obsid int64 2.26k 2.26k | source stringclasses 1
value | ra float64 3.69 3.69 | dec float64 -39.24 -39.24 | otype stringclasses 2
values | hardness_ratio float64 -0.87 -0.87 | bb_kt float64 0.19 0.19 | powlaw_gamma float64 5.03 5.03 | var_index_b int64 5 5 | var_prob_b float64 0.7 0.7 | source_flag int64 1 1 | bb_stat float64 3.97 3.97 | brems_stat float64 3.89 3.89 | powlaw_stat float64 3.8 3.8 | apec_stat float64 | answer stringclasses 5
values |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2,255 | 2CXO J001445.7-391435 | 3.690639 | -39.243245 | XB? | -0.866958 | 0.19266 | 5.02882 | 5 | 0.701548 | 1 | 3.969824 | 3.894318 | 3.800722 | null | [MENTIONED: YES]
### A) X-ray Properties
The source is classified as an EB* type, which generally refers to eclipsing binaries. In the context of X-ray observations, such sources can exhibit variability linked to their orbital motion. This variability often includes transient behavior, where the source might have peri... |
2,255 | 2CXO J001445.7-391435 | 3.690639 | -39.243245 | Unknown | -0.866958 | 0.19266 | 5.02882 | 5 | 0.701548 | 1 | 3.969824 | 3.894318 | 3.800722 | null | [MENTIONED: YES]
### A) X-ray Properties
The source classified as type EB* demonstrates notable variability patterns. |
2,255 | 2CXO J001445.7-391435 | 3.690639 | -39.243245 | Unknown | -0.866958 | 0.19266 | 5.02882 | 5 | 0.701548 | 1 | 3.969824 | 3.894318 | 3.800722 | null | [MENTIONED: YES]
The source is classified as type EB*, typically representing eclipsing binaries, which could include a wide range of variability characteristics.
### A) X-ray Properties
- **Variability**:
- Eclipsing binaries can exhibit transient behavior such as flaring during periastron passages due to grav... |
2,255 | 2CXO J001445.7-391435 | 3.690639 | -39.243245 | Unknown | -0.866958 | 0.19266 | 5.02882 | 5 | 0.701548 | 1 | 3.969824 | 3.894318 | 3.800722 | null | [MENTIONED: YES]
The source in question is classified as type EB*, which generally refers to eclipsing binaries, particularly those exhibiting variability.
### A) X-ray Properties
- **Variability**: The literature on X-ray sources of class EB* typically highlights their transient behavior, indicating significant v... |
2,255 | 2CXO J001445.7-391435 | 3.690639 | -39.243245 | Unknown | -0.866958 | 0.19266 | 5.02882 | 5 | 0.701548 | 1 | 3.969824 | 3.894318 | 3.800722 | null | [MENTIONED: YES]
### A) X-ray Properties
The source classified as type EB* exhibits variability characteristics typical of eclipsing binaries.
Spectral properties derived from analysis suggest that the source may be characterized using a variety of spectral models.
### B) Use in Scientific Hypotheses
Generally, the ... |
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