In total $753,864+2,953 Euro+30,000 Chinese Yuan grant under my control. Most of them were awarded in the past three years after I came to University of Michigan.
In total 1.17 Ms XMM-Newton data + 200 ks Chandra data + two-year archival Chandra program + 403 ks NuSTAR data + 100 ks Suzaku data + 22 ks Swift data + 3 hours SOFIA data.
[19] Jul. 2018, PI, Hot circum-galactic medium as a legacy of Chandra archive, Chandra Space Telescope Cycle 20 Proposal (archival; $90,000, two years); Proposal number: 20610246.
[18] Jul. 2018, PI, Non-thermal hard X-ray emission from a superbubble in a non-starburst galaxy, Chandra Space Telescope Cycle 20 Proposal (100 ks; approved ); Proposal number: 20610185.
[17] Dec. 2016, PI, XMM-Newton Legacy Survey of M31 Halo: Searching for the Missing Accreted Hot CGM, XMM-Newton Space Telescope AO-16 Proposal (510 ks, taken; $108,699); Proposal number: 080073.
[16] Jan. 2017 - Dec. 2018, PI, Non-thermal X-ray emission from a “Fermi bubble” in an external galaxy, Chandra Space Telescope Cycle 18 Proposal (100 ks, taken; $58,300, two years); Proposal number: 18610344.
[15] Oct. 2016 - Sep. 2018, PI, Neutral and Ionized Gas from the Most Energetic Extragalactic Nuclear Superbubble in NGC 3079, SOFIA Telescope Cycle 5 Proposal (3 hrs, scheduled; $40,000, two years); Proposal number: 05_0020.
[14] Sep. 2016, PI, A Systematical Spatially Resolved XMM-Newton Spectroscopy Study of X-ray Bright Galactic SNRs, AO2 AHEAD Visitor’s Programme (4 weeks travel grant to CEA, Saclay, France; 2,953 Euro).
[13] Oct. 2015, PI, Post-Outburst Multi-Wavelength Variation of Two Tidal Disruption Event Candidates, Swift Space Telescope Cycle 12 Proposal (22 ks, taken).
[12] Oct. 2015 - Sep. 2017, PI, Hard X-ray Emission from a Nearby Cosmic Ray Accelerator, NuSTAR Space Telescope Cycle-1 Proposal (403 ks, taken; $45,231, two years); Proposal number: NNX15AV24G.
[11] Jan. 2015 - Dec. 2017, Sponsor PI, Hot Coronae Around Local Spiral Galaxies: A Key Probe of Galaxy Formation Theory, NASA Astrophysics Data Analysis proposal ($361,634, three years); Proposal number: NNX15AM93G, University of Michigan PI: Joel N. Bregman; University of Massachusetts PI, co-I: Q. Daniel Wang.
[10] Feb. 2014, PI, Searching for Large Scale Diffuse X-ray Emission Around an Interacting Galaxy, Suzaku Space Telescope Cycle 9 Proposal (50 ks, Priority C); Proposal number: 92003.
[9] Dec. 2013, PI, Large Scale Circumgalactic Coronae around Massive Spiral Galaxies, XMM- Newton Space Telescope AO-13 Large Proposal (520.9 ks of five galaxies, taken in AO-13 and AO-14); Proposal number: 074130.
[8] Dec. 2013, PI, Supernova Remnant Evolving in Wind-Blown Bubbles: A Case Study of Kes 27, XMM-Newton Space Telescope AO-13 Proposal (80 ks, taken); Proposal number: 074064.
[7] Dec. 2013, PI, Mystery of the Unusually Strong X-ray Emission around an Interacting Galaxy Pair, XMM-Newton Space Telescope AO-13 Proposal (87 ks, Priority C); Proposal number: 074060.
[6] 2012, PI, X-raying the Matter Circulation around Nearby Disk Galaxies, NASA Astrophysics Data Analysis proposal ($50,000, one year); Grant number: NNX12AE78G.
[5] Jan. 2012, PI, Does Diffuse Soft X-ray Emission Produced by Galactic Feedback? — Spectral Diagnostics of NGC 4438, Suzaku Space Telescope Cycle 7 Proposal (300 ks, Priority C); Proposal number: 71501.
[4] 2011-2012, PI, Multi-wavelength Study of Nearby Galaxy Halos, Open Foundation of Key Lab- oratory of Modern Astronomy and Astrophysics, Nanjing University, Ministry of Education, China (30,000 Yuan, two years).
[3] Apr. 2011, PI, X-ray Spectroscopy of Stellar Feedback Processes in a Cool Gas-Rich S0 Galaxy, Suzaku Space Telescope Cycle 6 Proposal (100 ks, taken); Proposal number: 61502.
[2] Dec. 2010, PI, X-ray Emission from Galaxy Halos — Circulation and Environmental Effects, XMM-Newton Space Telescope AO-10 Proposal (56 ks of two galaxies, taken; 37 ks of one galaxy, Priority C); Proposal number: 067143.
[1] Dec. 2009, PI, NGC 5866: A Case Study of the Disk/Bulge/Halo Interaction in an S0 Galaxy, XMM-Newton Space Telescope AO-9 Proposal (53 ks, Priority C); Proposal number: 65049.