0920008

Monitoring of microquasars such as GRS 1915+105 and Cygnus X-1 during the previous INTEGRAL AOs has revealed a wealth of new observational information. The monitoring has revealed the dynamical behavior of these sources above 20 keV on all timescales as opposed to the snapshot observations available before. We propose to continue the monitoring of these canonical black holes with a dedicated Key Programme in INTEGRAL AO8 which will also include the soft X-rays through a strategy that allows the source to remain in the field of view of JEM-X. The proposed investigation will allow to study di erent emission models for the two extreme cases of microquasars with INTEGRAL and simultaneous optical IR and radio observations. This proposal is a continuation of our earlier accepted observations that started in AO1. [truncated! Please see actual data for full text]

针对GRS 1915+105与天鹅座X-1这类微类星体（microquasars）开展的监测工作，在INTEGRAL过往各轮观测征选提案周期（Announcement of Opportunity，AO）中已获取大量全新观测资料。相较于此前仅能获得的瞬时快照式观测，本次监测揭示了这批天体源在20 keV以上能段的全时标动力学行为。
我们提议在INTEGRAL第8轮观测征选提案周期（AO8）中，依托专属关键项目（Key Programme）继续监测这类典型黑洞（canonical black holes）；该项目将通过一种可让目标天体始终处于JEM-X视场范围内的观测策略，纳入软X射线波段的观测内容。
本次拟开展的研究将借助INTEGRAL观测设备以及同步开展的光学、红外与射电观测，针对两类极端微类星体样本展开不同辐射模型的研究。本提案是我们自AO1周期起获批的早期观测项目的延续。[内容已截断，请查阅完整原文以获取全部信息]