Dictionary of Nomenclature of Celestial Objects
(Last update: 16-Aug-2019)

Result of query: info cati CXOLV J005511.47-374015.3$



.
 

Details on Acronym:   CXOLV
   CXOLV (Chandra X-ray Observatory Local Volume Survey) Write:<<CXOLV JHHMMSS.s+DDMMSS>> N: about 700 Object:Poss. LMXB + Poss. HMXB  (SIMBAD class: X = X-ray source) Note:The Chandra Local Volume Survey is a deep, volume-limited X-ray survey of five nearby galaxies (NGC 55, NGC 300, NGC 404, NGC 2403, and NGC 4214) with matched Hubble Space Telescope observations down to an absolute V-band magnitude of ∼0. These galaxies contain ∼99% of the extragalactic stellar mass and 90% of the recent star formation outside of the Local Group out to a distance of 3.3 Mpc and span a range of stellar masses, morphologies, and metallicities. We are generating X-ray point source catalogs for each galaxy and correlating the properties of the X-ray binary populations (such as the X-ray luminosity function) to the host galaxy's star formation rate, thereby providing an observational test of theoretical predictions.
We will first be publishing the X-ray source catalog of NGC 300, with additional papers on the remaining four galaxies forthcoming. Each galaxy hosts 70-190 X-ray point sources, for a total survey sample of up to ∼700 X-ray sources requiring designations. in source:NGC 55 in source:NGC 300 in source:NGC 404 in source:NGC 2403 in source:NGC 4214 Auth.:Breanna Binder

University of Washington Originof the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym:   CXOLV
   CXOLV (Chandra X-ray Observatory Local Volume Survey) Write:<<CXOLV JHHMMSS.ss+DDMMSS.s>> N: 95+74+967 Object:Poss. LMXB + Poss. HMXB  (SIMBAD class: X = X-ray source) Note:Chandra ACIS observations of N=95+72+460 X-ray point sources as part of the Chandra Local Volume Survey.
See also [BWE2012], [BWE2013] and [BWE2015]. in source:NGC 55 in source:NGC 300 in source:NGC 404 in source:NGC 2403 in source:NGC 4214 Ref:=2012ApJ...758...15B byBINDER B. , WILLIAMS B.F., ERACLEOUS M., GAETZ T.J., PLUCINSKY P.P., SKILLMAN E.D., DALCANTON J.J., ANDERSON S.F., WEISZ D.R., KONG A.K.H. Astrophys. J., 758, 15 (2012) The Chandra Local Volume Survey: the X-ray point-source catalog of NGC 300. oTables 4-7, Col(ID): <CXOLV JHHMMSS.ss+DDMMSS.s> N=95 = Tables 4-7, Col(Seq): <[BWE2012] NGC 300 NN> (Nos 1-95). Ref:=2013ApJ...763..128B byBINDER B. , WILLIAMS B.F., ERACLEOUS M., GAETZ T.J., KONG A.K.H., SKILLMAN E.D., WEISZ D.R. Astrophys. J., 763, 128 (2013) The Chandra local volume survey: the X-ray point-source population of NGC 404. oTables 3-6, 10, 13, Col(ID): <CXOLV JHHMMSS.ss+DDMMSS.s> N=74 = Tables 3-6, 10, 13, Col(Seq): <[BWE2013] NGC 404 NN> (Nos 1-74). Ref:=2015AJ....150...94B byBINDER B. , WILLIAMS B.F., ERACLEOUS M., PLUCINSKY P.P., GAETZ T.J., ANDERSON S.F., SKILLMAN E.D., DALCANTON J.J., KONG A.K.H., WEISZ D.R. Astron. J., 150, 94 (2015) The Chandra Local Volume Survey. I. The X-ray point source populations of NGC 55, NGC 2403, and NGC 4214. oTable 5: <CXOLV JHHMMSS.ss+DDMMSS.s> N=967. Tables 8, 20 : <[BWE2015] NGC NNNN NNN> N=460.

University of Washington =E=Catalogue in electronic form as J/ApJ/758/15 =E=Catalogue in electronic form as J/ApJ/763/128 =E=Catalogue in electronic form as J/AJ/150/94 Originof the Acronym: A = Assigned by the author(s)

© Université de Strasbourg/CNRS

    • Contact