Dr. Jack Singal
Assistant Professor of Physics
Profile

My research connects several important topics in the emerging era of big data astrophysics. We carry out population studies of active galaxies and explore questions such as how they have changed over the history of the Universe. For this we utilize observational data from ground and satellite-based surveys in visible light, radio waves, gamma rays, and other kinds of light.  We also have a laboratory program to make precision measurements of subtle distortion effects on telescope images, which are an increasing challenge for coming astronomical surveys.  Additionally, we are involved in exploring survey issues such as photometric redshifts, and in ongoing projects characterizing the diffuse radio and microwave light from the cosmos.

Presentations

Public Talk: The Light Our Eyes Can't See
University of Richmond Downtown, June 6, 2017

Presentation: CMB@50 Conference
Princeton University, June 10, 2015

Colloquium: Harvard Smithsonian Center for Astrophysics
Harvard University, February 11, 2016

Professional Experience
Postdoctoral Scientist, Stanford University and SLAC National Accelerator Laboratory (2007-2013)
Postdoctoral Resesarcher, NASA Goddard Space Flight Center (2007)
Selected Publications
Articles
Axial Ratio of Edge-On Spiral Galaxies as a Test For Bright Radio Halos.  J. Singal, A. Kogut, E. Jones, and H. Dunlap, 2015, ApJL, 799, L10

Gamma-ray Luminosity and Photon Index Evolution of FSRQ Blazars and Contribution to the Gamma-ray Background. J. Singal, A. Ko, and V. Petrosian, 2014, ApJ, 786, 109

Geant4 Applications for Modeling Molecular Transport in Complex Vacuum Geometries. J. Singal, J. Langton, and R. Schindler, 2014, IJMSSC, 5, 2
Determination of the intrinsic Luminosity Time Correlation in the X-ray Afterglows of GRBs. M. Dainotti, V. Petrosian, J. Singal, and M. Ostrowski, 2013, ApJ, 774, 157
The Radio and Optical Luminosity Evolution of Quasars II – The SDSS Sample.” J. Singal, V. Petrosian, L. Stawarz, and A. Lawrence, 2013, ApJ, 764, 43
On The Radio and Optical Luminosity Evolution of Quasars.” J. Singal, V. Petrosian, A. Lawrence, and L. Stawarz, 2011, ApJ, 743, 104
The Efficacy of Galaxy Shape Parameters in Photometric Redshift Estimation: A Neural Network Approach.” J. Singal, M. Shmakova, B. Gerke, and J. Lotz, 2011, PASP, 615, 621
The ARCADE 2 Instrument.” J. Singal, D. Fixsen, A. Kogut, S. Levin, M. Limon, P. Lubin, P. Mirel, M. Seiffert, T. Villela, E. Wollack, and C.A. Wuensche, 2011, ApJ, 730, 138
ARCADE 2 Measurement of the Absolute Sky Brightness at 3-90 GHz.” D. Fixsen, A. Kogut, S. Levin, M. Limon, P. Lubin, P. Mirel, M. Seiffert, J. Singal, T. Villela, E. Wollack, and C.A. Wuensche, 2011, ApJ, 734, 5
ARCADE 2 Observations of Galactic Radio Emission.” A. Kogut, D. Fixsen, S. Levin, M. Limon, P. Lubin, P. Mirel, M. Seiffert, J. Singal, T. Villela, E. Wollack, and C.A. Wuensche, 2011, ApJ, 734, 4
Interpretation of the ARCADE 2 Absolute Sky Brightness Measurement.” M. Seiffert, D. Fixsen, A. Kogut, S. Levin, M. Limon, P. Lubin, P. Mirel, J. Singal, T. Villela, E. Wollack, and C.A. Wuensche, 2011, ApJ, 734, 6
Sources of the Radio Background Considered.” J. Singal, L. Stawarz, A. Lawrence, and V. Petrosian, 2010, MNRAS, 409, 1172
“The Cosmic Radio Background and AGN Connection.” J. Singal, L. Stawarz, A. Lawrence, and V. Petrosian, 2010, IJMPD, 19, 965
“A Multi-Chamber System for Analyzing the Outgassing, Deposition, and Associated Optical Degradation Properties of Materials in a Vacuum.” J. Singal, R. Schindler, C. Chang, P. Czodrowski, and P. Kim, 2010, Rev Sci Instrum, 81, 025101
“PHAT: Photo-z Accuracy Testing.” H. Hildebrandt, S. Arnouts, P. Capak, L. Moustakas, C. Wolf, F. Abdalla, R. Assef, M. Banerj, G. Brammer, S. Carliles, D. Coe, T. Dahlen, R. Feldmann, D. Gerdes, B. Gillis, R. Kotulla, I. Li, J.-M. Miralles, N. Purger, S. Schmidt, and J. Singal, 2010, A&A, 523, A31

Education
Ph.D., University of California, Santa Barbara
Physics
B.S., New York University
Physics
Contact Information
(804) 287-6537
Areas of Expertise
Multiwavelength astrophysics analysis
Data challenges in large survey astrophysics
Instrumentation methods in visible, radio, and microwave