signal-to-noise ratio of about 1000 per quasar image. This data qualityallows us to catch small photometric variations (a few mmag rms) of the quasar, acting on temporal scales much shorter than microlensing, and hence making the time delay measurement very robust against microlensing. In only seven months we very accurately measured one of the time delays in DES J04085354: - "t(AB) = 112.1 ± 2.1 days (1.8%) using only the MPIA 2.2 m data. In combination with data taken with the 1.2 m Euler Swiss telescope, we also measured two delays involving the D component of the system - "t(AD) = ± 12.8 days (8.2%) and - "t(BD) = 42.4 ± 17.6 days (41%), where all the error bars include systematics. Turning these time delays into cosmological constraints will require deep Hubble Space Telescope (HST) imaging or ground-based adaptive optics (AO), and information on the velocity field of the lensing galaxy.
- Published
- 2018
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7. COSMOGRAIL
- Author
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Bonvin, V., primary, Millon, M., additional, Chan, J. H.-H., additional, Courbin, F., additional, Rusu, C. E., additional, Sluse, D., additional, Suyu, S. H., additional, Wong, K. C., additional, Fassnacht, C. D., additional, Marshall, P. J., additional, Treu, T., additional, Buckley-Geer, E., additional, Frieman, J., additional, Hempel, A., additional, Kim, S., additional, Lachaume, R., additional, Rabus, M., additional, Chao, D. C.-Y., additional, Chijani, M., additional, Gilman, D., additional, Gilmore, K., additional, Rojas, K., additional, Williams, P., additional, Anguita, T., additional, Kochanek, C. S., additional, Morgan, C., additional, Motta, V., additional, Tewes, M., additional, and Meylan, G., additional
- Published
- 2019
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8. COSMOGRAIL
- Author
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Bonvin, V., primary, Chan, J. H. H., additional, Millon, M., additional, Rojas, K., additional, Courbin, F., additional, Chen, G. C.-F., additional, Fassnacht, C. D., additional, Paic, E., additional, Tewes, M., additional, Chao, D. C.-Y., additional, Chijani, M., additional, Gilman, D., additional, Gilmore, K., additional, Williams, P., additional, Buckley-Geer, E., additional, Frieman, J., additional, Marshall, P. J., additional, Suyu, S. H., additional, Treu, T., additional, Hempel, A., additional, Kim, S., additional, Lachaume, R., additional, Rabus, M., additional, Anguita, T., additional, Meylan, G., additional, Motta, V., additional, and Magain, P., additional
- Published
- 2018
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9. A hot Saturn on an eccentric orbit around the giant star K2-132
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Jones, M. I., primary, Brahm, R., additional, Espinoza, N., additional, Jordán, A., additional, Rojas, F., additional, Rabus, M., additional, Drass, H., additional, Zapata, A., additional, Soto, M. G., additional, Jenkins, J. S., additional, Vučković, M., additional, Ciceri, S., additional, and Sarkis, P., additional
- Published
- 2018
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10. High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP)
- Author
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Evans, D. F., primary, Southworth, J., additional, Smalley, B., additional, Jørgensen, U. G., additional, Dominik, M., additional, Andersen, M. I., additional, Bozza, V., additional, Bramich, D. M., additional, Burgdorf, M. J., additional, Ciceri, S., additional, D’Ago, G., additional, Figuera Jaimes, R., additional, Gu, S.-H., additional, Hinse, T. C., additional, Henning, Th., additional, Hundertmark, M., additional, Kains, N., additional, Kerins, E., additional, Korhonen, H., additional, Kokotanekova, R., additional, Kuffmeier, M., additional, Longa-Peña, P., additional, Mancini, L., additional, MacKenzie, J., additional, Popovas, A., additional, Rabus, M., additional, Rahvar, S., additional, Sajadian, S., additional, Snodgrass, C., additional, Skottfelt, J., additional, Surdej, J., additional, Tronsgaard, R., additional, Unda-Sanzana, E., additional, von Essen, C., additional, Wang, Yi-Bo, additional, and Wertz, O., additional
- Published
- 2018
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11. COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses
- Author
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Courbin, F., primary, Bonvin, V., additional, Buckley-Geer, E., additional, Fassnacht, C. D., additional, Frieman, J., additional, Lin, H., additional, Marshall, P. J., additional, Suyu, S. H., additional, Treu, T., additional, Anguita, T., additional, Motta, V., additional, Meylan, G., additional, Paic, E., additional, Tewes, M., additional, Agnello, A., additional, Chao, D. C.-Y., additional, Chijani, M., additional, Gilman, D., additional, Rojas, K., additional, Williams, P., additional, Hempel, A., additional, Kim, S., additional, Lachaume, R., additional, Rabus, M., additional, Abbott, T. M. C., additional, Allam, S., additional, Annis, J., additional, Banerji, M., additional, Bechtol, K., additional, Benoit-Lévy, A., additional, Brooks, D., additional, Burke, D. L., additional, Carnero Rosell, A., additional, Carrasco Kind, M., additional, Carretero, J., additional, D’Andrea, C. B., additional, da Costa, L. N., additional, Davis, C., additional, DePoy, D. L., additional, Desai, S., additional, Flaugher, B., additional, Fosalba, P., additional, García-Bellido, J., additional, Gaztanaga, E., additional, Goldstein, D. A., additional, Gruen, D., additional, Gruendl, R. A., additional, Gschwend, J., additional, Gutierrez, G., additional, Honscheid, K., additional, James, D. J., additional, Kuehn, K., additional, Kuhlmann, S., additional, Kuropatkin, N., additional, Lahav, O., additional, Lima, M., additional, Maia, M. A. G., additional, March, M., additional, Marshall, J. L., additional, McMahon, R. G., additional, Menanteau, F., additional, Miquel, R., additional, Nord, B., additional, Plazas, A. A., additional, Sanchez, E., additional, Scarpine, V., additional, Schindler, R., additional, Schubnell, M., additional, Sevilla-Noarbe, I., additional, Smith, M., additional, Soares-Santos, M., additional, Sobreira, F., additional, Suchyta, E., additional, Tarle, G., additional, Tucker, D. L., additional, Walker, A. R., additional, and Wester, W., additional
- Published
- 2018
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12. The 2014-2017 outburst of the young star ASASSN-13db: A time-resolved picture of a very low-mass star between EXors and FUors
- Author
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Sicilia-Aguilar, A., Oprandi, A., Froebrich, D., Fang, M., Prieto, J. L., Stanek, K., Scholz, A., Kochanek, C.S., Henning, Th., Gredel, R., Holoien, T.S.-W., Rabus, M., Shappee, B. J., Billington, S. J., Campbell-White, J., Zegmott, T.J., Sicilia-Aguilar, A., Oprandi, A., Froebrich, D., Fang, M., Prieto, J. L., Stanek, K., Scholz, A., Kochanek, C.S., Henning, Th., Gredel, R., Holoien, T.S.-W., Rabus, M., Shappee, B. J., Billington, S. J., Campbell-White, J., and Zegmott, T.J.
- Abstract
ASASSN-13db is a M5-type star with a protoplanetary disk, the lowest mass star known to experience accretion outbursts. Since its discovery in 2013, it has experienced two outbursts, the second of which started in November 2014 and lasted until February 2017. We use high- and low-resolution spectroscopy and time-resolved photometry from the ASAS-SN survey, the LCOGT and the Beacon Observatory to study the lightcurve and the dynamical and physical properties of the accretion flow. The 2014-2017 outburst lasted for nearly 800 days. A 4.15d period in the lightcurve likely corresponds to rotational modulation of a star with hot spot(s). The spectra show multiple emission lines with variable inverse P-Cygni profiles and a highly variable blueshifted absorption below the continuum. Line ratios from metallic emission lines (Fe I/Fe II, Ti I/Ti II) suggest temperatures of $\sim$5800-6000 K in the accretion flow. Photometrically and spectroscopically, the 2014-2017 event displays an intermediate behavior between EXors and FUors. The accretion rate (\.{M}=1-3$\times$10$^{-7}$M$_\odot$/yr), about 2 orders of magnitude higher than the accretion rate in quiescence, is not significantly different from the accretion rate observed in 2013. The absorption features in the spectra suggest that the system is viewed at a high angle and drives a powerful, non-axisymmetric wind, maybe related to magnetic reconnection. The properties of ASASSN-13db suggest that temperatures lower than those for solar-type stars are needed for modeling accretion in very low-mass systems. Finally, the rotational modulation during the outburst reveals that accretion-related structures settled after the begining of the outburst and can be relatively stable and long-lived. Our work also demonstrates the power of time-resolved photometry and spectroscopy to explore the properties of variable and outbursting stars. (Abridged).
- Published
- 2017
13. Estimating the parameters of globular cluster M 30 (NGC 7099) from time-series photometry (vol 555, pg A36, 2013)
- Author
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Kains, N, Bramich, DM, Ferro, AA, Jaimes, RF, Jorgensen, UG, Giridhar, S, Penny, MT, Alsubai, KA, Andersen, JM, Bozza, V, Browne, P, Burgdorf', M, Novati, SC, Damerdji, Y, Diehl, C, Dodds, P, Dominik, M, Elyiv, A, Fang, X-S, Giannini, E, Hardis, S, Harpsoe, K, Hinse, TC, Hornstrup, A, Hundertmark, M, Jessen-Hansen, J, Juncher, D, Kerins, E, Kjeldsen, H, Korhonen, H, Liebig, C, Lund, MN, Lundkvist, M, Mancini, L, Martin, R, Mathiasen, M, Rabus, M, Rahvar, S, Ricci, D, Sahu, K, Scarpetta, G, Skottfelt, J, Snodgrass, C, Southworth, J, Surdej, J, Tregloan-Reed, J, Vilela, C, Wertz, O, Williams, A, and Consortium, M
- Subjects
QC ,QB - Abstract
Aims. We present the analysis of 26 nights of V and I time-series observations from 2011 and 2012 of the globular cluster M 30 (NGC 7099). We\ud used our data to search for variable stars in this cluster and refine the periods of known variables; we then used our variable star light curves to\ud derive values for the cluster’s parameters.\ud Methods. We used difference image analysis to reduce our data to obtain high-precision light curves of variable stars. We then estimated the cluster\ud parameters by performing a Fourier decomposition of the light curves of RR Lyrae stars for which a good period estimate was possible. We also\ud derived an estimate for the age of the cluster by fitting theoretical isochrones to our colour-magnitude diagram (CMD).\ud Results. Out of 13 stars previously catalogued as variables, we find that only 4 are bona fide variables. We detect two new RR Lyrae variables,\ud and confirm two additional RR Lyrae candidates from the literature. We also detect four other new variables, including an eclipsing blue straggler\ud system, and an SX Phoenicis star. This amounts to a total number of confirmed variable stars in M 30 of 12. We perform Fourier decomposition of\ud the light curves of the RR Lyrae stars to derive cluster parameters using empirical relations. We find a cluster metallicity [Fe/H]ZW = −2.01±0.04,\ud or [Fe/H]UVES = −2.11 ± 0.06, and a distance of 8.32 ± 0.20 kpc (using RR0 variables), 8.10 kpc (using one RR1 variable), and 8.35 ± 0.42 kpc\ud (using our SX Phoenicis star detection in M 30). Fitting isochrones to the CMD, we estimate an age of 13.0 ± 1.0 Gyr for M 30.
- Published
- 2016
14. Erratum: Estimating the parameters of globular cluster M 30 (NGC 7099) from time-series photometry (Astronomy and Astrophysics (2013) 555 (A36))
- Author
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Kains, N, Bramich, Dm, Arellano Ferro, A, Figuera Jaimes, R, Jorgensen, Ug, Giridhar, S, Penny, Mt, Alsubai, Ka, Andersen, Jm, Bozza, V, Browne, P, Burgdorf, M, Calchi Novati, S, Damerdji, Y, Diehl, C, Dodds, P, Dominik, M, Elyiv, A, Fang, X, Giannini, E, S. -H., G, Hardis, S, Harpsoe, K, Hinse, Tc, Hornstrup, A, Hundertmark, M, Jessen-Hansen, J, Juncher, D, Kerins, E, Kjeldsen, H, Korhonen, H, Liebig, C, Lund, Mn, Lundkvist, M, Mancini, L, Martin, R, Mathiasen, M, Rabus, M, Rahvar, S, Ricci, D, Sahu, K, Scarpetta, G, Skottfelt, J, Snodgrass, C, Southworth, J, Surdej, J, Tregloan-Reed, J, Vilela, C, Wertz, O, and Williams, A
- Subjects
Settore FIS/05 - Astronomia e Astrofisica - Published
- 2016
15. The 2014–2017 outburst of the young star ASASSN-13db
- Author
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Sicilia-Aguilar, A., primary, Oprandi, A., additional, Froebrich, D., additional, Fang, M., additional, Prieto, J. L., additional, Stanek, K., additional, Scholz, A., additional, Kochanek, C. S., additional, Henning, Th., additional, Gredel, R., additional, Holoien, T. W.- S., additional, Rabus, M., additional, Shappee, B. J., additional, Billington, S. J., additional, Campbell-White, J., additional, and Zegmott, T. J., additional
- Published
- 2017
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16. Resolved astrometric orbits of ten O-type binaries
- Author
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Le Bouquin, J.-B., primary, Sana, H., additional, Gosset, E., additional, De Becker, M., additional, Duvert, G., additional, Absil, O., additional, Anthonioz, F., additional, Berger, J.-P., additional, Ertel, S., additional, Grellmann, R., additional, Guieu, S., additional, Kervella, P., additional, Rabus, M., additional, and Willson, M., additional
- Published
- 2017
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17. MiNDSTEp differential photometry of the gravitationally lensed quasars WFI 2033-4723 and HE 0047-1756: microlensing and a new time delay
- Author
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Giannini, E., primary, Schmidt, R. W., additional, Wambsganss, J., additional, Alsubai, K., additional, Andersen, J. M., additional, Anguita, T., additional, Bozza, V., additional, Bramich, D. M., additional, Browne, P., additional, Calchi Novati, S., additional, Damerdji, Y., additional, Diehl, C., additional, Dodds, P., additional, Dominik, M., additional, Elyiv, A., additional, Fang, X., additional, Figuera Jaimes, R., additional, Finet, F., additional, Gerner, T., additional, Gu, S., additional, Hardis, S., additional, Harpsøe, K., additional, Hinse, T. C., additional, Hornstrup, A., additional, Hundertmark, M., additional, Jessen-Hansen, J., additional, Jørgensen, U. G., additional, Juncher, D., additional, Kains, N., additional, Kerins, E., additional, Korhonen, H., additional, Liebig, C., additional, Lund, M. N., additional, Lundkvist, M. S., additional, Maier, G., additional, Mancini, L., additional, Masi, G., additional, Mathiasen, M., additional, Penny, M., additional, Proft, S., additional, Rabus, M., additional, Rahvar, S., additional, Ricci, D., additional, Scarpetta, G., additional, Sahu, K., additional, Schäfer, S., additional, Schönebeck, F., additional, Skottfelt, J., additional, Snodgrass, C., additional, Southworth, J., additional, Surdej, J., additional, Tregloan-Reed, J., additional, Vilela, C., additional, Wertz, O., additional, and Zimmer, F., additional
- Published
- 2016
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18. A census of variability in globular cluster M 68 (NGC 4590)
- Author
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Kains, N, Arellano Ferro, A, Jaimes, RF, Bramich, DM, Skottfelt, J, Jorgensen, UG, Tsapras, Y, Street, RA, Browne, P, Dominik, M, Horne, K, Hundertmark, M, Ipatov, S, Snodgrass, C, Steele, IA, Alsubai, KA, Bozza, V, Novati, SC, Ciceri, S, D'Ago, G, Galianni, P, Gu, S-H, Harpsoe, K, Hinse, TC, Juncher, D, Korhonen, H, Mancini, L, Popovas, A, Rabus, M, Rahvar, S, Southworth, J, Surdej, J, Vilela, C, Wang, X-B, Wertz, O, Consortium, LCOGTR, Consortium, M, The Royal Society, Science & Technology Facilities Council, and University of St Andrews. School of Physics and Astronomy
- Subjects
Metallicity ,Globular clusters: individual: M 68 ,Stars: variables: general ,NDAS ,FOS: Physical sciences ,Astrophysics ,variables: RR Lyrae [Stars] ,RR Lyrae variable ,variables: general [Stars] ,Stars: variables: RR Lyrae ,Astronomy and Astrophysics ,Space and Planetary Science ,Photometry (optics) ,Settore FIS/05 - Astronomia e Astrofisica ,QB Astronomy ,Astrophysics::Solar and Stellar Astrophysics ,Solar and Stellar Astrophysics (astro-ph.SR) ,QC ,Astrophysics::Galaxy Astrophysics ,QB ,Physics ,Light curve ,individual: M 68 [Globular clusters] ,Distance modulus ,Stars ,QC Physics ,Astrophysics - Solar and Stellar Astrophysics ,Globular cluster ,Variable star - Abstract
We analyse 20 nights of CCD observations in the V and I bands of the globular cluster M68 (NGC 4590), using these to detect variable objects. We also obtained electron-multiplying CCD (EMCCD) observations for this cluster in order to explore its core with unprecedented spatial resolution from the ground. We reduced our data using difference image analysis, in order to achieve the best possible photometry in the crowded field of the cluster. In doing so, we showed that when dealing with identical networked telescopes, a reference image from any telescope may be used to reduce data from any other telescope, which facilitates the analysis significantly. We then used our light curves to estimate the properties of the RR Lyrae (RRL) stars in M68 through Fourier decomposition and empirical relations. The variable star properties then allowed us to derive the cluster's metallicity and distance. We determine new periods for the variable stars, and search for new variables, especially in the core of the cluster where our method performs particularly well. We detect an additional 4 SX Phe stars, and confirm the variability of another star, bringing the total number of confirmed variable stars in this cluster to 50. We also used archival data stretching back to 1951 in order to derive period changes for some of the single-mode RRL stars, and analyse the significant number of double-mode RRL stars in M68. Furthermore, we find evidence for double-mode pulsation in one of the SX Phe stars in this cluster. Using the different types of variables, we derived an estimate of the metallicity, [Fe/H]=$-2.07 \pm 0.06$ on the ZW scale, and 4 independent estimates of the distance modulus ($\mu_0 \sim$ 15.00 mag) for this cluster. Thanks to the first use of difference image analysis on time-series observations of M68, we are now confident that we have a complete census of the RRL stars in this cluster., Comment: 25 pages, 18 figures, A&A in press
- Published
- 2015
19. COSMOGRAIL: XVIII. time delays of the quadruply lensed quasar WFI2033−4723.
- Author
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Bonvin, V., Millon, M., Chan, J. H.-H., Courbin, F., Rusu, C. E., Sluse, D., Suyu, S. H., Wong, K. C., Fassnacht, C. D., Marshall, P. J., Treu, T., Buckley-Geer, E., Frieman, J., Hempel, A., Kim, S., Lachaume, R., Rabus, M., Chao, D. C.-Y., Chijani, M., and Gilman, D.
- Subjects
QUASARS ,TIME delay systems ,TIME measurements ,GRAVITATIONAL lenses ,TELESCOPES ,HUBBLE constant - Abstract
We present new measurements of the time delays of WFI2033−4723. The data sets used in this work include 14 years of data taken at the 1.2 m Leonhard Euler Swiss telescope, 13 years of data from the SMARTS 1.3 m telescope at Las Campanas Observatory and a single year of high-cadence and high-precision monitoring at the MPIA 2.2 m telescope. The time delays measured from these different data sets, all taken in the R-band, are in good agreement with each other and with previous measurements from the literature. Combining all the time-delay estimates from our data sets results in Δt
AB = 36.2+0.7 −0.8 Δ t AB = 36. 2 − 0.8 + 0.7 $ \Delta t_{\mathrm{AB}} = 36.2_{-0.8}^{+0.7} $ days (2.1% precision), ΔtAC = −23.3+1.2 −1.4 Δ t AC = − 23. 3 − 1.4 + 1.2 $ \Delta t_{\mathrm{AC}} = -23.3_{-1.4}^{+1.2} $ days (5.6%) and ΔtBC = −59.4+1.3 −1.3 Δ t BC = − 59. 4 − 1.3 + 1.3 $ \Delta t_{\mathrm{BC}} = -59.4_{-1.3}^{+1.3} $ days (2.2%). In addition, the close image pair A1-A2 of the lensed quasars can be resolved in the MPIA 2.2 m data. We measure a time delay consistent with zero in this pair of images. We also explore the prior distributions of microlensing time-delay potentially affecting the cosmological time-delay measurements of WFI2033−4723. Our time-delay measurements are not precise enough to conclude that microlensing time delay is present or absent from the data. This work is part of a H0LiCOW series focusing on measuring the Hubble constant from WFI2033−4723. [ABSTRACT FROM AUTHOR]- Published
- 2019
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20. Erratum: Estimating the parameters of globular cluster M 30 (NGC 7099) from time-series photometry (Astronomy and Astrophysics (2013) 555 (A36))
- Author
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Kains, N., Bramich, D., Arellano Ferro, A., Figuera Jaimes, R., Jørgensen, U., Giridhar, S., Penny, M., Alsubai, K., Andersen, J., Bozza, V., Browne, P., Burgdorf, M., Calchi Novati, S., Damerdji, Y., Diehl, C., Dodds, P., Dominik, M., Elyiv, A., Fang, X., Giannini, E., Gu, S., Hardis, S., Harpsøe, K., Hinse, T., Hornstrup, A., Hundertmark, M., Jessen-Hansen, J., Juncher, D., Kerins, E., Kjeldsen, H., Korhonen, H., Liebig, C., Lund, M., Lundkvist, M., Mancini, L., Martin, R., Mathiasen, M., Rabus, M., Rahvar, S., Ricci, D., Sahu, K., Scarpetta, G., Skottfelt, J., Snodgrass, C., Southworth, J., Surdej, J., Tregloan-Reed, J., Vilela, C., Wertz, O., Williams, Andrew, Kains, N., Bramich, D., Arellano Ferro, A., Figuera Jaimes, R., Jørgensen, U., Giridhar, S., Penny, M., Alsubai, K., Andersen, J., Bozza, V., Browne, P., Burgdorf, M., Calchi Novati, S., Damerdji, Y., Diehl, C., Dodds, P., Dominik, M., Elyiv, A., Fang, X., Giannini, E., Gu, S., Hardis, S., Harpsøe, K., Hinse, T., Hornstrup, A., Hundertmark, M., Jessen-Hansen, J., Juncher, D., Kerins, E., Kjeldsen, H., Korhonen, H., Liebig, C., Lund, M., Lundkvist, M., Mancini, L., Martin, R., Mathiasen, M., Rabus, M., Rahvar, S., Ricci, D., Sahu, K., Scarpetta, G., Skottfelt, J., Snodgrass, C., Southworth, J., Surdej, J., Tregloan-Reed, J., Vilela, C., Wertz, O., and Williams, Andrew
- Published
- 2016
21. High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP)
- Author
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Evans, D. F., primary, Southworth, J., additional, Maxted, P. F. L., additional, Skottfelt, J., additional, Hundertmark, M., additional, Jørgensen, U. G., additional, Dominik, M., additional, Alsubai, K. A., additional, Andersen, M. I., additional, Bozza, V., additional, Bramich, D. M., additional, Burgdorf, M. J., additional, Ciceri, S., additional, D’Ago, G., additional, Figuera Jaimes, R., additional, Gu, S.-H., additional, Haugbølle, T., additional, Hinse, T. C., additional, Juncher, D., additional, Kains, N., additional, Kerins, E., additional, Korhonen, H., additional, Kuffmeier, M., additional, Mancini, L., additional, Peixinho, N., additional, Popovas, A., additional, Rabus, M., additional, Rahvar, S., additional, Schmidt, R. W., additional, Snodgrass, C., additional, Starkey, D., additional, Surdej, J., additional, Tronsgaard, R., additional, von Essen, C., additional, Wang, Yi-Bo, additional, and Wertz, O., additional
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- 2016
- Full Text
- View/download PDF
22. Exploring the crowded central region of ten Galactic globular clusters using EMCCDs
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Figuera Jaimes, R., primary, Bramich, D. M., additional, Skottfelt, J., additional, Kains, N., additional, Jørgensen, U. G., additional, Horne, K., additional, Dominik, M., additional, Alsubai, K. A., additional, Bozza, V., additional, Calchi Novati, S., additional, Ciceri, S., additional, D’Ago, G., additional, Galianni, P., additional, Gu, S.-H., additional, W Harpsøe, K. B., additional, Haugbølle, T., additional, Hinse, T. C., additional, Hundertmark, M., additional, Juncher, D., additional, Korhonen, H., additional, Mancini, L., additional, Popovas, A., additional, Rabus, M., additional, Rahvar, S., additional, Scarpetta, G., additional, Schmidt, R. W., additional, Snodgrass, C., additional, Southworth, J., additional, Starkey, D., additional, Street, R. A., additional, Surdej, J., additional, Wang, X.-B., additional, and Wertz, O., additional
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- 2016
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23. Rotation periods and astrometric motions of the Luhman 16AB brown dwarfs by high-resolution lucky-imaging monitoring
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Mancini, L., primary, Giacobbe, P., additional, Littlefair, S. P., additional, Southworth, J., additional, Bozza, V., additional, Damasso, M., additional, Dominik, M., additional, Hundertmark, M., additional, Jørgensen, U. G., additional, Juncher, D., additional, Popovas, A., additional, Rabus, M., additional, Rahvar, S., additional, Schmidt, R. W., additional, Skottfelt, J., additional, Snodgrass, C., additional, Sozzetti, A., additional, Alsubai, K., additional, Bramich, D. M., additional, Calchi Novati, S., additional, Ciceri, S., additional, D’Ago, G., additional, Figuera Jaimes, R., additional, Galianni, P., additional, Gu, S.-H., additional, Harpsøe, K., additional, Haugbølle, T., additional, Henning, Th., additional, Hinse, T. C., additional, Kains, N., additional, Korhonen, H., additional, Scarpetta, G., additional, Starkey, D., additional, Surdej, J., additional, Wang, X.-B., additional, and Wertz, O., additional
- Published
- 2015
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24. HATS-13b and HATS-14b: two transiting hot Jupiters from the HATSouth survey
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Mancini, L., primary, Hartman, J. D., additional, Penev, K., additional, Bakos, G. Á., additional, Brahm, R., additional, Ciceri, S., additional, Henning, Th., additional, Csubry, Z., additional, Bayliss, D., additional, Zhou, G., additional, Rabus, M., additional, de Val-Borro, M., additional, Espinoza, N., additional, Jordán, A., additional, Suc, V., additional, Bhatti, W., additional, Schmidt, B., additional, Sato, B., additional, Tan, T. G., additional, Wright, D. J., additional, Tinney, C. G., additional, Addison, B. C., additional, Noyes, R. W., additional, Lázár, J., additional, Papp, I., additional, and Sári, P., additional
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- 2015
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25. Strong near-infrared carbon in the Type Ia supernova iPTF13ebh
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Hsiao, E. Y., primary, Burns, C. R., additional, Contreras, C., additional, Höflich, P., additional, Sand, D., additional, Marion, G. H., additional, Phillips, M. M., additional, Stritzinger, M., additional, González-Gaitán, S., additional, Mason, R. E., additional, Folatelli, G., additional, Parent, E., additional, Gall, C., additional, Amanullah, R., additional, Anupama, G. C., additional, Arcavi, I., additional, Banerjee, D. P. K., additional, Beletsky, Y., additional, Blanc, G. A., additional, Bloom, J. S., additional, Brown, P. J., additional, Campillay, A., additional, Cao, Y., additional, De Cia, A., additional, Diamond, T., additional, Freedman, W. L., additional, Gonzalez, C., additional, Goobar, A., additional, Holmbo, S., additional, Howell, D. A., additional, Johansson, J., additional, Kasliwal, M. M., additional, Kirshner, R. P., additional, Krisciunas, K., additional, Kulkarni, S. R., additional, Maguire, K., additional, Milne, P. A., additional, Morrell, N., additional, Nugent, P. E., additional, Ofek, E. O., additional, Osip, D., additional, Palunas, P., additional, Perley, D. A., additional, Persson, S. E., additional, Piro, A. L., additional, Rabus, M., additional, Roth, M., additional, Schiefelbein, J. M., additional, Srivastav, S., additional, Sullivan, M., additional, Suntzeff, N. B., additional, Surace, J., additional, Woźniak, P. R., additional, and Yaron, O., additional
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- 2015
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26. Physical properties of the WASP-67 planetary system from multi-colour photometry
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Mancini, L., primary, Southworth, J., additional, Ciceri, S., additional, Calchi Novati, S., additional, Dominik, M., additional, Henning, Th., additional, Jørgensen, U. G., additional, Korhonen, H., additional, Nikolov, N., additional, Alsubai, K. A., additional, Bozza, V., additional, Bramich, D. M., additional, D’Ago, G., additional, Figuera Jaimes, R., additional, Galianni, P., additional, Gu, S.-H., additional, Harpsøe, K., additional, Hinse, T. C., additional, Hundertmark, M., additional, Juncher, D., additional, Kains, N., additional, Popovas, A., additional, Rabus, M., additional, Rahvar, S., additional, Skottfelt, J., additional, Snodgrass, C., additional, Street, R., additional, Surdej, J., additional, Tsapras, Y., additional, Vilela, C., additional, Wang, X.-B., additional, and Wertz, O., additional
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- 2014
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27. Orbital and physical parameters of eclipsing binaries from the All-Sky Automated Survey catalogue
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Hełminiak, K. G., primary, Brahm, R., additional, Ratajczak, M., additional, Espinoza, N., additional, Jordán, A., additional, Konacki, M., additional, and Rabus, M., additional
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- 2014
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28. Physical properties and transmission spectrum of the WASP-80 planetary system from multi-colour photometry
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Mancini, L., primary, Southworth, J., additional, Ciceri, S., additional, Dominik, M., additional, Henning, Th., additional, Jørgensen, U. G., additional, Lanza, A. F., additional, Rabus, M., additional, Snodgrass, C., additional, Vilela, C., additional, Alsubai, K. A., additional, Bozza, V., additional, Bramich, D. M., additional, Calchi Novati, S., additional, D’Ago, G., additional, Figuera Jaimes, R., additional, Galianni, P., additional, Gu, S.-H., additional, Harpsøe, K., additional, Hinse, T., additional, Hundertmark, M., additional, Juncher, D., additional, Kains, N., additional, Korhonen, H., additional, Popovas, A., additional, Rahvar, S., additional, Skottfelt, J., additional, Street, R., additional, Surdej, J., additional, Tsapras, Y., additional, Wang, X.-B., additional, and Wertz, O., additional
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- 2014
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29. Estimating the parameters of globular cluster M 30 (NGC 7099) from time-series photometry
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Kains, N., Bramich, D., Arellano Ferro, A., Figuera Jaimes, R., Jørgensen, U., Giridhar, S., Penny, M., Alsubai, K., Andersen, J., Bozza, V., Browne, P., Burgdorf, M., Calchi Novati, S., Damerdji, Y., Diehl, C., Dodds, P., Dominik, M., Elyiv, A., Fang, X., Giannini, E., Gu, S., Hardis, S., Harpsoe, K., Hinse, T., Hornstrup, A., Hundertmark, M., Jessen-Hansen, J., Juncher, D., Kerins, E., Kjeldsen, H., Korhonen, H., Liebig, C., Lund, M., Lundkvist, M., Mancini, L., Martin, R., Mathiasen, M., Rabus, M., Rahvar, S., Ricci, D., Sahu, K., Scarpetta, G., Skottfelt, J., Snodgrass, C., Southworth, J., Surdej, J., Tregloan-Reed, J., Vilela, C., Wertz, O., Williams, Andrew, Kains, N., Bramich, D., Arellano Ferro, A., Figuera Jaimes, R., Jørgensen, U., Giridhar, S., Penny, M., Alsubai, K., Andersen, J., Bozza, V., Browne, P., Burgdorf, M., Calchi Novati, S., Damerdji, Y., Diehl, C., Dodds, P., Dominik, M., Elyiv, A., Fang, X., Giannini, E., Gu, S., Hardis, S., Harpsoe, K., Hinse, T., Hornstrup, A., Hundertmark, M., Jessen-Hansen, J., Juncher, D., Kerins, E., Kjeldsen, H., Korhonen, H., Liebig, C., Lund, M., Lundkvist, M., Mancini, L., Martin, R., Mathiasen, M., Rabus, M., Rahvar, S., Ricci, D., Sahu, K., Scarpetta, G., Skottfelt, J., Snodgrass, C., Southworth, J., Surdej, J., Tregloan-Reed, J., Vilela, C., Wertz, O., and Williams, Andrew
- Abstract
Aims. We present the analysis of 26 nights of V and I time-series observations from 2011 and 2012 of the globular cluster M30 (NGC 7099). Weused our data to search for variable stars in this cluster and refine the periods of known variables; we then used our variable star light curves toderive values for the cluster’s parameters.Methods. We used difference image analysis to reduce our data to obtain high-precision light curves of variable stars.We then estimated the clusterparameters by performing a Fourier decomposition of the light curves of RR Lyrae stars for which a good period estimate was possible. We alsoderived an estimate for the age of the cluster by fitting theoretical isochrones to our colour-magnitude diagram (CMD).Results. Out of 13 stars previously catalogued as variables, we find that only 4 are bona fide variables. We detect two new RR Lyrae variables,and confirm two additional RR Lyrae candidates from the literature. We also detect four other new variables, including an eclipsing blue stragglersystem, and an SX Phoenicis star. This amounts to a total number of confirmed variable stars in M30 of 12. We perform Fourier decomposition ofthe light curves of the RR Lyrae stars to derive cluster parameters using empirical relations.We find a cluster metallicity [Fe/H]ZW = -2.01±0.04,or [Fe/H]UVES = -2.11 ± 0.06, and a distance of 8.32 ± 0.20 kpc (using RR0 variables), 8.10 kpc (using one RR1 variable), and 8.35 ± 0.42 kpc(using our SX Phoenicis star detection in M30). Fitting isochrones to the CMD, we estimate an age of 13.0 ± 1.0 Gyr for M30.
- Published
- 2013
30. EMCCD photometry reveals two new variable stars in the crowded central region of the globular cluster NGC 6981
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Skottfelt, J., Bramich, D., Figuera Jaimes, R., Jorgensen, U., Kains, N., Harpsoe, K., Liebig, C., Penny, M., Alsubai, K., Andersen, J., Bozza, V., Browne, P., Calchi Novati, S., Damerdji, Y., Diehl, C., Dominik, M., Elyiv, A., Giannini, E., Hessman, F., Hinse, T., Hundertmark, M., Juncher, D., Kerins, E., Korhonen, H., Mancini, L., Martin, R., Rabus, M., Rahvar, S., Scarpetta, G., Southworth, J., Snodgrass, C., Street, R., Surdej, J., Tregloan-Reed, J., Vilela, C., Williams, Andrew, Skottfelt, J., Bramich, D., Figuera Jaimes, R., Jorgensen, U., Kains, N., Harpsoe, K., Liebig, C., Penny, M., Alsubai, K., Andersen, J., Bozza, V., Browne, P., Calchi Novati, S., Damerdji, Y., Diehl, C., Dominik, M., Elyiv, A., Giannini, E., Hessman, F., Hinse, T., Hundertmark, M., Juncher, D., Kerins, E., Korhonen, H., Mancini, L., Martin, R., Rabus, M., Rahvar, S., Scarpetta, G., Southworth, J., Snodgrass, C., Street, R., Surdej, J., Tregloan-Reed, J., Vilela, C., and Williams, Andrew
- Abstract
Two previously unknown variable stars in the crowded central region of the globular cluster NGC 6981 are presented. The observations were made using the electron multiplying CCD (EMCCD) camera at the Danish 1.54 m Telescope at La Silla, Chile. The two variables were not previously detected by conventional CCD imaging because of their proximity to a bright star. This discovery demonstrates that EMCCDs are a powerful tool for performing high-precision time-series photometry in crowded fields and near bright stars, especially when combined with difference image analysis.
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- 2013
31. HATS-2b: A transiting extrasolar planet orbiting aK-type star showing starspot activity
- Author
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Mohler-Fischer, M., primary, Mancini, L., additional, Hartman, J. D., additional, Bakos, G. Á., additional, Penev, K., additional, Bayliss, D., additional, Jordán, A., additional, Csubry, Z., additional, Zhou, G., additional, Rabus, M., additional, Nikolov, N., additional, Brahm, R., additional, Espinoza, N., additional, Buchhave, L. A., additional, Béky, B., additional, Suc, V., additional, Csák, B., additional, Henning, T., additional, Wright, D. J., additional, Tinney, C. G., additional, Addison, B. C., additional, Schmidt, B., additional, Noyes, R. W., additional, Papp, I., additional, Lázár, J., additional, Sári, P., additional, and Conroy, P., additional
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- 2013
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32. EMCCD photometry reveals two new variable stars in the crowded central region of the globular cluster NGC 6981 (Corrigendum)
- Author
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Skottfelt, J., primary, Bramich, D. M., additional, Figuera Jaimes, R., additional, Jørgensen, U. G., additional, Kains, N., additional, W Harpsøe, K. B., additional, Liebig, C., additional, Penny, M. T., additional, Alsubai, K. A., additional, Andersen, J. M., additional, Bozza, V., additional, Browne, P., additional, Calchi Novati, S., additional, Damerdji, Y., additional, Diehl, C., additional, Dominik, M., additional, Elyiv, A., additional, Giannini, E., additional, Hessman, F., additional, Hinse, T. C., additional, Hundertmark, M., additional, Juncher, D., additional, Kerins, E., additional, Korhonen, H., additional, Mancini, L., additional, Martin, R., additional, Rabus, M., additional, Rahvar, S., additional, Scarpetta, G., additional, Southworth, J., additional, Snodgrass, C., additional, Street, R. A., additional, Surdej, J., additional, Tregloan-Reed, J., additional, Vilela, C., additional, and Williams, A., additional
- Published
- 2013
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33. Planetary transit candidates in the CoRoT-SRc01 field
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Erikson, A., primary, Santerne, A., additional, Renner, S., additional, Barge, P., additional, Aigrain, S., additional, Alapini, A., additional, Almenara, J.-M., additional, Alonso, R., additional, Auvergne, M., additional, Baglin, A., additional, Benz, W., additional, Bonomo, A. S., additional, Bordé, P., additional, Bouchy, F., additional, Bruntt, H., additional, Cabrera, J., additional, Carone, L., additional, Carpano, S., additional, Csizmadia, Sz., additional, Deleuil, M., additional, Deeg, H. J., additional, Díaz, R. F., additional, Dvorak, R., additional, Ferraz-Mello, S., additional, Fridlund, M., additional, Gandolfi, D., additional, Gazzano, J.-C., additional, Gillon, M., additional, Guenther, E. W., additional, Guillot, T., additional, Hatzes, A., additional, Hébrard, G., additional, Jorda, L., additional, Lammer, H., additional, Léger, A., additional, Llebaria, A., additional, Mayor, M., additional, Mazeh, T., additional, Moutou, C., additional, Ollivier, M., additional, Ofir, A., additional, Pätzold, M., additional, Pepe, F., additional, Pont, F., additional, Queloz, D., additional, Rabus, M., additional, Rauer, H., additional, Régulo, C., additional, Rouan, D., additional, Samuel, B., additional, Schneider, J., additional, Shporer, A., additional, Tingley, B., additional, Udry, S., additional, and Wuchterl, G., additional
- Published
- 2012
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34. Planetary transit candidates in the CoRoT LRa01 field
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Carone, L., primary, Gandolfi, D., additional, Cabrera, J., additional, Hatzes, A. P., additional, Deeg, H. J., additional, Csizmadia, Sz., additional, Pätzold, M., additional, Weingrill, J., additional, Aigrain, S., additional, Alonso, R., additional, Alapini, A., additional, Almenara, J.-M., additional, Auvergne, M., additional, Baglin, A., additional, Barge, P., additional, Bonomo, A. S., additional, Bordé, P., additional, Bouchy, F., additional, Bruntt, H., additional, Carpano, S., additional, Cochran, W. D., additional, Deleuil, M., additional, Díaz, R. F., additional, Dreizler, S., additional, Dvorak, R., additional, Eislöffel, J., additional, Eigmüller, P., additional, Endl, M., additional, Erikson, A., additional, Ferraz-Mello, S., additional, Fridlund, M., additional, Gazzano, J.-C., additional, Gibson, N., additional, Gillon, M., additional, Gondoin, P., additional, Grziwa, S., additional, Günther, E. W., additional, Guillot, T., additional, Hartmann, M., additional, Havel, M., additional, Hébrard, G., additional, Jorda, L., additional, Kabath, P., additional, Léger, A., additional, Llebaria, A., additional, Lammer, H., additional, Lovis, C., additional, MacQueen, P. J., additional, Mayor, M., additional, Mazeh, T., additional, Moutou, C., additional, Nortmann, L., additional, Ofir, A., additional, Ollivier, M., additional, Parviainen, H., additional, Pepe, F., additional, Pont, F., additional, Queloz, D., additional, Rabus, M., additional, Rauer, H., additional, Régulo, C., additional, Renner, S., additional, de la Reza, R., additional, Rouan, D., additional, Santerne, A., additional, Samuel, B., additional, Schneider, J., additional, Shporer, A., additional, Stecklum, B., additional, Tal-Or, L., additional, Tingley, B., additional, Udry, S., additional, and Wuchterl, G., additional
- Published
- 2012
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35. Transit timing analysis of the exoplanets TrES-1 and TrES-2
- Author
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Rabus, M., primary, Deeg, H. J., additional, Alonso, R., additional, Belmonte, J. A., additional, and Almenara, J. M., additional
- Published
- 2009
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36. Transiting exoplanets from the CoRoT space mission
- Author
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Rauer, H., primary, Queloz, D., additional, Csizmadia, Sz., additional, Deleuil, M., additional, Alonso, R., additional, Aigrain, S., additional, Almenara, J. M., additional, Auvergne, M., additional, Baglin, A., additional, Barge, P., additional, Bordé, P., additional, Bouchy, F., additional, Bruntt, H., additional, Cabrera, J., additional, Carone, L., additional, Carpano, S., additional, De la Reza, R., additional, Deeg, H. J., additional, Dvorak, R., additional, Erikson, A., additional, Fridlund, M., additional, Gandolfi, D., additional, Gillon, M., additional, Guillot, T., additional, Guenther, E., additional, Hatzes, A., additional, Hébrard, G., additional, Kabath, P., additional, Jorda, L., additional, Lammer, H., additional, Léger, A., additional, Llebaria, A., additional, Magain, P., additional, Mazeh, T., additional, Moutou, C., additional, Ollivier, M., additional, Pätzold, M., additional, Pont, F., additional, Rabus, M., additional, Renner, S., additional, Rouan, D., additional, Shporer, A., additional, Samuel, B., additional, Schneider, J., additional, Triaud, A. H. M. J., additional, and Wuchterl, G., additional
- Published
- 2009
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37. Planetary transit candidates in CoRoT-LRc01 field
- Author
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Cabrera, J., primary, Fridlund, M., additional, Ollivier, M., additional, Gandolfi, D., additional, Csizmadia, Sz., additional, Alonso, R., additional, Aigrain, S., additional, Alapini, A., additional, Almenara, J.-M., additional, Barge, P., additional, Bonomo, A. S., additional, Bordé, P., additional, Bouchy, F., additional, Bruntt, H., additional, Carone, L., additional, Carpano, S., additional, Deeg, H. J., additional, De la Reza, R., additional, Deleuil, M., additional, Dvorak, R., additional, Erikson, A., additional, Gillon, M., additional, Gondoin, P., additional, Guenther, E. W., additional, Guillot, T., additional, Hartmann, M., additional, Hatzes, A., additional, Hebrard, G., additional, Jorda, L., additional, Lammer, H., additional, Léger, A., additional, Llebaria, A., additional, Lovis, C., additional, Magain, P., additional, Mayor, M., additional, Mazeh, T., additional, Moutou, C., additional, Ofir, A., additional, Pätzold, M., additional, Pepe, F., additional, Pont, F., additional, Queloz, D., additional, Rabus, M., additional, Rauer, H., additional, Régulo, C., additional, Renner, S., additional, Rouan, D., additional, Samuel, B., additional, Santerne, A., additional, Schneider, J., additional, Shporer, A., additional, Stecklum, B., additional, Tingley, B., additional, Udry, S., additional, and Wuchterl, G., additional
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- 2009
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38. Ground-based photometry of space-based transit detections: photometric follow-up of the CoRoT mission
- Author
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Deeg, H. J., primary, Gillon, M., additional, Shporer, A., additional, Rouan, D., additional, Stecklum, B., additional, Aigrain, S., additional, Alapini, A., additional, Almenara, J. M., additional, Alonso, R., additional, Barbieri, M., additional, Bouchy, F., additional, Eislöffel, J., additional, Erikson, A., additional, Fridlund, M., additional, Eigmüller, P., additional, Handler, G., additional, Hatzes, A., additional, Kabath, P., additional, Lendl, M., additional, Mazeh, T., additional, Moutou, C., additional, Queloz, D., additional, Rauer, H., additional, Rabus, M., additional, Tingley, B., additional, and Titz, R., additional
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- 2009
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39. Planetary transit candidates in the CoRoT initial run: resolving their nature
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Moutou, C., primary, Pont, F., additional, Bouchy, F., additional, Deleuil, M., additional, Almenara, J. M., additional, Alonso, R., additional, Barbieri, M., additional, Bruntt, H., additional, Deeg, H. J., additional, Fridlund, M., additional, Gandolfi, D., additional, Gillon, M., additional, Guenther, E., additional, Hatzes, A., additional, Hébrard, G., additional, Loeillet, B., additional, Mayor, M., additional, Mazeh, T., additional, Queloz, D., additional, Rabus, M., additional, Rouan, D., additional, Shporer, A., additional, Udry, S., additional, Aigrain, S., additional, Auvergne, M., additional, Baglin, A., additional, Barge, P., additional, Benz, W., additional, Bordé, P., additional, Carpano, S., additional, De la Reza, R., additional, Dvorak, R., additional, Erikson, A., additional, Gondoin, P., additional, Guillot, T., additional, Jorda, L., additional, Kabath, P., additional, Lammer, H., additional, Léger, A., additional, Llebaria, A., additional, Lovis, C., additional, Magain, P., additional, Ollivier, M., additional, Pätzold, M., additional, Pepe, F., additional, Rauer, H., additional, Schneider, J., additional, and Wuchterl, G., additional
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- 2009
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40. A cool starspot or a second transiting planet in the TrES-1 system?
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Rabus, M., primary, Alonso, R., additional, Belmonte, J. A., additional, Deeg, H. J., additional, Gilliland, R. L., additional, Almenara, J. M., additional, Brown, T. M., additional, Charbonneau, D., additional, and Mandushev, G., additional
- Published
- 2008
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41. Transiting exoplanets from the CoRoT space mission
- Author
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Moutou, C., primary, Bruntt, H., additional, Guillot, T., additional, Shporer, A., additional, Guenther, E., additional, Aigrain, S., additional, Almenara, J. M., additional, Alonso, R., additional, Auvergne, M., additional, Baglin, A., additional, Barbieri, M., additional, Barge, P., additional, Benz, W., additional, Bordé, P., additional, Bouchy, F., additional, Deeg, H. J., additional, De la Reza, R., additional, Deleuil, M., additional, Dvorak, R., additional, Erikson, A., additional, Fridlund, M., additional, Gillon, M., additional, Gondoin, P., additional, Hatzes, A., additional, Hébrard, G., additional, Jorda, L., additional, Kabath, P., additional, Lammer, H., additional, Léger, A., additional, Llebaria, A., additional, Loeillet, B., additional, Magain, P., additional, Mayor, M., additional, Mazeh, T., additional, Ollivier, M., additional, Pätzold, M., additional, Pepe, F., additional, Pont, F., additional, Queloz, D., additional, Rabus, M., additional, Rauer, H., additional, Rouan, D., additional, Schneider, J., additional, Udry, S., additional, and Wuchterl, G., additional
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- 2008
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42. Misaligned spin-orbit in the XO-3 planetary system?
- Author
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Hébrard, G., primary, Bouchy, F., additional, Pont, F., additional, Loeillet, B., additional, Rabus, M., additional, Bonfils, X., additional, Moutou, C., additional, Boisse, I., additional, Delfosse, X., additional, Desort, M., additional, Eggenberger, A., additional, Ehrenreich, D., additional, Forveille, T., additional, Lagrange, A.-M., additional, Lovis, C., additional, Mayor, M., additional, Pepe, F., additional, Perrier, C., additional, Queloz, D., additional, Santos, N. C., additional, Ségransan, D., additional, Udry, S., additional, and Vidal-Madjar, A., additional
- Published
- 2008
- Full Text
- View/download PDF
43. Limits to the planet candidate GJ 436c
- Author
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Alonso, R., primary, Barbieri, M., additional, Rabus, M., additional, Deeg, H. J., additional, Belmonte, J. A., additional, and Almenara, J. M., additional
- Published
- 2008
- Full Text
- View/download PDF
44. HATS-2b: A transiting extrasolar planet orbiting a K-type star showing starspot activity.
- Author
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Mohler-Fischer, M., Mancini, L., Hartman, J. D., Bakos, G. Á., Penev, K., Bayliss, D., Jordán, A., Csubry, Z., Zhou, G., Rabus, M., Nikolov, N., Brahm, R., Espinoza, N., Buchhave, L. A., Béky, B., Suc, V., Csák, B., Henning, T., Wright, D. J., and Tinney, C. G.
- Subjects
EXTRASOLAR planets ,K stars ,WAVELENGTHS ,LIGHT curves ,PARAMETER estimation - Abstract
We report the discovery of HATS-2b, the second transiting extrasolar planet detected by the HATSouth survey. HATS-2b is moving on a circular orbit around a V = 13:6 mag, K-type dwarf star (GSC 6665-00236), at a separation of 0:0230 ± 0:0003 AU and with a period of 1:3541 days. The planetary parameters have been robustly determined using a simultaneous fit of the HATSouth, MPG/ESO 2.2m/GROND, Faulkes Telescope South/Spectral transit photometry, and MPG/ESO 2.2m/FEROS, Euler 1.2m/CORALIE, AAT 3.9m/CYCLOPS radial-velocity measurements. HATS-2b has a mass of 1:37 ± 0:16 MJ, a radius of 1:14 ± 0:03 RJ, and an equilibrium temperature of 1567 ± 30 K. The host star has a mass of 0:88 ± 0:04 M☉ and a radius of 0:89 ± 0:02 R☉, and it shows starspot activity. We characterized the stellar activity by analyzing two photometric follow-up transit light curves taken with the GROND instrument, both obtained simultaneously in four optical bands (covering the wavelength range of 3860-9520 Å). The two light curves contain anomalies compatible with starspots on the photosphere of the host star along the same transit chord. [ABSTRACT FROM AUTHOR]
- Published
- 2013
- Full Text
- View/download PDF
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