J/MNRAS/537/931          Chandra X-ray flares and dips         (Dillmann+, 2025)

Representation learning for time-domain high-energy astrophysics: Discovery of extragalactic fast X-ray transient XRT 200515. Dillmann S., Martinez-Galarza J.R., Soria R., Di Stefano R., Kashyap V.L. <Mon. Not. R. Astron. Soc. 537, 931 (2025)> =2025MNRAS.537..931D 2025MNRAS.537..931D (SIMBAD/NED BibCode)
ADC_Keywords: X-ray sources ; Transient ; Photometry, infrared ; Photometry, SDSS ; Optical Keywords: methods: data analysis - software: machine learning - stars: magnetars - stars: peculiar - X-rays: bursts - (transients:) gamma-ray bursts Abstract: We present a novel representation learning method for downstream tasks like anomaly detection, unsupervised classification, and similarity searches in high- energy data sets. This enabled the discovery of a new extragalactic fast X-ray transient (FXT) in Chandra archival data, XRT 200515, a needle-in-the-haystack event and the first Chandra FXT of its kind. Recent serendipitous discoveries in X-ray astronomy, including FXTs from binary neutron star mergers and an extragalactic planetary transit candidate, highlight the need for systematic transient searches in X-ray archives. We introduce new event file representations, E-t maps and E-t-dt cubes, that effectively encode both temporal and spectral information, enabling the seamless application of machine learning to variable-length event file time series. Our unsupervised learning approach employs PCA or sparse autoencoders to extract low-dimensional, informative features from these data representations, followed by clustering in the embedding space with DBSCAN. New transients are identified within transient- dominant clusters or through nearest-neighbour searches around known transients, producing a catalogue of 3559 candidates (3447 flares and 112 dips). XRT 200515 exhibits unique temporal and spectral variability, including an intense, hard <10s initial burst, followed by spectral softening in an ∼800s oscillating tail. We interpret XRT 200515 as either the first giant magnetar flare observed at low X-ray energies or the first extragalactic Type I X-ray burst from a faint, previously unknown low-mass X-ray binary in the LMC. Our method extends to data sets from other observatories such as XMM-Newton, Swift-XRT, eROSITA, Einstein Probe, and upcoming missions like AXIS. Description: We tabulate the meta-data of X-ray flares and dips from the Chandra Source Catalog (CSC) found as part of the paper. Please get in touch with Steven Dillmann (stevendi(at)stanford.edu, steven.dillmann(at)outlook.com) for further information or data (e.g. the individual region eventfiles associated with each flaring/dipping source, that can be used to plot the lightcurves). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 1837 3559 Chandra X-ray flares and dips -------------------------------------------------------------------------------- See also: IX/70 : Chandra Source Catalog Release 2 (CSC 2.1) (Evans+, 2024) II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016) I/345 : Gaia DR2 (Gaia Collaboration, 2018) I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022) Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh Right ascension (J2000) 3 A1 --- --- [:] 4- 5 I2 min RAm Right ascension (J2000) 6 A1 --- --- [:] 7- 11 F5.2 s RAs Right ascension (J2000) 13 A1 --- DE- Declination sign (J2000) 14- 15 I2 deg DEd Declination (J2000) 16 A1 --- --- [:] 17- 18 I2 arcmin DEm Declination (J2000) 19 A1 --- --- [:] 20- 24 F5.2 arcsec DEs Declination (J2000) 26- 35 A10 --- CatId Catalog ID, NNNNN_NNNN 37- 58 A22 --- CSCName Name of the source in the CSC, 2CXO JHHMMSS.s+DDMMSS 60 A1 --- TransType [F/D] Transient (F:flare, D:dip) 62- 78 A17 --- CSCcoord J2000 coordinates in the CSC, JHHMMSS.s+DDMMSS 80- 99 F20.16 deg RACdeg Right ascension of the source in the CSC 101- 120 F20.16 deg DECdeg Declination of the source in the CSC 122- 126 I5 --- CSCobsId Observation ID in the CSC 128- 131 I4 --- CSCregId Region ID in the CSC 133- 152 F20.16 --- CSCsigni Highest flux significance 154- 175 E22.17 --- CSCFluxap-b ? Broad band flux in the CSC 177- 195 F19.16 --- CSChardhm ? Hard-to-medium hardness ratio 197- 215 F19.16 --- CSChard-ms ? Medium-to-soft hardness ratio 217- 235 E19.16 --- CSChard-hs ? Hard-to-soft hardness ratio 237- 255 E19.15 --- CSCvarProb-b ? Variability probability in broad band 257- 273 F17.15 --- CSCvarProb-h ? Variability probability in soft band 275- 292 F18.16 --- CSCvarProb-m ? Variability probability in medium band 294- 310 F17.15 --- CSCvarProb-s ? Variability probability in hard band 312- 315 F4.1 --- CSCvarIndx-b ? Variability index in broad band 317- 335 A19 "datime" CSCgti-obs Start time of observation 337- 355 A19 "datime" CSCgti-end End time of observation 357- 375 F19.16 arcmin CSCtheta Off-axis angle of the source 377- 381 I5 ct CSCctapb Source region counts 383- 387 I5 ct CSCctapbkgb Background region counts 389 A1 --- CSCtype [P/X] Source type (P:point, X:ext.) 391- 395 A5 --- CSC2.1Flag True: CSC2.1, False: CSC2.0 397- 414 I18 --- PSid ?=0 PanSTARRS-1 unique object ID 416- 432 F17.1 --- PSintId ? PanSTARRS-1 internal object ID 434- 443 F10.8 arcsec sepCSC-PS ? Distance CSC-PS source 445- 461 F17.12 mag PSgmag ?=- PanSTARRS-1 g magnitude 463- 479 F17.12 mag PSrmag ?=- PanSTARRS-1 r magnitude 481- 497 F17.12 mag PSimag ?=- PanSTARRS-1 i magnitude 499- 515 F17.12 mag PSzmag ?=- PanSTARRS-1 z magnitude 517- 535 I19 --- GaiaId ?=0 Gaia unique object ID 537- 549 E13.7 arcsec sepCSC-Gaia ? Distance CSC-GAIA source 551- 565 F15.12 mag Gmag ? Gaia G magnitude 567- 579 F13.8 km/s RV ? Gaia radial velocity 581- 599 F19.16 mas plx ? Gaia parallax 601- 611 F11.8 mag Bp-Rp ? Gaia BP-RP magnitude 613- 622 F10.7 mag GMAG ? Gaia absolute magnitude 624- 640 I17 --- LSId ?=0 Legacy Survey DR10 ID 642- 648 F7.1 --- LSobjectId ? Legacy Survey DR10 object ID 650- 661 E12.8 arcsec sepCSC-LS ? Distance CSC-LS source 663- 671 F9.6 mag LSgmag ? Legacy Survey DR10 g magnitude 673- 681 F9.6 mag LSrmag ? Legacy Survey DR10 r magnitude 683- 691 F9.6 mag LSzmag ? Legacy Survey DR10 z magnitude 693- 708 A16 --- 2MASSId 2MASS name 710- 720 F11.9 arcsec sepCSC-2M ? Distance CSC-2MASS source 722- 727 F6.3 mag Jmag ? 2MASS J magnitude 729- 734 F6.3 mag Hmag ? 2MASS H magnitude 736- 741 F6.3 mag Kmag ? 2MASS K magnitude 743- 760 F18.16 arcsec sepCSC-Sp ? Distance CSC-SPEC source 762- 767 A6 --- Spclass SDSS spectroscopic clas 769- 787 A19 --- Spsubclass SDSS spectroscopic subclass 789- 802 E14.11 --- Spz ? SDSS spectroscopic redshift 804- 817 E14.11 --- e_Spz ? SDSS spectroscopic redshift error 819- 827 F9.4 0.1nm Spwavemin ? SDSS spectroscopic minimum wavelength 829- 837 F9.3 0.1nm Spwavemax ? SDSS spectroscopic maximum wavelength 839- 841 F3.1 --- Spzwarning ? SDSS spectroscopic redshift warning 843- 852 E10.7 --- Spsn ? SDSS spectroscopy median SN 854- 872 I19 --- SDSSId ? SDSS object ID 874- 881 F8.6 --- sepCSC-SDSS ? Distance CSC-SDSS source 883 A1 --- SDSSType [S/G] SDSS type (S:star, G:galaxy) 885-1718 A834 --- SIM-ids SIMBAD object ID 1720-1741 A22 --- SIM-otype SIMBAD object type 1743-1763 A21 --- SIM-sptype SIMBAD spectral type 1765-1771 F7.4 mas SIM-plx ? SIMBAD parallax 1773-1780 F8.3 mas/yr SIM-pmRA ? SIMBAD proper motion in RA 1782-1789 F8.3 mas/yr SIM-pmDE ? SIMBAD proper motion in DEC 1791-1808 E18.14 km/s SIM-RV ? SIMBAD radial velocity 1810-1818 E9.6 --- SIM-z ? SIMBAD redshift 1820-1837 F18.16 arcsec sepCSC-SIM ? Distance CSC-SIMBAD source -------------------------------------------------------------------------------- Acknowledgements: Steven Dillmann, stevendi(at)stanford.edu
(End) Patricia Vannier [CDS] 17-Feb-2025
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line