Andreea Petric

JWST’s PEARLS: A JWST/NIRCam View of ALMA Sources

Are JWST/NIRCam Color Gradients in the Lensed z = 2.3 Dusty Star-forming Galaxy El Anzuelo Due to Central Dust Attenuation or Inside-out Galaxy Growth?

JWST’s PEARLS: Dust Attenuation and Gravitational Lensing in the Backlit-galaxy System VV 191

JWST PEARLS. Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results

Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past

Obscured active galactic nuclei and the need for optical to near‐infrared, massively multiplexed, spectroscopic facilities

SIGNALS: I. Survey description

Mapping the Inner Structure of Quasars with Time-Domain Spectroscopy

High Redshift Obscured Quasars and the Need for Optical to NIR, Massively Multiplexed, Spectroscopic Facilities

Mapping the Inner Structure of Quasars with Time-Domain Spectroscopy

Star formation in quasar hosts and the origin of radio emission in radio-quiet quasars

EXTENDED [C II] EMISSION IN LOCAL LUMINOUS INFRARED GALAXIES

EXPLAINING THE [C II]157.7 μm DEFICIT IN LUMINOUS INFRARED GALAXIES—FIRST RESULTS FROM A<i>HERSCHEL</i>/PACS STUDY OF THE GOALS SAMPLE

MID-INFRARED PROPERTIES OF NEARBY LUMINOUS INFRARED GALAXIES. I. <i>SPITZER</i> INFRARED SPECTROGRAPH SPECTRA FOR THE GOALS SAMPLE

MID-INFRARED ATOMIC FINE-STRUCTURE EMISSION-LINE SPECTRA OF LUMINOUS INFRARED GALAXIES:<i>SPITZER</i>/IRS SPECTRA OF THE GOALS SAMPLE

The Spitzer Extragalactic Representative Volume Survey (SERVS): Survey Definition and Goals*

<i>SPITZER</i>OBSERVATIONS OF YOUNG RED QUASARS