Results 121 to 130 of about 200,741 (275)

High-redshift, Restframe Far-infrared Selected Galaxies [PDF]

arXiv, 2006
I discuss our current understanding of the properties and nature of high redshift, far-infrared luminous galaxies selected through their observed-frame submillimeter emission.
arxiv  

The X-ray emission of local luminous infrared galaxies [PDF]

Astronomy & Astrophysics, 2011
We study the X-ray emission of a representative sample of 27 local luminous infrared galaxies (LIRGs). The median IR luminosity of our sample is log L_IR/L_sun = 11.2, thus the low-luminosity end of the LIRG class is well represented. We used new XMM-Newton data as well as Chandra and XMM-Newton archive data. The soft X-ray (0.5-2 keV) emission of most
Rieke, George, Esquej, Pilar, Ward, Martin, Longinotti, Anna, Jimenez-Bailon, Elena, Colina, Luis, Santos-Lleo, Maria, Alonso-Herrero, Almudena, Pereira-Santaella, Miguel   +8 more
openaire   +3 more sources

Spitzer observations of extended Lyman-alpha Clouds in the SSA22 field

, 2008
We present the results of a Spitzer IRAC and MIPS 24 micron study of extended Lyman-alpha clouds (or Lyman-alpha Blobs, LABs) within the SSA22 filamentary structure at z = 3.09.
Alonso-Herrero, Basu-Zych, Bauer, Chapman, Chapman, Chapman, Cirasuolo, Coil, Colbert, Dey, E. Egami, Egami, Fazio, Francis, Geach, Geach, Giavalisco, Hayashino, J.-S. Huang, Keel, Kohno, Lacy, M. Gonzalez, M. L. N Ashby, Matsuda, Matsuda, Matsuda, Palunas, Patton, Prescott, Reuland, Rieke, Rudnick, Saito, Saito, Schuster, Shapley, Smith, Steidel, Steidel, Steidel, Stern, T. Hayashimo, T. M. A. Webb, T. Yamada, Taniguchi, Taniguchi, Webb, Werner, Y. Matsuda   +49 more
core   +1 more source

THE FIRST HYPER-LUMINOUS INFRARED GALAXY DISCOVERED BYWISE [PDF]

The Astrophysical Journal, 2012
We report the discovery by the Wide-field Infrared Survey Explorer of the z = 2.452 source WISE J181417.29+341224.9, the first hyperluminous source found in the WISE survey. WISE 1814+3412 is also the prototype for an all-sky sample of ~1000 extremely luminous "W1W2-dropouts" (sources faint or undetected by WISE at 3.4 and 4.6 microns and well detected
Eisenhardt, PRM, Wu, J, Assef, R, Stern, D, Tsai, C-W, Cutri, R, Gelino, C, Griffith, RL, Grillmair, CJ, Jarrett, T, Masci, FJ, Yan, L, Benford, D, Blain, A, Bridge, C, Sayers, J, Condon, JJ, Lonsdale, CJ, Mason, BS, Cushing, MC, Evans II NJ, Petty, S, Wright, EL, Stanford, SA   +23 more
openaire   +6 more sources

Spatially Resolved [FeII] 1.64 \mu m Emission in NGC 5135. Clues for Understanding the Origin of the Hard X-rays in Luminous Infrared Galaxies [PDF]

, 2012
Spatially resolved near-IR and X-ray imaging of the central region of the Luminous Infrared Galaxy NGC 5135 is presented. The kinematical signatures of strong outflows are detected in the [FeII]1.64 \mu m emission line in a compact region at 0.9 kpc from
A. Alonso-Herrero, A. G. Bedregal, Alonso-Herrero, Alonso-Herrero, Alonso-Herrero, Arnaud, Ballo, Bedregal, Bondi, Genzel, Gonzalez-Delgado, Grimes, Iwasawa, L. Colina, Lehmer, Levenson, M. Pereira-Santaella, McDowell, Mitsuishi, Mouri, Nussbaumer, Piqueras, Robitaille, S. Arribas, Strateva, Strickland, Strickland, Strickland, Strickland, Weaver, Wilms, Zezas, Zezas   +32 more
core   +2 more sources

GOALS-JWST: Gas Dynamics and Excitation in NGC 7469 Revealed by NIRSpec

The Astrophysical Journal
We present new JWST NIRSpec integral field spectroscopy (IFS) data for the luminous infrared galaxy NGC 7469, a nearby (70.6 Mpc) active galaxy with a Seyfert 1.5 nucleus that drives a highly ionized gas outflow and a prominent nuclear star-forming ring.
Marina Bianchin, Vivian U, Yiqing Song, Thomas S.-Y. Lai, Raymond P. Remigio, Loreto Barcos-Muñoz, Tanio Díaz-Santos, Lee Armus, Hanae Inami, Kirsten L. Larson, Aaron S. Evans, Torsten Böker, Justin A. Kader, Sean T. Linden, Vassilis Charmandaris, Matthew A. Malkan, Jeff Rich, Thomas Bohn, Anne M. Medling, Sabrina Stierwalt, Joseph M. Mazzarella, David R. Law, George C. Privon, Susanne Aalto, Philip Appleton, Michael J. I. Brown, Victorine A. Buiten, Luke Finnerty, Christopher C. Hayward, Justin Howell, Kazushi Iwasawa, Francisca Kemper, Jason Marshall, Jed McKinney, Francisco Müller-Sánchez, Eric J. Murphy, Paul P. van der Werf, David B. Sanders, Jason Surace   +38 more
doaj   +1 more source

EXTENDED [C II] EMISSION IN LOCAL LUMINOUS INFRARED GALAXIES [PDF]

The Astrophysical Journal, 2014
Accepted for publication in ApJ Letters.
Hanae Inami, Joseph M. Mazzarella, C. K. Xu, Jason Surace, Eric J. Murphy, Tanio Díaz-Santos, P. van der Werf, S. Malhotra, Lee Armus, Vassilis Charmandaris, N. Y. Lu, D. B. Sanders, Sylvain Veilleux, Andreea Petric, D. Elbaz, P. N. Appleton, S. Haan, Sabrina Stierwalt, Rowin Meijerink, Justin Howell, G. Stacey, Aaron S. Evans, Aaron S. Evans, Georgios E. Magdis   +23 more
openaire   +10 more sources

A population of z> 2 far-infrared Herschel-spire-selected starbursts [PDF]

, 2012
We present spectroscopic observations for a sample of 36 Herschel-SPIRE 250-500um selected galaxies (HSGs) at 210% of the estimated total star formation rate density (SFRD) of the Universe from optical surveys.
A. Conley, A. Cooray, Alexander, B. Magnelli, Blain, Bridge, C. Bridge, C. J. Conselice, C. M. Casey, Caputi, Cardamone, Chapman, Chapman, Chapman, Chapman, Chary, Conley, Coppin, Cox, D. B. Sanders, D. Burgarella, D. Farrah, D. L. Clements, D. Lutz, D. Rigopoulou, Daddi, Dale, Davé, Douglas Scott, Draine, E. Chapin, E. Hatziminaoglou, E. le Floc'h, Eales, F. Pozzi, G. Magdis, Hainline, Hinshaw, Hopkins, I. G. Roseboom, I. Valtchanov, Ilbert, Ivison, J. Bock, J. D. Vieira, J. Wardlow, Kennicutt, Kovács, L. Riguccini, Le Floc'h, Le Floc'h, M. Béthermin, M. J. Page, M. Viero, Madau, Madau, Menéndez-Delmestre, Mobasher, N. Seymour, Pope, R. J. Ivison, S. Berta, S. C. Chapman, S. J. Oliver, Sanders, Scarlata, Shapley, Siana, Siana, Smail, Smolčić, Strazzullo, Swinbank, Tacconi, Wang, Wang, Wang, Wardlow   +77 more
core   +5 more sources

Submillimetre surveys: The prospects for Herschel [PDF]

, 2009
Using the observed submillimetre source counts, from 250-1200 microns (including the most recent 250, 350 and 500 micron counts from BLAST), we present a model capable of reproducing these results, which is used as a basis to make predictions for upcoming surveys with the SPIRE instrument aboard the Herschel Space Observatory.
arxiv   +1 more source

Unveiling the Progenitors of GRBs through Observations of their Host Galaxies

, 2002
I discuss the possibility of differentiating between popular models for gamma-ray bursts by using multiwavelength observations to constrain the characteristics of their host galaxies, in particular the age of the stellar populations.Comment: 3 pages ...
Chary, Ranga-Ram
core   +2 more sources