REVIEW 21 cited by
Friends and Foes in Learning from Noisy Labels
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
Learning from examples with noisy labels has attracted increasing attention recently. But, this paper will show that the commonly used CIFAR-based datasets and the accuracy evaluation metric used in the literature are both inappropriate in this context. An alternative valid evaluation metric and new datasets are proposed in this paper to promote proper research and evaluation in this area. Then, friends and foes are identified from existing methods as technical components that are either beneficial or detrimental to deep learning from noisy labeled examples, respectively, and this paper improves and combines technical components from the friends category, including self-supervised learning, new warmup strategy, instance filtering and label correction. The resulting F&F method significantly outperforms existing methods on the proposed nCIFAR datasets and the real-world Clothing1M dataset.
Forward citations
Cited by 21 Pith papers
-
Spectropolarimetric detection of baryonic mass loading in a transient relativistic jet: application to the black hole X-ray binary Swift J1727.8$-$1613
Transient Faraday-complex spectropolarimetric structure detected during radio flaring of Swift J1727 implies internal Faraday rotation from electron-proton jet plasma with rotating mass ~10^21 g, a small fraction of a...
-
Accretion Regimes of Neutrino-Cooled Flows onto Black Holes
A 1D relativistic disk model charts the accretion regimes of neutrino-cooled flows and predicts r-process outflows up to black hole masses of about 3000 solar masses.
-
Einstein Probe Fast X-ray Transients Extend the Physical Parameter Space of Relativistic Jets
Einstein Probe fast X-ray transients are too spectrally soft to be ordinary long GRBs viewed off-axis, pointing to a distinct or intrinsically softer class of relativistic explosions.
-
How Low Can We Go? Minimum Spectroscopic Requirements For Supernova Subtype Classification
ABC-SN classifies ten supernova subtypes with no performance loss down to R_λ=50 and SNR=5, and only minimal loss at R_λ=25.
-
The Environments of Luminous Fast Blue Optical Transients: Evidence for a Compact Object and Wolf-Rayet Star Merger Origin
LFBOT hosts are star-forming and moderately metal-poor, with many events offset from bright light, favoring a compact-object–Wolf-Rayet merger origin over TDEs or standard CCSNe.
-
EP250827b/SN 2025wkm: An X-ray Flash-Supernova Powered by a Central Engine and Circumstellar Interaction
EP250827b/SN 2025wkm is an X-ray flash supernova at z=0.1194 powered by a long-lived magnetar and disk winds interacting with extended circumstellar medium, without an on-axis relativistic jet.
-
Fine-Tuned Supernova or Failed Explosion? Decoding the Origins of the G3425 Binary
G3425's nearly circular orbit points to a 4 to 4.4 solar-mass black hole from a failed supernova rather than a neutron star from a standard explosion.
-
Identifying Merger-Driven Long Gamma-Ray Bursts based on Machine Learning
Machine learning on the three-episode structure of 29 Fermi/GBM bursts separates eight merger-driven long GRBs, six of which are newly identified, using short precursor duration, short waiting time, and short precurso...
-
Multi-Instrument Search for Gamma-Ray Counterpart of X-ray Transients detected by EP/WXT
A multi-instrument search pipeline called ETJASMIN finds gamma-ray counterparts for 14 of 63 EP/WXT X-ray transients, with improved upper limits for the rest.
-
Fermi-GBM Observations of GRB 230307A: An Exceptionally Bright Long-Duration Gamma-ray Burst with an Associated Kilonova
GRB 230307A shows spectral evolution consistent with fast-cooling synchrotron emission, a bulk Lorentz factor of about 1600, and late high-latitude emission, supporting a compact merger origin for this long burst.
-
The peak flux of long gamma-ray bursts in the E$_{\rm p,i}$--L$_{\rm iso}$ diagram and in the classification
Peak flux selection biases the best-fit Ep,i-Liso correlation of long GRBs, and a small set of low-luminosity high-flux bursts may be non-collapsars.
-
Magnetic Burial in Millisecond Magnetars and Late GRB Afterglow Signatures
A magnetar whose dipole field was submerged by fallback accretion and re-emerges in about 5.5 years can explain the late-time X-ray brightening of the neutron-star merger GW170817.
-
Prospects for the Detection of High-Redshift Gamma-Ray Bursts in the Era of EP and SVOM
Using a Swift-calibrated population model, the paper forecasts 5.1 high-redshift (z>6) GRB detections per year for EP/WXT and 0.7 per year for SVOM/ECLAIRs.
-
Observational Properties of Thermal Emission from Relativistic Jets Embedded in AGN Disks
Relativistic jets embedded in AGN disks should produce soft X-ray thermal flares lasting 100 to 100,000 seconds, with UV/optical flares only from the most powerful jets.
-
A Roadmap for Transient Hunters: Mapping Stellar Mass and Star Formation Rate Anisotropies in the Local Universe
All-sky maps of stellar mass and star formation rate in the local universe, binned by telescope field-of-view and distance, provide optimized pointing priors for transient surveys.
-
Tightening Bounds on Warm Dark Matter with High-Redshift Gamma-Ray Bursts
Using the redshift distribution of 118 luminous Swift GRBs, warm dark matter particles are bounded to mx ≥ 1.3 keV at 95% CL (≥3.4 keV if GRBs exactly trace the SFR).
-
Gamma-ray bursts reveal the history and faint contributors of cosmic reionization
Long gamma-ray bursts imply a higher cosmic star formation rate density at z>6 than galaxy surveys detect, sufficient to drive reionization with moderate ionizing efficiency and escape fraction, implying a large popul...
-
Deciphering the Physical Origin of GRB 240825A: A Long GRB Lacking a Bright Supernova
GRB 240825A is best explained as a collapsar with a faint or dust-obscured supernova, despite several merger-like prompt signatures.
-
The Event Rate and Luminosity Function of Fermi/GBM Gamma-Ray Bursts
Bright Fermi/GBM gamma-ray bursts form at a rate that matches star formation, while faint and medium bursts show an excess at low redshift.
-
GRB 221009A and the Apparently Most Energetic Gamma-Ray Bursts
Using 185 energetic gamma-ray bursts, the authors confirm a cutoff near Eiso = 4×10^54 erg that is not invalidated by GRB 221009A.
-
Stellar-Mass Black Holes
A concise review of stellar-mass black hole physics and observations, plus a speculative interstellar mission concept.
Discussion (0). Continue with ORCID to comment.