Hakkı Boran Ögelman

Hakkı Boran Ögelman

Ögelman in front of the Cukurova University (CÜ) Solar House construction in 1981.

Hakkı Boran Ögelman (July 8, 1940 – September 4, 2011) was a Turkish physicist and astrophysicist. He was an expert on gamma ray astronomy, the physics of neutron stars, and solar energy and worked on several key topics in modern astrophysics. He made many contributions to high energy astrophysics. In his early professional career he engaged in the SAS-II Small Gamma Ray Astronomy Satellite experiment development, data analysis, and first detection and imaging of our universe in gamma rays with his NASA colleagues, as well as in other fields of physics. His main interests in the field of astrophysics were the study of gamma ray astronomy and compact objects such as neutron stars and pulsars. Ögelman worked at NASA Goddard Space Flight Center, Middle East Technical University (METU) in Ankara, Turkey, Cukurova University in Adana, Turkey, Max Planck Institute (MPI) at Garching, Germany and the University of Wisconsin.

First years

Hakkı Ögelman was born in Ankara, Turkey, on July 8, 1940. His father was Salehettin Ögelman, a lawyer, and his mother Vedya Özlem Ögelman, a schoolteacher.[1]

Education

Hakkı Ögelman attended English-language Robert College in Istanbul, receiving his baccalaureate in 1957, then went to the U.S. to further his education. He received his B.A. in physics from DePauw University in June 1960 and his M.Sc. and Ph.D. from Cornell University in 1963 and 1966, respectively. [2] He married a DePauw classmate, Ivy White.[3]

Early career

After his 1966 graduation from Cornell, Ögelman did one year of postdoctoral research at the University of Sydney, Australia.[4] He then worked at Goddard Space Flight Center from September 1967 to January 1970 as National Academy of Sciences Research Associate.[5]

Turkey and METU

In February 1970 Ögelman decided to return to Turkey, so that he could contribute his experimental research and teaching capabilities to his country.[6] He was hired as an associate professor in the Middle East Technical University (METU) Physics Department, and was appointed department chairman that same year. [5] [7] He started an experimental High Energy Astrophysics group specializing in gamma ray astronomy—at the time, a fledgling new field—and took on graduate students for the group’s M.Sc. and Ph.D. programs. [3] Ögelman also started a new solar energy group to train graduate students to address Turkey’s energy needs. Additionally, he worked with the METU’s Carbon-14 Dating Group, led by Yeter Goksu, a physics department colleague who would later become his second wife.[3]

During Ögelman’s time at METU, his astrophysics group’s major projects used data of NASA’s SAS-II (Second Small Astronomy Satellite) gamma ray telescope. With this group and his former NASA colleagues, Ögelman co-authored several critical papers on gamma ray astronomy published using the SAS II data. Their work covered the premiere satellite based detection of gamma rays from celestial objects, the observation of galactic gamma ray emission from compact objects including the Crab Nebula, and the discovery of Geminga.

The SAS II gamma ray telescope’s successful results during the 1970s brought gamma ray astronomy of age and established it as the newest astrophysics field. Under Ögelman’s leadership, his group carried out actual data analysis at METU with graduate and undergraduate students, and contributed significantly to the SAS II project’s success. By that time the once-fledgling field of gamma ray astronomy had since grown into a major science utilizing numerous other space-based and balloon-born telescopes, and many important discoveries have been made extending astronomy to the high energy region.

In 1973 Ögelman took a leave of absence from METU to complete his army service. In 1974 he took a sabbatical leave of absence to serve as a National Academy of Sciences Senior Research Associate at the Goddard Space Flight Center in Greenbelt, Maryland, working with his colleagues at NASA’s Gamma Ray Astronomy Group led by Dr. Carl E. Fichtel. Ögelman returned to METU in 1975, becoming a full professor in 1976.

In 1977, at the invitation of the president of Çukurova University (CÜ) in Adana, Turkey, Ögelman took another leave of absence and with three of his METU colleagues (and, later, some of his graduate and post graduate students from METU, who formed the core of the new Physics Department) moved to CÜ to start and establish its Faculty of Arts and Sciences.[8] Becoming the founding Dean of the faculty, he decided to take students without delay, and the group started classes in barracks. Eventually, Ögelman arranged for funding from the Ford Foundation and the USAID to start a modern research laboratory in the campus. He also took an interest in the local economy and needs of the people, and encouraged the faculty to research in fields with most benefit to the region. One of the most important topics to address at that time concerning physics was Turkish society's energy needs. Ögelman gave priority to solar energy research in the Physics Department because in the Cukurova region there is plenty of sunshine throughout the year. To this end, as he had at METU, he started research in solar energy, building Turkey’s first energy efficient solar house and a solar pond. Ögelman left CÜ in 1982 to return to METU but continued working with his previous students as colleagues on astrophysics.

From July 1983 to July 1985, Ögelman again took a leave of absence from METU, spending the period as a guest scientist at the Max Planck Institute for Extraterrestrial Physics (MPE) in Munich, Germany. Ögelman then became a resident scientist at MPE and worked there from July 1985 to January 1991.[5] He started working on X-ray data of the Einstein and Exosat satellites. After the launch of the hugely successful ROSAT (Röntgensatellit - German X-Ray Satellite) Observatory (June 1, 1990 – February 12, 1999) led by Principal Investigator (PI) Joachim Trümper at MPE and developed through a cooperative program between Germany, the United States, and the United Kingdom, Ögelman became one of the main investigators with this satellite. ROSAT performed the first all sky surveys with imaging telescopes, leading to the discovery of 125,000 X-ray and 479 EUV sources. In addition the diffuse galactic X-ray emission was mapped with unprecedented angular resolution (< 1 arcmin). Most of the mission time was devoted to pointed observations at selected targets. In total 4,580 PSPC (Position Sensitive Proportional Counter) and 4482 HRI fields were covered with observation times between ~ 2,000 sec and ~ 1 Million sec. 700 Scientists (PIs) from 24 countries were involved in these pointed observations. The total number of ROSAT based publications is 4787, with 54,9 % in referred journals (status August 2001).[9] Ögelman took part in the analysis of ROSAT data from the beginning and published some of his most exciting research work.

In 1983 he proposed X-ray observations of a classical nova in outburst (GQ Mus) with Exosat. The nova turned to be a luminous X-ray source in the lowest range of X-ray energy (called "supersoft") proving the thermonuclear burning on the surface of a white dwarf, thought to be the cause of the outburst. With ROSAT Ögelman and collaborators could establish that novae in outburst are among the most luminous sources in the X-ray sky.

In 1988 Ögelman was awarded Turkey’s highest scientific honor, the Sedat Simavi Prize.[2] In 1991, he received the Turkish Scientific and Technical Research Council Prize. He represented Turkey on international science councils and co-operations, and served on NASA committees and working groups. He was instrumental in the 1991 establishment of the Turkish national astronomic observatory for TÜBİTAK. Around this time Ögelman's second marriage ended. He began seeing and subsequently married an Italian astronomer, Marina Orio; they spent the remainder of his life together. [10]

University of Wisconsin

At Max Planck, Ögelman had met the University of Wisconsin astrophysicist Prof. William F. “Jack” Fry, who would become a good friend and mentor. Fry returned to the University of Wisconsin from MPE with an interest in building up the Wisconsin astrophysics program by adding a high energy astrophysics group to complement the astroparticle/neutrino group. He persuaded Hakki Ögelman to join the Wisconsin faculty, first as a visiting professor from January 1991 to September 1992, and, then, from the end of 1992, as a full-time professor. One of Ögelman’s METU students, Prof. A. Baha Balantekin, was already at Wisconsin University Physics Department, having arrived in 1986. (Balantekin served as department chairman between 2008 and 2011.)

During Ögelman’s tenure at Wisconsin, he continued to pursue his interest in compact objects, and published roughly sixty papers on the subject between 1991 and 1998. As time passed and experiments became larger and more institutional, Ögelman devoted an increasing amount of time to data analysis and worked on analyzing the data from major X-ray missions such as the ROSAT Telescope, Beppo-SAX, and AXAF.

While at Wisconsin, Ögelman visited METU, Sabanci and/or Çukurova Universities in Turkey regularly, practically every summer.[2] He visited and worked with his former graduate students Profs. Umit Kiziloglu, Mehmet Emin Özel, Akif Esendemir, Solen Balman and with Ilhami Yegingil at CÜ—all of whom had become professors by this time—and also with Prof. Altan Baykal. Ögelman especially spent significant amount of time with Prof. Ali Alpar at Sabanci University, a private, technically oriented school in Istanbul on pulsar research and jointly publishing several papers, which he considered to be some of his best work. Ögelman also took part and/or organized several scientific symposiums, conferences meetings with his colleagues in Turkey.

In 1997, Ögelman suffered a major stroke. His life was saved by the intervention and treatment of University of Wisconsin doctors. He returned to work after his recovery and carried on working on his research but at a slower pace. Life was difficult for him because his movement was limited. In the spring of 2011 Ögelman’s declining health forced his retirement.

Personal life

Ögelman loved music, literature, sports, and was very concerned about finding a sustainable solution to the world's energy needs. He was a competitive wrestler in college and a black belt in judo.

Hakki Ögelman died on September 4, 2011. In his memory, the Turkish Astronomical Society established the Hakki Ögelman Summer Schools, intended to "offer intense summer training to undergraduate and graduate students of astronomy from all over Turkey, in physics, computation and other subjects related to research in astronomy.” The Turkish Philanthropy Funds coordinates international contributions to this project.[11]

Positions held

Awards, prizes and honors

Selected publications

  • Achterberg, A., Ogelman, H.; et al. (February 2008). "The search for muon neutrinos from northern hemisphere gamma-ray bursts with AMANDA". Astrophysical Journal 674 (1): 357–370. arXiv:0705.1186. Bibcode:2008ApJ...674..357A. doi:10.1086/524920. 
  • Ackermann, T. Ogelman, H.; et al. (January 2006). "Limits to the muon flux from neutralino annihilations in the sun with the AMANDA detector". Astroparticle Physics 24 (6): 459–466. arXiv:astro-ph/0508518. Bibcode:2006APh....24..459A. doi:10.1016/j.astropartphys.2005.09.006. 
  • Ahrens, J., Ogelman, H.; et al. (April 2004). "Status of the IceCube neutrino observatory - 2nd VERITAS symposium on the astrophysics of extragalactic sources, April 24-26, 2003". New Astronomy Reviews 48 (5-6): 519–525. Bibcode:2004NewAR..48..519A. doi:10.1016/j.newar.2003.12.031. 
  • Alpar, M., Ogelman, H., Shaham, J. (June 1993). "Is Geminga A Glitching Pulsar". Astronomy and Astrophysics 273 (1): L35–L37. Bibcode:1993A&A...273L..35A. 
  • Ayasli, S., Ogelman, H., (April 1980). "Gamma-rays from pulsars". Astrophysical Journal 237 (1): 227–235. Bibcode:1980ApJ...237..227A. doi:10.1086/157862. 
  • Balman, S., Orio, M., Ogelman, H. (August 1995). "ROSAT observation of the old classical nova CP Puppis". The Astrophysical Journal 449 (1): L47–L50. Bibcode:1995ApJ...449L..47B. doi:10.1086/309628. 
  • Baykal, A., Ogelman, H. (1993). "An empirical torque noise and spin-up model for accretion-powered x-ray pulsars". Astronomy and Astrophysics 267 (1): 119–125. Bibcode:1993A&A...267..119B. 
  • Bignami, G., Fichtel, C., Hartman, R., Kniffen, D., Ogelman, H., Thompson, D., Ozel, M., Tümer, T. (January 1975). "High-energy galactic gamma-radiation from Sas-2 satellite". Bulletin of the American Physical Society 20 (4): 656. 
  • Brinkmann, W., Ogelman, H. (August 1987). "Soft x-ray observations of the radio pulsar PSR-1055-52". Astronomy and Astrophysics 182 (1): 71–74. Bibcode:1987A&A...182...71B. 
  • Buccheri, R., Ogelman, H., (January 1988). "Two neutrino periodicities from supernova 1987A". Nature 331 (6154): 309–310. Bibcode:1988Natur.331..309O. doi:10.1038/331309d0. 
  • Fichtel, C., Hartman, R., Kniffen, D., Thompson, D., Bignami, G., Ogelman, H., Ozel, M., Tümer, T. (May 1975). "High-energy gamma-ray results from second small astronomy satellite". Astrophysical Journal 198 (1): 163–182. Bibcode:1975ApJ...198..163F. doi:10.1086/153590. 
  • Fichtel, C., Hartman, R., Kniffen, D., Thompson, D., Ogelman, H., Ozel, M., Tümer, T. (October 1977). "SAS-2 Observations of the diffuse gamma-radiation in the galactic latitude interval 10-degrees less than (B) less than or equal to 90-degrees". Astrophysical Journal 217 (1): L9–L13. Bibcode:1977ApJ...217L...9F. doi:10.1086/182528. 
  • Finley, J., Ogelman, H. (October 1994). "The PSR 1800-21/G8.7-0.1 association - a view from ROSAT". Astrophysical Journal 434 (1, Part 2): L25–L28. Bibcode:1994ApJ...434L..25F. doi:10.1086/187563. 
  • Gurkan, M., Baykal, A., Alpar, M., Ogelman, H., Strohmayer, T. (April 2000). "Post-glitch RXTE-PCA observations of the Vela pulsar". Astronomy & Astrophysics 356 (3): 1136–1140. Bibcode:2000A&A...356.1136G. 
  • Hartman, R., Kniffen, D., Thompson, D., Fichtel, C., Ogelman, H., Tümer, T., Ozel, M. (June 1979). "Galactic plane gamma-radiation". Astrophysical Journal 230 (2): 597–606. Bibcode:1979ApJ...230..597H. doi:10.1086/157118. 
  • Kiziloglu, U., Derman, E., Ogelman, H., Tokdemir, F., (June 1983). "Ultraviolet observations of AR-Lacertae". Astronomy and Astrophysics 123 (1): 17–21. Bibcode:1983A&A...123...17K. 
  • Kniffen, D., Hartman, R., Thompson, D., Bignami, G., Fichtel, C., Tümer, T., Ogelman, H. (October 1974). "Gamma radiation from the Crab Nebula above 35 MeV.". Nature 251 (5474): 397–399. Bibcode:1974Natur.251..397K. doi:10.1038/251397a0. 
  • Krautter, J., Ogelman, H., Starrfield, S., Wichmann, R., Pfeffermann, E. (January 1996). "ROSAT X-Ray Observations of Nova V1974 Cygni: the rise and fall of the brightest supersoft x-ray source". Astrophysical Journal 456 (2, Part 1): 788–797. Bibcode:1996ApJ...456..788K. doi:10.1086/176697. 
  • Maran, S., Ogelman, H. (October 1969). "Pulsar periods and rapid changes in terrestrial rotation rate". Nature 224 (5217): 349. Bibcode:1969Natur.224..349M. doi:10.1038/224349a0. 
  • Markwardt, C., Ogelman, H. (May 1995). "An x-ray jet from the Vela pulsar". Nature 375 (6526): 40–42. Bibcode:1995Natur.375...40M. doi:10.1038/375040a0. 
  • Ogelman, H. (February 1969). "Discrete source interpretation of recent high energy cosmic gamma ray measurements". Nature 221 (5182): 753–754. Bibcode:1969Natur.221..753O. doi:10.1038/221753a0. 
  • Ogelman, H. (December 1970). "Extensive air shower arrays as detectors of prompt gamma rays from supernovae explosions". Nature 228 (5277): 1181. Bibcode:1970Natur.228.1181O. doi:10.1038/2281181a0. 
  • Ogelman, H. (June 1973). "Millisecond time scale atmospheric light pulses associated with solar and magnetospheric activity". American Geophysical Union 78 (16): 3033–3039. Bibcode:1973JGR....78.3033O. doi:10.1029/JA078i016p03033. 
  • Ogelman, H. (December 1993). "ROSAT observations of single pulsars". Advances in Space Research 13 (12): 135–137. Bibcode:1993AdSpR..13..135O. doi:10.1016/0273-1177(93)90105-k. 
  • Ogelman, H., Fichtel, C., Kniffen, D. (May 1975). "Observations of low-energy gamma-ray bursts with Sas-2". Nature 255 (5505): 208–210. Bibcode:1975Natur.255..208O. doi:10.1038/255208b0. 
  • Ogelman, H., Finley, J., Zimmermann, H. (January 1993). "Pulsed x-rays from the Vela pulsar". Nature 361 (6408): 136–138. Bibcode:1993Natur.361..136O. doi:10.1038/361136a0. 
  • Ogelman, H., Orio, M., Krautter, J., Starrfield, S. (January 1993). "Detection of supersoft x-ray emission from GQ-Muscae nine years after a nova outburst". Nature 361 (6410): 331–333. Bibcode:1993Natur.361..331O. doi:10.1038/361331a0. 
  • Ogelman, H., Sobieski, S. (July 1969). "Search for ultra-short light pulses from pulsars". Nature 223 (5201): 47–48. Bibcode:1969Natur.223...47O. doi:10.1038/223047a0. 
  • Ogelman, H., Swank, J. (December 1974). "Neutron stars with main-sequence binary companions as low luminosity x-ray sources". Astronomy and Astrophysics 37 (1): 101–104. Bibcode:1974A&A....37..101O. 
  • Ogelman, H., Tepedelenlioglu, E. (2004). "Chandra observations of two pulsars PSR 0628-28 and PSR 1813-36". Advances in Space Research 33 (4): 597–600. Bibcode:2004AdSpR..33..597O. doi:10.1016/j.asr.2003.02.018. 
  • Ogelman, H., Zimmermann, H. (April 1989). "Soft x-ray observations of the VELA pulsar PSR 0833-45". Astronomy and Astrophysics 214 (1-2): 179–185. Bibcode:1989A&A...214..179O. 
  • Orio, M., Balman, S., DellaValle, M., Gallagher, J., Ogelman, H. (July 1996). "X-ray emission of nova Puppis 1991: accretion or a shocked shell?". Astrophysical Journal 466 (1, Part 1): 410–414. Bibcode:1996ApJ...466..410O. doi:10.1086/177520. 
  • Seward, F., Alpar, M., Flanagan, C., Kiziloglu, U., Markwardt, C., Mcculloch, P., Ogelman, H. (June 2000). "ROSAT observations of the Vela pulsar". Astrophysical Journal 536 (2): 948–953. arXiv:astro-ph/0004015. Bibcode:2000ApJ...536..948S. doi:10.1086/308961. 
  • Tepedelenlioglu, E., Ogelman, H. (April 2007). "Discovery of extended emission around the pulsar B0355+54". Astrophysical Journal 658 (2): 1183–1187. Bibcode:2007ApJ...658.1183T. doi:10.1086/510995. 
  • Thompson, D., Bailes, M., Bertsch, D., Cordes, J., D’Amico, N., Esposito, J., Finley, J., Hartman, R., Hermsen, W., Kanbach, G., Kaspi, V., Kniffen, D., Kuiper, L., Lin, Y., Lyne, A., Manchester, R., Matz, S., Mayer-Hasselwander, H., Michelson, P., Nolan, P., Ogelman, H., Pohl, M., Ramanamurthy, P., Sreekumar, P., Reimer, O., Taylor, J., Ulmer, M. (May 1999). "Gamma radiation from PSR B1055-52". Astrophysical Journal 516 (1): 297–306. arXiv:astro-ph/9811219. Bibcode:1999ApJ...516..297T. doi:10.1086/307083. 
  • Trumper, J., Kahabka, P., Ogelman, H., Pietsch, W., Voges, W. (January 1986). "EXOSAT observations of the 35 day cycle of Hercules X-1 - evidence for neutron-star precession". Astrophysical Journal 300 (2, Part 2): L63–L67. Bibcode:1986ApJ...300L..63T. doi:10.1086/184604. 
  • Tümer, T., Gordon, E., Hamilton, W., Hurley, K., Maeding, D., Mohanty, G., Ogelman, H., Paulos, R., Puetter, R., Souchkov, V., Zweerink, J. (December 1999). "Preliminary test results of pixel detectors developed for the all-sky x-ry & gamma-ray astronomy monitor (AXGAM)". Nuclear Science Symposium, 1999. Conference Record. 1999 IEEE 2: 626, 632. doi:10.1109/NSSMIC.1999.845748. 
  • Yegingil, I., Ogelman, H., Kiziloglu, N. (1980). "Investigation of sodium in the upper atmosphere". Journal of Geophysical Research - Oceans and Atmospheres 85 (C10): 5507–5510. Bibcode:1980JGR....85.5507Y. doi:10.1029/JC085iC10p05507. 

References

  1. ↑ Orio, Marina (2011). "Obituary of Hakki Ögelman". Bulletin of the American Astronomical Society 43 (38). Bibcode:2011BAAS...43..037O. doi:10.3847/baasobit2011038.
  2. 1 2 3 Orio 2011.
  3. 1 2 3 Work 2012.
  4. ↑ Ögelman, Hakki (1998). "Curriculum Vitae of Prof. Hakki B. Ögelman". Compact Objects at Wisconsin. Retrieved 16 December 2013.
  5. 1 2 3 Ögelman 1998.
  6. ↑ Work, Peter; Allen, Joe (July 2012). "Remembering Hakki Ogelman". DePauw University News & Media. Retrieved 16 December 2013.
  7. ↑ "History". Middle East Technical University Department of Physics. Retrieved 16 September 2014.
  8. ↑ Balantekin, Baha; Timbie, Peter (2012). "Memorial Resolution of the Faculty of the University of Wisconsin-Madison on the Death of Professor Emeritus Hakki B. Ögelman" (PDF). Office of the Secretary of the Faculty University of Wisconsin-Madison. Retrieved 16 December 2013.
  9. ↑ X-Ray Group at MPE. "X-Ray Astronomy: ROSAT". Max-Planck-Institut für extraterrestrische Physik. Retrieved 16 December 2013.
  10. ↑ Balantekin 2012.
  11. ↑ "Hakki Ögelman Summer Schools". Turkish Philanthropy Funds. Retrieved 2 June 2014.

Further reading

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