Positions: | Research Staff; Deputy Chief Designer of the Science Application System, the Einstein Probe Mission |
---|---|
Academic Title: | Dr. |
E-mail: | ccjin@nao.cas.cn |
Mailing Address: | Chichuan Jin |
Research Staff, NAOC, Beijing, China, 2017-current
Postdoc, MPE, Garching, Germany, 2015-2017
Research Scientist, Qianxuesen Lab, CAST, Beijing, China, 2014-2015
Visiting Scholar, IHEP, Beijing, China, 2012-2013
PhD: Durham University, Durham, United Kingdom, 2008-2012
BSc: Tsinghua University, Beijing, China, 2004-2008
Active Galactic Nuclei: X-ray Spectral Variability, Multi-wavelength Study
Intersteller Medium: X-ray Dust Scattering
X-ray Transients
Fundings:
National Natural Science Foundation of China: No. 11873054 (Lead)
Proposals Accepted as PI:
1. PI: Swift ToO,2020,20 ksec, ID: 36528 (triggered)
2. PI: XMM-Newton GO, AO-19, 123 ksec,ID: 08637901 (accepted)
3. PI: Chandra ToO,Cycle-21, 40 ksec Chandra + 40 ksec XMM-Newton,ID: 21910146 (accepted, waiting for trigger)
4. PI: XMM-Newton GO, AO-18, 133 ksec XMM-Newton + 200 ksec Nustar, ID: 0841801 (observed)
5. PI: XMM-Newton GO, AO-18, 132 ksec, ID: 8418201 (observed)
6. PI: XMM-Newton GO, AO-17, 396 ksec XMM-Newton + 260 ksec NuSTAR, Large Program, ID: 08240801 (observed)
7. PI: XMM-Newton GO, AO-17, 72 ksec XMM-Newton + 100 ksec NuSTAR, ID: 08240301 (observed)
8. PI: XMM-Newton ToO, AO-16, 43 ksec, ID: 08032301 (accepted)
9. PI: XMM-Newton GO, AO-15, 124 ksec, ID: 07849301 (observed)
10. PI: XMM-Newton GO, AO-15, 132 ksec, ID: 07849701 (accepted)
11. PI: XMM-Newton GO, AO-14, 124 ksec, ID: 07645301 (accepted)
12. PI: XMM-Newton GO, AO-12, 123 ksec, ID: 07248401 (observed)
13. PI: XMM-Newton GO, AO-12, 63 ksec, ID: 07251301 (accepted)
14. PI: XMM-Newton GO, AO-11, 102 ksec, ID: 06910601 (observed)
15. PI: XMM-Newton GO, AO-10, 122 ksec, ID: 06753201 (accepted)
First-author Publications:
1. Jin C., Done C., Ward M., 2020, MNRAS, accepted, Re-observing the NLS1 Galaxy RE J1034+396. II. New Insights on the Soft X-ray Excess, QPO and the Analogy with GRS 1915+105
2. Jin C., Done C., Ward M., 2020, MNRAS, 495, 3538, Re-observing the NLS1 Galaxy RE J1034+396. I. the Long-term, Recurrent X-ray QPO with a High Significance
3. Jin C., Ponti G., Guang X., Bogensberger D., 2019, ApJ, 875, 157, Exploring the Interstellar Medium Using an Asymmetric X-Ray Dust Scattering Halo
4. Jin C., Ponti G., Haberl F., Smith R., Valencic L., 2018, MNRAS, 477, 3480, Effects of interstellar dust scattering on the X-ray eclipses of the LMXB AX J1745.6-2901 in the Galactic Centre
5. Jin C., Done C., Ward M., 2017a, MNRAS, 468, 3663, Super-Eddington QSO RX J0439.6-5311 – I. Origin of the soft X-ray excess and structure of the inner accretion flow
6. Jin C., Done C., Ward M., Gardner E., 2017b, MNRAS, 471, 706, Super-Eddington QSO RX J0439.6-5311 – II. Multiwavelength constraints on the global structure of the accretion flow
7. Jin C., Ponti G., Haberl F., Smith R., 2017c, MNRAS, 468, 2532, Probing the interstellar dust towards the Galactic Centre: dust-scattering halo around AX J1745.6-2901
8. Jin C., Done C., Ward M., 2016, MNRAS, 455, 691, Strong constraints on a super-Eddington accretion flow: XMM-Newton observations of an intermediate-mass black hole
9. Jin C., Done C., Middleton M., Ward M., 2013, MNRAS, 436, 3173, A long XMM-Newton observation of an extreme narrow-line Seyfert 1: PG 1244+026
10. Jin C., Ward M., Done C., Gelbord J., 2012a, MNRAS, 420, 1825, A combined optical and X-ray study of unobscured type 1 active galactic nuclei – I. Optical spectra and spectral energy distribution modelling
11. Jin C., Ward M., Done C., 2012b, MNRAS, 422, 3268, A combined optical and X-ray study of unobscured type 1 active galactic nuclei – II. Relation between X-ray emission and optical spectra
12. Jin C., Ward M., Done C., 2012c, MNRAS, 425, 907, A combined optical and X-ray study of unobscured type 1 active galactic nuclei – III. Broad-band SED properties
13. Jin C., Done C., Ward M., Gerlinski M., Mullaney J., 2009, MNRAS, 398, L16, The Seyfert AGN RX J0136.9-3510 and the spectral state of super Eddington accretion flows