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sb25101602

GCN Circular 42311

Subject
sb25101602: Swift-XRT counterpart detection
Date
2025-10-16T20:00:35Z (4 days ago)
From
Phil Evans at U of Leicester <pae9@star.le.ac.uk>
Via
email
P.A. Evans (U. Leicester), J.A. Kennea (PSU), E. Ambrosi  (INAF-IASFPA) , A.P.
Beardmore (U. Leicester), M.G. Bernardini (INAF-OAB), R. Brivio (INAF-OAB), D.N.
Burrows (PSU), S. Campana (INAF-OAB), M. Capalbi (INAF-OAR), A. D'Ai (INAF-IASFPA),
P. D'Avanzo (INAF-OAB), V. D'Elia (SSDC & INAF-OAR), S. Dichiara (PSU), M. Ferro
(INAF-OAB), A. Melandri (INAF-OAR), J.P. Osborne (U. Leicester), K.L. Page (U.
Leicester), M. Perri (SSDC & INAF-OAR), C. Salvaggio (INAF-OAB), T. Sbarrato
(INAF-OAB), B. Sbarufatti (INAF-OAB), M.A. Williams (PSU) report on behalf of the
Swift-XRT team:

Swift-XRT has performed follow-up observations of the SVOM/ECLAIRs-detected
GRB251016A (sb25101602), collecting 749 s of Photon Counting (PC) mode data between
T0+6.6 ks and T0+7.4 ks after the trigger. A likely counterpart has been found. The
details of this source are:

  Source 1 (SWIFT J174512.5-393337):
  ==================================
    RA (J2000.0):   266.3024  =  17 45 12.58
    Dec (J2000.0):  -39.5606  =  -39 33 38.2
    Error:	    4.6 (arcsec, radius, 90% confidence).
    Detect flag:    GOOD
    Distance:	    4.5 arcmin from the SVOM/ECLAIRs position.
    Mean rate:	    0.057 +/- 0.011 ct s^-1
    Mean flux:	    (3.41 +/- 0.64)e-12 erg cm^-2 s^-1
    Peak rate:	    0.072 +/- 0.019 ct s^-1
    Peak flux:	    (4.4 +/- 1.1)e-12 erg cm^-2 s^-1
    ECF:	    6.02e-11 erg cm^-2 ct^-1
		      assuming NH=7.85e+21 cm^-2, gamma=1.55
		      determined from a spectral fit.
    XMM UL:	    6.5e-13 erg cm^-2 s^-1, (0.3-10 keV)
		      so the source is 3.2-sigma above this 3-sigma upper limit.
    The source may be fading, at the 1.1-sigma level.
    There are 2 2MASS objects within the source's 3-sigma error radius.


We have detected a total of 9 sources.	These have been automatically classified as
follows:
  * 1 likely counterpart
  * 0 candidate counterparts
  * 8 uncatalogued X-ray sources
  * 0 known X-ray sources

Uncatalogued X-ray sources
--------------------------

  Source 2 (SWIFT J174439.5-394550):
  ==================================
    RA (J2000.0):   266.1646  =  17 44 39.50
    Dec (J2000.0):  -39.7642  =  -39 45 51.1
    Error:	    6.1 (arcsec, radius, 90% confidence).
    Detect flag:    POOR
    Distance:	    11.4 arcmin from the SVOM/ECLAIRs position.
    Mean rate:	    0.0300 [+0.0096, -0.0079] ct s^-1
    Mean flux:	    (1.29 [+0.41, -0.34])e-12 erg cm^-2 s^-1
    Peak rate:	    0.0300 [+0.0096, -0.0079] ct s^-1
    Peak flux:	    (1.29 [+0.41, -0.34])e-12 erg cm^-2 s^-1
    XMM UL:	    7.9e-13 erg cm^-2 s^-1, (0.3-10 keV)
		      so the source is not above this 3-sigma upper limit.
    There is no evidence for fading.
    There are 5 2MASS objects within the source's 3-sigma error radius.

  Source 3 (SWIFT J174431.8-393913):
  ==================================
    RA (J2000.0):   266.1326  =  17 44 31.82
    Dec (J2000.0):  -39.6537  =  -39 39 13.3
    Error:	    5.9 (arcsec, radius, 90% confidence).
    Detect flag:    POOR
    Distance:	    5.7 arcmin from the SVOM/ECLAIRs position.
    Mean rate:	    (-1.0 +/- -1.0)e0 ct s^-1
    Mean flux:	    (-4.3 +/- -4.3)e-11 erg cm^-2 s^-1
    Peak rate:	    0.0123 [+0.0069, -0.0053] ct s^-1
    Peak flux:	    (5.3 [+2.9, -2.3])e-13 erg cm^-2 s^-1
    XMM UL:	    1.3e-12 erg cm^-2 s^-1, (0.3-10 keV)
		      so the source is not above this 3-sigma upper limit.
    There is no evidence for fading.
    There are 5 2MASS objects within the source's 3-sigma error radius.

  Source 4 (SWIFT J174456.1-392739):
  ==================================
    RA (J2000.0):   266.2340  =  17 44 56.16
    Dec (J2000.0):  -39.4609  =  -39 27 39.2
    Error:	    14.0 (arcsec, radius, 90% confidence).
    Detect flag:    POOR
    Distance:	    7.1 arcmin from the SVOM/ECLAIRs position.
    Mean rate:	    (-1.0 +/- -1.0)e0 ct s^-1
    Mean flux:	    (-3.5 +/- -3.5)e-9 erg cm^-2 s^-1
    Peak rate:	    (6.3 [+5.6, -4.0])e-3 ct s^-1
    Peak flux:	    (2.2 [+1.9, -1.4])e-11 erg cm^-2 s^-1
    ECF:	    3.48e-09 erg cm^-2 ct^-1
		      assuming NH=3.52e+22 cm^-2, gamma=5.05
		      determined from a spectral fit.
    XMM UL:	    1.0e-12 erg cm^-2 s^-1, (0.3-10 keV)
		      so the source is 1.3-sigma above this 3-sigma upper limit.
    There is no evidence for fading.
    There are 34 2MASS objects within the source's 3-sigma error radius.

  Source 5 (SWIFT J174354.6-392827):
  ==================================
    RA (J2000.0):   265.9777  =  17 43 54.65
    Dec (J2000.0):  -39.4743  =  -39 28 27.5
    Error:	    9.8 (arcsec, radius, 90% confidence).
    Detect flag:    POOR
    Distance:	    12.2 arcmin from the SVOM/ECLAIRs position.
    Mean rate:	    0.0128 [+0.0066, -0.0050] ct s^-1
    Mean flux:	    (5.5 [+2.8, -2.1])e-13 erg cm^-2 s^-1
    Peak rate:	    0.0128 [+0.0066, -0.0050] ct s^-1
    Peak flux:	    (5.5 [+2.8, -2.1])e-13 erg cm^-2 s^-1
    XMM UL:	    7.2e-13 erg cm^-2 s^-1, (0.3-10 keV)
		      so the source is not above this 3-sigma upper limit.
    There is no evidence for fading.
    There are 22 2MASS objects within the source's 3-sigma error radius.

  Source 6 (SWIFT J174500.5-394402):
  ==================================
    RA (J2000.0):   266.2523  =  17 45 00.55
    Dec (J2000.0):  -39.7341  =  -39 44 02.8
    Error:	    11.1 (arcsec, radius, 90% confidence).
    Detect flag:    POOR
    Distance:	    9.7 arcmin from the SVOM/ECLAIRs position.
    Mean rate:	    0.0156 [+0.0070, -0.0055] ct s^-1
    Mean flux:	    (6.7 [+3.0, -2.4])e-13 erg cm^-2 s^-1
    Peak rate:	    0.0156 [+0.0070, -0.0055] ct s^-1
    Peak flux:	    (6.7 [+3.0, -2.4])e-13 erg cm^-2 s^-1
    XMM UL:	    1.3e-12 erg cm^-2 s^-1, (0.3-10 keV)
		      so the source is not above this 3-sigma upper limit.
    There is no evidence for fading.
    There are 18 2MASS objects within the source's 3-sigma error radius.

  Source 7 (SWIFT J174411.2-392428):
  ==================================
    RA (J2000.0):   266.0470  =  17 44 11.28
    Dec (J2000.0):  -39.4079  =  -39 24 28.4
    Error:	    13.9 (arcsec, radius, 90% confidence).
    Detect flag:    POOR
    Distance:	    12.5 arcmin from the SVOM/ECLAIRs position.
    Mean rate:	    0.0167 [+0.0073, -0.0057] ct s^-1
    Mean flux:	    (7.2 [+3.2, -2.4])e-13 erg cm^-2 s^-1
    Peak rate:	    0.0167 [+0.0073, -0.0057] ct s^-1
    Peak flux:	    (7.2 [+3.2, -2.4])e-13 erg cm^-2 s^-1
    XMM UL:	    1.1e-12 erg cm^-2 s^-1, (0.3-10 keV)
		      so the source is not above this 3-sigma upper limit.
    There is no evidence for fading.
    A SIMBAD object `OGLE BLG-DSCT-13120' is 43.9" away.
    There are 33 2MASS objects within the source's 3-sigma error radius.

  Source 8 (SWIFT J174427.1-393500):
  ==================================
    RA (J2000.0):   266.1131  =  17 44 27.14
    Dec (J2000.0):  -39.5835  =  -39 35 00.6
    Error:	    11.9 (arcsec, radius, 90% confidence).
    Detect flag:    POOR
    Distance:	    4.3 arcmin from the SVOM/ECLAIRs position.
    Mean rate:	    (-1.0 +/- -1.0)e0 ct s^-1
    Mean flux:	    (-4.3 +/- -4.3)e-11 erg cm^-2 s^-1
    Peak rate:	    (8.7 [+6.1, -4.5])e-3 ct s^-1
    Peak flux:	    (3.7 [+2.6, -1.9])e-13 erg cm^-2 s^-1
    XMM UL:	    6.6e-13 erg cm^-2 s^-1, (0.3-10 keV)
		      so the source is not above this 3-sigma upper limit.
    There is no evidence for fading.
    There are 28 2MASS objects within the source's 3-sigma error radius.

  Source 9 (SWIFT J174502.9-392734):
  ==================================
    RA (J2000.0):   266.2622  =  17 45 02.93
    Dec (J2000.0):  -39.4596  =  -39 27 34.6
    Error:	    8.8 (arcsec, radius, 90% confidence).
    Detect flag:    POOR
    Distance:	    7.5 arcmin from the SVOM/ECLAIRs position.
    Mean rate:	    (-1.0 +/- -1.0)e0 ct s^-1
    Mean flux:	    (-4.3 +/- -4.3)e-11 erg cm^-2 s^-1
    Peak rate:	    (8.9 [+6.4, -4.7])e-3 ct s^-1
    Peak flux:	    (3.8 [+2.7, -2.0])e-13 erg cm^-2 s^-1
    XMM UL:	    7.1e-13 erg cm^-2 s^-1, (0.3-10 keV)
		      so the source is not above this 3-sigma upper limit.
    There is no evidence for fading.
    There are 11 2MASS objects within the source's 3-sigma error radius.

All fluxes are 0.3-10 keV, observed. For all flux conversions and comparisons with
catalogues and upper limits  from other missions, we assumed a power-law spectrum
with NH=3x10^20 cm^-2 and photon index (Gamma)=1.7 unless otherwise stated.

The results of the XRT-team automatic analysis of the XRT observations, including a
position-specific upper limit calculator, are available at
https://www.swift.ac.uk/SVOM/SVOM_FIELD00042.

This circular is an official product of the Swift-XRT team.




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