[ Previous | Next | ADS ]

SWIFT/BAT Detections of Hard X-ray Sources II

ATel #669; J. Tueller (NASA/GSFC), S. Barthelmy (NASA/GSFC), D. Burrows (PSU), A. Falcone (PSU), N. Gehrels (NASA/GSFC), D. Grupe (PSU), J. Kennea (PSU), C. B. Markwardt (U. Md. & NASA/GSFC), R. F. Mushotzky (NASA/GSFC), G. K. Skinner (CESR)
on 5 Dec 2005; 19:14 UT
Credential Certification: Jack Tueller (jack.tueller-1@nasa.gov)

Subjects: X-ray, Gamma Ray, AGN, Black Hole, Cataclysmic Variable, Quasar

Referred to by ATel #: 677, 684, 697, 715, 720, 735, 785, 847, 853, 859

Table of BAT survey source identifications described in ATEL #668.

  
   BAT Name           RA    (J2000) Dec      ER    Notes Type  Identification
SWIFT J0444.1+2813 04 44 09.0 +28 13 00.1 3.4 - G 2MASX J04440903+2813003
SWIFT J0505.7-2348 05 05 45.7 -23 51 14.4 3.4 1 G 2MASX J05054575-2351139
SWIFT J0519.5-3140 05 19 35.7 -32 39 25.0 3.3 - Sy1.5 ESO 362-G018
SWIFT J0746.3+2548 07 46 25.7 +25 49 00.0 3.3 - QSO SDSS J074625.87+254902.2
SWIFT J0750.9+1439 07 51 17.2 +14 44 21.2 3.2 - CV PQ Gem
SWIFT J0917.2-6221 09 16 08.9 -62 19 29.6 3.3 - Sy1 IRAS 09149-6206
SWIFT J1010.1-5747 10 11 03.0 -57 48 14.7 4.3 2 - SWIFT J101103.3-574814
SWIFT J1038.8-4942 10 38 45.0 -49 46 55.1 3.3 - G 2MASX J10384520-4946531
SWIFT J1142.7+7149 11 43 38.2 +71 41 20.6 3.3 - CV DO Draconis
SWIFT J1238.9-2720 12 38 54.5 -27 18 27.8 3.6 - G ESO 506-G027
SWIFT J1559.5+2553 15 59 30.2 +25 55 14.2 3.3 - Sym T CrB
SWIFT J1922.7-1716 19 22 37.0 -17 17 02.6 3.2 - - SWIFT J192237.0-171702
SWIFT J2000.6+3210 20 00 21.9 +32 11 21.9 3.6 3 - 2MASS J20002185+3211232
SWIFT J2127.4+5654 21 27 45.4 +56 56 34.6 3.4 - - NVSS J212745+565633

ER - 90% error radius
1 - identified as XSS J05054-2348 by BAT as noted in Revnivtsev et al, astro-ph/0511444
2 - position is 30' from GRO J1008-57
3 - ref. 2MASS All-Sky Point Source Catalog (PSC)
G - galaxy
CV - cataclysmic variable, DQ Her
Sym - symbiotic star

LOG NH* Z COMMENTS
SWIFT J0444.1+2813 ~23 .011 not classified as a Seyfert
SWIFT J0505.7-2348 ~23 .035 unclassified
SWIFT J0519.5-3140 ~0 .013 The XRT flux should have been detected by ROSAT RASS
at 0.06 cnts s-1.
Two component XRT spectrum.
SWIFT J0746.3+2548 ~0 3.0 blazar, variable XRT spectrum, BAT photon spectrum
is E-0.6 to 200 keV.
SWIFT J0750.9+1439 DQ Her type
SWIFT J0917.2-6221 ~22 .057 bright UV counterpart in UVOT
SWIFT J1010.1-5747 no cataloged source, gal b = -1.3 deg.
SWIFT J1038.8-4942 ~22 unclassified
SWIFT J1142.7+7149 DQ Her type
SWIFT J1238.9-2720 ~23 .025 compton thick object, EW of the Fe K line is ~500 ev
SWIFT J1559.5+2553 KT = 12±4 keV
SWIFT J1922.7-1716 ~21 power law photon index = 2.05 ± 0.05,
no cataloged source, UVOT counterpart not consistent
with Palomar survey, gal l = 20.7 deg, b = -14.5 deg
SWIFT J2000.6+3210 ~22 gal b = +1.1 deg.
SWIFT J2127.4+5654 ~22 variable radio source, 1RXH J212745.4+565634

* LOG NH derived from preliminary fits to XRT spectra, uncertainty ± 0.5
due to model dependence of fit values