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Object name *

Dec

Start time *

End time *

Time unit

Gamma-rays

INTEGRAL SPI-ACS
Modelling-EM

Synch-IC-Brems
radio

STIX-MWA Solar Activity
Modelling-GW

SGWB
Gamma-rays

MAGIC
Gamma-rays

LST
neutrino

IceCube
Gamma-rays

IACT simulators
Gamma-rays

HESS
GRB detection
Visible

gaia
Gamma-rays

Fermi-LAT
Visible/Infrared

DESI Legacy Survey
Gamma-rays

CTA
cosmic rays

Auger
radio

MWA

Query parameters :

Query Type

Product Type

Light curve

Time bin

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 :

Product Type

Sic brems

Gamma

Ecut

Back_norm

version: 4bb3381a

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

Stix-wma-workflow

Source

STIX

Energy Range (min)

Energy Range (max)

version: e404086b

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

Image public dl3

Lightcurve public dl3

Magic simulator-v1.9

Spectrum 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)

Source region radius for aperture photometry deg

Number of time bins

Slope of the model powerlaw

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

Minimal energy for spectral fitting TeV

Maximal energy for spectral fitting TeV

version: 10c7a861

Service generated from the repository

Query parameters :

Product Type

Visibility predictor

Lst1 spectrum simulator

Lst1 events simulator

Minimal zenith deg

Maximal zenith deg

maximal moon (between 0 and 1) deg

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

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

version: 6c108754

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

Lightcurve

Spectrum

IC40

True

False

IC59

True

False

IC79

True

False

IC86_I

True

False

IC86_II_VII

True

False

Radius deg

pixel_size deg

TSmap_type

Slope

Spectrum_type

version: a166bf24

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.

Query parameters :

Product Type

Magic simulator-v1.9

Visibility predictor

Lst1 spectrum

Ctao

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)

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

Minimal zenith deg

Maximal zenith deg

maximal moon (between 0 and 1) deg

Gamma-hadron separation cut efficiency

Zenith angle

Number of backgorund regions

Exposure time in hours

Source extension in degrees

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

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 public dl3

Lightcurve public dl3

Spectrum public dl3

Image radius deg

Pixel size deg

Minimal energy TeV

Maximal energy TeV

R_s deg

NTbins

NEbins

Efit_min TeV

Efit_max TeV

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

Integralallsky

Detectgrb

RA_rename

Dec

tstart_rel_mseconds

tstop_rel_seconds

t0_utc

required_completeness

mode

global_snr_threshold

negative_excesses

detection_time_scales

lc_time_scale

background_age s

min_sn

Service generated from the repository

Query parameters :

Product Type

Period folded lightcurve

Spectrum from photometry

Continuum spectra

Lightcurve from photometry

search_radius arcsec

data_release

flux_band

flux_units

radius_photometry arcsec

radius arcsec

wl_min

wl_max

d_wl

sampling_type

calib_output

True

False

bprp_output

True

False

version: 80936ff0

Service generated from the repository

Query parameters :

Product Type

Image

Lightcurve

Spectrum likelihood

Spectrum aperture

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

time_binning

Number of time bins

Number of energy bins

Sky model xml file

Upload a file

Provide a URL

File URL

Upload a file

version: f7cecd5c

This is an example acknowledgements with link

Query parameters :

Product Type

Image

Catalog

Spectrum

Radius arcmin

Pixel size arcsec

Band

Data Release

version: 35a28123

Service generated from the repository

Query parameters :

Product Type

Pre-defined model

Model cube file

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

data_cube

Upload a file

Provide a URL

File URL

Upload a file

Telescopes_LST

True

False

Telescopes_MST

True

False

Telescopes_SST

True

False

version: d655f12f

This service 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.

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

Spectrum

Radius deg

pixsize deg

Frequency

version: 3f4b0d49

This service is based on GLEAM

version: 7.x-1.0