The James Webb Space Telescope Feed

Harvard ADS: GA-NIFS & EIGER: A merging quasar host at z=7 with an overmassive black hole

Harvard ADS: GA-NIFS & EIGER: A merging quasar host at z=7 with an overmassive black hole

EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at z >= 6

EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at z >= 6

EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at z >= 6

EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at z >= 6

EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at z >= 6

Harvard ADS: EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at z\gtrsim6

Arxiv: Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys Published: 6/8/2023 9:00:00 PM Updated: 2/1/2024 12:58:14 PM

Arxiv: Little Red Dots: an abundant population of faint AGN at z\sim5 revealed by the EIGER and FRESCO JWST surveys Published: 6/8/2023 9:00:00 PM Updated: 1/23/2024 11:59:22 AM

EIGER V. Characterizing the Host Galaxies of Luminous Quasars at z\gtrsim6

Searching for hidden accreting supermassive black holes in the first JWST-EIGER field

EIGER | background of J0100+2802 quasar

EIGER IV: The cool 10^4K circumgalactic environment of high-z galaxies reveals remarkably efficient IGM enrichment

Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys

Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys

Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys

Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys

Little Red Dots: an abundant population of faint AGN at z\sim5 revealed by the EIGER and FRESCO JWST surveys Published: 6/8/2023 9:00:00 PM Updated: 6/8/2023 9:00:00 PM

EIGER III. JWST/NIRCam observations of the ultra-luminous high-redshift quasar J0100+2802

EIGER III. JWST/NIRCam observations of the ultra-luminous high-redshift quasar J0100+2802

EIGER III. JWST/NIRCam observations of the ultra-luminous high-redshift quasar J0100+2802

EIGER III. JWST/NIRCam observations of the ultra-luminous high-redshift quasar J0100+2802 Published: 11/29/2022 4:48:57 PM Updated: 5/18/2023 4:41:57 PM

EIGER | JWST NIRCam observations of the eld of the quasar J0100+2802. The background is the coadded pseudo-color image in the F115W (blue), F200W (green) and F356W (red) bands

EIGER I. a large sample of [OIII]-emitting galaxies at 5.3 < z < 6.9 and direct evidence for local reionization by galaxies

EIGER | highlighting isolated systems. These sources are representative for the fainter objects in our sample, which are typically small, compact systems with high EWs

EIGER | Overview of the information that we can measure for two example [OIII] emitters identified in the JWST data

EIGER | highlighting isolated systems. These sources are representative for the fainter objects in our sample, which are typically small, compact systems with high EWs

EIGER | Overview of the information that we can measure for two example [OIII] emitters identified in the JWST data

EIGER | NIRCam F115W+F200W+F356W

EIGER

EIGER | Example false-color F115W/F200W/F356W stamps of regions where we detect multiple [OIII] emitting systems within 2'', highlighting the diversity of these groups

EIGER | Example false-color F115W/F200W/F356W stamps of regions where we detect multiple [OIII] emitting systems within 2'', highlighting the diversity of these groups

EIGER | Example false-color F115W/F200W/F356W stamps of regions where we detect multiple [OIII] emitting systems within 2'', highlighting the diversity of these groups

EIGER II. first spectroscopic characterisation of the young stars and ionised gas associated with strong Hβ and [OIII] line-emission in galaxies at z=5-7 with JWST Published: 11/15/2022 6:00:50 PM Updated: 3/17/2023 10:50:56 PM

EIGER | A pseudo-color JWST/NIRCam image in the field of the z=6.3 J0100+2802 quasar field. The three broadband images in F115W (blue), F200W (green), and F356W (red) are composite. The quasar is the red "star" at the center

EIGER | A pseudo-color JWST/NIRCam image in the field of the z=6.3 J0100+2802 quasar field. The three broadband images in F115W (blue), F200W (green), and F356W (red) are composite. The quasar is the red "star" at the center (high resolution)

EIGER | A compilation of pseudo-color stamp images of example [OIII]-emitters (3 arcsec on a side). They often look relatively "red" due to the strong [OIII] fluxes sampled in the F356W band images

EIGER | Examples of stacked 2D spectra of [O iii]-emitters, shown in order of redshift from top to bottom. The [OIII]?5008 line is marked by ticks. Taken from EIGER Paper I (Kashino et al.)

EIGER III. JWST/NIRCam observations of the ultra-luminous high-redshift quasar J0100+2802

EIGER II. first spectroscopic characterisation of the young stars and ionised gas associated with strong H$β$ and [OIII] line-emission in galaxies at z=5-7 with JWST