The identification of z-dropouts in Pan-STARRS1: three quasars at 6.5
Autor:
Venemans, B. P., Bañados, E., Decarli, R., Farina, E. P., Walter, F., Chambers, K. C., Fan, X., Rix, H-W., Schlafly, E., McMahon, R. G., Simcoe, R., Stern, D., Burgett, W. S., Draper, P. W., Flewelling, H., Hodapp, K. W., Kaiser, N., Magnier, E. A., Metcalfe, N., Morgan, J. S., Price, P. A., Tonry, J. L., Waters, C., AlSayyad, Y., Banerji, M., Chen, S. S., González-Solares, E. A., Greiner, J., Mazzucchelli, C., McGreer, I., Miller, D. R., Reed, S., Sullivan, P. W.
Rok vydání:
2015
Předmět:
Zdroj:
The Astrophysical Journal Letters, Volume 801, Issue 1, article id. L11, 7 pp. (2015)
Druh dokumentu:
Working Paper
DOI:
10.1088/2041-8205/801/1/L11
Popis:
Luminous distant quasars are unique probes of the high redshift intergalactic medium (IGM) and of the growth of massive galaxies and black holes in the early universe. Absorption due to neutral Hydrogen in the IGM makes quasars beyond a redshift of z~6.5 very faint in the optical $z$-band, thus locating quasars at higher redshifts require large surveys that are sensitive above 1 micron. We report the discovery of three new z>6.5 quasars, corresponding to an age of the universe of <850 Myr, selected as z-band dropouts in the Pan-STARRS1 survey. This increases the number of known z>6.5 quasars from 4 to 7. The quasars have redshifts of z=6.50, 6.52, and 6.66, and include the brightest z-dropout quasar reported to date, PSO J036.5078+03.0498 with M_1450=-27.4. We obtained near-infrared spectroscopy for the quasars and from the MgII line we estimate that the central black holes have masses between 5x10^8 and 4x10^9 M_sun, and are accreting close to the Eddington limit (L_Bol/L_Edd=0.13-1.2). We investigate the ionized regions around the quasars and find near zone radii of R_NZ=1.5-5.2 proper Mpc, confirming the trend of decreasing near zone sizes with increasing redshift found for quasars at 5.7
Databáze:
arXiv
Externí odkaz:
| Autor: | Venemans, B. P., Bañados, E., Decarli, R., Farina, E. P., Walter, F., Chambers, K. C., Fan, X., Rix, H-W., Schlafly, E., McMahon, R. G., Simcoe, R., Stern, D., Burgett, W. S., Draper, P. W., Flewelling, H., Hodapp, K. W., Kaiser, N., Magnier, E. A., Metcalfe, N., Morgan, J. S., Price, P. A., Tonry, J. L., Waters, C., AlSayyad, Y., Banerji, M., Chen, S. S., González-Solares, E. A., Greiner, J., Mazzucchelli, C., McGreer, I., Miller, D. R., Reed, S., Sullivan, P. W. |
|---|---|
| Rok vydání: | 2015 |
| Předmět: | |
| Zdroj: | The Astrophysical Journal Letters, Volume 801, Issue 1, article id. L11, 7 pp. (2015) |
| Druh dokumentu: | Working Paper |
| DOI: | 10.1088/2041-8205/801/1/L11 |
| Popis: | Luminous distant quasars are unique probes of the high redshift intergalactic medium (IGM) and of the growth of massive galaxies and black holes in the early universe. Absorption due to neutral Hydrogen in the IGM makes quasars beyond a redshift of z~6.5 very faint in the optical $z$-band, thus locating quasars at higher redshifts require large surveys that are sensitive above 1 micron. We report the discovery of three new z>6.5 quasars, corresponding to an age of the universe of <850 Myr, selected as z-band dropouts in the Pan-STARRS1 survey. This increases the number of known z>6.5 quasars from 4 to 7. The quasars have redshifts of z=6.50, 6.52, and 6.66, and include the brightest z-dropout quasar reported to date, PSO J036.5078+03.0498 with M_1450=-27.4. We obtained near-infrared spectroscopy for the quasars and from the MgII line we estimate that the central black holes have masses between 5x10^8 and 4x10^9 M_sun, and are accreting close to the Eddington limit (L_Bol/L_Edd=0.13-1.2). We investigate the ionized regions around the quasars and find near zone radii of R_NZ=1.5-5.2 proper Mpc, confirming the trend of decreasing near zone sizes with increasing redshift found for quasars at 5.7 |
| Databáze: | arXiv |
| Externí odkaz: |
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