eRASS1_HMXB_LMC_v1.0.fitsContent of the page (HDU means "Header Data Unit" of a fits file).
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Multi-wavelength counterparts and properties, assigne confidence classes.
| Key | Value | Type | Comment |
|---|
| Name | Type | Unit | Description |
|---|---|---|---|
| XrayName | char[23] | None | |
| eRASS1_name | char[23] | None | |
| seqno_Kaltenbrunner | int64 | None | Seqno in Kaltenbrunner+ submitted |
| DETUID_eRASS1 | char[36] | None | |
| RA_eRASS1 | float64 | deg | |
| DEC_eRASS1 | float64 | deg | |
| Pspin | float32 | sec | Spin period |
| Porb | float32 | days | Orbital period |
| Gaia_DR3_name | char[28] | None | Gaia DR3Name |
| Gmag_Gaia | float64 | None | Gaia Gmag |
| RA_Gaia | float64 | degree | Gaia RA |
| DEC_Gaia | float64 | degree | Gaia Dec |
| ps | char[3] | None | Flag: spin period known |
| xrb | char[3] | None | Flag: known HMXB due to other reason than spin period |
| px | char[2] | None | Flag: orbital period known from X-rays |
| po | char[3] | None | Flag: orbital period known from optical |
| os | char[3] | None | Flag: orbital solution |
| xv | char[8] | None | Flag: X-ray variability |
| xs | char[3] | None | Flag: X-ray spectrum matches HMXB |
| oi | char[3] | None | Flag: good optical match |
| em | char[2] | None | Flag: emission line in spectrum |
| sx | char[3] | None | Flag: IR excess in SED fit |
| ix | char[2] | None | Flag: IR excess in IR colours |
| qc | char[2] | None | Flag: position matches AGN candidate |
| nv | char[2] | None | Flag: no match in VMC selection |
| nm | char[2] | None | Flag: no match in MCPS selection |
| ns | char[2] | None | Flag: SED fit does not match high-mass star |
| confclass_Kaltenbrunner | char | None | Confidence class in Kaltenbrunner+ submitted |
| RA_MCPS | float64 | deg | |
| DEC_MCPS | float64 | deg | |
| Vmag_MCPS | float32 | mag | |
| e_Vmag_MCPS | float32 | mag | |
| POS_ERR | float64 | None | POS_ERR eRAS1 |
| IAUNAME_VMC | char[29] | None | |
| RA2000_VMC | float64 | deg | |
| DEC2000_VMC | float64 | deg |
Kaltenbrunner at al., submitted to A&A;, A comprehensive catalogue of High-Mass X-ray binaries in the Large Magellanic Cloud detected during the first eROSITA all-sky survey
This work is based on data from eROSITA, the soft X-ray instrument aboard SRG, a joint Russian-German science mission supported by the Russian Space Agency (Roskosmos), in the interests of the Russian Academy of Sciences represented by its Space Research Institute (IKI), and the Deutsches Zentrum für Luft- und Raumfahrt (DLR). The SRG spacecraft was built by Lav- ochkin Association (NPOL) and its subcontractors, and is operated by NPOL with support from the Max Planck Institute for Extraterrestrial Physics (MPE). The development and construction of the eROSITA X-ray instrument was led by MPE, with contributions from the Dr. Karl Remeis Observatory Bamberg & ECAP (FAU Erlangen-Nuernberg), the University of Hamburg Observatory, the Leibniz Institute for Astrophysics Potsdam (AIP), and the Institute for As- tronomy and Astrophysics of the University of Tübingen, with the support of DLR and the Max Planck Society. The Argelander Institute for Astronomy of the University of Bonn and the Ludwig Maximilians Universität Munich also participated in the science preparation for eROSITA. The eROSITA data shown here were processed using the eSASS software system developed by the Ger- man eROSITA consortium. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France (Ochsenbein 1996). The original descrip- tion of the VizieR service was published in Ochsenbein et al. (2000). This re- search has made use of the Spanish Virtual Observatory (https://svo.cab.inta- csic.es) project funded by MCIN/AEI/10.13039/501100011033/ through grant PID2020-112949GB-I00. The LCO observations have been made possible by the support of the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy-EXC-2094-390783311. RW is funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) – 446281683. GV acknowledges support from the Hellenic Foun- dation for Research and Innovation (H.F.R.I.) through the project ASTRAPE (Project ID 7802).