'Qsos' presentation slideshows

From ULIRGs to QSOs

From ULIRGs to QSOs. XiaoYang, Xia Center for Astrophysics Tianjin Normal University Collaborators: H. Wu, Deng, Zou, Z. Zheng, Mao, X.Z. Zheng, Hao, Huo, Y. Gao, Wang,J.L, Tan. Outline. The morphology and environment of ULIRGs and LIRGs May give hint for high-z SMGs

1.37k views • 118 slides

Mid- Infrared Spectroscopic Properties of IR QSOs

Mid- Infrared Spectroscopic Properties of IR QSOs. XiaoYang, Xia Center for Astrophysics Tianjin Normal University. Outline. Infrared Luminous QSOs (IR QSO) Spitzer IRS Spectra of IR QSOs.

782 views • 65 slides

IR QSOs at low and high redshift

IR QSOs at low and high redshift. X.Y.Xia Tianjin Normal University, China Collaborators: C.N.Hao, S.Mao, H.Wu & Z.G.Deng. Motivation. The tight correlation between Mbh and ? of host galaxy Kommendy&Gebhardt 2001, Merritt & Ferrarese 2001 The relation of SFR/Mdot vs. Mbh

556 views • 44 slides

The Coeval Growth of Black Holes and their host Spheriods

The Coeval Growth of Black Holes and their host Spheriods. X.Y.Xia Tianjin Normal University, China Collaborators: C.N.Hao, S.Mao, Z.G.Deng &H.Wu. Motivation. The tight correlation between Mbh and the mass of host spheriod Kommendy&Gebhardt 2001, Merritt & Ferrarese 2001

394 views • 32 slides

Traversing a money storm when planning a DXpedition May 19, 2012 By N1DG, Don Greenbaum

Traversing a money storm when planning a DXpedition May 19, 2012 By N1DG, Don Greenbaum. Why This Discussion?. Financial transparency rarely done on DXpeditions . It should be.

376 views • 30 slides

Traversing a money storm when planning a DXpedition May 19, 2012 By N1DG, Don Greenbaum

Traversing a money storm when planning a DXpedition May 19, 2012 By N1DG, Don Greenbaum. Why This Discussion?. Financial transparency rarely done on DXpeditions . It should be.

358 views • 30 slides

Traversing a money storm when planning a DXpedition May 19, 2012 By N1DG, Don Greenbaum

Traversing a money storm when planning a DXpedition May 19, 2012 By N1DG, Don Greenbaum. Why This Discussion?. Financial transparency rarely done on DXpeditions . It should be.

306 views • 30 slides

High-z (z > 3) QSOs studied with Subaru/HSC

High-z (z > 3) QSOs studied with Subaru/HSC. Masa Imanishi (NAOJ) Tohru Nagao (NAOJ). Outline. Importance and current understanding of high-z QSOs (AGNs). 2. QSOs at z > 7. (M.Imanishi). (Subaru/HSC + UKIRT/WFCAM). 3. Low-luminosity QSOs at z = 3-6. (Subaru/HSC). (T.Nagao).

394 views • 25 slides

High-z (z > 3) QSOs studied with Subaru/HSC

High-z (z > 3) QSOs studied with Subaru/HSC. Masa Imanishi (NAOJ) Tohru Nagao (NAOJ). Outline. Importance and current understanding of high-z QSOs (AGNs). 2. QSOs at z > 7. (M.Imanishi). (Subaru/HSC + UKIRT/WFCAM). 3. Low-luminosity QSOs at z = 3-6. (Subaru/HSC). (T.Nagao).

253 views • 25 slides

AKARI View of Distant Quasars and Galaxies

AKARI View of Distant Quasars and Galaxies. Myungshin Im CEOU/Department of Physics & Astronomy, Seoul National University. Hyungsun Jun, Dohyeong Kim, Hyung Mok Lee , Myung Gyoon Lee, Jonghak Woo (SNU), Y. Ohyama (ASIAA), Minjin Kim (KASI/Carnegie),

335 views • 24 slides

High-redshift QSOs and Galaxies in the GOODS

High-redshift QSOs and Galaxies in the GOODS. Pierluigi Monaco & Stefano Cristiani DAUT - University of Trieste INAF-Trieste Observatory. THE GOODS TEAM

323 views • 23 slides

The BH mass of nearby QSOs

210 views • 14 slides