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TILED_GRB00092
NEWGRB
92
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GRB 200803A: Swift observation summary
  
  
    | Mission: | Fermi/LAT | 
|---|
    | GRB RA: | 311.290° | 
|---|
    | GRB Dec: | -63.080° | 
|---|
    | GRB Err: | 27.6 arcmin | 
|---|
    | T0: | 2020-08-03 03:34:26 UT | 
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    | Galactic: | 332.73° -36.76° | 
|---|
    | Galactic NH: | 4.04× 1020 cm-2 | 
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    | Galactic E(B-V): | 0.05207005 | 
|---|
  
  
  
   
  
  
    
Source 1 has been manually confirmed as the GRB afterglow; data for this object are now available through the main GRB results area for this GRB.
  About tiled field analysis.
  
  
    So far 3 fields have been scheduled for observations.
    Data are available and processed for 4 of these.
    The list gives the exposure time used in source detection. If any individual sources
    were selected for follow-up observations, the source detection is not repeated for the follow up
    observations and the table below is not updated.
  
  
- 21021 — 1.2 ks of cleaned data taken between 2020-08-03 13:38:57 and 2020-08-03 16:43:07
- 21022 — 1.2 ks of cleaned data taken between 2020-08-03 13:44:41 and 2020-08-03 16:48:57
- 21023 — 1.2 ks of cleaned data taken between 2020-08-03 13:50:05 and 2020-08-03 16:54:03
- 21024 — 1.2 ks of cleaned data taken between 2020-08-03 13:55:49 and 2020-08-03 16:36:26
Probable afterglow details
A source was found which matches the afterglow criteria.
    
    
    
    
    
    
      | # | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2
 | Dist from LAT pos
 | Exposure | Notes | Vizier | 
    
    
  
      | 1 [details]
 | 20h 44m 22.35s311.09311° | -62° 56′ 41.5″-62.94487° | 2.6′′ | Good | 9.7′ | 2.3 ks | The source is 7.6-σ above the 2SXPS limit. |  | 
  | 
  Mean XRT rate: 2.4 (±0.4) ×10-2 ct s-1Peak XRT rate: 4.8 (±1.2) ×10-2 ct s-1RASS PSPC 3-σ upper limit: 0.02 ct s-1 (XRT equiv count-rate)Mean XRT flux: 6.3 (±1.0) ×10-13 erg cm-1s-1Peak XRT flux: 1.3 (±0.3) ×10-12 erg cm-1s-1Products: Light curve | Spectrum | Enhanced positionExpected serendipitous sources: ~0.1 [What is this?] | 
  
1 Radius, 90% confidence.
2 Indicates how likely the source is to be real. See the 1SXPS documentation.
* The position was enhanced using astrometry derived from the Swift UVOT.
† The position was astrometrically corrected using the XRT sources and the 2MASS catalogue.
  Find an upper limit.
  
Sources found so far
So far 7 sources have been found in the XRT data. 3 sources match catalogued sources.
    
    
    
    
    
    
    
    
      | # | RA (J2000) | Dec (J2000) | Err901 | Detection Flag2
 | Dist from LAT pos
 | Exposure | Notes | Vizier | 
    
    
  
      | 1 [details]
 | 20h 44m 22.35s311.09311° | -62° 56′ 41.5″-62.94487° | 2.6′′ | Good | 9.7′ | 2.3 ks | The source is 7.6-σ above the 2SXPS limit. |  | 
  | 
  Mean XRT rate: 2.4 (±0.4) ×10-2 ct s-1Peak XRT rate: 4.8 (±1.2) ×10-2 ct s-1RASS PSPC 3-σ upper limit: 0.02 ct s-1 (XRT equiv count-rate)Mean XRT flux: 6.3 (±1.0) ×10-13 erg cm-1s-1Peak XRT flux: 1.3 (±0.3) ×10-12 erg cm-1s-1Products: Light curve | Spectrum | Enhanced positionExpected serendipitous sources: ~0.1 [What is this?] | 
    
      | 2 [details]
 | 20h 42m 28.09s310.61703° | -63° 06′ 43.7″-63.11215° | 6.5′′ | Poor | 18.4′ | 1.2 ks |  |  | 
  | 
  Mean XRT rate: 2.8 (+2.8, -1.7) ×10-3 ct s-1Peak XRT rate: 2.8 (+2.8, -1.7) ×10-3 ct s-1RASS PSPC 3-σ upper limit: 0.04 ct s-1 (XRT equiv count-rate)Products: Light curve | 
    
      | 3 [details]
 | 20h 45m 22.11s311.34211° | -63° 00′ 24.9″-63.00692° | 5.2′′ | Good | 4.6′ | 2.4 ks | Matches SIMBAD source: MOST 2041-631, 1.6″ away. |  | 
  | 
  Mean XRT rate: 1.06 (+0.32, -0.27) ×10-2 ct s-1Peak XRT rate: 1.06 (+0.32, -0.27) ×10-2 ct s-1RASS PSPC 3-σ upper limit: 0.06 ct s-1 (XRT equiv count-rate)Mean XRT flux: 5.7 (+1.7, -1.4) ×10-13 erg cm-1s-1Peak XRT flux: 5.7 (+1.7, -1.4) ×10-13 erg cm-1s-1Products: Light curve | Spectrum | Enhanced positionExpected serendipitous sources: ~0.5 [What is this?] | 
    
      | 4 [details]
 | 20h 48m 03.63s312.01512° | -63° 01′ 58.8″-63.03299° | 10.3′′ | Reasonable | 19.9′ | 1.2 ks |  |  | 
  | 
  Mean XRT rate: 6.0 (+3.3, -2.4) ×10-3 ct s-1Peak XRT rate: 6.0 (+3.3, -2.4) ×10-3 ct s-1RASS PSPC 3-σ upper limit: 0.05 ct s-1 (XRT equiv count-rate)Mean XRT flux: 2.48 (+1.35, -1.00) ×10-13 erg cm-1s-1Peak XRT flux: 2.48 (+1.35, -1.00) ×10-13 erg cm-1s-1Products: Light curve | SpectrumExpected serendipitous sources: ~0.9 [What is this?] | 
    
      | 5 [details]
 | 20h 45m 19.44s311.33098° | -63° 06′ 55.5″-63.11542° | 4.8′′ | Good | 2.4′ | 2.5 ks |  |  | 
  | 
  Mean XRT rate: 7.6 (+2.6, -2.1) ×10-3 ct s-1Peak XRT rate: 7.6 (+2.6, -2.1) ×10-3 ct s-1RASS PSPC 3-σ upper limit: 0.08 ct s-1 (XRT equiv count-rate)Mean XRT flux: 4.3 (+1.5, -1.2) ×10-13 erg cm-1s-1Peak XRT flux: 4.3 (+1.5, -1.2) ×10-13 erg cm-1s-1Products: Light curve | Spectrum | Enhanced positionExpected serendipitous sources: ~0.8 [What is this?] | 
    
      | 6 [details]
 | 20h 45m 40.07s311.41694° | -62° 54′ 36.5″-62.91013° | 4.6′′ | Good | 10.8′ | 1.2 ks | Matches known X-ray source: 2SXPS J204540.1-625438 (from 2SXPS), 2.2″ away. Matches SIMBAD source: UCAC3 55-399254, 2.1″ away.
 |  | 
  | 
  Mean XRT rate: 6.6 (+3.3, -2.5) ×10-3 ct s-1Peak XRT rate: 6.6 (+3.3, -2.5) ×10-3 ct s-1RASS PSPC 3-σ upper limit: 0.0×100 ct s-1 (XRT equiv count-rate)Mean XRT flux: 2.23 (+1.10, -0.84) ×10-13 erg cm-1s-1Peak XRT flux: 2.23 (+1.10, -0.84) ×10-13 erg cm-1s-1Products: Light curve | SpectrumExpected serendipitous sources: ~0.9 [What is this?] | 
    
      | 7 [details]
 | 20h 43m 15.96s310.81649° | -62° 55′ 56.6″-62.93239° | 4.6′′ | Good | 15.6′ | 1.2 ks | Matches known X-ray source: 2SXPS J204316.1-625603 (from 2SXPS), 6.8″ away. Matches SIMBAD source: PMN J2043-6256, 5.5″ away.
 |  | 
  | 
  Mean XRT rate: 1.1 (+0.5, -0.4) ×10-2 ct s-1Peak XRT rate: 1.1 (+0.5, -0.4) ×10-2 ct s-1RASS PSPC 3-σ upper limit: 0.0×100 ct s-1 (XRT equiv count-rate)Products: Light curve | SpectrumExpected serendipitous sources: ~0.5 [What is this?] | 
  
1 Radius, 90% confidence.
2 Indicates how likely the source is to be real. See the 1SXPS documentation.
* The position was enhanced using astrometry derived from the Swift UVOT.
† The position was astrometrically corrected using the XRT sources and the 2MASS catalogue.
Image
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