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----- Attempting Submission 1 (Thu Dec 09 12:34:54 GMT 2021) -----Joint XMM/HST ProposalINEFFICIENT ORDERING OF FP-POS POSITIONS0----- Attempting Submission 1 (Wed Jan 19 12:21:19 GMT 2022) -----
----- Attempting Submission 2 (Wed Feb 09 17:47:12 GMT 2022) -----FP-POS should be efficient as it isAn accretion disk wind across the electromagnetic spectrumAccretion inevitably produces disk winds, which has vast consequences. These outflows can regulate the accretion process, affect the long-term orbital evolution of the X-ray binary, and impact their cosmic envi- ronment. However, it is not established exactly how disk winds are launched, and how much mass is carried away by them. We propose to study the disk wind of a persistently accreting neutron star across the elec- tromagnetic spectrum with XMM-Newton, HST and VLT. These simultaneous multi-wavelength data will determine the launch mechanism and mass content of the disk wind. This show-case study will highlight the impact of studying disk winds across the electromagnetic spectrum and pave the way for future observations.We propose to observe the low-mass X-ray binary IGR J17062-6143 in 6 orbits all within the same visit.
The first orbit, will consist of an ACQ/IMAGE taken with COS/NUV and complemented with the spectroscopic exposures taken with the COS/FUV G140L.
The preffered window to coordinate with XMM and VLT/XShooter is 19-24 September.n/aSupermassive Black Holes and Active Galaxies6falsefalsefalsefalsefalsefalsefalseSUPPORTEDSTARACCRETION DISKNEUTRON STARX-RAY TRANSIENTNOThis object was obtained from GAIA EDR3 id: "Gaia EDR3 5913619493527584768"J2000J2000COS/FUVSpectroscopicNoNoG140L/private/var/folders/f9/f1hshrrd6mx_rnl1gt9vywkw0000gn/T/OPVisit1847838498290068555.xmlThe scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.The object is faint.
In order to optimise the exposure time, we use a single FP-POS per orbit with the exception of the last two where we use 2 per orbit.(Tic-Visit
:proposal-id 16897
:visit-id "01"
:proposal-version -1
:trans-version "20210514"
:date "09-Feb-2022 16:56:03.0"
:trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 6
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191616
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16897
:visit-id "01"
:obset-id "01"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16897
:visit-id "01"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 3018
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3411
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16897
:visit-id "01"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 3019
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3411
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16897
:visit-id "01"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 3019
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3411
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16897
:visit-id "01"
:orbit-number 4
:pcs-time 392
:si-vis-utilization 3019
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3411
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16897
:visit-id "01"
:orbit-number 5
:pcs-time 392
:si-vis-utilization 3019
:al-overhead-at-end 0
:internal-dur-at-end 48
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3411
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16897
:visit-id "01"
:orbit-number 6
:pcs-time 392
:si-vis-utilization 3019
:al-overhead-at-end 0
:internal-dur-at-end 344
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3411
:pcs-gap 0
)true60We used a blackbody with Teff = 50000 K normalized to the magnitudes reported in https://arxiv.org/pdf/1801.03006.pdf for the UW2 filter (central wav. 1928).
The source show small variability so we secure the aquisition aiming for a S/N=40