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pro vyhledávání: '"Roche, Paul"'
Autor:
Roche, Paul, Certon, Dominique, Calle, Samuel, Bunetel, Jean-Charles Le, Poulin-Vittrant, Guylaine, Nadaud, Kevin
Publikováno v:
In Sensors and Actuators: A. Physical 1 December 2024 379
Autor:
Roche, Paul, Nadaud, Kevin, Galayko, Dimitri, Calle, Samuel, Barcella, Flavien, Bunetel, Jean-Charles Le, Certon, Dominique, Poulin-Vittrant, Guylaine
Publikováno v:
In Sensors and Actuators: A. Physical 1 December 2024 379
Autor:
Hsieh, Henry H., Chandler, Colin O., Denneau, Larry, Fitzsimmons, Alan, Erasmus, Nicolas, Kelley, Michael S. P., Knight, Matthew M., Lister, Tim A., Pittichova, Jana, Sheppard, Scott S., Thirouin, Audrey, Trujillo, Chadwick A., Usher, Helen, Gomez, Edward, Chatelain, Joey, Greenstreet, Sarah, Angel, Tony, Miles, Richard, Roche, Paul, Wooding, Ben
We report results from new and archival observations of the newly discovered active asteroid (248370) 2005 QN_137, which has been determined to be a likely main-belt comet based on a subsequent discovery that it is recurrently active near perihelion.
Externí odkaz:
http://arxiv.org/abs/2109.14822
Seeing the Bigger Picture: The Rosetta Mission Amateur Observing Campaign and Lessons for the Future
Amateur astronomers can make useful contributions to the study of comets. They add temporal coverage and multi-scale observations which can aid the study of fast-changing, and large-scale comet features. We document and review the amateur observing c
Externí odkaz:
http://arxiv.org/abs/2011.07123
Hard X-ray observations with the Neil Gehrels Swift Observatory Burst Alert Telescope (BAT) reveal superorbital modulation in the wind-accreting supergiant high-mass X-ray binary (HMXB) 4U 1538-52 at a period of 14.9130 +/- 0.0026 days that is consis
Externí odkaz:
http://arxiv.org/abs/2010.12556
Autor:
Monageng, Itumeleng, Coe, Malcolm, Kennea, Jamie, Townsend, Lee, Buckley, David, McBride, Vanessa, Udalski, Andrzej, Evans, Phil, Roche, Paul
In this paper we report on the optical and X-ray behaviour of the Be X-ray binary, SXP 91.1, during a recent type I outburst. We monitored the outburst using the Neil Gehrels Swift Observatory. These data were supported by optical data from the South
Externí odkaz:
http://arxiv.org/abs/1908.04638
Autor:
Monageng, Itumeleng, Coe, Malcolm, Townsend, Lee, Buckley, David, McBride, Vanessa, Roche, Paul, Kennea, Jamie, Udalski, Andrzej, Evans, Phil
SXP4.78 was originally discovered in 2000 as a pulsar in the Small Magellanic Cloud (SMC) by the Rossi X-ray Timing Explorer (RXTE) but it was not spatially located at that time. A new detection in 2018 with the Neil Gehrels Swift Observatory during
Externí odkaz:
http://arxiv.org/abs/1902.00677
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