The dataset viewer is not available for this dataset.
Error code: JWTInvalidSignature
Exception: InvalidSignatureError
Message: Signature verification failed
Traceback: Traceback (most recent call last):
File "/src/libs/libapi/src/libapi/jwt_token.py", line 286, in validate_jwt
decoded = jwt.decode(
jwt=token,
...<2 lines>...
options=options,
)
File "/usr/local/lib/python3.14/site-packages/jwt/api_jwt.py", line 368, in decode
decoded = self.decode_complete(
jwt,
...<8 lines>...
leeway=leeway,
)
File "/usr/local/lib/python3.14/site-packages/jwt/api_jwt.py", line 265, in decode_complete
decoded = self._jws.decode_complete(
jwt,
...<3 lines>...
detached_payload=detached_payload,
)
File "/usr/local/lib/python3.14/site-packages/jwt/api_jws.py", line 270, in decode_complete
self._verify_signature(
~~~~~~~~~~~~~~~~~~~~~~^
signing_input,
^^^^^^^^^^^^^^
...<4 lines>...
options=merged_options,
^^^^^^^^^^^^^^^^^^^^^^^
)
^
File "/usr/local/lib/python3.14/site-packages/jwt/api_jws.py", line 417, in _verify_signature
raise InvalidSignatureError("Signature verification failed")
jwt.exceptions.InvalidSignatureError: Signature verification failedNeed help to make the dataset viewer work? Make sure to review how to configure the dataset viewer, and open a discussion for direct support.
SPECTRA Fermi-LAT Simulated Sky Maps
This repository contains the simulated dataset associated with the manuscript:
“Self-Supervised ConvLSTM for Fermi Large Area Telescope Transient Detection”
The associated manuscript is currently under review at Astronomy and Computing.
Overview
This dataset was generated to support the development and validation of self-supervised, spatio-temporal anomaly-detection methods for gamma-ray transient searches in Fermi-LAT-like observations.
Starting from long-duration gtobssim simulations within the Fermitools ecosystem, the pipeline produces daily full-sky maps of:
- counts
- exposure
The primary dataset released here is the original energy-resolved tensor with shape:
(3649, 2, 10, 360, 180)
where:
3649= valid daily frames over approximately 10 years2= channels (counts,exposure)10= logarithmically spaced energy bins spanning 100 MeV–500 GeV360 x 180= all-sky spatial grid in celestial coordinates- spatial resolution = 1 degree/pixel
One daily frame was discarded during preprocessing and quality control; therefore, the public release contains 3649 valid daily observations.
An energy-integrated representation can be derived by summing over the energy axis, yielding:
(3649, 2, 360, 180)
This reduced representation is the one used in the main ConvLSTM experiments discussed in the manuscript, whereas the full tensor released here preserves the complete spectral structure of the simulation.
Scientific context
The dataset is designed as a controlled testbed for:
- self-supervised next-frame prediction
- residual-based anomaly detection
- transient-search benchmarking
- future extensions to energy-resolved spatio-temporal modeling
It reproduces the structure of daily Fermi-LAT-like observations while keeping the simulation environment fully controlled.
Data description
Tensor axes
The main tensor follows the convention:
(time, channel, energy, x, y)
with:
time = 3649daily frameschannel = 2→counts,exposureenergy = 10logarithmic binsx = 360y = 180
Channels
channel 0: counts mapchannel 1: exposure map
Energy range
- 100 MeV to 500 GeV
- 10 logarithmically spaced bins
Spatial grid
- celestial coordinates
- Cartesian (CAR) projection
360 x 180pixels1 degree/pixel
Time coverage
- 3649 valid daily maps
- approximately 10 years of simulated observations
Repository contents
The repository structure is:
README.mdmetadata.jsondata/spectra_tensor_part_00.npyspectra_tensor_part_01.npyspectra_tensor_part_02.npyspectra_tensor_part_03.npy
load_example.py
Intended use
This dataset is intended for research purposes, including:
- anomaly detection in gamma-ray astronomy
- self-supervised spatio-temporal modeling
- benchmarking of ConvLSTM and related architectures
- methodological studies on synthetic Fermi-LAT-like sky maps
Citation
If you use this dataset, please cite the associated manuscript.
Suggested citation text:
Garinei et al., “Self-Supervised ConvLSTM for Fermi Large Area Telescope Transient Detection”, under review at Astronomy and Computing.
Important notes
- This dataset is simulated, not a redistribution of official Fermi-LAT survey data products.
- The exposure channel is included because exposure variations are an essential part of the predictive and anomaly-detection problem addressed in the manuscript.
- The repository is intended to improve reproducibility and public accessibility of the simulation products described in the paper.
Contact
For questions regarding the dataset, simulation pipeline, or manuscript status, please contact the corresponding author listed in the associated paper.
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