Prof.Dr. Şölen BALMAN İKşi şTiesleflo Bniul:g +il9e0r 212 440 0000 Dahili: 10668-7 DE-ipğeors tEa-:p soosletna.:b saolmleann.b@[email protected] PWoesbta: hAtdtprse:/s/i:a vPersoifs. .iDstra. nSbouleln.e dBua.ltmr/a6n9 I2s1ta4nbul University Astronomy and Space Sciences Beyazit, 34119, Istanbul, Turkey EBüğtiütnimleş iBk iDlgokilteorai, University of Wisconsin-Madison, Colledge of Letters and Science, Physics, Amerika Birleşik LDiesvalnest,l eBroi ğ1a9z9iç2i -Ü 1n9iv9e7rsitesi, Fen-Edebiyat Fakültesi, Fizik Bölümü, Türkiye 1987 - 1991 Yİnagbiliazcnec, Cı 1D İilellreir SMeerslteikfi kEğai,t iKmu, Irnstr ovdeu cEtiğoint itmo SlPeArCE SYSTEMS ENGINEERING” course by Prof. Dr. S. Gabriel, School of Engineering DSciğieenrc, eFsin, Ae eArrotssp (aMcein Eonrg),i nBeoegrainzigc,i UUnniivv. eorfs Sitoyu, 1th9a8m7pton, European Space Agency, 2006 Yaptığı Tezler GBaültaücntilce şNiko vDaoek, tUonraiv, eXr-sRiatyy oEfm Wisisicoonn sfrino-mM aCdlaisosinc,a Fl eNno-vEadee ibni yOaut tFbaukrüsltt:e Nsio, vFaiz Ciky, g1n9i 917992 and Other ROSAT Detections of ATermaeşlt Bırilmimale rA, Mlaünhleanrdıislik ve Teknoloji Akademik Unvanlar / Görevler ÖYrğdre.Dtiomç .DGör.r, eOvrltiasi DDorğ., uO Trteak Dniokğ Üun Tiveekrnsiikt eÜsni, iFverns-iEtedseib, Fiyeant -FEadkeüblityeasti , FFaizkiükl tBeösliü, Fmizüik, 1 B9ö9l9ü m- 2ü0, 109297 - 1999 ABAkPa Bdielimsiekl Kİodmairsiy oDne Ünyeeysii, mOrta Doğu Teknik Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, 2013 - 2018 FBaÖkLüÜltMe KBuArŞuKluA NÜ yDeAsiN, OIŞrMtaA DNoI,ğ Our Ttae kDnoiğku Ü Tneivkenriski tÜensii,v Feernsi-tEedsie, bFieyna-tE Fdaekbüiyltaets iF, aFkizüiklt eBsöi,l üFmiziük, B2ö0l0ü0m -ü 2, 020309 - 2012 SCI. I, STShCe IU vLeX AsoHuCrcIe İ nX-d3e ikns NleGrCi n4e2 5G8i:r ae nse Darecrhg ifloerr idtse XY-raayyı nalnadn oapnt iMcaal kparolepleerrties MAkOyNuTz HAL., YA NvdOaTnI CSE., SA OllaFk T SH.,E A RksOaYkAeLr NAS., TORrOalNhOanM II.C AA. L, BSaOlCmIaEnT YŞ,. cilt.499, sa.2, ss.2138-2147, 2020 (SCI İndekslerine II. XG-irreany Dperrogpi)erties of dwarf nova EY Cyg and the companion star using an XMM-Newton observation ANDabViAzaNdCeEhS A IN., B SAPLAMCEA NR EŞS.EARCH, cilt.66, sa.5, ss.1139-1146, 2020 (SCI İndekslerine Giren Dergi) III. ABAccLrMeAtiNo nŞ .flows in nonmagnetic white dwarf binaries as observed in X-rays IV. PArDeVfAaNceC:E NS oINv aS PeArCuEp tRiEoSnEsA, RcaCtHa, ccliylts.6m6i, cs sv.1a0r9ia7b-1le1s2 2a,n 2d0 2r0e l(aStCeId İ nsdyesktselmersin: eC Ghiarlelne nDgeersg ii)n the 2020 era ABDALVMANACNE ŞS. IN SPACE RESEARCH, cilt.66, sa.5, ss.1001-1003, 2020 (SCI İndekslerine Giren Dergi) V. XDRisBks structure of cataclysmic variables and broadband noise characteristics in comparison with ABSATLRMOANNO ŞM.ISCHE NACHRICHTEN, cilt.340, sa.4, ss.296-301, 2019 (SCI İndekslerine Giren Dergi) 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, Mcil tA.8 7sp5,a scae.1 m, 2i0ss1i9o (nS CfoI rİn MdeekVs-leGreinVe gGairmenm Da-erragyi) 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, ecrilvt.a1t9i,o sns. 1o-f1 0th6e, 2 i0n1te8r (mSCeId İinadtek psloelrainre X GYir Aenr iDergi) MCaOmNuTrHdLaYn NDO. ZT. I,C BEAS LOMFA TNH EŞ. ,R BOuYrAwLit zA SVT.RONOMICAL SOCIETY, cilt.477, sa.3, ss.4035-4045, 2018 (SCI İndekslerine IX. MGioredni fDyeinrgi )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 ctilito.8n4 6X,M saM.1-,N 2e0w17to (nS CdI aİntad eokfs lVe2ri4n9e 1G iCreyng nDie urgsii)ng models of collisionally ionized hBoAtL MabAsNo Şr.b, Gerasmsizkan C. XI. XA-SRTAROYN SOPMEYC T&R AASLT RAONPDH YOSPICTSI,C cAilLt.5 P9R8,O 2P0E1R7T (ISECSI İOnFde Aks UleLriXn eI NG iNreGnC D 4er2g5i)8 (M106) ASvTdRanO PHH., YASvIdCaAnL SJ.O, AUKRYNÜAZL ,A c.i, lBt.8A2L8M, AsaN.2 Ş, .2, A01K6S A(KSCEIR İ nNd., eOkrsalelhrainne I G. Air.en Dergi) XII. PBrAeL-MoAuNtb Şu.rst Chandra observations of the recurrent nova T Pyxidis XIII. SAWSTIRFOTN XO-MRYA Y& IALSLTERSOCPOHPYESI COSB, SciEltR.5V7A2,T 2I0O1N4S ( SOCFI İTnHdEek NslOerVinAe- LGIirKeEn CDAerTgAi)CLYSMIC VARIABLES MV Lyr, BZ CBaAmLM, AN DŞ. , VG5o9d2on C Pa.s, Sion E. M. ASTROPHYSICAL JOURNAL, cilt.794, sa.1, 2014 (SCI İndekslerine Giren Dergi) 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 c iLlt.U3M52I,N sOa.U1,S s sS.1O2U3R-1C2E8S, 2IN01 N4 E(ASCRIB İnYd GekAsLleArXinIeE GS irNeGnC D 4er3g9i)5, 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 cnilte.1r4 a5c, csrae.3t,i o20n1 f3lo (wSC oI İfn ddwekasrlef rninoev Gaieren Dergi) ABSATLRMOANNO ŞM.,Y R &ev AnSivTtRseOvP MHY.SICS, cilt.546, 2012 (SCI İndekslerine Giren Dergi) 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, cilt.545, 2012 (SCI İndekslerine Giren Dergi) XVIII. NOREWBITOANL- OPHBSAESREV-RAETSOORLYV EDDA TSAPECTROSCOPY OF THE INTERMEDIATE POLAR FO AQR USING XMM- APeSkToRnO NY.O, BMAICLAMLA JNO UŞ.RNAL, cilt.144, sa.2, 2012 (SCI İndekslerine Giren Dergi) 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 c. iMlt.7. ,4 N1e, ssa .J2.,, S2c0h1l1eg (eSlC EI. ,İ Bndarerkestlte rPi.n Ee. G, Sirzekno dDye Prg.i) 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, cilt.411, sa.2, ss.1177-1196, 2011 (SCI İndekslerine XXI. FGrireeqnu Deenrcgyi)-resolved spectroscopy of XB1323-619 using XMM-Newton data: detection of a reflection rBeAgLiMonA Nin Ş .the disc GMiOreNnT DHeLrYg iN)OTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.407, sa.3, ss.1895-1902, 2010 (SCI İndekslerine 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, ocifl te.5x1t7e,n 2d0e1d0 e(SmCiIs İsnidoenk sflreormine t hGeir enno Dvaer rgei)mnant of T Pyxidis MBAOLNMTAHNLY Ş .NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.404, sa.1, 2010 (SCI İndekslerine Giren Dergi) 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, -cRilAt.3Y3 B1,I sNaA.2R, sYs .D15IP6 -S1O59U, R2C0E10S (XSBC I1 İ9nd1e6k-s0le5r3in, eX BGi r1e3n2 D3e-r6g1i)9, X 1624-490 ABANLDM 4AUN 1Ş.746-371 OBSERVED WITH INTEGRAL XXVI. TAhSTeR bOrNoOaMd-ICbAaLn dJO nUoRiNseA Lc,h cailrt.a1c3t8e, rsias.1ti,c sss .o50f -s6e2l,e 2c0te0d9 (aSnCoI mİnadleokussle rXi-nrea Gyi rpeunl sDaerrsg ia)nd soft gamma-ray rKeupleebai tBe.r, sBALMAN Ş. GMiOreNnT DHeLrYg iN)OTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.395, sa.4, ss.2356-2362, 2009 (SCI İndekslerine XXVII. An optical search for supernova remnants in the nearby spiral galaxy NGC 2903 ASoSnTbRaOsN EO.,M AYK Y&Ü AZS AT.R, BOAPLHMYSAINCS Ş, .cilt.493, sa.3, ss.1061-1065, 2009 (SCI İndekslerine Giren Dergi) 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 c iLlt..,4 M9o3t, csha .C1,. , sTsa.1la4v5e-r1a5 A7,. , 2B0A0L9M (ASCNI Şİn.dekslerine Giren Dergi) XXIX. RPeRk oPeicn (Y1., 9B2A5L)M: AAN C Şh.andra X-ray view GMiOreNnT DHeLrYg iN)OTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.388, sa.2, ss.921-926, 2008 (SCI İndekslerine 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, c pilte.6r4io2d, s ian.1 t, hsse. 4c3la8s-4s4ic2a, l2 n00o6v a( SVCeI lİonrduekms le1r9in9e9 G (iVre3n8 D2e Vrgeil)) and the long-term bBeAhLaMvAioNr Ş o., fR ethtte rN Ao.,v Bao lsi gMh.t curve XXXII. ASnT aRrOcNhOivMaIlC sAtLu dJOyU oRfN eAxLt, ecniltd.1e3d1 X, s-ar.a5y, s es.m26is2s8i-o2n6 3f3ro, 2m0 0c6la (sSsCiIc aİnl daenkdsl erreincue rGrierennt Dneorvgai)e ABDalVmAaNnC ŞE.S IN SPACE RESEARCH, cilt.38, sa.12, ss.2840-2843, 2006 (SCI İndekslerine Giren Dergi) 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, schilte.4ll3 o9,f sNa.o3v, sas .P1e1r3s1e-1i 113940, 12 0(0G5K ( SPCeIr İsnedie)k: sDleertineec tGioirne no Df elorgcia)lized nBoAnLMthAeNrm Ş.al X-ray emission from a miniature supernova remnant XXXV. DASisTcRoOvPeHrYyS oICfA iLrr JaOdUiRaNtiAoLn,- ciniltd.6u2c7e, ds av.2a,r sisa.9ti3o3n-s9 5in2, t2h0e0 5li g(ShCt Ic İunrdveeks olefr itnhee G cilraesns Dicearlg ni)ova V2275 Cyg (N Cyg 2B0al0m1a nN Şo.., Y2ı)lmaz A., Retter A., Saygac T., Esenoglu H. H. GMiorennth Dlye rNgoi)tices of the Royal Astronomical Society, cilt.356, sa.2, ss.773-777, 2005 (SCI Expanded İndekslerine 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, cilt.609, sa.1, 2004 (SCI İndekslerine Giren Dergi) 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, cVil.t, .5W9i4c,h sma.a2n, n2 0R0.,3 H (aSuCsIc hİnilddet kPs.l, eDrrinaek eG Jir., eWn aDgenregri )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 c idlt.a3t8a4 o, sfa N.1o, svsa.1 M90u-s1 9149, 82300 u2s (inSCgI wİnhdietkes dlewrianref G airtemno Dseprhgei)re emission models MBaolnmtahnly Ş N., oKtricaeust toefr tJh.e Royal Astronomical Society, cilt.326, sa.4, ss.1441-1447, 2001 (SCI İndekslerine Giren XL. TDhereg ei)mission nebula associated with V1974 Cygni: a unique object? ACaSsTaRleOgNnOoM RY., O&r AioS TMR.,O MPaHtYhSisI CJ.S, ,C coilnt.s3e6li1c,e s Ca.,2 G, sasll.a7g2h5e-7r 3J.3, B, 2A0L0M0A (NSC ŞI. ,İ Dndeellkas Vlearlilne eM G.,i rHeonm Deeierrg iN)., Ogelman H. 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, cilt.25, ss.363-368, 2000 (SCI İndekslerine Giren Dergi) 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, tciioltn.5 1o8f, cslaa.2s,s 1ic9a9l9 N (oSCvIa İ nVd1e9k7sl4e rCinyeg Gniir 1en9 9D2e:r gAi) reanalysis of the ROSAT data ABSATLRMOAPNH YŞ.S, IKCrAaLu tJtOeUr RJ.,N OAgLe,l mcilat.n4 9H9., sa.1, ss.395-406, 1998 (SCI İndekslerine Giren Dergi) 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, c iTltH.4E6 6O, LsaD.1 C, sLsA.4S1S0I-C4A14L, N19O9V6A ( SCCPI İPnUdPekPsIlSerine Giren Dergi) ABSATLRMOAPNH YŞ.S, IOCRAILO JMOU., RONGAELM, cAiltN.4 H49., sa.1, 1995 (SCI İndekslerine Giren Dergi) HIa. keXmIPlEi :K Tohne gXr-era /y Simemagpinogz pyoulmar iBmieltdriyr ei xKpiltoarpelrarında Yer Alan Yayınlar GSoofofistmtaa Pn.n, B Re.l, leatz zailn.i R., Bozzo E., Burwitz V., Castro-Tirado A. J. , Costa E., Courvoisier T., Feng H., Gburek S., TSpemacme uTze l2e0sc1o6p, ecisl ta.9n9d0 I5nstrumentation 2016: Ultraviolet to Gamma Ray, Edinburgh, İngiltere, 26 Haziran - 01 II. TFehreo cLiO MF.,T B mozizsos iEo.,n B croanndcte Sp.,t H- eArn satnazt uMs. , uvpand adteer Klis M., Liu L. -. , Orleanski P., Pohl M., Santangelo A., Schanne S., Ceto anlf.erence on Space Telescopes and Instrumentation - Ultraviolet to Gamma Ray, Edinburgh, Saint Helena, 26 III. PHraozibrainng - d01is Tke smtrmuuczt u2r0e1 6o, fc idltw.9a9r0f5 novae and cataclysmic variables using broadband noise FBraolmntaienr Ş R.esearch in Astrophysics, FRAPWS 2014, Mondello, Palermo, İtalya, 26 - 31 Mayıs 2014 IV. Pehkaosne YR.,e BsAoLlvMeAdN X Ş-.Ray Spectral Analysis of Intermediate Polars EX Hya and FO Aqr V. TCohnef eLraerngce oOnb sPehryvsiactso arty t hFeo Mr axg-nreatyo sTpihmeirnicg Boundary, Geneva, İsviçre, 25 - 28 Haziran 2013, cilt.64 LF.e, reot cail .M., den Herder J. W. , Bozzo E., Barret D., Brandt S., Hernanz M., van der Klis M., Pohl M., Santangelo A., Stella HCoanzifrearne n2c0e1 o4n, c Silpt.a9c1e4 T4elescopes and Instrumentation - Ultraviolet to Gamma Ray, Montreal, Kanada, 22 - 26 VI. HBAigLhM RAeNs Şo.,l uPteikoonn XYM.M-Newton Data of Nova Outbursts using Warm & Hot Absorber Models VII. L28O1FsTt S-y tmhpeo Lsaiurmge o fO tbhsee Irnvteartnoartyio Fnoalr-A xs-trraoyn oTmimicainl-gUnion, Padova, İtalya, 4 - 08 Temmuz 2011, ss.124-125 LF.e, reot cail .M., den Herder J. W. , Bozzo E., Barret D., Brandt S., Hernanz M., van der Klis M., Pohl M., Santangelo A., Stella 0C6o nTfemremncuez o2n0 1S2p,a ccielt .T8e4l4e3scopes and Instrumentation 2012 - Ultraviolet to Gamma Ray, Amsterdam, Hollanda, 1 - VIII. FBrAeLqMuAeNn cŞy. Resolved Spectroscopy of XB 1323-619 and EXO 0748-676 International Conference on X-Ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future IX. OPerrbsiptaecl tPivheas,s Beo Rloegsnoal,v İetadly Sap, 7e c- t1r1o sEcyolüpl y2 0o0f 9E, Xci lHt.1y2a4 U8,s sins.g1 3X5M-1M36-NEWTON IPnetkeorna Yti.,o BnAalL CMoAnNfe Şre.nce on X-Ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future X. VPearrsipaeticotinvess i, nB othloeg ndaip, İ tparlyoap, 7e r-t 1ie1s E oyflü Xl B20 10295, c4il-t6.192 4o8b, sses.r1v3e7d-1 w38ith XMM-newton and INTEGRAL 7Ttrhig Mo iMcr. oDq. u, aPsaarrm Waro Ark.,s Bhooipr:i nM Lic.,r Moqoutcahs aCr.,s T aanladv Beeray oAn.,d B, aMlmQWan 2Ş0.08, Foca, Izmir, Türkiye, 1 - 05 Eylül 2008 XI. ABa slmtuadny Ş o.f selected low-mass X-ray binary dip sources observed with INTEGRAL s4s0.5 Y3e0a-r5s3 O2f Pulsars: Millisecond Pulsars, Magnetars and More, Montreal, Kanada, 12 - 17 Ağustos 2007, cilt.983, XII. TKhülee bbir Bo.,a Bda-lbmaannd Ş n.oise characteristics of selected AXPs and SGRs: Probing the magnetar coronae s4s0.2 Y8e3a-r2s8 O5f Pulsars: Millisecond Pulsars, Magnetars and More, Montreal, Kanada, 12 - 17 Ağustos 2007, cilt.983, XIII. TGhelein ion Dcl.i Mna. t, iBoAnL aMnAgNle Ş .a, nKdiz imlogalsus U o.,f Y tihlmea bz lAa.c, kK ahleomlec ii nE. ,X TToEm Js1ic1k1 J.8 A+.480 DCoenvlfetrlenric, e2 8o nE kNiamtu -r 0e2 a Knda sEımvo 2lu0t0io7n, coilft .X1-0R1a0y, Bssin.8a2r-i8es3 in Diverse Environments, Florida, Amerika Birleşik XIV. ASonn obapst iEc.a, Al KseYaÜrZc Ah. ,f BoAr LSMuApNer Şn.,o Cveak mReecmelnioagnluts E i.n NGC 3184 and NGC 2903 163th6 International Conference of the Balkan-Physical-Union, İstanbul, Türkiye, 22 - 26 Ağustos 2006, cilt.899, ss.135- XV. TBiamlmea-na vŞe., rPaagremda rb Aro., aSdid-oblai Ln.d, P sapizeisc tAr.a, D oiaf zt hTrei gdoi pMp.,i nOgo sltoewrb-rmoeaks sT .X-ray binaries observed with INTEGRAL XVI. A6t hs tIundteyg roafl tWemorpkoshroapl c- hTahrea Ocbtescruisrteidc sU onifv seersle,c Mteods ccoawta, cRluyssyma,i c2 v- a0r8i aTbemlems u: zT 2h0e0 b6,r sosa.4d1-7b-a4n2d0 noise sBtarlumcatnu rŞe., Kbüeltewbie Be.n, B 2e-k2le0n kEe.y XVII. OX-prtaiyc aUln siveearrsceh 2 0fo0r5 ,s Muapderrind,o İvspaa rneyma, n2a6n -t 3s 0i nE ytlwülo 2-s0p0i5r, acli ltg.1a,l assx.2ie3s7-238 XA-KrYayÜ ZU nAi.v, eBraslem 2a0n0 Ş5.,, BMhaadttraidch, İasrpyaan Dya., , S2o6n -b 3as0 EE.y, Clüelk 2m0e0c5e,l icoilgt.l1u, Ess..441-442 XVIII. sAt rsutuctduyr eo fb teetmweepeonr 2a-l2 c0h akreavcteristics of selected Cataclysmic Variables: The broad-band noise SByAmLpMoAsNiu mŞ., oKnu ltehbei XB-.r, aBye kUlneniv eEr.se 2005, El Escorial, İspanya, 26 - 30 Eylül 2005, cilt.604, ss.237-238 XIX. DBAisLcMoAveNr Şy. of localized non-thermal X-ray emission from the nova remnant of GK Persei (1901) 2C0o0n4fe, rceilnt.c3e3 o0n, s As.s4t3ro3p-4h3y4sics of Cataclysmic Variables and Related Objects, Strasbourg, Fransa, 11 - 16 Temmuz XX. CBCADLM pAhNo tŞo., mYIeLtMryA Zo fA .V, R2e2t7te5r CAy., gSnayi g(aNc TC.y, EgS 2E0N0O1G LNUo H.2. )H .in 2002-2003 2C0o0n4fe, rceilnt.c3e3 o0n, s As.s4t3ro1p-4h3y2sics of Cataclysmic Variables and Related Objects, Strasbourg, Fransa, 11 - 16 Temmuz XXI. TIbhrea hdimis cAo.,v Mearryk owfa rad Tt rCa., nSswiaennkt Jm., Raganseotmar S., Roberts M., Kaspi V., Woods P., Safi-Harb S., BALMAN Ş., Parke W., et Calo.nference on X-Ray Timing 2003 - Rossi and Beyond, Cambridge, Kanada, 3 - 05 Kasım 2003, cilt.714, ss.294-297 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, Güney Afrika, 8 - 13 Aralık 2002, XXIII. Ocinlt. 3th15e, psso.1s7si2b-1il7it3y of detecting 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, eİscptaendy cal, a2s0s -i c2a4l Mnoayvıas 2sh00e2ll, icnil tX.6-3r7a,y sss:.3 T6h5e-3 s7h1ell oBfA LNMoAvaN PŞ.ersei 1901 (GK Per) XXV. AX-pRpalyi cAasttiroonn oomf yth 2e0 0h0o tC ownhfeitree ndcwe,a MrfO NatDmEoLsLpOh, İetarley am, 4o d- e0l9s Etyol ütlh 2e0 X00-r, aciylt .d2a3t4a, sosf.2 c6l9a-s2s7i4cal novae CBoAnLfMerAeNn cŞe. of the NATO-Advanced-Study-Institute on Variable Stars as Essential Astrophysical Tools, CESME, XXVI. Tührek iryeea, n31a lAyğsuiss toofs t-h 1e0 REOylSüAl 1T9 d9a8t, aci lot.f5 4c4la, sss.i7c7a3l -n7o8v2a V1974 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, ATm oebrsikear Bvairtlieoşniks D oefv lceltalesrsii, c1a4l -n 1o9v aHeaziran 1997, cilt.137, ss.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 oHnaz oirfa nth 1e9 o95ld, ccillta.2s0s8ic, assl .2n8o9va CP PUPPIS CBoAnLfMerAeNn cŞe., oOnr iCoa Mta.,c Olygsemlmic aVna Hri.ables, ABANO TERME, İtalya, 20 - 24 Haziran 1994, cilt.205, ss.469 Atıflar hT-oinpdlaemks Ai t(ıWf SOaSy)ıs:1ı 3(WOS):856 ASivkial Tdoepmlumi D Kıuşrıu Dluşeun, eEuyriompean Space Agency, RSSD (Research and Science Division)