Prof. Şölen BALMAN OPfefricseo Pnhaol nIen:f +or9m0 2a1t2io 4n40 0000 Extension: 10668-7 OEmthaeirl: Esmolaenil.:b saolmleann.b@[email protected] AWdedbr:e hstst:p sP:r/o/fa. vDers.i sS.oislteann Bbual.medaun. tIrs/ta6n9b2u1l4 University Astronomy and Space Sciences Beyazit, 34119, Istanbul, Turkey EDodcutocraatteio, Unn iIvnefrosirtym oaf Wtioisnconsin-Madison, Colledge of Letters and Science, Physics, United States Of America 1992 - U19n9d7ergraduate, Bogazici University, Faculty Of Arts And Scıences, Department Of Physıcs, Turkey 1987 - 1991 FEnogrliesihg, nC1 L Aadnvagnucaedges CVoecrattiiofincaal tTersai,n Cinogu, Irnstreosd uacntidon T tor aSiPnAiCnEg SsYSTEMS ENGINEERING” course by Prof. Dr. S. Gabriel, School of OEnthgeinr,e Feirnineg A Srctsie (nMceins,o Ar)e,r Boospgaczeic iE Ungniinveersriitnyg, ,1 U9n8i7v. of Southampton, European Space Agency, 2006 Dissertations NDovctaoer, aUtne,i vXe-rRsaityy E omf iWssiisocno nfrsoinm-M Caladsisiocna,l FNeonv-aEed einb iOyuatb Fuarksüt:l tNesoiv, aF iCziykg, n1i9 199792 and Other ROSAT Detections of Galactic RNaetsueraalr Scchie nAcrese, aEsngineering and Technology Academic Titles / Tasks LAescstisutraenrt PPhrDof, eMssidodr,l eM Eidadstl eT Eecahstn Ticeacl hUnnicivael rUsnitiyv,e Frascituyl,t Fy aOcfu Altryt sO fA Anrdt sS cAienndc Secsi,e Dnecpesa,r Dtmepenart tOmf ePnhty Osfic Psh, 1y9si9c7s, -1 19999 - 2002 ABAcPa dSceiemntiicfi ca Cnodm mAidssmioinneirs, Mtriaddtilev eEa Estx Tpeechrnieicnalc Ueniversity, Faculty Of Arts And Sciences, Department Of Physics, B20Ö1L3Ü M- 2 B0A1Ş8KAN DANIŞMANI, Middle East Technical University, Faculty Of Arts And Sciences, Department Of Physics, F2a0k0ü9l t-e 2 K0u1r2ulu Üyesi, Middle East Technical University, Faculty Of Arts And Sciences, Department Of Physics, 2000 - 2003 AIr. ticTlhees UPLuXb lsiosuhrecde Xin-3 J oinu NrnGCa l4s2 T5h8a: ta Esenatrecrhe dfo rS CitIs, XS-SrCayI andd oApHticCaIl Ipnrdopeexretsies MAkOyNuTz HAL., YA NvdOaTnI CSE., SA OllaFk T SH.,E A RksOaYkAeLr NAS., TORrOalNhOanM II.C AA. L, BSaOlCmIaEnT YŞ,. vol.499, no.2, pp.2138-2147, 2020 (Journal Indexed II. Xin- rSaCyI) properties of dwarf nova EY Cyg and the companion star using an XMM-Newton observation ANDabViAzaNdCeEhS A IN., B SAPLAMCEA NR EŞS.EARCH, vol.66, no.5, pp.1139-1146, 2020 (Journal Indexed in SCI) III. ABAccLrMeAtiNo nŞ .flows in nonmagnetic white dwarf binaries as observed in X-rays IV. PArDeVfAaNceC:E NS oINv aS PeArCuEp tRiEoSnEsA, RcaCtHa, cvloyls.6m6i, cp pv.a1r0i9a7b-l1e1s2 a2n, 2d0 r2e0l a(tJoeudr snyasl tInedmesx:e Cd hina lSlCeIn)ges in the 2020 era ABDALVMANACNE ŞS. IN SPACE RESEARCH, vol.66, no.5, pp.1001-1003, 2020 (Journal Indexed in SCI) V. XDRisBks structure of cataclysmic variables and broadband noise characteristics in comparison with ABSATLRMOANNO ŞM.ISCHE NACHRICHTEN, vol.340, no.4, pp.296-301, 2019 (Journal Indexed in SCI) VI. OAvpdtiacna Sl .C, AoKuYnÜteZr Ap.,a Vritnso okfu rUoLvX As. , aAnKdS ATKhEeRir N H., oAsvtd aEnn vHi.r, Foanbmriekna tSs. , iVna NleGevC A 4.,4 A9k0k/ay4a4-8O5ralhan I., BALMAN Ş. VII. SAcSiTeRnOcPeH wYiStIhC AeL-A JOSUTRNOAGLA, Mvo Al.8 s7p5a, ncoe. 1m, 2is0s1io9 n( Jfoourr nMale IVn-dGeexVed g ianm SCmI)a-ray astrophysics ADreg Aan gAe.l, ies tA a.,l .Tatischeff V., Grenier I. A. , McEnery J., Mallamaci M., Tavani M., Oberlack U., Hanlon L., Walter R., VIII. AJO UloRnNgA sLe OrFe nHdIGipHit EoNuEsR XGMY MAS-NTReOwPtHonYS oICbSs, evrovl.a1t9i,o pnp .o1f- 1t0h6e, 2in0t1e8r m(Joeudriantael Ipnodelaxre dX iYn ASCrIi) MCaOmNuTrHdLaYn NDO. ZT. I,C BEAS LOMFA TNH EŞ. ,R BOuYrAwLit zA SVT.RONOMICAL SOCIETY, vol.477, no.3, pp.4035-4045, 2018 (Journal Indexed IX. Min oSdCiIf)ying the Standard Disk Model for the Ultraviolet Spectral Analysis of Disk-dominated CGaotdaocnl yPs.,m Siiocn V Ea. rMia. b, Bleaslm. Ia. nT Şh.,e B Nlaoirv Wal.i kPe.s MV Lyrae, BZ Camelopardalis, and V592 Cassiopeiae X. RASeTaRnOaPlyHsYisS IoCfA Lh iJgOhU-RrNesAoLl,u vtoiol.8n4 X6,M nMo.1-N, 2e0w1t7o (nJ oduartnaa lo Ifn Vde2x4e9d1 in C SyCgIn)i using models of collisionally ionized hBoAtL MabAsNo Şr.b, Gerasmsizkan C. XI. XA-SRTAROYN SOPMEYC T&R AASLT RAONPDH YOSPICTSI,C vAoLl.5 P9R8O, 2P0E1R7T (IJEoSu rOnFal AIn dUeLxXe dI Nin NSCGIC) 4258 (M106) ASvTdRanO PHH., YASvIdCaAnL SJ.O, AUKRYNÜAZL ,A v.,o Bl.8A2L8M, AnNo. 2Ş,. ,2 A0K1S6A (KJEoRur Nn.a, lO Irnadlhexaend I .i nA .SCI) XII. PBrAeL-MoAuNtb Şu.rst Chandra observations of the recurrent nova T Pyxidis XIII. SAWSTIRFOTN XO-MRYA Y& IALSLTERSOCPOHPYESI COSB, SvoElR.5V7A2,T 2I0O1N4S ( OJoFu rTnHalE I nNdOeVxeAd- LinI KSCEI )CATACLYSMIC VARIABLES MV Lyr, BZ Cam, AND V592 Cas ABSATLRMOAPNH YŞ.S, IGCoAdLo JnO PU.R, SNioAnL ,E v. oMl..794, no.1, 2014 (Journal Indexed in SCI) XIV. Av sdeaanr Hch., Afovdra pne Sr. iKo.d , iAcKitYieÜsZ fAr.o, BmA aL MUALNX Şin. the LINER galaxy NGC 4736 XV. XAMSTMRO-NPEHWYSTICOSN A ONBDS SEPRAVCEA TSCIOIENNSC EO,F v oLlU.3M52I,N nOoU.1S, pSpO.1U2R3C-1E2S8 ,I N20 N14E A(JRoBurYn aGlA InLdAeXxIeEdS i nN SGCCI) 4395, NGC 4736, AKNYDÜ ZN GA.C, K 4a2y5ac8i S., Avdan H., Ozel M. E. , Sonbas E., BALMAN Ş. XVI. XA-SrTaRyO vNaOrMiaICtiAoLn sJO iUnR tNhAeL i,n vnoel.1r 4a5c, cnroe.3ti,o 2n0 1fl3o (wJo oufr ndawl Ianrdfe nxeodv aine SCI) ABSATLRMOANNO ŞM.,Y R &ev AnSivTtRseOvP MHY.SICS, vol.546, 2012 (Journal Indexed in SCI) XVII. TBheaer domutobrue rAs.t P o. ,f ONsobovran Ce SJ.S P 0. ,8 P1a0g0e 7K:.0 L3. 0, H5a5k9a+la0 P5. 4J. 7, 1Sc5h w(HarVz CGe. Jt.i ), Rauch T., BALMAN Ş., Evans P. A. , Goad M. R. A, NSTesRsO JN. -O. M, eYt a&l. ASTROPHYSICS, vol.545, 2012 (Journal Indexed in SCI) XVIII. NOREWBITOANL- OPHBSAESREV-RAETSOORLYV EDDA TSAPECTROSCOPY OF THE INTERMEDIATE POLAR FO AQR USING XMM- APeSkToRnO NY.O, BMAICLAMLA JNO UŞ.RNAL, vol.144, no.2, 2012 (Journal Indexed in SCI) XIX. BXMOUMN-NDEAWRYT OLNAY OEBRSERVATIONS OF THE DWARF NOVA RU Peg IN QUIESCENCE: PROBE OF THE ABSATLRMOAPNH YŞ.S, IGCoAdLo JnO PU.R, SNioAnL ,E v. oMl..7 ,4 N1e, snso J.2., ,S 2c0h1le1g e(lJ oEu., rBnaarl rIentdt ePx. eEd. ,i nSz SkCoId)y P. XX. dOartbaital and spin phase-resolved spectroscopy of the intermediate polar EX Hya using XMM-Newton MPeOkNoTnH YL., YB NALOMTIACNES Ş O.F THE ROYAL ASTRONOMICAL SOCIETY, vol.411, no.2, pp.1177-1196, 2011 (Journal Indexed XXI. Finr SeCqIu)ency-resolved spectroscopy of XB1323-619 using XMM-Newton data: detection of a reflection rBeAgLiMonA Nin Ş .the disc iMn OSNCIT)HLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, vol.407, no.3, pp.1895-1902, 2010 (Journal Indexed XXII. ASo snebaarsc Eh., fAoKrY sÜuZp Ae.,r BnAoLvMa ArNem Ş.n, Oanzetls M in. E t.he nearby spiral galaxy M74 (NGC 628) XXIII. TAhSTeR XOMNMOM-NYe &w AtoSTnR dOePtHeYctSiIoCnS, ovof le.5x1t7e,n 2d0e1d0 e(Jmouisrsniaoln In fdreoxmed t hine S nCoI)va remnant of T Pyxidis MBAOLNMTAHNLY Ş .NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, vol.404, no.1, 2010 (Journal Indexed in SCI) XXIV. SBweairftd mobosre rAv. aPt. i,o Onssb oorfn CeS JS. P0.8 , 1P0ag0e7 K:0. 3L.0 , 5S5ch9w+a0r5z 4G7., 1S5tarrfield S., Hakala P., Ness J. -. , BALMAN Ş., Wagner R. M. XXV. AS STTRUODNYO MOIFS CTHHEE N LAOCWHR-IMCHATSESN X, -vRoAl.3Y3 B1,I NnoA.2R, Yp pD.1IP56 S-1O5U9R, C20E1S0 X (BJo 1u9rn1a6l -I0n5de3x, eXdB i n1 S3C2I3)-619, X 1624-490 ABANLDM 4AUN 1Ş.746-371 OBSERVED WITH INTEGRAL XXVI. TAhSTeR bOrNoOaMd-ICbAaLn dJO nUoRiNseA Lc,h vaorl.a1c3t8e, rniost.1ic, sp po.5f 0s-e6l2e,c 2t0e0d9 a (nJoumranlaol uInsd Xex-ready i np SuClsI)ars and soft gamma-ray rKeupleebai tBe.r, sBALMAN Ş. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, vol.395, no.4, pp.2356-2362, 2009 (Journal Indexed XXVII. Ainn S CoIp)tical search for supernova remnants in the nearby spiral galaxy NGC 2903 ASoSnTbRaOsN EO.,M AYK Y&Ü AZS AT.R, BOAPLHMYSAINCS Ş, .vol.493, no.3, pp.1061-1065, 2009 (Journal Indexed in SCI) XXVIII. NVaerwiatotino nasn din I NthTeE dGiRpA pLroperties of the low-mass X-ray binary XB 1254-690 observed with XMM- ATrSiTgRoO MN. ODM. ,Y P &ar AmSaTrR AO. PNH. Y, BSIoCirSi,n v oLl.,. 4M9o3t, cnho C.1.,, Tpapl.a1v4e5r-a1 5A7., ,B 2A0L0M9 A(JNo uŞr.nal Indexed in SCI) XXIX. RPeRk oPeicn (Y1., 9B2A5L)M: AAN C Şh.andra X-ray view SMCOI)NTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, vol.388, no.2, pp.921-926, 2008 (Journal Indexed in XXX. TGhelein ion Dcl.i, nBaAtLioMnA Nan Şg.,l Ke izainlodg lmu aUs., sY iolmf athz eA .b, Klaaclekm hcoi lEe., iTno mXTsiEck J 1J.118+480 XXXI. TAhSTeR dOePtHeYctSiIoCnA Lo JfO aU R3N.5A hLr, v poel.6ri4o2d, nion. 1t,h pep c.4l3a8ss-4ic4a2l, 2n0o0v6a (VJoeulornraulm In 1de9x9e9d (inV S3C8I2) Vel) and the long-term bBeAhLaMvAioNr Ş o., fR ethtte rN Ao.,v Bao lsi gMh.t curve XXXII. ASnT aRrOcNhOivMaIlC sAtLu dJOyU oRfN eAxLt, evnodl.1e3d1 X, n-roa.5y, pepm.2is6s2i8o-n2 6f3r3o,m 2 0c0la6s (sJiocuarln aanl Idn drexceudr rine nSCt In)ovae ABDalVmAaNnC ŞE.S IN SPACE RESEARCH, vol.38, no.12, pp.2840-2843, 2006 (Journal Indexed in SCI) XXXIII. XB-aryakya l oAu., tKbiuzirlosgt lou fU 4., UK i0zi1lo1g5lu+ N6.3, B4A aLnMdA RNO ŞT., SInEa mob Ss.ervations of its optical counterpart V635 Cas XXXIV. CAhSTaRnOdNraO MobY s&e rAvSaTtRioOnP HoYfS tIhCeS, svhoel.4ll3 o9f, nNoo.3v, ap pP.1e1rs3e1i- 11193041, 2 (0G0K5 (PJeorusrenia)l: I nDdeetxeecdti ionn S CoIf) localized nBoAnLMthAeNrm Ş.al X-ray emission from a miniature supernova remnant XXXV. DASisTcRoOvPeHrYyS oICfA iLrr JaOdUiRaNtiAoLn,- vinodl.6u2c7e,d n ov.a2r, ipapt.i9o3n3s- 9i5n2 t, h2e0 0li5g h(Jto cuurnravle I nodfe txheed cinla SsCsIi)cal nova V2275 Cyg (N Cyg 2B0al0m1a nN Şo.., Y2ı)lmaz A., Retter A., Saygac T., Esenoglu H. H. EMxopnatnhdlye dN)otices of the Royal Astronomical Society, vol.356, no.2, pp.773-777, 2005 (Journal Indexed in SCI XXXVI. DIbirsachoimve Ary., Moaf rak wtraarndst iCe.,n Stw manakg nJ.e, Rtaarn:s oXmTE S .J, 1R8o1b0er-t1s9 M7., Kaspi V., Woods P., Safi-Harb S., BALMAN Ş., Parke W., et AalS.TROPHYSICAL JOURNAL, vol.609, no.1, 2004 (Journal Indexed in SCI) XXXVII. sAu Cphearsnodfrta X l-orway e snoeurrgcye t raannds am visiosiloen tglyr avtainrgia sbplee clitgrhotm ceutrevre observation of V4743 Sagittarii: A ANSeTssR OJ.,P SHtaYrSrIfCieAlLd JSO., UBRuNrwAiLtz, vVo.,l .W59i4ch, nmoa.2n,n 2 R0.0, H3 a(uJosuchrnildalt IPn.,d Dexraekde i nJ. ,S WCIa)gner R., Bond H., Krautter J., Orio M., et al. XXXVIII. CYoHlAdaNsD AR., AB AdLeMteAcNti oŞ.n of 16 new X-ray sources XXXIX. TAhSTeR rOeN-aOnMaYly &s iAsS oTfR tOhPeH RYSOISCAS,T v odla.3t8a4 o, nf oN.1o, vpap .M19u0s- 119948, 230 u0s2i n(Jgo uwrhniatle I nddwexaerdf aint mSCoIs)phere emission models MBaolnmtahnly Ş N., oKtricaeust toefr tJh.e Royal Astronomical Society, vol.326, no.4, pp.1441-1447, 2001 (Journal Indexed in SCI) XL. TCahsea leemgnioss Rio., nO rnioe bMu.,l Ma aatshsiso cJ.i, aCtoends ewliicteh C V., 1G9al7la4g hCeyrg Jn., iB: AaL uMnAiqNu Şe., oDbeljleac Vt?alle M., Homeier N., Ogelman H. ASTRONOMY & ASTROPHYSICS, vol.361, no.2, pp.725-733, 2000 (Journal Indexed in SCI) XLI. dTehtee cfitriostn rse osfo hlvaerdd aXn-dra dye etemcitsesdio cnla fsrsoicma lc lnaosvsaic sahl enlol vina Xin- roauytsb iunr sctomparison with the ROSAT ABdalvmanance Şs. ,i nÖ gSeplamcaen R Hes.earch, vol.25, pp.363-368, 2000 (Journal Indexed in SCI) XLII. TBhAeL MfiArNst Şr.,e Osgoellvmeadn a Hn.d detected classical nova shell in X-rays: The shell of Nova Persei 1901 XLIII. TAhSTeR XO-PrHayY SsIpCAecLt JrOaUl ReNvoAlLu, tviooln.5 1o8f , cnloa.s2s, i1c9a9l 9N (oJovuar Vna1l9 I7nd4e Cxeydg nini S1C9I9)2: A reanalysis of the ROSAT data ABSATLRMOAPNH YŞ.S, IKCrAaLu tJtOeUr RJ.,N OAgLe,l mvoaln.4 9H9., no.1, pp.395-406, 1998 (Journal Indexed in SCI) XLIV. XO-rrioa yM e., mBAisLsMioAnN oŞf., NDeolvlaaV Palulep Mpi.,s G 1a9lla9g1h:e Ar cJ.c, rOegteilomna no rH a. shocked shell? XLV. RASOTSRAOTP HOYBSSIECRALV AJOTUIRONNA OLF, v TolH.4E6 6O, LnDo. 1C, LpAp.S4S1I0C-A41L4 N, 1O9V9A6 (CJPou PrUnaPlP InISdexed in SCI) ABSATLRMOAPNH YŞ.S, IOCRAILO JMOU., RONGAELM, vAoNl.4 H4.9, no.1, 1995 (Journal Indexed in SCI) Refereed Congress / Symposium Publications in Proceedings I. XSoIPffEit:t aT Ph.,e B Xe-llraazyzi nimi Ra.,g Binogzz poo El.a, Briumrwetitrzy V e.,x Cpalsotroe-rTirado A. J. , Costa E., Courvoisier T., Feng H., Gburek S., SGpoaocsem Taenlens Rco., peet sa la.nd Instrumentation 2016: Ultraviolet to Gamma Ray, Edinburgh, United Kingdom, 26 June - 01 II. TJuhlye 2L0O1F6T, v moli.9s9si0o5n concept - A status update eFte arol.ci M., Bozzo E., Brandt S., Hernanz M., van der Klis M., Liu L. -. , Orleanski P., Pohl M., Santangelo A., Schanne S., -C 0o1n fJeurleyn 2c0e1 o6n, vSopla.9c9e 0T5elescopes and Instrumentation - Ultraviolet to Gamma Ray, Edinburgh, Saint Helena, 26 June III. PBraolmbain gŞ .disk structure of dwarf novae and cataclysmic variables using broadband noise IV. PFrhoansteie Rr eRseoselvaercdh Xin-R Aasytr oSpheycstircasl, FARnAaPlyWsSis 2 o0f1 4In, Mteornmdedlloia, tPea lPeromlaor, sI tEalXy , H26y a- 3a1n dM aFyO 2 A0q14r CPoeknofenr eYn., cBeA oLnM PAhNy sŞi.cs at the Magnetospheric Boundary, Geneva, Switzerland, 25 - 28 June 2013, vol.64 V. TFehreo cLia Mrg., ed eOnb Hserrdveart oJ. rWy . F, oBro zxz-or aEy., BTairmreint gD., Brandt S., Hernanz M., van der Klis M., Pohl M., Santangelo A., Stella CLo., nefte arle.nce on Space Telescopes and Instrumentation - Ultraviolet to Gamma Ray, Montreal, Canada, 22 - 26 June VI. H20ig1h4 , Rvoels.9o1lu4t4ion XMM-Newton Data of Nova Outbursts using Warm & Hot Absorber Models 2B8A1LsMt ASyNm Şp.,o Pseiukmon o Yf .the International-Astronomical-Union, Padova, Italy, 4 - 08 July 2011, pp.124-125 VII. LFeOrFoTci -M t.h, dee Lna Hregred eOrb Js. eWr.v ,a Btozrzyo FEo., rB axr-reaty D T., iBmrianngdt S., Hernanz M., van der Klis M., Pohl M., Santangelo A., Stella CLo., nefte arle.nce on Space Telescopes and Instrumentation 2012 - Ultraviolet to Gamma Ray, Amsterdam, Netherlands, VIII. F1 r-e 0q6u Jeunlyc y2 0R1e2s, ovolvl.e8d4 4S3pectroscopy of XB 1323-619 and EXO 0748-676 BALMAN Ş. PInetresrpneacttiiovneasl, BConlofgenrean, Ictea loyn, 7 X - R1a1y S Aespttreomnboemry 2-2000099, v: oPlr.1es2e4n8t, Sptpa.t1u3s5, M-1u3l6ti-Wavelength Approach and Future IX. OPerkboitna Yl .P, BhAaLsMe ARNe sŞo.lved Spectroscopy of EX Hya Using XMM-NEWTON PInetresrpneacttiiovneasl, BConlofgenrean, Ictea loyn, 7 X - R1a1y S Aespttreomnboemry 2-2000099, v: oPlr.1es2e4n8t, Sptpa.t1u3s7, M-1u3l8ti-Wavelength Approach and Future X. VTrairgioa Mtio. Dn.s , iPna rtmhea rd Aip., Bporioripne Lr.t, iMeso tochf XC.B, T 1a2la5v4er-a6 9A .,o Bbaslemravne Şd. with XMM-newton and INTEGRAL XI. A7t hs tMudicyro oqfu saesaler cWteodr klsohwo-pm: Masicsr oXq-ruaaysa brsin aanrdy B deiypo nsod,u MrcQeWs o20b0s8e,r Fvoecda ,w Izimthi rI, NTTurEkGeRy,A 1L - 05 September 2008 4B0a lYmeaanr sŞ .Of Pulsars: Millisecond Pulsars, Magnetars and More, Montreal, Canada, 12 - 17 August 2007, vol.983, XII. Tpph.e5 3b0r-o5a3d2-band noise characteristics of selected AXPs and SGRs: Probing the magnetar coronae 4K0ü lYeebai rBs. , OBfa Plmulasna rŞs.: Millisecond Pulsars, Magnetars and More, Montreal, Canada, 12 - 17 August 2007, vol.983, XIII. Tpph.e2 8in3-c2li8n5ation angle and mass of the black hole in XTE J1118+480 CGoenlinfeor eDn. cMe . o, nB ANLaMtuAreN aŞn.,d K Eizviloolgultuio Un. ,o Yfi lXm-Raaz yA B., iKnaalreimesc in E D., Tivoemrsseic Ekn Jv. iAr.onments, Florida, United States Of America, XIV. A28n Oocptotibcearl -s 0e2a rNcohv efomrb Seru p20e0rn7,o vvoal. 1R0e1m0,n papn.8ts2 -i8n3 NGC 3184 and NGC 2903 6Sothn bInatse rEn., aAtiKoYnÜaZl C Ao.,n BfeArLeMncAeN o Şf .t, hCee kBmalekcaenl-ioPghlyus iEc.al-Union, İstanbul, Turkey, 22 - 26 August 2006, vol.899, pp.135- XV. T13im6e-averaged broad-band spectra of the dipping low-mass X-ray binaries observed with INTEGRAL 6Btahlm Inatne gŞr.,a Pl aWrmorakrs Aho., pS i-d Tohli eL O., bPsacizuirse Ad. , UDniaivze Trsreig, oM Mos.,c Ooows,t Rerubsrsoiae, k2 T -. 08 July 2006, pp.417-420 XVI. sAt rsutuctduyr eo fb teetmwpeoenra 2l -c2h0a rkaecyteristics of selected cataclysmic variables : The broad-band noise XB-arlamya Unn Şiv., eKrüslee b2i0 B0.5, ,B Mekalderni dE, .Spain, 26 - 30 September 2005, vol.1, pp.237-238 XVII. OAKpYtiÜcZa lA s.,e Baarlcmha nfo Şr., sBuhpaettranchoavray ar eDm., Snoannbtass i nE. ,t Cweok-msepcierlaiol gglaul Ea.xies XVIII. AX- rsatyu dUyn iovef rtseem 2e0p0o5,r Mala cdhriadr, aScptaeinr,i s2t6ic -s 3 o0f S seepltecmtbeedr C2a0t0a5c,l vyoslm.1i, cp pV.a4r4i1a-b4l4e2s: The broad-band noise sBtArLuMctAuNr eŞ .b, Keutwleebei Bn. ,2 B-e2k0le kne Ev. XIX. DSyimscpoovseiurmy ofn ltohcea Xli-zraeyd Unnoivne-rtshee 2rm00a5l, XE-l rEasyco ermiali,s Sspioainn ,f 2r6o m- 3 t0h See nptoevmab reer m20n0a5n, tv olf. 6G0K4 , Ppepr.2s3e7i -(2139801) CBoAnLfMerAeNn cŞe. on Astrophysics of Cataclysmic Variables and Related Objects, Strasbourg, France, 11 - 16 July 2004, XX. CvoClD.3 3p0h, optpo.4m3e3t-4ry3 4of V2275 Cygni (N Cyg 2001 No.2) in 2002-2003 CBoAnLfMerAeNn cŞe., oYnIL AMsAtrZo pAh., yRseictste orf A C.,a Stacylgyascm Tic., VEaSrEiNabOlGeLs Ua nHd. HRe.lated Objects, Strasbourg, France, 11 - 16 July 2004, XXI. Tvohle.3 3d0is, cpopv.4e3r1y- 4o3f2 a Transient magnetar aIbl.rahim A., Markwardt C., Swank J., Ransom S., Roberts M., Kaspi V., Woods P., Safi-Harb S., BALMAN Ş., Parke W., et pCpo.n2f9e4re-2n9c7e on X-Ray Timing 2003 - Rossi and Beyond, Cambridge, Canada, 3 - 05 November 2003, vol.714, XXII. cTahned CidHaAteNDRA data of the classical nova RR Pic (1925): A possible magnetic cataclysmic variable IBAAUL CMoAllNo qŞu., iKumup 1cu9-0Y oWldoarsk sAh.op on Magnetic Cataclysmic Variables, Cape-Town, South Africa, 8 - 13 December XXIII. O20n0 t2h, ev opl.o3s1s5i,b pipli.t1y7 2o-f1 d73etecting remnants of novae in the X-rays and recovering the remains of an eBxApLlMoAsiNo nŞ. after a century XXIV. TInhter CnaHtAioNnaDl RCAon ofebrseenrcvea otnio Cnl aosfs itchale N foirvsat Erxepsloslvioends ,a SnITdG dEeSt, eScptaeind, 2cl0a -s s2i4c aMl anyo 2v0a0 2sh, veoll. 6in3 7X, -prpa.3y6s:5 -T3h7e1 shell oBfA LNMoAvaN PŞ.ersei 1901 (GK Per) XXV. AX-pRpalyi cAasttiroonn oomf yth 2e0 0h0o tC ownhfeitree ndcwe,a MrfO NatDmEoLsLpOh, Ietarley ,m 4 o- d0e9l sS etpot etmheb eXr- 2ra0y0 0d, avtoal. 2o3f4 c, lpaps.s2i6c9a-l2 n7o4vae CBoAnLfMerAeNn cŞe. of the NATO-Advanced-Study-Institute on Variable Stars as Essential Astrophysical Tools, CESME, XXVI. Tuhrek erye,a 3n1a Alyusgius sot f- 1th0e S eRpOteSmATbe dr a1t9a9 o8f, vcolal.5s4si4c, aplp n.7o7v3a-7 V812974 Cygni 1992 WBAilLdM SAtaNr sŞ i.,n O tgheel mOladn W He., sKt r-a 1u3tttehr N J.orth American Workshop on Cataclysmic Variables and Related Objects, XXVII. TWhyeo mROinSgA, UTn oitbeds eSrtavtaetsi oOnf sA mofe rcilcaas, s1i4c a- l1 n9o Juvnae 1997, vol.137, pp.400-405 1O5ri8ot hM C., oOllgoeqlmuiaunm H o.,f BthAeL MInAteNr nŞa.tional-Astronomical-Union on Cataclysmic Variables and Related Objects, KEELE, XXVIII. RENOGSLAATN oDb, s2e6r -v 3a0ti oJunn eo f1 9th9e5 , ovlodl. 2c0la8s, spipc.a2l8 9nova CP PUPPIS CBoAnLfMerAeNn cŞe., oOnr iCoa Mta.,c Olygsemlmic aVna Hri.ables, ABANO TERME, Italy, 20 - 24 June 1994, vol.205, pp.469 Citations hT-ointadl eCxi t(aWtioOnSs) :(1W3OS):856 Noonn-p Arocfait dOergmanicis aEtixopn,e Eruireonpceean Space Agency, RSSD (Research and Science Division)