GitHub - abubakryagob/xray-radio-transient-analysis: the computational backbone for my first-author publications on magnetars and transients, showcasing robust, multi-wavelength scientific data pipelines.

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Name		Name	Last commit message	Last commit date
Latest commit History 5 Commits
.ipynb_checkpoints		.ipynb_checkpoints
X-ray-pulsars-Pulse-Profile-master		X-ray-pulsars-Pulse-Profile-master
askap_scripts		askap_scripts
pdot_daigram		pdot_daigram
.DS_Store		.DS_Store
2BB_source_diffuse_xmm_michelas_checks.qdp		2BB_source_diffuse_xmm_michelas_checks.qdp
2BB_source_diffuse_xmm_michelas_checks_2.qdp		2BB_source_diffuse_xmm_michelas_checks_2.qdp
3901_0.3-2keV.png		3901_0.3-2keV.png
Calculate the shift of the pulse phase.ipynb		Calculate the shift of the pulse phase.ipynb
Calculate_Obs_Flux.ipynb		Calculate_Obs_Flux.ipynb
Calculate_UnObs_Flux.ipynb		Calculate_UnObs_Flux.ipynb
F0_measurements_F1fit.png		F0_measurements_F1fit.png
Luminosity_mdel_exp.pdf		Luminosity_mdel_exp.pdf
Luminosity_mdel_power-law-model.pdf		Luminosity_mdel_power-law-model.pdf
MJDes.txt		MJDes.txt
Model_R_Lum_PF.ipynb		Model_R_Lum_PF.ipynb
NuSTAR_Magnetars_ObsIDs.txt		NuSTAR_Magnetars_ObsIDs.txt
PF_0.3-10kev.qdp		PF_0.3-10kev.qdp
PF_0.3-10kev.txt		PF_0.3-10kev.txt
PF_mdel.pdf		PF_mdel.pdf
Phase_fitting.ipynb		Phase_fitting.ipynb
Pulsars Death Line calculation .ipynb		Pulsars Death Line calculation .ipynb
Pulse_profile_layout_plots.pptx		Pulse_profile_layout_plots.pptx
Radius_mdel.pdf		Radius_mdel.pdf
Radius_mdel_exp.pdf		Radius_mdel_exp.pdf
SGR_J1935_nu1002.pdf		SGR_J1935_nu1002.pdf
SGR_J1935_nu1004.pdf		SGR_J1935_nu1004.pdf
SLMC_magnetars.py		SLMC_magnetars.py
SWJ1818.0_pulse_profiles.pdf		SWJ1818.0_pulse_profiles.pdf
SWJ1818_Pulsed_Fraction.pdf		SWJ1818_Pulsed_Fraction.pdf
SWJ1818_Pulsed_Fraction_in-time.pdf		SWJ1818_Pulsed_Fraction_in-time.pdf
SWJ1818_Pulsed_Fraction_max-min.pdf		SWJ1818_Pulsed_Fraction_max-min.pdf
SWJ1818_Pulsed_Fraction_max-min_energy.pdf		SWJ1818_Pulsed_Fraction_max-min_energy.pdf
SWJ1818_Pulsed_Fraction_new.pdf		SWJ1818_Pulsed_Fraction_new.pdf
SWJ1818_pul.pdf		SWJ1818_pul.pdf
SWJ1818_pulse_profile.pdf		SWJ1818_pulse_profile.pdf
SWJ1818_pulse_profile1-03-10.pdf		SWJ1818_pulse_profile1-03-10.pdf
SWJ1818_pulse_profile1-03-2.pdf		SWJ1818_pulse_profile1-03-2.pdf
SWJ1818_pulse_profile1-2-3.pdf		SWJ1818_pulse_profile1-2-3.pdf
SWJ1818_pulse_profile1-3-5.pdf		SWJ1818_pulse_profile1-3-5.pdf
SWJ1818_pulse_profile1-5-10.pdf		SWJ1818_pulse_profile1-5-10.pdf
SWJ1818_pulse_profile2-03-10.pdf		SWJ1818_pulse_profile2-03-10.pdf
SWJ1818_pulse_profile2-03-2.pdf		SWJ1818_pulse_profile2-03-2.pdf
SWJ1818_pulse_profile2-2-3.pdf		SWJ1818_pulse_profile2-2-3.pdf
SWJ1818_pulse_profile2-3-5.pdf		SWJ1818_pulse_profile2-3-5.pdf
SWJ1818_pulse_profile2-5-10.pdf		SWJ1818_pulse_profile2-5-10.pdf
SWJ1818_pulse_profile3-03-10.pdf		SWJ1818_pulse_profile3-03-10.pdf
SWJ1818_pulse_profile3-03-2.pdf		SWJ1818_pulse_profile3-03-2.pdf
SWJ1818_pulse_profile3-2-3.pdf		SWJ1818_pulse_profile3-2-3.pdf
SWJ1818_pulse_profile3-3-5.pdf		SWJ1818_pulse_profile3-3-5.pdf
SWJ1818_pulse_profile3-5-10.pdf		SWJ1818_pulse_profile3-5-10.pdf
SWJ1818_pulse_profile4-03-10.pdf		SWJ1818_pulse_profile4-03-10.pdf
SWJ1818_pulse_profile4-03-2.pdf		SWJ1818_pulse_profile4-03-2.pdf
SWJ1818_pulse_profile4-2-3.pdf		SWJ1818_pulse_profile4-2-3.pdf
SWJ1818_pulse_profile4-3-5.pdf		SWJ1818_pulse_profile4-3-5.pdf
SWJ1818_pulse_profile4-5-10.pdf		SWJ1818_pulse_profile4-5-10.pdf
SWJ1818_pulse_profile_0.3-10keV.pdf		SWJ1818_pulse_profile_0.3-10keV.pdf
SWJ1818_pulse_profile_0.3-10keV_all_combined.pdf		SWJ1818_pulse_profile_0.3-10keV_all_combined.pdf
SWJ1818_pulse_profile_1801.pdf		SWJ1818_pulse_profile_1801.pdf
SWJ1818_pulse_profile_3901.pdf		SWJ1818_pulse_profile_3901.pdf
SWJ1818_pulse_profile_4001.pdf		SWJ1818_pulse_profile_4001.pdf
SWJ1818_pulse_profile_4201.pdf		SWJ1818_pulse_profile_4201.pdf
SWJ1818_pulse_profile_new.pdf		SWJ1818_pulse_profile_new.pdf
Untitled.ipynb		Untitled.ipynb
Untitled1.ipynb		Untitled1.ipynb
absorbed_flux.png		absorbed_flux.png
bayesian_blok_burst.py		bayesian_blok_burst.py
calculate_pdot.ipynb		calculate_pdot.ipynb
calculate_phase_nustar.ipynb		calculate_phase_nustar.ipynb
chi_psi_Swift_1818_Abu_April_Upper_Lower.pdf		chi_psi_Swift_1818_Abu_April_Upper_Lower.pdf
compile_NuSTAR_IDs.ipynb		compile_NuSTAR_IDs.ipynb
compile_ObsIDs.py		compile_ObsIDs.py
datetime.ipynb		datetime.ipynb
del_persistent_spectra_SGRJ1935.pdf		del_persistent_spectra_SGRJ1935.pdf
del_persistent_spectra_SGRJ1935_Epoch1.pdf		del_persistent_spectra_SGRJ1935_Epoch1.pdf
del_persistent_spectra_SGRJ1935_Epoch2.pdf		del_persistent_spectra_SGRJ1935_Epoch2.pdf
del_plot_persistent spectra_SGRJ1935.ipynb		del_plot_persistent spectra_SGRJ1935.ipynb
diffuse2_fit_J1818.ipynb		diffuse2_fit_J1818.ipynb
diffuse_spec.qdp		diffuse_spec.qdp
diffuse_spec.txt		diffuse_spec.txt
diffuse_spectra.ipynb		diffuse_spectra.ipynb
diffuse_spectra.pdf		diffuse_spectra.pdf
eeufspac_SRC_diffuse_spectra_SWJ1818.pdf		eeufspac_SRC_diffuse_spectra_SWJ1818.pdf
eeufspac_diffuse_spectra_SWJ1818.pdf		eeufspac_diffuse_spectra_SWJ1818.pdf
eeufspac_same_epoch_only_spectra.qdp		eeufspac_same_epoch_only_spectra.qdp
eeufspac_spectra_SWJ1818.pdf		eeufspac_spectra_SWJ1818.pdf
eeufspac_spectra_SWJ1818_updated.pdf		eeufspac_spectra_SWJ1818_updated.pdf
eeufspac_src_diffuse_spectra_SWJ1818_2.pdf		eeufspac_src_diffuse_spectra_SWJ1818_2.pdf
eeufspec_del_plot_SGRJ1935.pdf		eeufspec_del_plot_SGRJ1935.pdf
eeufspec_del_plot_SGRJ1935_Epoch1.pdf		eeufspec_del_plot_SGRJ1935_Epoch1.pdf
eeufspec_del_plot_SGRJ1935_Epoch2.pdf		eeufspec_del_plot_SGRJ1935_Epoch2.pdf
eeufspec_del_plots_persistent_spectra_SGRJ1935.ipynb		eeufspec_del_plots_persistent_spectra_SGRJ1935.ipynb
eeufspec_persistent_spectra_J1935.ipynb		eeufspec_persistent_spectra_J1935.ipynb
eeufspec_persistent_spectra_SGRJ1935.pdf		eeufspec_persistent_spectra_SGRJ1935.pdf
eeufspec_persistent_spectra_SGRJ1935_Epoch1.pdf		eeufspec_persistent_spectra_SGRJ1935_Epoch1.pdf
eeufspec_persistent_spectra_SGRJ1935_Epoch2.pdf		eeufspec_persistent_spectra_SGRJ1935_Epoch2.pdf
fdot_nustar_obs.png		fdot_nustar_obs.png
fdot_swift_obs.dat		fdot_swift_obs.dat
fdot_xmm-nustar_obs.dat		fdot_xmm-nustar_obs.dat
fdot_xmm-nustar_obs.txt		fdot_xmm-nustar_obs.txt

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the computational backbone for my first-author publications on magnetars and transients, showcasing robust, multi-wavelength scientific data pipelines.

python sas radio-astronomy xspec heasoft

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