Results 111 to 120 of about 35,402 (267)

Radio continuum and far-infrared emission from the galaxies in the Eridanus group

, 2005
The Eridanus galaxies follow the well-known radio-FIR correlation. Majority (70%) of these galaxies have their star formation rates below that of the Milky Way.
A. Omar, A. Omar, C. A. Heisler, C. N. A. Willmer, D. B. Sanders, G. Gavazzi, G. Helou, G. Neugebauer, H. Roussel, J. J. Condon, J. J. Condon, J. J. Condon, J. J. Condon, K. S. Dwarakanath, M. A. W. Verheijen, M. Harwit, M. S. Yun, M. Scodeggio, N. A. Reddy, N. Miller, P. C. Kruit van der, R. C. Kennicutt, S. Hameed, S. Veilleux, T. Elfhag, T. K. Menon   +25 more
core   +2 more sources

Discovery of two infrared supernovae: a new window on the SN search [PDF]

, 2002
We report the discovery of two supernovae (SN 1999gw and SN 2001db) obtained within the framework of an infrared monitoring campaign of Luminous Infrared Galaxies, aimed at detecting obscured supernovae.
Alard, Aretxaga, Baffa, Barbon, Barbon, Benetti, Calzetti, Cappellaro, Cresci, Dwek, F. Ghinassi, F. Mannucci, Fassia, Filippenko, G. Cresci, Genzel, Grossan, Hamuy, Hunt, L. Vanzi, Li, M. Della Valle, Maiolino, Maiolino, Maiolino, Marconi, Mattila, R. Maiolino, Richmond, Sanders, Sato, Schlegel, Schmidt, Soifer, van Buren, van Buren, Xu   +36 more
core   +2 more sources

Measuring the Interstellar Medium Content of Nearby, Luminous, Type 1 and Type 2 QSOs through CO and [C ii]

The Astrophysical Journal
We present observations of CO(1–0) and CO(2–1) lines from the Institut de radioastronomie millimétrique 30 m telescope toward 20 nearby, optically luminous type 2 quasars (QSO2s) and observations of the [C ii ] 158 μ m line from the Stratospheric ...
Yuanze Luo, A. O. Petric, R. M. J. Janssen, D. Fadda, N. Flagey, A. Omont, A. M. Jacob, K. Rowlands, K. Alatalo, N. Billot, T. Heckman, B. Husemann, D. Kakkad, M. Lacy, J. Marshall, R. Minchin, R. Minsley, N. Nesvadba, J. A. Otter, P. Patil, T. Urrutia   +20 more
doaj   +1 more source

Spitzer Power-law AGN Candidates in the Chandra Deep Field-North [PDF]

, 2007
We define a sample of 62 galaxies in the Chandra Deep Field-North whose Spitzer IRAC SEDs exhibit the characteristic power-law emission expected of luminous AGN. We study the multiwavelength properties of this sample, and compare the AGN selected in this
A. Alonso‐Herrero, Devriendt J. E. G., G. H. Rieke, Hasinger G., J. L. Donley, J. R. Rigby, Klaas U., Lacy M., Lawrence A., Maiolino R., Origlia L., P. G. Perez‐Gonzalez, Sturm E.   +12 more
core   +3 more sources

Morphology of luminous IRAS galaxies: Summary talk [PDF]

The author discusses the morphology of luminous Infrared Astronomy Satellite (IRAS) galaxies.
Becklin, E. E.
core   +1 more source

PEARLS: Discovery of Point-source Features within Galaxies in the North Ecliptic Pole Time Domain Field

The Astrophysical Journal
The first public 0.9–4.4 μ m NIRCam images of the North Ecliptic Pole Time Domain Field uncovered galaxies displaying point-source features in their cores as seen in the longer-wavelength filters. We visually identified a sample of 66 galaxies (∼1 galaxy
Rafael Ortiz III, Rogier A. Windhorst, Seth H. Cohen, Steven P. Willner, Rolf A. Jansen, Timothy Carleton, Patrick S. Kamieneski, Michael J. Rutkowski, Brent M. Smith, Jake Summers, Cheng Cheng, Dan Coe, Christopher J. Conselice, Jose M. Diego, Simon P. Driver, Jordan C. J. D’Silva, Brenda L. Frye, Hansung B. Gim, Norman A. Grogin, Heidi B. Hammel, Nimish P. Hathi, Benne W. Holwerda, Minhee Hyun, Myungshin Im, William C. Keel, Anton M. Koekemoer, Juno Li, Madeline A. Marshall, Tyler J. McCabe, Noah J. McLeod, Stefanie N. Milam, Rosalia O’Brien, Nor Pirzkal, Aaron S. G. Robotham, Russell E. Ryan Jr., Christopher N. A. Willmer, Haojing Yan, Min S. Yun, Adi Zitrin   +38 more
doaj   +1 more source

Modelling the Spectral Energy Distribution of Compact Luminous Infrared Galaxies: Constraints from High Frequency Radio Data [PDF]

, 2004
We have performed 23 GHz VLA observations of 7 compact, luminous infrared galaxies, selected to have evidence of starburst activity. New and published multi-frequency data are combined to obtain the spectral energy distributions of all 7 galaxies from ...
A. Bressan, A. Franceschini, Barger, Becker, Berta, Beswick, Bohlin, Bressan, Cavaliere, Clemens, Condon, Condon, Condon, Condon, Downes, Downes, Dunne, Efstathiou, Elbaz, Farrah, Ferrarese, Franceschini, Franceschini, G. L. Granato, Galliano, Granato, Granato, Granato, Haas, Helou, Högbom, Jarrett, Kennicutt, L. Silva, Lancon, Lonsdale, M. Clemens, Maiolino, Maiolino, Mayya, Miles, Miles, Mirabel, Mulchaey, Mundell, Nikolic, O. R. Prouton, Panuzzo, Pier, Roche, Sanders, Sanders, Sanders, Scoville, Silva, Smail, Smail, Smith, Soifer, Soifer, Soifer, Soifer, Sopp, Spinoglio, Veilleux, Veilleux, Wunderlich   +66 more
core   +1 more source

Outflows in Infrared-Luminous Starbursts at z < 0.5. II. Analysis and Discussion

, 2005
We have performed an absorption-line survey of outflowing gas in 78 starburst-dominated, infrared-luminous galaxies. This is the largest study of superwinds at z < 3. Superwinds are found in almost all infrared-luminous galaxies, and changes in detection
Rupke, David S., Sanders, D. B., Veilleux, Sylvain   +2 more
core   +1 more source

SMILES Initial Data Release: Unveiling the Obscured Universe with MIRI Multiband Imaging

The Astrophysical Journal
The James Webb Space Telescope is revolutionizing our view of the Universe through unprecedented sensitivity and resolution in the infrared, with some of the largest gains realized at its longest wavelengths.
Stacey Alberts, Jianwei Lyu, Irene Shivaei, George H. Rieke, Pablo G. Pérez-González, Nina Bonaventura, Yongda Zhu, Jakob M. Helton, Zhiyuan Ji, Jane Morrison, Brant E. Robertson, Meredith A. Stone, Yang Sun, Christina C. Williams, Christopher N. A. Willmer   +14 more
doaj   +1 more source

High Redshift HCN Emission: Dense Star-Forming Molecular Gas in IRAS F10214+4724

, 2004
Hydrogen cyanide emission in the J=1-0 transition has been detected at redshift z=2.2858 in IRAS F10214+4724 using the Green Bank Telescope . This is the second detection of HCN emission at high redshift.
Bout, P. A. Vanden, Maddalena, R. J., Solomon, P. M.   +2 more
core   +1 more source