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Object name *

Dec

Start time *

End time *

Time unit

Hard X-rays

INTEGRAL ISGRI
X-rays

INTEGRAL JEM-X
Gamma-rays

INTEGRAL SPI-ACS
Gamma-rays

Polar
Cosmic rays

Auger
Gamma-rays

CTAO LST1 simulators
Visible/Infrared

DESI Legacy Survey
Visible

GAIA
Gamma-rays

HESS DL3 Demo
Neutrino

IceCube
Gamma-rays

MAGIC DL3 Demo
Gamma-rays

MAGIC simulator
Modelling-GW

SGWB
Gravitational waves

LIGO-VIRGO-KAGRA

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 :

Product Type

Spectrum

Source signal region radius deg

Minimal energy eV

Maximal energy eV

Number of energy bins

version: 5f1f7352

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

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?

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: 6e369d27

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

Spectrum

Catalog

Radius arcmin

Pixel size arcsec

Band

Data Release

version: 68935f0d

Service generated from the repository

Query parameters :

Product Type

Spectrum from photometry

Period folded lightcurve

Lightcurve from photometry

Continuum spectra

radius_photometry arcsec

data_release

search_radius arcsec

flux_band

flux_units

radius arcsec

wl_min

wl_max

d_wl

sampling_type

calib_output

bprp_output

version: a7de4ed2

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: 22853434

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

Lightcurve

Image

Spectrum

Slope

IC40

IC59

IC79

IC86_I

IC86_II_VII

Radius deg

pixel_size deg

TSmap_type

Spectrum_type

version: 95d5c71f

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

Image public dl3

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)

Source region radius for aperture photometry deg

Plotting

NEbins

Minimal energy for spectral fitting TeV

Maximal energy for spectral fitting TeV

Number of time bins

Slope of the model powerlaw

version: 86efc721

Service generated from the repository

Query parameters :

Product Type

Magic simulator-v1.9

Observation time hour

Source extension deg

Source redshift

Zenith angle

Sum Trigger?

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

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

Pulsar analysis

Pulsar analysis?

range of ON phases

range of OFF phases

isLSTmode

version: e42f9e35

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: aed7b03b

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

Skymap search

Parameters estimation

Catalogs statistics

Catalogs event selection

RA std (deg) deg

DEC std (deg) deg

Probability envelop [0-1]

Waveform approximant

use_glade

use_grb

The model or combination of waveform models used to generate the posterior samples

The waveform model used to generate the time-domain waveform for overlay with the detector strain

Time window low (in seconds, float)

Time window high (in seconds, float)

Low strain frequency cut-off (Hz)

High strain frequency cut-off (Hz)

use_gwtc4

use_gwtc3

use_gwtc2

use_gwtc1

M1 Low (solar mass)

M1 High (solar mass)

M2 Low (solar mass)

M2 High (solar mass)

Dist Low (Mpc)

Dist High (Mpc)

use_time

version: 0d9a7eae

The module relies on data curated by GWOSC. Please follow https://gwosc.org/acknowledgement/ if your work uses this data product.

For any help or questions related to this LIGO-VIRGO-KAGRA GitLab project, please contact Daniel Sentenac

This work was made possible thanks to the ACME program, the LVK collaboration, the GWOSC team, and AstroOrdas project team. Particular thanks to Denys Savchenko who helped me to set-up the module.

version: 7.x-1.0