Welcome to MMODA

Query parameters :

OSA Version

Radius deg

Use INTEGRAL pointing Science Windows (ScWs)

Select for time range

Custom list

Custom list in file

Maximum number of ScWs

ScWs List

ScWs file

INTEGRAL data access priviledge

Public

All Private

Energy Min * keV

Energy Max * keV

Query Type

Detection Threshold

Product Type

Image

Spectrum

Light curve

Time bin

Unit

User catalog

If needed, create a custom catalog following one of the templates : ASCII or FITS.

If you use results or material from this instrument in our application, ODA, do not forget to quote our paper:
A. Neronov, V. Savchenko, A. Tramacere, M. Meharga, C. Ferrigno, S.Paltani
An online data analysis system of INTEGRAL telescope

Query parameters :

OSA Version

Radius deg

Use INTEGRAL pointing Science Windows (ScWs)

Select for time range

Custom list

Custom list in file

Maximum number of ScWs

ScWs List

ScWs file

INTEGRAL data access priviledge

Public

All Private

JEMX module number

JEMX-1

JEMX-2

Energy Min * keV

Energy Max * keV

Query Type

Detection Threshold

Product Type

Image

Spectrum

Light curve

Time bin

Unit

User catalog

If needed, create a custom catalog following one of the templates : ASCII or FITS.

Query parameters :

Query Type

Product Type

Light curve

Time bin

Query parameters :

Energy Min * keV

Energy Max * keV

Query Type

Product Type

Light curve

Time bin

Unit

Query parameters :

Data Release

Product Type

Image & Catalog

Photometry

Photometry collection radius arcsec

Image size arcmin

Pixel size arcsec per pixel

Image Band

If this result is used for publicaiton, please cite https://doi.org/10.5281/zenodo.6376844 and include an acknowledgement of the Legacy Survey: https://www.legacysurvey.org/acknowledgment/

Query parameters :

Product Type

Synchrotron external-compton bremsstrahlung

Synchrotron-self-compton bremsstrhalung

Electron spectrum dN/dE

Electron spectrum ascii file (overrides analytical formula)

Upload a file

Provide a URL

File URL

Upload a file

minimal energy for calculations eV

maximal energy for calculations eV

magnetic field [G]

density of the medium [1/cm3]

average atomic charge of the medium

Temperature of black body photon background [K]

Normalization of blackbody photon background (<=1)

Custom background spectral energy density [1/(eV cm3)]

Background spectrum ascii file (overrides parameters above)

Upload a file

Provide a URL

File URL

Upload a file

Energy density of synchrotron radiation [eV/cm3]

version: 3ac9b4fd

Modelling implemented in this service is based on formulae from Ref. Blumenthal&Gould Rev. Mod. Phys. 42, 237 (1970) [BG]).

Python notebook for the modelling can be found at renkulab.io and in a related GitLab repository. Contact mainteiners of the repository for questions / suggestions or if you want to contribute.

Query parameters :

Product Type

Spectrogram

Time resolution (sec)

Frequency resolution (MHz)

version: 0988c12b

Service generated from the repository

Query parameters :

Product Type

Lst1 spectrum simulator

Lst1 events simulator

Visibility predictor

Source redshift

Gamma-hadron separation cut efficiency

Zenith angle

Number of backgorund regions

Exposure time in hours

Source extension in degrees

Source spectrum dN/dE [1/(TeV cm2 s)]

Pulsar analysis

Pulsar analysis?

range of ON phases

range of OFF phases

Plotting

Image radius deg

Pixel size deg

Minimal energy TeV

Maximal energy TeV

Source off-axis angle deg

Number of wobble positions

Exposure time in hours hour

Sky model yaml file (overrides parameters above)

Upload a file

Provide a URL

File URL

Upload a file

Minimal zenith deg

Maximal zenith deg

maximal moon (between 0 and 1) deg

version: d13301e5

The LST1 spectrum simulator has been developed by Abellardo Moralejo, it is based on the instrument response functions corresponding to the performance paper Astrophys.J. 956 (2023) 2, 80.

The LST1 event generator is based on a code srcsim developed by Ievgen Vovk, Marcel Strzys and Elise Lagarde.

The spectrum simulator and event generator services are staged from the LST project on the collaborative data science platform Renku.

Query parameters :

Product Type

Image public dl3

Magic simulator-v1.9

Spectrum public dl3

Lightcurve public dl3

Cone search radius deg

Image radius deg

Pixel size deg

Minimal energy TeV

Maximal energy TeV

Source off-axis angle

Night sky background level (0-8)

Observation time hour

Source extension deg

Source redshift

Zenith angle

Sum Trigger?

True

False

numoff

minimum number of events

minimum ratio of excess to background

PSF deg

degradation factor (for offset >0.4 deg)

Plotting

minimal energy GeV

maximal energy GeV

minimal flux [TeV/(cm2 s)]

maximal flux [TeV/(cm2 s)]

Minimal errorbar (signal-to-noise)

NEbins

drawsigma

True

False

Source spectrum dN/dE [1/(TeV cm2 s)]

Pulsar analysis

Pulsar analysis?

True

False

range of ON phases

range of OFF phases

isLSTmode

True

False

Source region radius for aperture photometry deg

Minimal energy for spectral fitting TeV

Maximal energy for spectral fitting TeV

Number of time bins

Slope of the model powerlaw

version: 10c7a861

Service generated from the repository

Query parameters :

Product Type

Image

Spectrum

Radius deg

pixsize deg

Frequency

version: fae2c134

This service is based on GLEAM

Query parameters :

Product Type

Workflow

STIX

Energy Range (min)

Energy Range (max)

MWA

Time resolution (sec)

Frequency resolution (MHz)

version: ac46eefc

Service generated from the repository

Query parameters :

Product Type

Multi-instrument spectrum

MWA (radio)

INTEGRAL/JEM-X (X-ray)

INTEGRAL/ISGRI (hard X-ray)

Fermi/LAT (gamma-ray)

MAGIC (gamma-ray)

IceCube (neutrino)

Auger (UHECR)

HESS (gamma-ray)

GAIA (visible)

DESI Legacy Survey (visible/infrared)

version: 9f46e181

Service generated from the repository

Query parameters :

Product Type

Phase transition parameters

Model spectrum

epsilon_turb

Phase transition temperature GeV

Number of effective degrees of freedom

alpha: latent heat in units of radiation density

beta: phase transition rate in units of Hubble rate

ternminal velocity of bubles

Hubble parameter

model parameterisation

version: 2a082b5c

This service provides power spectra of Stochastic Gravitational Wave Background from cosmological phase transitions based on parameterisations described by Roper Pol et al. (2023).

Query parameters :

Product Type

Workflow

STIX

Energy Range (min)

Energy Range (max)

version: af0ae5ac

Service generated from the repository

Query parameters :

Product Type

Spectrum

Source spectrum dN/dp

secondary particle channel

version: b4a550df

Service generated from the repository

Query parameters :

Product Type

Spectrum

Source signal region radius deg

Minimal energy eV

Maximal energy eV

Number of energy bins

version: a4c47884

This service uses the publicly available data of Pierre Auger Observatory, (see description of the dataset in Ref. Pierre Auger collaboration, arXiv:2206.13492).

Query parameters :

Product Type

Image

Lightcurve

Spectrum

Instrument

radius deg

E_min keV

E_max keV

Detection threshold

Include new sources

Upload to the gallery

Host Type

Host Type Reference catalog URL

Upload a file

Provide a URL

File URL

Upload a file

Token for MMODA

Grouping minimum energy keV

Grouping maximum energy keV

Grouping bin number

Systmatic fraction

version: 74d843ff

Service generated from the repository

Query parameters :

Product Type

Image

Catalog

Spectrum

Radius arcmin

Pixel size arcsec

Band

Data Release

version: cfd5a99c

Service generated from the repository

Query parameters :

Product Type

Image

Spectrum aperture

Spectrum likelihood

Lightcurve

Size of the Region-Of-Interest (ROI) deg

Pixel size for the countmap deg

Minimal energy MeV

Maximal energy MeV

Radius of the source region deg

Outer radius of the background ring deg

Number of energy bins

Sky model xml file

Upload a file

Provide a URL

File URL

Upload a file

time_binning

Number of time bins

version: 14a3e87e

This is an example acknowledgements with link

Query parameters :

Product Type

Lightcurve from photometry

Period folded lightcurve

Spectrum from photometry

Continuum spectra

radius_photometry arcsec

data_release

flux_band

flux_units

search_radius arcsec

radius arcsec

wl_min

wl_max

d_wl

sampling_type

calib_output

True

False

bprp_output

True

False

version: ba1ad5f6

Service generated from the repository

Query parameters :

Product Type

Detectgrb

Integralallsky

detection_time_scales

lc_time_scale

background_age s

min_sn

RA_rename

Dec

tstart_rel_mseconds

tstop_rel_seconds

t0_utc

required_completeness

mode

global_snr_threshold

negative_excesses

version: 4a3181dc

Service generated from the repository

Query parameters :

Product Type

Image public dl3

Spectrum public dl3

Lightcurve public dl3

Image radius deg

Pixel size deg

Minimal energy TeV

Maximal energy TeV

R_s deg

NEbins

Efit_min TeV

Efit_max TeV

NTbins

version: 9de5ab92

This service uses the publicly available data of HESS telescope, (see description of the dataset in Ref. HESS collaboration, arXiv:1810.04516).

Query parameters :

Product Type

Lst1 spectrum

Magic simulator-v1.9

Ctao

Visibility predictor

Source redshift

Gamma-hadron separation cut efficiency

Zenith angle

Number of backgorund regions

Exposure time in hours

Source extension in degrees

Source spectrum dN/dE [1/(TeV cm2 s)]

Pulsar analysis

Pulsar analysis?

True

False

range of ON phases

range of OFF phases

Observation time hour

Source extension deg

Zenith angle

Sum Trigger?

True

False

numoff

minimum number of events

minimum ratio of excess to background

PSF deg

degradation factor (for offset >0.4 deg)

Plotting

minimal energy GeV

maximal energy GeV

minimal flux [TeV/(cm2 s)]

maximal flux [TeV/(cm2 s)]

Minimal errorbar (signal-to-noise)

drawsigma

True

False

isLSTmode

True

False

OffAxis_angle deg

Texp hour

E0 TeV

Gamma

Radius_spectal_extraction

Radius_sky_image deg

Site

Telescope_LST

True

False

Telescope_MST

True

False

Telescope_SST

True

False

Minimal zenith deg

Maximal zenith deg

maximal moon (between 0 and 1) deg

version: 04e1905c

CTAO simulator uses the publicly available instrument response functions derived from simulations of performance of Cherenkov Telescope Array (CTA) observatory, (see description ). The analysis is done using Gammapy package.

The MAGIC simulator has been developed by Julian Sitarek, the code can be found in the repository.

The LST1 simulator has been developed by Abellardo Moralejo, it is based on the instrument response functions corresponding to the performance paper Astrophys.J. 956 (2023) 2, 80.

Query parameters :

Product Type

Image

Lightcurve

Spectrum

IC40

IC59

IC79

IC86_I

IC86_II_VII

Radius deg

pixel_size deg

TSmap_type

Slope

Spectrum_type

version: e99209d0

This service uses the publicly available data of ten-year exposure of IceCube, (see description of the dataset in Ref. IceCube collaboration, arXiv:2101.09836). The analysis is done using the SkyLLH package, see SkyLLH documentation.

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Incident on the platform: jobs delayed, services reduced