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← Revision 8 as of 2024-04-05 17:20:59 ⇥
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| David Kaltenbrunner [[attachment:]] | Adrien Hoornaert [[attachment:BWM_AH_24_04_04.pptx]] - Study of an X-Ray source (MC Bridge): eRASSU J031038.2-734935with eROSITA / XMM / NuSTAR Haonan Yang [[attachment:20240403_LEIA_Data_Brief.pptx]] - Study of XRBs in the Magellanic Clouds with LEIA David Kaltenbrunner [[attachment:Biweekly_meetings_2024_04_04.pdf]] - Created source products for all catalogs - Solved the problem of variable background for bright objects (LMC X-1, X-2, X-3) by choosing background in the scan direction - Working on the paper draft |
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| Robert Willer [[attachment:MC_meeting_04_04_24.pdf]] | |
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| - used MESA to simulate for a 0.53 Msolar WD, including mass-loss prescription, diffusion and convective mixing for several nova cycles | |
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Robert Willer [[attachment:]] |
-- Need to simulate over wider WD range |
Minutes of the Magellanic Cloud meeting, April 04, 2024
Attendants: Chandreyee, Robert, David, Frank, Jochen, Haonan, Adrien
Adrien Hoornaert BWM_AH_24_04_04.pptx
- Study of an X-Ray source (MC Bridge): eRASSU J031038.2-734935with eROSITA / XMM / NuSTAR
Haonan Yang 20240403_LEIA_Data_Brief.pptx
- Study of XRBs in the Magellanic Clouds with LEIA
David Kaltenbrunner Biweekly_meetings_2024_04_04.pdf
- Created source products for all catalogs
- Solved the problem of variable background for bright objects (LMC X-1, X-2, X-3) by choosing background in the scan direction
- Working on the paper draft
Robert Willer MC_meeting_04_04_24.pdf
- used MESA to simulate for a 0.53 Msolar WD, including mass-loss prescription, diffusion and convective mixing for several nova cycles
-- Need to simulate over wider WD range
Next telecon on April 18, 2024