Zobrazeno 1 - 10
of 412
pro vyhledávání: '"Goessl C"'
Autor:
Queirolo, G., Seitz, S., Riffeser, A., Kluge, M., Bender, R., Gössl, C., Hopp, U., Ries, C., Schmidt, M., Zöller, R.
The goal of this work is to obtain a Hubble constant estimate through the study of the quadruply lensed, variable QSO SDSSJ1433+6007. To achieve this we combine multi-filter, archival $\textit{HST}$ data for lens modelling and a dedicated time delay
Externí odkaz:
http://arxiv.org/abs/2312.09311
Autor:
Borsato, N. W., Hoeijmakers, H. J., Cont, D., Kitzmann, D., Ehrhardt, J., Gössl, C., Ries, C., Prinoth, B., Molaverdikhani, K., Ercolano, B., Kellerman, H., Heng, Kevin
When observing transmission spectra produced by atmospheres of ultra-hot Jupiters, large telescopes are typically the instrument of choice due to the very weak signal of the planet's atmosphere. This study aims to alleviate the desire for large teles
Externí odkaz:
http://arxiv.org/abs/2308.05149
We explore several ways to dissect Brightest Cluster Galaxies (BCGs) and their surrounding Intracluster Light (ICL) using a surface brightness cut, a luminosity cut, excess light above a de Vaucouleurs profile, or a double S\'ersic decomposition. Ass
Externí odkaz:
http://arxiv.org/abs/2011.12992
Autor:
Kluge, M., Neureiter, B., Riffeser, A., Bender, R., Goessl, C., Hopp, U., Schmidt, M., Ries, C., Brosch, N.
Publikováno v:
The Astrophysical Journal Supplement Series, Volume 247, Issue 2, id.43, 34 pp. (2020)
Observations of 170 local ($z\lesssim0.08$) galaxy clusters in the northern hemisphere have been obtained with the Wendelstein Telescope Wide Field Imager (WWFI). We correct for systematic effects such as point-spread function broadening, foreground
Externí odkaz:
http://arxiv.org/abs/1908.08544
Autor:
Chambers, K. C., Magnier, E. A., Metcalfe, N., Flewelling, H. A., Huber, M. E., Waters, C. Z., Denneau, L., Draper, P. W., Farrow, D., Finkbeiner, D. P., Holmberg, C., Koppenhoefer, J., Price, P. A., Rest, A., Saglia, R. P., Schlafly, E. F., Smartt, S. J., Sweeney, W., Wainscoat, R. J., Burgett, W. S., Chastel, S., Grav, T., Heasley, J. N., Hodapp, K. W., Jedicke, R., Kaiser, N., Kudritzki, R. -P., Luppino, G. A., Lupton, R. H., Monet, D. G., Morgan, J. S., Onaka, P. M., Shiao, B., Stubbs, C. W., Tonry, J. L., White, R., Bañados, E., Bell, E. F., Bender, R., Bernard, E. J., Boegner, M., Boffi, F., Botticella, M. T., Calamida, A., Casertano, S., Chen, W. -P., Chen, X., Cole, S., Deacon, N., Frenk, C., Fitzsimmons, A., Gezari, S., Gibbs, V., Goessl, C., Goggia, T., Gourgue, R., Goldman, B., Grant, P., Grebel, E. K., Hambly, N. C., Hasinger, G., Heavens, A. F., Heckman, T. M., Henderson, R., Henning, T., Holman, M., Hopp, U., Ip, W. -H., Isani, S., Jackson, M., Keyes, C. D., Koekemoer, A. M., Kotak, R., Le, D., Liska, D., Long, K. S., Lucey, J. R., Liu, M., Martin, N. F., Masci, G., McLean, B., Mindel, E., Misra, P., Morganson, E., Murphy, D. N. A., Obaika, A., Narayan, G., Nieto-Santisteban, M. A., Norberg, P., Peacock, J. A., Pier, E. A., Postman, M., Primak, N., Rae, C., Rai, A., Riess, A., Riffeser, A., Rix, H. W., Röser, S., Russel, R., Rutz, L., Schilbach, E., Schultz, A. S. B., Scolnic, D., Strolger, L., Szalay, A., Seitz, S., Small, E., Smith, K. W., Soderblom, D. R., Taylor, P., Thomson, R., Taylor, A. N., Thakar, A. R., Thiel, J., Thilker, D., Unger, D., Urata, Y., Valenti, J., Wagner, J., Walder, T., Walter, F., Watters, S. P., Werner, S., Wood-Vasey, W. M., Wyse, R.
Pan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the $3\pi$ Steradian Survey and the Medium Deep Survey in 5 bands ($grizy_{P1}$). The mean 5$\sigma$ point source limiting sensitivities in the stacked 3$\pi$ Sterad
Externí odkaz:
http://arxiv.org/abs/1612.05560
Akademický článek
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Autor:
Lee, C. -H., Koppenhoefer, J., Seitz, S., Bender, R., Riffeser, A., Kodric, M., Hopp, U., Snigula, J., Goessl, C., Kudritzki, R. -P., Burgett, W., Chambers, K., Hodapp, K., Kaiser, N., Waters, C.
The goal of this work is to conduct a photometric study of eclipsing binaries in M31. We apply a modified box-fitting algorithm to search for eclipsing binary candidates and determine their period. We classify these candidates into detached, semi-det
Externí odkaz:
http://arxiv.org/abs/1411.1115
Autor:
Lee, C. -H., Seitz, S., Kodric, M., Riffeser, A., Koppenhoefer, J., Bender, R., Snigula, J., Hopp, U., Goessl, C., Bianchi, L., Price, P. A., Fraser, M., Burgett, W., Chambers, K. C., Draper, P. W., Flewelling, H., Kaiser, N., Kudritzki, R. -P., Magnier, E. A.
We perform a study on the optical and infrared photometric properties of known luminous blue variables (LBVs) in M31 using the sample of LBV candidates from the Local Group Galaxy Survey (Massey et al. 2007). We find that M31 LBV candidates show phot
Externí odkaz:
http://arxiv.org/abs/1403.6859
Autor:
Lee, C. -H., Kodric, M., Seitz, S., Riffeser, A., Koppenhoefer, J., Bender, R., Hopp, U., Goessl, C., Snigula, J., Burgett, W. S., Chambers, K. C., Flewelling, H., Hodapp, K. W., Kaiser, N., Kudritzki, R. -P., Price, P. A., Tonry, J. L., Wainscoat, R. J.
Publikováno v:
2013, ApJ, 777, 35
We present a sample of M31 beat Cepheids from the Pan-STARRS 1 PAndromeda campaign. By analyzing three years of PAndromeda data, we identify seventeen beat Cepheids, spreading from a galactocentric distance of 10 to 16 kpc. Since the relation between
Externí odkaz:
http://arxiv.org/abs/1308.6576
Autor:
Robson, M.E. *, Tung, N., Conte, P., Im, S.-A., Senkus, E., Xu, B., Masuda, N., Delaloge, S., Li, W., Armstrong, A., Wu, W., Goessl, C., Runswick, S. †, Domchek, S.M.
Publikováno v:
In Annals of Oncology April 2019 30(4):558-566
