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JWST/MIRI Simulated Imaging: Insights into Obscured Star-Formation and AGN for Distant Galaxies in Deep Surveys
Guang Yang, Casey Papovich, Micaela B. Bagley +13
The JWST MIRI instrument will revolutionize extragalactic astronomy with unprecedented sensitivity and angular resolution in mid-IR. Here, we assess the potential of MIRI photometr…
Transformative Planetary Science with the US ELT Program
Michael H. Wong, Karen J. Meech, Mark Dickinson +4
The proposed US Extremely Large Telescope (ELT) Program would secure national open access to at least 25% of the observing time on the Thirty Meter Telescope in the north and the G…
Texas Spectroscopic Search for Ly Emission at the End of Reionization III. the Ly Equivalent-width Distribution and Ionized Structures at
Intae Jung, Steven L. Finkelstein, Mark Dickinson +11
Ly emission from galaxies can be utilized to characterize the ionization state in the intergalactic medium (IGM). We report our search for Ly emission at using a compre…
GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5
L. Zhou, D. Elbaz, M. Franco +30
In this paper we study the properties of the six optically dark galaxies detected in the 69 arcmin^2 GOODS-ALMA 1.1mm continuum survey. While none of them are listed in the deepest…
CO emission in distant galaxies on and above the main sequence
Francesco Valentino, Emanuele Daddi, Annagrazia Puglisi +17
We present the detection of multiple CO line transitions with ALMA in a few tens of infrared-selected galaxies on and above the main sequence at z=1.1-1.7. We reliably detected the…
Selection of massive evolved galaxies at in the CANDELS fields
Abtin Shahidi, Bahram Mobasher, Hooshang Nayyeri +14
Using the CANDELS photometric catalogs for the HST/ACS and WFC3, we identified massive evolved galaxies at , employing three different selection methods. We find the c…
COLDz: A High Space Density of Massive Dusty Starburst Galaxies ~1 Billion Years after the Big Bang
Dominik A. Riechers, Jacqueline A. Hodge, Riccardo Pavesi +15
We report the detection of CO(=21) emission from three massive dusty starburst galaxies at 5 through molecular line scans in the NSF's Karl G. Jansky Very Large Array…
GOODS-ALMA: The slow downfall of star-formation in = 2-3 massive galaxies
M. Franco, D. Elbaz, L. Zhou +34
We investigate the properties of a sample of 35 galaxies, detected with ALMA at 1.1 mm in the GOODS-ALMA field (area of 69 arcmin, resolution = 0.60", RMS 0.18 mJy bea…
GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies
M. Franco, D. Elbaz, L. Zhou +33
In this paper, we extend the source detection in the GOODS-ALMA field (69 arcmin, rms sensitivity 0.18 mJy.beam), to deeper levels than presented in Franco…
The Typical Massive Quiescent Galaxy at z3 is a Post-starburst
C. D'Eugenio, E. Daddi, R. Gobat +10
We have obtained spectroscopic confirmation with Hubble Space Telescope WFC3/G141 of a first sizeable sample of nine quiescent galaxies at 2.4<z<3.3. Their average near-UV/optical…
Measuring the Heating and Cooling of the Interstellar Medium at High redshift: PAH and [C II] Observations of the Same Star Forming Galaxies at z~2
Jed McKinney, Alexandra Pope, Lee Armus +4
Star formation depends critically on cooling mechanisms in the interstellar medium (ISM); however, thermal properties of gas in galaxies at the peak epoch of star formation (z ~ 2)…