The total number of Primary Orbits used in all Cycles must equal the total number of Primary Orbits specified on all the Observations. (Compare totals reported on the first and second pages of the PDF Preview.)
This investigator has not been uniquely identified in the STScI database.
This investigator has not been uniquely identified in the STScI database.
This investigator has not been uniquely identified in the STScI database.
This investigator has not been uniquely identified in the STScI database.
This investigator has not been uniquely identified in the STScI database.
This investigator has not been uniquely identified in the STScI database.
This investigator has not been uniquely identified in the STScI database.
This investigator has not been uniquely identified in the STScI database.
This investigator has not been uniquely identified in the STScI database.
This investigator has not been uniquely identified in the STScI database.
At least one target must be specified in Phase I
At least one observation must be specified0Assigned ID: 4943
----- Attempting Submission 1 (Mon Dec 18 18:36:51 GMT 2023) -----Joint XMMupdated mock visits for the tentative observing strategy.-776684107----- Attempting Submission 1 (Fri Jan 19 17:40:46 GMT 2024) -----
Your proposal could not be saved.
Submission aborted.
----- Attempting Submission 2 (Mon Jan 22 18:55:23 GMT 2024) -----Legacy Observations of BHXRBs: wind driving mechanism and relation with the jetEdge-on black hole transients show blue-shifted absorption lines in their X-ray spectra due to hot equatorial disk winds. Blue-shifted absorption lines also been discovered in optical and UV. These features must be produced in an outflow, but the physical conditions required to form them are very different. The three features have never been observed at the same time. It is unclear if they are linked to distinct outflows or simply to different regions. We propose to answer this question with simultaneous time-resolved spectroscopy of a transient BHXRB in X-ray, UV, optical and mid-IR during their hard- intermediate- and soft-states. This will allow us to test if all types of wind features are present simultaneously and whether they display correlated variability among them and with the jetThis proposal aims follow the ouburst of a transient LMXB covering different parts of the outburst evolution.
The distribution of the orbits may vary based on the brigthness of the actual transient.naStellar Physics and Stellar Types6falsefalsefalsefalsefalsefalsefalsefalseSUPPORTEDSTARLMXBX-RAY NOVAENext LMXB in outburstCOS/FUVSpectroscopicNoNoG140L1280STIS/NUV-MAMASpectroscopicNoNoG230L2376The scheduling data was generated by CASM 32.0.CASM was run in Phase II mode./private/var/folders/qw/bm7knqg9493_9mh63wbjwdkh0000gp/T/OPVisit17367571352499746882.xml(Tic-Visit
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COS.ta.1417131
COS.ta.1417132
COS.ta.1417134Otther spetral shapes are considered here:
COS.sp.1416844
COS.sp.1416867
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