Zobrazeno 1 - 10
of 305
pro vyhledávání: '"Mommert M"'
Autor:
Strauss, R., Trilling, D. E., Bernardinelli, P. H., Beach, C., Oldroyd, W. J., Sheppard, S. S., Schlichting, H. E., Gerdes, D. W., Adams, F. C., Chandler, C. O., Fuentes, C., Holman, M. J., Jurić, M., Lin, H. W., Markwardt, L., McNeill, A., Mommert, M., Napier, K. J., Payne, M. J., Ragozzine, D., Rivkin, A. S., Smotherman, H., Trujillo, C. A.
We present the methods and results from the discovery and photometric measurement of 26 bright (VR $>$ 24 trans-Neptunian objects (TNOs) during the first year (2019-20) of the DECam Ecliptic Exploration Project (DEEP). The DEEP survey is an observati
Externí odkaz:
http://arxiv.org/abs/2309.04034
Autor:
Farkas-Takács, A., Kiss, Cs., Vilenius, E., Marton, G., Müller, T. G., Mommert, M., Stansberry, J., Lellouch, E., Lacerda, P., Pál, A.
Publikováno v:
A&A 638, A23 (2020)
The goal of this work is to determine the physical characteristics of resonant, detached and scattered disk objects in the transneptunian region, observed mainly in the framework of the "TNOs are Cool!" Herschel Open Time Key Program. Based on therma
Externí odkaz:
http://arxiv.org/abs/2002.12712
The {\it Transiting Exoplanet Survey Satellite} (TESS) searches for planets transiting bright and nearby stars using high-cadence, large-scale photometric observations. Full Frame Images provided by the TESS mission include large number of serendipit
Externí odkaz:
http://arxiv.org/abs/1911.01495
Autor:
Vilenius, E., Stansberry, J., Müller, T., Mueller, M., Kiss, C., Santos-Sanz, P., Mommert, M., Pál, A., Lellouch, E., Ortiz, J. L., Peixinho, N., Thirouin, A., Lykawka, P. S., Horner, J., Duffard, R., Fornasier, S., Delsanti, A.
Publikováno v:
Astronomy and Astrophysics, Vol. 618, 2018, A136
A group of trans-Neptunian objects (TNO) are dynamically related to the dwarf planet 136108 Haumea. Ten of them show strong indications of water ice on their surfaces, are assumed to have resulted from a collision, and are accepted as the only known
Externí odkaz:
http://arxiv.org/abs/1904.06333
We present here multi-band photometry for over 2000 Main-belt asteroids. For each target we report the probabilistic taxonomy using the measured V-R and V-I colors in combination with a machine-learning generated decision surface in color-color space
Externí odkaz:
http://arxiv.org/abs/1903.08019
Autor:
Snodgrass, C., Carry, B., Berthier, J., Eggl, S., Mommert, M., Petit, J. -M., Spoto, F., Granvik, M., Laureijs, R., Altieri, B., Vavrek, R., Conversi, L., Nucita, A., Popescu, M., Kleijn, G. Verdoes, Kidger, M., Jones, G. H., Oszkiewicz, D., Juric, M., Jones, L.
The ESA Euclid mission is a space telescope that will survey ~15,000 square degrees of the sky, primarily to study the distant universe (constraining cosmological parameters through the lensing of galaxies). It is also expected to observe ~150,000 So
Externí odkaz:
http://arxiv.org/abs/1812.00607
Autor:
Müller, T., Kiss, Cs., Ali-Lagoa, V., Ortiz, J. L., Lellouch, E., Santos-Sanz, P., Fornasier, S., Marton, G., Mommert, M., Farkas-Takacs, A., Thirouin, A., Vilenius, E.
A recent occultation measurement of the dwarf planet Haumea (Ortiz et al. 2017) revealed an elongated shape with the longest axis comparable to Pluto's mean diameter. The chords also indicate a ring around Haumea's equatorial plane, where its largest
Externí odkaz:
http://arxiv.org/abs/1811.09476
Autor:
Trilling, DE, Mommert, M, Hora, JL, Farnocchia, D, Chodas, P, Giorgini, J, Smith, HA, Carey, S, Lisse, CM, Werner, M, McNeill, A, Chesley, SR, Emery, JP, Fazio, G, Fernandez, YR, Harris, A, Marengo, M, Mueller, M, Roegge, A, Smith, N, Weaver, HA, Meech, K, Micheli, M
Publikováno v:
Published in the Astronomical Journal, 156, 261 (2018)
1I/`Oumuamua is the first confirmed interstellar body in our Solar System. Here we report on observations of `Oumuamua made with the Spitzer Space Telescope on 2017 November 21--22 (UT). We integrated for 30.2~hours at 4.5 micron (IRAC channel 2). We
Externí odkaz:
http://arxiv.org/abs/1811.08072
We present VRI spectrophotometry of 1003 Main-Belt Asteroids (MBAs) observed with the Sutherland, South Africa, node of the Korea Microlensing Telescope Network (KMTNet). All of the observed MBAs were serendipitously captured in KMTNet's large 2deg $
Externí odkaz:
http://arxiv.org/abs/1805.04478
Autor:
Cibulková, H., Nortunen, H., Ďurech, J., Kaasalainen, M., Vereš, P., Jedicke, R., Wainscoat, R. J., Mommert, M., Trilling, D. E., Schunová-Lilly, E., Magnier, E. A., Waters, C., Flewelling, H.
Publikováno v:
A&A 611, A86 (2018)
Context. A lot of photometric data is produced by surveys such as Pan-STARRS, LONEOS, WISE or Catalina. These data are a rich source of information about the physical properties of asteroids. There are several possible approaches for utilizing these
Externí odkaz:
http://arxiv.org/abs/1709.05640