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Start Over Author "Sanders D. B." Publisher american astronomical society
248 results on '"Sanders D. B."'

1. The Farmer: A Reproducible Profile-fitting Photometry Package for Deep Galaxy Surveys

Author

Weaver, J. R., primary, Zalesky, L., additional, Kokorev, V., additional, McPartland, C. J. R., additional, Chartab, N., additional, Gould, K. M. L., additional, Shuntov, M., additional, Davidzon, I., additional, Faisst, A., additional, Stickley, N., additional, Capak, P. L., additional, Toft, S., additional, Masters, D., additional, Mobasher, B., additional, Sanders, D. B., additional, Kauffmann, O. B., additional, McCracken, H. J., additional, Ilbert, O., additional, Brammer, G., additional, and Moneti, A., additional

Published
2023
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2. Characterizing Compact 15–33 GHz Radio Continuum Sources in Local U/LIRGs

Author

Song, Y., primary, Linden, S. T., additional, Evans, A. S., additional, Barcos-Muñoz, L., additional, Murphy, E. J., additional, Momjian, E., additional, Díaz-Santos, T., additional, Larson, K. L., additional, Privon, G. C., additional, Huang, X., additional, Armus, L., additional, Mazzarella, J. M., additional, U, V., additional, Inami, H., additional, Charmandaris, V., additional, Ricci, C., additional, Emig, K. L., additional, McKinney, J., additional, Yoon, I., additional, Kunneriath, D., additional, Lai, T. S.-Y., additional, Rodas-Quito, E. E., additional, Saravia, A., additional, Gao, T., additional, Meynardie, W., additional, and Sanders, D. B., additional

Published
2022
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3. COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs

Author

Weaver, J. R., primary, Kauffmann, O. B., additional, Ilbert, O., additional, McCracken, H. J., additional, Moneti, A., additional, Toft, S., additional, Brammer, G., additional, Shuntov, M., additional, Davidzon, I., additional, Hsieh, B. C., additional, Laigle, C., additional, Anastasiou, A., additional, Jespersen, C. K., additional, Vinther, J., additional, Capak, P., additional, Casey, C. M., additional, McPartland, C. J. R., additional, Milvang-Jensen, B., additional, Mobasher, B., additional, Sanders, D. B., additional, Zalesky, L., additional, Arnouts, S., additional, Aussel, H., additional, Dunlop, J. S., additional, Faisst, A., additional, Franx, M., additional, Furtak, L. J., additional, Fynbo, J. P. U., additional, Gould, K. M. L., additional, Greve, T. R., additional, Gwyn, S., additional, Kartaltepe, J. S., additional, Kashino, D., additional, Koekemoer, A. M., additional, Kokorev, V., additional, Le Fèvre, O., additional, Lilly, S., additional, Masters, D., additional, Magdis, G., additional, Mehta, V., additional, Peng, Y., additional, Riechers, D. A., additional, Salvato, M., additional, Sawicki, M., additional, Scarlata, C., additional, Scoville, N., additional, Shirley, R., additional, Silverman, J. D., additional, Sneppen, A., additional, Smolc̆ić, V., additional, Steinhardt, C., additional, Stern, D., additional, Tanaka, M., additional, Taniguchi, Y., additional, Teplitz, H. I., additional, Vaccari, M., additional, Wang, W.-H., additional, and Zamorani, G., additional

Published
2022
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4. Euclid Preparation. XIV. The Complete Calibration of the Color–Redshift Relation (C3R2) Survey: Data Release 3

Author

Stanford, S. A., primary, Masters, D., additional, Darvish, B., additional, Stern, D., additional, Cohen, J. G., additional, Capak, P., additional, Hernitschek, N., additional, Davidzon, I., additional, Rhodes, J., additional, Sanders, D. B., additional, Mobasher, B., additional, Castander, F. J., additional, Paltani, S., additional, Aghanim, N., additional, Amara, A., additional, Auricchio, N., additional, Balestra, A., additional, Bender, R., additional, Bodendorf, C., additional, Bonino, D., additional, Branchini, E., additional, Brinchmann, J., additional, Capobianco, V., additional, Carbone, C., additional, Carretero, J., additional, Casas, R., additional, Castellano, M., additional, Cavuoti, S., additional, Cimatti, A., additional, Cledassou, R., additional, Conselice, C. J., additional, Corcione, L., additional, Costille, A., additional, Cropper, M., additional, Degaudenzi, H., additional, Douspis, M., additional, Dubath, F., additional, Dusini, S., additional, Fosalba, P., additional, Frailis, M., additional, Franceschi, E., additional, Franzetti, P., additional, Fumana, M., additional, Garilli, B., additional, Giocoli, C., additional, Grupp, F., additional, Haugan, S. V. H., additional, Hoekstra, H., additional, Holmes, W., additional, Hormuth, F., additional, Hudelot, P., additional, Jahnke, K., additional, Kiessling, A., additional, Kilbinger, M., additional, Kitching, T., additional, Kubik, B., additional, Kümmel, M., additional, Kunz, M., additional, Kurki-Suonio, H., additional, Laureijs, R., additional, Ligori, S., additional, Lilje, P. B., additional, Lloro, I., additional, Maiorano, E., additional, Marggraf, O., additional, Markovic, K., additional, Massey, R., additional, Meneghetti, M., additional, Meylan, G., additional, Moscardini, L., additional, Niemi, S. M., additional, Padilla, C., additional, Pasian, F., additional, Pedersen, K., additional, Pettorino, V., additional, Pires, S., additional, Poncet, M., additional, Popa, L., additional, Pozzetti, L., additional, Raison, F., additional, Roncarelli, M., additional, Rossetti, E., additional, Saglia, R., additional, Scaramella, R., additional, Schneider, P., additional, Secroun, A., additional, Seidel, G., additional, Serrano, S., additional, Sirignano, C., additional, Sirri, G., additional, Taylor, A. N., additional, Teplitz, H. I., additional, Tereno, I., additional, Toledo-Moreo, R., additional, Valentijn, E. A., additional, Valenziano, L., additional, Verdoes Kleijn, G. A., additional, Wang, Y., additional, Zamorani, G., additional, Zoubian, J., additional, Brescia, M., additional, Congedo, G., additional, Conversi, L., additional, Copin, Y., additional, Kermiche, S., additional, Kohley, R., additional, Medinaceli, E., additional, Mei, S., additional, Moresco, M., additional, Morin, B., additional, Munari, E., additional, Polenta, G., additional, Sureau, F., additional, Tallada Crespí, P., additional, Vassallo, T., additional, Zacchei, A., additional, Andreon, S., additional, Aussel, H., additional, Baccigalupi, C., additional, Balaguera-Antolínez, A., additional, Baldi, M., additional, Bardelli, S., additional, Biviano, A., additional, Borsato, E., additional, Bozzo, E., additional, Burigana, C., additional, Cabanac, R., additional, Camera, S., additional, Cappi, A., additional, Carvalho, C. S., additional, Casas, S., additional, Castignani, G., additional, Colodro-Conde, C., additional, Coupon, J., additional, Courtois, H. M., additional, Cuby, J.-G., additional, Da Silva, A., additional, de la Torre, S., additional, Di Ferdinando, D., additional, Duncan, C. A. J., additional, Dupac, X., additional, Fabricius, M., additional, Farina, M., additional, Farrens, S., additional, Ferreira, P. G., additional, Finelli, F., additional, Flose-Reimberg, P., additional, Fotopoulou, S., additional, Galeotta, S., additional, Ganga, K., additional, Gillard, W., additional, Gozaliasl, G., additional, Graciá-Carpio, J., additional, Keihanen, E., additional, Kirkpatrick, C. C., additional, Lindholm, V., additional, Mainetti, G., additional, Maino, D., additional, Martinet, N., additional, Marulli, F., additional, Maturi, M., additional, Maurogordato, S., additional, Metcalf, R. B., additional, Nakajima, R., additional, Neissner, C., additional, Nightingale, J. W., additional, Nucita, A. A., additional, Patrizii, L., additional, Potter, D., additional, Renzi, A., additional, Riccio, G., additional, Romelli, E., additional, Sánchez, A. G., additional, Sapone, D., additional, Schirmer, M., additional, Schultheis, M., additional, Scottez, V., additional, Stanco, L., additional, Tenti, M., additional, Teyssier, R., additional, Torradeflot, F., additional, Valiviita, J., additional, Viel, M., additional, Whittaker, L., additional, and Zucca, E., additional

Published
2021
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5. Star-forming Clumps in Local Luminous Infrared Galaxies

Author

Larson, K. L., primary, Díaz-Santos, T., additional, Armus, L., additional, Privon, G. C., additional, Linden, S. T., additional, Evans, A. S., additional, Howell, J., additional, Charmandaris, V., additional, U, V., additional, Sanders, D. B., additional, Stierwalt, S., additional, Barcos-Muñoz, L., additional, Rich, J., additional, Medling, A., additional, Cook, D., additional, Oklopĉić, A., additional, Murphy, E. J., additional, and Bonfini, P., additional

Published
2020
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6. A 33 GHz Survey of Local Major Mergers: Estimating the Sizes of the Energetically Dominant Regions from High-resolution Measurements of the Radio Continuum

Author

Barcos-Muñoz, L., Leroy, A. K., Evans, A. S., Condon, J., Privon, G. C., Thompson, T. A., Armus, L., Díaz-Santos, T., Mazzarella, J. M., Meier, D. S., Momjian, E., Murphy, E. J., Ott, J., Sanders, D. B., Schinnerer, E., Stierwalt, S., Surace, J. A., and Walter, F.

Subjects
Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

We present Very Large Array observations of the 33 GHz radio continuum emission from 22 local ultraluminous and luminous infrared (IR) galaxies (U/LIRGs). These observations have spatial (angular) resolutions of 30–720 pc (0.”07–0.”67) in a part of the spectrum that is likely to be optically thin. This allows us to estimate the size of the energetically dominant regions. We find half-light radii from 30 pc to 1.7 kpc. The 33 GHz flux density correlates well with the IR emission, and we take these sizes as indicative of the size of the region that produces most of the energy. Combining our 33 GHz sizes with unresolved measurements, we estimate the IR luminosity and star formation rate per area and the molecular gas surface and volume densities. These quantities span a wide range (4 dex) and include some of the highest values measured for any galaxy (e.g., Σ^(33 GHz)_(SFR) ⩽ 10^(4.1) M⊙ yr^(-1) kpc^(-2)). At least 13 sources appear Compton thick (N^(33 GHz)_H ⩾ 10^(24) cm(-2)). Consistent with previous work, contrasting these data with observations of normal disk galaxies suggests a nonlinear and likely multivalued relation between star formation rate and molecular gas surface density, though this result depends on the adopted CO-to-H2 conversion factor and the assumption that our 33 GHz sizes apply to the gas. Eleven sources appear to exceed the luminosity surface density predicted for starbursts supported by radiation pressure and supernova feedback; however, we note the need for more detailed observations of the inner disk structure. U/LIRGs with higher surface brightness exhibit stronger [C II] 158 μm deficits, consistent with the suggestion that high energy densities drive this phenomenon.

Published
2017

7. First Data Release of the COSMOS Ly α Mapping and Tomography Observations: 3D Ly α Forest Tomography at 2.05 < z < 2.55

Author

Lee, Khee-Gan, primary, Krolewski, Alex, additional, White, Martin, additional, Schlegel, David, additional, Nugent, Peter E., additional, Hennawi, Joseph F., additional, Müller, Thomas, additional, Pan, Richard, additional, Prochaska, J. Xavier, additional, Font-Ribera, Andreu, additional, Suzuki, Nao, additional, Glazebrook, Karl, additional, Kacprzak, Glenn G., additional, Kartaltepe, Jeyhan S., additional, Koekemoer, Anton M., additional, Le Fèvre, Olivier, additional, Lemaux, Brian C., additional, Maier, Christian, additional, Nanayakkara, Themiya, additional, Rich, R. Michael, additional, Sanders, D. B., additional, Salvato, Mara, additional, Tasca, Lidia, additional, and Tran, Kim-Vy H., additional

Published
2018
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8. Erratum: “A 33 GHz Survey of Local Major Mergers: Estimating the Sizes of the Energetically Dominant Regions from High-resolution Measurements of the Radio Continuum” (2017, ApJ, 843, 117)

Author

Barcos-Muñoz, L., primary, Leroy, A. K., additional, Evans, A. S., additional, Condon, J., additional, Privon, G. C., additional, Thompson, T. A., additional, Armus, L., additional, Díaz-Santos, T., additional, Mazzarella, J. M., additional, Meier, D. S., additional, Momjian, E., additional, Murphy, E. J., additional, Ott, J., additional, Sanders, D. B., additional, Schinnerer, E., additional, Stierwalt, S., additional, Surace, J. A., additional, and Walter, F., additional

Published
2017
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9. AHerschel/PACS Far-infrared Line Emission Survey of Local Luminous Infrared Galaxies

Author

Díaz-Santos, T., primary, Armus, L., additional, Charmandaris, V., additional, Lu, N., additional, Stierwalt, S., additional, Stacey, G., additional, Malhotra, S., additional, Werf, P. P. van der, additional, Howell, J. H., additional, Privon, G. C., additional, Mazzarella, J. M., additional, Goldsmith, P. F., additional, Murphy, E. J., additional, Barcos-Muñoz, L., additional, Linden, S. T., additional, Inami, H., additional, Larson, K. L., additional, Evans, A. S., additional, Appleton, P., additional, Iwasawa, K., additional, Lord, S., additional, Sanders, D. B., additional, and Surace, J. A., additional

Published
2017
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10. A 33 GHz Survey of Local Major Mergers: Estimating the Sizes of the Energetically Dominant Regions from High-resolution Measurements of the Radio Continuum

Author

Barcos-Muñoz, L., primary, Leroy, A. K., additional, Evans, A. S., additional, Condon, J., additional, Privon, G. C., additional, Thompson, T. A., additional, Armus, L., additional, Díaz-Santos, T., additional, Mazzarella, J. M., additional, Meier, D. S., additional, Momjian, E., additional, Murphy, E. J., additional, Ott, J., additional, Sanders, D. B., additional, Schinnerer, E., additional, Stierwalt, S., additional, Surace, J. A., additional, and Walter, F., additional

Published
2017
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12. The Great Observatories All-Sky LIRG Survey: Herschel Image Atlas and Aperture Photometry

Author

Chu, Jason K., primary, Sanders, D. B., additional, Larson, K. L., additional, Mazzarella, J. M., additional, Howell, J. H., additional, Díaz-Santos, T., additional, Xu, K. C., additional, Paladini, R., additional, Schulz, B., additional, Shupe, D., additional, Appleton, P., additional, Armus, L., additional, Billot, N., additional, Chan, B. H. P., additional, Evans, A. S., additional, Fadda, D., additional, Frayer, D. T., additional, Haan, S., additional, Ishida, C. M., additional, Iwasawa, K., additional, Kim, D.-C., additional, Lord, S., additional, Murphy, E., additional, Petric, A., additional, Privon, G. C., additional, Surace, J. A., additional, and Treister, E., additional

Published
2017
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13. The Bright and Dark Sides of High-redshift Starburst Galaxies from Herschel and Subaru Observations

Author

Puglisi, A., primary, Daddi, E., additional, Renzini, A., additional, Rodighiero, G., additional, Silverman, J. D., additional, Kashino, D., additional, Rodríguez-Muñoz, L., additional, Mancini, C., additional, Mainieri, V., additional, Man, A., additional, Franceschini, A., additional, Valentino, F., additional, Calabrò, A., additional, Jin, S., additional, Darvish, B., additional, Maier, C., additional, Kartaltepe, J. S., additional, and Sanders, D. B., additional

Published
2017
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14. Optical Identification ofInfrared Space ObservatoryFar-Infrared Sources in the Lockman Hole Using a Deep Very Large Array 1.4 GHz Continuum Survey

Author

Yun, Min S., Sanders, D. B., Oyabu, Sinki, Murayama, T., Kawara, K., Taniguchi, Y., Veilleux, S., Okuda, H., Matsuhara, Hideo, Cowie, L. L., Sato, Y., Wakamatsu, K., and Sofue, Y.

Subjects
Physics, Luminous infrared galaxy, education.field_of_study, Active galactic nucleus, Star formation, Astrophysics::High Energy Astrophysical Phenomena, Population, Astronomy and Astrophysics, Quasar, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Galaxy, Luminosity, Space and Planetary Science, ROSAT, education, Astrophysics::Galaxy Astrophysics
Abstract

著者人数：13名, Accepted: 2005-07-02, 資料番号: SA1001299000

Published
2005
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15. ALMA Observations of Warm Dense Gas in NGC 1614 — Breaking of Star Formation Law in the Central kpc

Author

Xu, C. K., Cao, C., Lu, N., Gao, Y., Diaz-Santos, T., Herrero-Illana, R., Meijerink, R., Privon, G., Zhao, Y. -H., Evans, A. S., K��nig, S., Mazzarella, J. M., Aalto, S., Appleton, P., Armus, L., Charmandaris, V., Chu, J., Haan, S., Inami, H., Murphy, E. J., Sanders, D. B., Schulz, B., and van der Werf, P.

Subjects
Astrophysics of Galaxies (astro-ph.GA), FOS: Physical sciences, Astrophysics - Astrophysics of Galaxies
Abstract

We present ALMA Cycle-0 observations of the CO (6-5) line emission and of the 435um dust continuum emission in the central kpc of NGC 1614, a local luminous infrared galaxy (LIRG) at a distance of 67.8 Mpc (1 arcsec = 329 pc). The CO emission is well resolved by the ALMA beam (0".26 x 0".20) into a circum-nuclear ring, with an integrated flux of f_{CO(6-5)} = 898 (+-153) Jy km/s, which is 63(+-12)% of the total CO(6-5) flux measured by Herschel. The molecular ring, located between 100pc < r < 350pc from the nucleus, looks clumpy and includes seven unresolved (or marginally resolved) knots with median velocity dispersion of 40 km/s. These knots are associated with strong star formation regions with \Sigma_{SFR} 100 M_\sun/yr/kpc^{2} and \Sigma_{Gas} 1.0E4 M_\sun/pc^{2}. The non-detections of the nucleus in both the CO (6-5) line emission and the 435um continuum rule out, with relatively high confidence, a Compton-thick AGN in NGC 1614. Comparisons with radio continuum emission show a strong deviation from an expected local correlation between \Sigma_{Gas} and \Sigma_{SFR}, indicating a breakdown of the Kennicutt-Schmidt law on the linear scale of 100 pc., Comment: 13 pages, 10 figures; accepted by ApJ

Published
2015

17. THE COSMOS2015 CATALOG: EXPLORING THE 1 < z < 6 UNIVERSE WITH HALF A MILLION GALAXIES

Author

Laigle, C., primary, McCracken, H. J., additional, Ilbert, O., additional, Hsieh, B. C., additional, Davidzon, I., additional, Capak, P., additional, Hasinger, G., additional, Silverman, J. D., additional, Pichon, C., additional, Coupon, J., additional, Aussel, H., additional, Le Borgne, D., additional, Caputi, K., additional, Cassata, P., additional, Chang, Y.-Y., additional, Civano, F., additional, Dunlop, J., additional, Fynbo, J., additional, Kartaltepe, J. S., additional, Koekemoer, A., additional, Le Fèvre, O., additional, Le Floc’h, E., additional, Leauthaud, A., additional, Lilly, S., additional, Lin, L., additional, Marchesi, S., additional, Milvang-Jensen, B., additional, Salvato, M., additional, Sanders, D. B., additional, Scoville, N., additional, Smolcic, V., additional, Stockmann, M., additional, Taniguchi, Y., additional, Tasca, L., additional, Toft, S., additional, Vaccari, Mattia, additional, and Zabl, J., additional

Published
2016
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19. The role of galaxy interaction in the SFR-M_* relation: characterizing morphological properties of Herschel-selected galaxies at 0.2 <z <1.5

Author

Hung, Chao-Ling, Sanders, D. B., Casey, C. M., Lee, N., Barnes, J. E., Capak, P., Kartaltepe, J. S., Koss, M., Larson, K. L., Le Floc'h, E., Lockhart, K., Man, A. W. S., Mann, A. W., Riguccini, L., Scoville, N., and Symeonidis, M.

Subjects
Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

Galaxy interactions/mergers have been shown to dominate the population of IR-luminous galaxies (L_(IR) ≳ 10^(11.6) L_☉) in the local universe (z ≾ 0.25). Recent studies based on the relation between galaxies' star formation rates and stellar mass (the SFR-M_* relation or the "galaxy main sequence") have suggested that galaxy interaction/mergers may only become significant when galaxies fall well above the galaxy main sequence. Since the typical SFR at a given M_* increases with redshift, the existence of the galaxy main sequence implies that massive, IR-luminous galaxies at high z may not necessarily be driven by galaxy interactions. We examine the role of galaxy interactions in the SFR-M_* relation by carrying out a morphological analysis of 2084 Herschel-selected galaxies at 0.2 < z < 1.5 in the COSMOS field. Using a detailed visual classification scheme, we show that the fraction of "disk galaxies" decreases and the fraction of "irregular" galaxies increases systematically with increasing L_(IR) out to z ≾ 1.5 and z ≾ 1.0, respectively. At L_(IR) >10^(11.5) L_☉, ≳ 50% of the objects show evident features of strongly interacting/merger systems, where this percentage is similar to the studies of local IR-luminous galaxies. The fraction of interacting/merger systems also systematically increases with the deviation from the SFR-M_* relation, supporting the view that galaxies falling above the main sequence are more dominated by mergers than the main-sequence galaxies. Meanwhile, we find that ≳ 18% of massive IR-luminous "main-sequence galaxies" are classified as interacting systems, where this population may not evolve through the evolutionary track predicted by a simple gas exhaustion model.

Published
2013

20. Hubble Space Telescope ACS Imaging of the GOALS Sample: Quantitative Structural Properties of Nearby Luminous Infrared Galaxies with L_(IR) > 10^(11.4) L_☉

Author

Kim, D.-C., Evans, A. S., Vavilkin, T., Armus, L., Mazzarella, J. M., Sheth, K., Surace, J. A., Haan, S., Howell, J. H., Díaz-Santos, T., Petric, A., Iwasawa, K., Privon, G. C., and Sanders, D. B.

Subjects
Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

A Hubble Space Telescope/Advanced Camera for Surveys study of the structural properties of 85 luminous and ultraluminous (L_(IR) > 10^(11.4) L_☉) infrared galaxies (LIRGs and ULIRGs) in the Great Observatories All-sky LIRG Survey (GOALS) sample is presented. Two-dimensional GALFIT analysis has been performed on F814W "I-band" images to decompose each galaxy, as appropriate, into bulge, disk, central point-spread function (PSF) and stellar bar components. The fraction of bulge-less disk systems is observed to be higher in LIRGs (35%) than in ULIRGs (20%), with the disk+bulge systems making up the dominant fraction of both LIRGs (55%) and ULIRGs (45%). Further, bulge+disk systems are the dominant late-stage merger galaxy type and are the dominant type for LIRGs and ULIRGs at almost every stage of galaxy-galaxy nuclear separation. The mean I-band host absolute magnitude of the GOALS galaxies is –22.64 ± 0.62 mag (1.8^(+1.4)_(-0.4) L^*_I), and the mean bulge absolute magnitude in GOALS galaxies is about 1.1 mag fainter than the mean host magnitude. Almost all ULIRGs have bulge magnitudes at the high end (–20.6 to –23.5 mag) of the GOALS bulge magnitude range. Mass ratios in the GOALS binary systems are consistent with most of the galaxies being the result of major mergers, and an examination of the residual-to-host intensity ratios in GOALS binary systems suggests that smaller companions suffer more tidal distortion than the larger companions. We find approximately twice as many bars in GOALS disk+bulge systems (32.8%) than in pure-disk mergers (15.9%) but most of the disk+bulge systems that contain bars are disk-dominated with small bulges. The bar-to-host intensity ratio, bar half-light radius, and bar ellipticity in GOALS galaxies are similar to those found in nearby spiral galaxies. The fraction of stellar bars decreases toward later merger stages and smaller nuclear separations, indicating that bars are destroyed as the merger advances. In contrast, the fraction of nuclear PSFs increases toward later merger stages and is highest in late-stage systems with a single nucleus. Thus, light from an active galactic nucleus or compact nuclear star cluster is more visible at I band as ULIRGs enter their latter stages of evolution. Finally, both GOALS elliptical hosts and nearby Sloan Digital Sky Survey (SDSS) ellipticals occupy the same part of the surface brightness versus half-light radius plot (i.e., the "Kormendy Relation") and have similar slopes, consistent with the possibility that the GOALS galaxies belong to the same parent population as the SDSS ellipticals.

Published
2013

21. MERGER SIGNATURES IN THE DYNAMICS OF STAR-FORMING GAS

Author

Hung (洪肇伶), Chao-Ling, primary, Hayward, Christopher C., additional, Smith, Howard A., additional, Ashby, Matthew L. N., additional, Lanz, Lauranne, additional, Martínez-Galarza, Juan R., additional, Sanders, D. B., additional, and Zezas, Andreas, additional

Published
2016
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22. THE QUASAR-LBG TWO-POINT ANGULAR CROSS-CORRELATION FUNCTION ATz∼ 4 IN THE COSMOS FIELD

Author

Ikeda, H., primary, Nagao, T., additional, Taniguchi, Y., additional, Matsuoka, K., additional, Kajisawa, M., additional, Akiyama, M., additional, Miyaji, T., additional, Kashikawa, N., additional, Morokuma, T., additional, Shioya, Y., additional, Enoki, M., additional, Capak, P., additional, Koekemoer, A. M., additional, Masters, D., additional, Salvato, M., additional, Sanders, D. B., additional, Schinnerer, E., additional, and Scoville, N. Z., additional

Published
2015
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23. A Far-infrared Characterization of 24 μm Selected Galaxies at 0 < z < 2.5 using Stacking at 70 μm and 160 μm in the COSMOS Field

Author

Lee, Nicholas, Le Floc'h, Emeric, Sanders, D. B., Frayer, D. T., Arnouts, Stephane, Ilbert, Olivier, Aussel, Herve, Salvato, Mara, Scoville, N. Z., and Kartaltepe, Jeyhan S.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

We present a study of the average properties of luminous infrared galaxies detected directly at 24 μm in the COSMOS field using a median stacking analysis at 70 μm and 160 μm. Over 35,000 sources spanning 0 ≤ z ≤ 3 and 0.06 mJy ≤ S_(24) ≤ 3.0 mJy are stacked, divided into bins of both photometric redshift and 24 μm flux. We find no correlation of S_(70)/S_(24) flux density ratio with S_(24), but find that galaxies with higher S_(24) have a lower S_(160)/S_(24) flux density ratio. These observed ratios suggest that 24 μm selected galaxies have warmer spectral energy distributions (SEDs) at higher mid-IR fluxes, and therefore have a possible higher fraction of active galactic nuclei. Comparisons of the average S_(70)/S_(24) and S_(160)/S_(24) colors with various empirical templates and theoretical models show that the galaxies detected at 24 μm are consistent with "normal" star-forming galaxies and warm mid-IR galaxies such as Mrk 231, but inconsistent with heavily obscured galaxies such as Arp 220. We perform a χ^2 analysis to determine best-fit galactic model SEDs and total IR luminosities for each of our bins. We compare our results to previous methods of estimating L IR and find that previous methods show considerable agreement over the full redshift range, except for the brightest S_(24) sources, where they overpredict the bolometric IR luminosity at high redshift, most likely due to their warmer dust SED. We present a table that can be used as a more accurate and robust method for estimating bolometric infrared luminosity from 24 μm flux densities.

Published
2010

25. REST-FRAME OPTICAL EMISSION LINES IN FAR-INFRARED-SELECTED GALAXIES AT z < 1.7 FROM THE FMOS-COSMOS SURVEY

Author

Kartaltepe, Jeyhan S., primary, Sanders, D. B., additional, Silverman, J. D., additional, Kashino, D., additional, Chu, J., additional, Zahid, H., additional, Hasinger, G., additional, Kewley, L., additional, Matsuoka, K., additional, Nagao, T., additional, Riguccini, L., additional, Salvato, M., additional, Schawinski, K., additional, Taniguchi, Y., additional, Treister, E., additional, Capak, P., additional, Daddi, E., additional, and Ohta, K., additional

Published
2015
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26. No Evolution in the IR–Radio Relation for IR-luminous Galaxies at z < 2 in the COSMOS Field

Author

Sargent, M. T., Schinnerer, E., Murphy, E., Carilli, C. L., Helou, G., Aussel, H., Le Floc'h, E., Frayer, D. T., Ilbert, O., Oesch, P., Salvato, M., Smolčić, V., Kartaltepe, J., and Sanders, D. B.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

Previous observational studies of the infrared (IR)-radio relation out to high redshift employed any detectable star-forming systems at a given redshift within the restricted area of cosmological survey fields. Consequently, the evolution inferred relies on a comparison between the average IR/radio properties of (1) very IR-luminous high-z sources and (2) more heterogeneous low(er)-z samples that often lack the strongest IR emitters. In this Letter, we consider populations of objects with comparable luminosities over the last 10 Gyr by taking advantage of deep IR (especially Spitzer 24 μm) and Very Large Array 1.4 GHz observations of the COSMOS field. Consistent with recent model predictions, both Ultra Luminous Infrared Galaxies and galaxies on the bright end of the evolving IR luminosity function do not display any change in their average IR/radio ratios out to z ~ 2 when corrected for bias. Uncorrected data suggested ~0.3 dex of positive evolution.

Published
2010

28. A TURNOVER IN THE GALAXY MAIN SEQUENCE OF STAR FORMATION ATM*∼ 1010M☉FOR REDSHIFTSz< 1.3

Author

Lee, Nicholas, primary, Sanders, D. B., additional, Casey, Caitlin M., additional, Toft, Sune, additional, Scoville, N. Z., additional, Hung, Chao-Ling, additional, Le Floc'h, Emeric, additional, Ilbert, Olivier, additional, Zahid, H. Jabran, additional, Aussel, Hervé, additional, Capak, Peter, additional, Kartaltepe, Jeyhan S., additional, Kewley, Lisa J., additional, Li, Yanxia, additional, Schawinski, Kevin, additional, Sheth, Kartik, additional, and Xiao, Quanbao, additional

Published
2015
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29. THEHERSCHELCOMPREHENSIVE (U)LIRG EMISSION SURVEY (HERCULES): CO LADDERS, FINE STRUCTURE LINES, AND NEUTRAL GAS COOLING

Author

Rosenberg, M. J. F., primary, van der Werf, P. P., additional, Aalto, S., additional, Armus, L., additional, Charmandaris, V., additional, Díaz-Santos, T., additional, Evans, A. S., additional, Fischer, J., additional, Gao, Y., additional, González-Alfonso, E., additional, Greve, T. R., additional, Harris, A. I., additional, Henkel, C., additional, Israel, F. P., additional, Isaak, K. G., additional, Kramer, C., additional, Meijerink, R., additional, Naylor, D. A., additional, Sanders, D. B., additional, Smith, H. A., additional, Spaans, M., additional, Spinoglio, L., additional, Stacey, G. J., additional, Veenendaal, I., additional, Veilleux, S., additional, Walter, F., additional, Weiß, A., additional, Wiedner, M. C., additional, van der Wiel, M. H. D., additional, and Xilouris, E. M., additional

Published
2015
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30. The Hα luminosity function and star formation rate at z ≈ 0.24 in the COSMOS 2 square degree field

Author

Shioya, Y., Taniguchi, Y., Sasaki, S. S., Nagao, T., Murayama, T., Takahashi, M. I., Ajiki, M., Ideue, Y., Mihara, S., Nakajima, A., Scoville, N. Z., Mobasher, B., Aussel, H., Giavalisco, M., Guzzo, L., Hasinger, G., Impey, C., Le Fèvre, O., Lilly, S., Renzini, A., Rich, M., Sanders, D. B., Schinnerer, E., Shopbell, P., Leauthaud, A., Kneib, J. P., Rhodes, J., and Massey, R.

Abstract

To derive a new Hα luminosity function and to understand the clustering properties of star-forming galaxies at z≈ 0.24, we have made a narrowband imaging survey for Hα-emitting galaxies in the Hubble Space Telescope (HST) COSMOS 2 square degree field. We used the narrowband filter NB816 (λ_c = 8150 Å, Δ λ = 120 Å) and sampled Hα emitters with EW_(obs)(H α + [N II]) > 12Å in a redshift range between z = 0.233 and 0.251 corresponding to a depth of 70 Mpc. We obtained 980 Hα-emitting galaxies in a sky area of 5540 arcmin^2, corresponding to a survey volume of 3.1 × 10^4 Mpc^3. We derive a Hα luminosity function with a best-fit Schechter function parameter set of α = − 1.35_(−0.13)^(+0.11), log ф_* = − 2.65_(−0.38)^(+0.27), and log L_*(ergs s^(−1)) = 41.94_(−0.23)^(+0.38). The Hα luminosity density is 2.7_(−0.6)^(+0.7) × 10^(39) ergs s^(−1) Mpc^(−3). After subtracting the AGN contribution (15%) to the Hα luminosity density, the star formation rate density is evaluated as 1.8_(−0.4)^(+0.7) × 10^(−2) M_סּ yr^(−1) Mpc^(−3). The angular two-point correlation function of Hα-emitting galaxies of log L(H α) > 39.8 is well fit by a power-law form of w(θ) = 0.013−_(0.001)^(+0.002)θ^(−0.88 ± 0.03), corresponding to the correlation function of ξ (r) = (r/1.9 Mpc)^(−1.88). We also find that the Hα emitters with higher Hα luminosity are more strongly clustered than those with lower luminosity.

Published
2008

31. ALMA OBSERVATIONS OF WARM DENSE GAS IN NGC 1614—BREAKING OF THE STAR FORMATION LAW IN THE CENTRAL KILOPARSEC

Author

Xu, C. K., primary, Cao, C., additional, Lu, N., additional, Gao, Y., additional, Diaz-Santos, T., additional, Herrero-Illana, R., additional, Meijerink, R., additional, Privon, G., additional, Zhao, Y.-H., additional, Evans, A. S., additional, König, S., additional, Mazzarella, J. M., additional, Aalto, S., additional, Appleton, P., additional, Armus, L., additional, Charmandaris, V., additional, Chu, J., additional, Haan, S., additional, Inami, H., additional, Murphy, E. J., additional, Sanders, D. B., additional, Schulz, B., additional, and van der Werf, P., additional

Published
2015
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32. HIGH-RESOLUTION RADIO CONTINUUM MEASUREMENTS OF THE NUCLEAR DISKS OF Arp 220

Author

Barcos-Muñoz, L., primary, Leroy, A. K., additional, Evans, A. S., additional, Privon, G. C., additional, Armus, L., additional, Condon, J., additional, Mazzarella, J. M., additional, Meier, D. S., additional, Momjian, E., additional, Murphy, E. J., additional, Ott, J., additional, Reichardt, A., additional, Sakamoto, K., additional, Sanders, D. B., additional, Schinnerer, E., additional, Stierwalt, S., additional, Surace, J. A., additional, Thompson, T. A., additional, and Walter, F., additional

Published
2015
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33. ARE DUSTY GALAXIES BLUE? INSIGHTS ON UV ATTENUATION FROM DUST-SELECTED GALAXIES

Author

Casey, C. M., primary, Scoville, N. Z., additional, Sanders, D. B., additional, Lee, N., additional, Cooray, A., additional, Finkelstein, S. L., additional, Capak, P., additional, Conley, A., additional, De Zotti, G., additional, Farrah, D., additional, Fu, H., additional, Le Floc'h, E., additional, Ilbert, O., additional, Ivison, R. J., additional, and Takeuchi, T. T., additional

Published
2014
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34. ERRATUM: “ SPITZER QUASAR AND ULIRG EVOLUTION STUDY (QUEST). IV. COMPARISON OF 1 Jy ULTRALUMINOUS INFRARED GALAXIES WITH PALOMAR-GREEN QUASARS” (2009, ApJS, 182, 628)

Author

Veilleux, S., primary, Rupke, D. S. N., additional, Kim, D.-C., additional, Genzel, R., additional, Sturm, E., additional, Lutz, D., additional, Contursi, A., additional, Schweitzer, M., additional, Tacconi, L. J., additional, Netzer, H., additional, Sternberg, A., additional, Mihos, J. C., additional, Baker, A. J., additional, Mazzarella, J. M., additional, Lord, S., additional, Sanders, D. B., additional, Stockton, A., additional, Joseph, R. D., additional, and Barnes, J. E., additional

Published
2014
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35. A COMPARISON OF THE MORPHOLOGICAL PROPERTIES BETWEEN LOCAL ANDz∼ 1 INFRARED LUMINOUS GALAXIES: ARE LOCAL AND HIGH-z(U)LIRGS DIFFERENT?

Author

Hung, Chao-Ling, primary, Sanders, D. B., additional, Casey, Caitlin M., additional, Koss, Michael, additional, Larson, Kirsten L., additional, Lee, Nicholas, additional, Li, Yanxia, additional, Lockhart, Kelly, additional, Shih, Hsin-Yi, additional, Barnes, Joshua E., additional, Kartaltepe, Jeyhan S., additional, and Smith, Howard A., additional

Published
2014
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36. EXTENDED [C II] EMISSION IN LOCAL LUMINOUS INFRARED GALAXIES

Author

Díaz-Santos, T., primary, Armus, L., additional, Charmandaris, V., additional, Stacey, G., additional, Murphy, E. J., additional, Haan, S., additional, Stierwalt, S., additional, Malhotra, S., additional, Appleton, P., additional, Inami, H., additional, Magdis, G. E., additional, Elbaz, D., additional, Evans, A. S., additional, Mazzarella, J. M., additional, Surace, J. A., additional, van der Werf, P. P., additional, Xu, C. K., additional, Lu, N., additional, Meijerink, R., additional, Howell, J. H., additional, Petric, A. O., additional, Veilleux, S., additional, and Sanders, D. B., additional

Published
2014
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37. WARM MOLECULAR GAS IN LUMINOUS INFRARED GALAXIES

Author

Lu, N., primary, Zhao, Y., additional, Xu, C. K., additional, Gao, Y., additional, Armus, L., additional, Mazzarella, J. M., additional, Isaak, K. G., additional, Petric, A. O., additional, Charmandaris, V., additional, Díaz-Santos, T., additional, Evans, A. S., additional, Howell, J., additional, Appleton, P., additional, Inami, H., additional, Iwasawa, K., additional, Leech, J., additional, Lord, S., additional, Sanders, D. B., additional, Schulz, B., additional, Surace, J., additional, and van der Werf, P. P., additional

Published
2014
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38. ALMA OBSERVATIONS OF WARM MOLECULAR GAS AND COLD DUST IN NGC 34

Author

Xu, C. K., primary, Cao, C., additional, Lu, N., additional, Gao, Y., additional, van der Werf, P., additional, Evans, A. S., additional, Mazzarella, J. M., additional, Chu, J., additional, Haan, S., additional, Diaz-Santos, T., additional, Meijerink, R., additional, Zhao, Y.-H., additional, Appleton, P., additional, Armus, L., additional, Charmandaris, V., additional, Lord, S., additional, Murphy, E. J., additional, Sanders, D. B., additional, Schulz, B., additional, and Stierwalt, S., additional

Published
2014
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39. ERRATUM: “THE FMOS-COSMOS SURVEY OF STAR-FORMING GALAXIES AT z ∼ 1.6. I. Hα-BASED STAR FORMATION RATES AND DUST EXTINCTION” (2013, ApJL, 777, L8)

Author

Kashino, D., primary, Silverman, J. D., additional, Rodighiero, G., additional, Renzini, A., additional, Arimoto, N., additional, Daddi, E., additional, Lilly, S. J., additional, Sanders, D. B., additional, Kartaltepe, J., additional, Zahid, H. J., additional, Nagao, T., additional, Sugiyama, N., additional, Capak, P., additional, Carollo, C. M., additional, Chu, J., additional, Hasinger, G., additional, Ilbert, O., additional, Kajisawa, M., additional, Kewley, L. J., additional, Koekemoer, A. M., additional, Kovač, K., additional, Le Fèvre, O., additional, Masters, D., additional, McCracken, H. J., additional, Onodera, M., additional, Scoville, N., additional, Strazzullo, V., additional, Symeonidis, M., additional, and Taniguchi, Y., additional

Published
2014
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41. Evidence for CO shock excitation in NGC 6240 from Herschel Spire spectroscopy

Author

Meijerink, R., Kristensen, L. E., Weiß, A., Werf, Paul P. van der, Walter, F., Spaans, M., Loenen, A. F., Fischer, J., Israel, F. P., Isaak, K., Papadopoulos, P. P., Aalto, S., Armus, L., Charmandaris, V., Dasyra, K.M., Díaz-Santos, T., Evans, A., Gao, Y., González-Alfonso, E., Güsten, R., Henkel, Christian, Kramer, C., Lord, S., Martín-Pintado, Jesús, Naylor, D., Sanders, D. B., Smith, H., Spinoglio, L., Stacey, G., Veilleux, S., Wiedner, M. C., Meijerink, R., Kristensen, L. E., Weiß, A., Werf, Paul P. van der, Walter, F., Spaans, M., Loenen, A. F., Fischer, J., Israel, F. P., Isaak, K., Papadopoulos, P. P., Aalto, S., Armus, L., Charmandaris, V., Dasyra, K.M., Díaz-Santos, T., Evans, A., Gao, Y., González-Alfonso, E., Güsten, R., Henkel, Christian, Kramer, C., Lord, S., Martín-Pintado, Jesús, Naylor, D., Sanders, D. B., Smith, H., Spinoglio, L., Stacey, G., Veilleux, S., and Wiedner, M. C.

Abstract

We present Herschel SPIRE FTS spectroscopy of the nearby luminous infrared galaxy NGC 6240. In total 20 lines are detected, including CO J = 4-3 through J = 13-12, 6 H2O rotational lines, and [C I] and [N II] fine-structure lines. The CO to continuum luminosity ratio is 10 times higher in NGC 6240 than Mrk 231. Although the CO ladders of NGC 6240 and Mrk 231 are very similar, UV and/or X-ray irradiation are unlikely to be responsible for the excitation of the gas in NGC 6240. We applied both C and J shock models to the H2 v = 1-0 S(1) and v = 2-1 S(1) lines and the CO rotational ladder. The CO ladder is best reproduced by a model with shock velocity vs = 10 km s -1 and a pre-shock density nH = 5 × 104 cm-3. We find that the solution best fitting the H2 lines is degenerate. The shock velocities and number densities range between v s = 17-47 km s-1 and nH = 107-5 × 104 cm-3, respectively. The H2 lines thus need a much more powerful shock than the CO lines. We deduce that most of the gas is currently moderately stirred up by slow (10 km s-1) shocks while only a small fraction (≲ 1%) of the interstellar medium is exposed to the high-velocity shocks. This implies that the gas is rapidly losing its highly turbulent motions. We argue that a high CO line-to-continuum ratio is a key diagnostic for the presence of shocks. © 2013. The American Astronomical Society. All rights reserved.

Published
2013

42. MULTI-WAVELENGTH SEDs OFHERSCHEL-SELECTED GALAXIES IN THE COSMOS FIELD

Author

Lee, Nicholas, primary, Sanders, D. B., additional, Casey, Caitlin M., additional, Scoville, N. Z., additional, Hung, Chao-Ling, additional, Le Floc'h, Emeric, additional, Ilbert, Olivier, additional, Aussel, Hervé, additional, Capak, Peter, additional, Kartaltepe, Jeyhan S., additional, Roseboom, Isaac, additional, Salvato, Mara, additional, Aravena, M., additional, Berta, S., additional, Bock, J., additional, Oliver, S. J., additional, Riguccini, L., additional, and Symeonidis, M., additional

Published
2013
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43. THE ROLE OF GALAXY INTERACTION IN THE SFR-M*RELATION: CHARACTERIZING MORPHOLOGICAL PROPERTIES OFHerschel-SELECTED GALAXIES AT 0.2 < 1.5

Author

Hung, Chao-Ling, primary, Sanders, D. B., additional, Casey, C. M., additional, Lee, N., additional, Barnes, J. E., additional, Capak, P., additional, Kartaltepe, J. S., additional, Koss, M., additional, Larson, K. L., additional, Le Floc'h, E., additional, Lockhart, K., additional, Man, A. W. S., additional, Mann, A. W., additional, Riguccini, L., additional, Scoville, N., additional, and Symeonidis, M., additional

Published
2013
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44. THE FMOS-COSMOS SURVEY OF STAR-FORMING GALAXIES AT z ∼ 1.6. I. Hα-BASED STAR FORMATION RATES AND DUST EXTINCTION

Author

Kashino, D., primary, Silverman, J. D., additional, Rodighiero, G., additional, Renzini, A., additional, Arimoto, N., additional, Daddi, E., additional, Lilly, S. J., additional, Sanders, D. B., additional, Kartaltepe, J., additional, Zahid, H. J., additional, Nagao, T., additional, Sugiyama, N., additional, Capak, P., additional, Carollo, C. M., additional, Chu, J., additional, Hasinger, G., additional, Ilbert, O., additional, Kajisawa, M., additional, Kewley, L. J., additional, Koekemoer, A. M., additional, Kovač, K., additional, Le Fèvre, O., additional, Masters, D., additional, McCracken, H. J., additional, Onodera, M., additional, Scoville, N., additional, Strazzullo, V., additional, Symeonidis, M., additional, and Taniguchi, Y., additional

Published
2013
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45. EXPLAINING THE [C II]157.7 μm DEFICIT IN LUMINOUS INFRARED GALAXIES—FIRST RESULTS FROM AHERSCHEL/PACS STUDY OF THE GOALS SAMPLE

Author

Díaz-Santos, T., primary, Armus, L., additional, Charmandaris, V., additional, Stierwalt, S., additional, Murphy, E. J., additional, Haan, S., additional, Inami, H., additional, Malhotra, S., additional, Meijerink, R., additional, Stacey, G., additional, Petric, A. O., additional, Evans, A. S., additional, Veilleux, S., additional, van der Werf, P. P., additional, Lord, S., additional, Lu, N., additional, Howell, J. H., additional, Appleton, P., additional, Mazzarella, J. M., additional, Surace, J. A., additional, Xu, C. K., additional, Schulz, B., additional, Sanders, D. B., additional, Bridge, C., additional, Chan, B. H. P., additional, Frayer, D. T., additional, Iwasawa, K., additional, Melbourne, J., additional, and Sturm, E., additional

Published
2013
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46. A COMPARATIVE ANALYSIS OF VIRIAL BLACK HOLE MASS ESTIMATES OF MODERATE-LUMINOSITY ACTIVE GALACTIC NUCLEI USING SUBARU/FMOS

Author

Matsuoka, K., primary, Silverman, J. D., additional, Schramm, M., additional, Steinhardt, C. L., additional, Nagao, T., additional, Kartaltepe, J., additional, Sanders, D. B., additional, Treister, E., additional, Hasinger, G., additional, Akiyama, M., additional, Ohta, K., additional, Ueda, Y., additional, Bongiorno, A., additional, Brandt, W. N., additional, Brusa, M., additional, Capak, P., additional, Civano, F., additional, Comastri, A., additional, Elvis, M., additional, Lilly, S. J., additional, Mainieri, V., additional, Masters, D., additional, Mignoli, M., additional, Salvato, M., additional, Trump, J. R., additional, Taniguchi, Y., additional, Zamorani, G., additional, Alexander, D. M., additional, and Schawinski, K., additional

Published
2013
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47. HUBBLE SPACE TELESCOPEACS IMAGING OF THE GOALS SAMPLE: QUANTITATIVE STRUCTURAL PROPERTIES OF NEARBY LUMINOUS INFRARED GALAXIES WITHLIR> 1011.4L☉

Author

Kim, D.-C., primary, Evans, A. S., additional, Vavilkin, T., additional, Armus, L., additional, Mazzarella, J. M., additional, Sheth, K., additional, Surace, J. A., additional, Haan, S., additional, Howell, J. H., additional, Díaz-Santos, T., additional, Petric, A., additional, Iwasawa, K., additional, Privon, G. C., additional, and Sanders, D. B., additional

Published
2013
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48. EVOLUTION OF GALAXIES AND THEIR ENVIRONMENTS AT z = 0.1-3 IN COSMOS

Author

Scoville, N., primary, Arnouts, S., additional, Aussel, H., additional, Benson, A., additional, Bongiorno, A., additional, Bundy, K., additional, Calvo, M. A. A., additional, Capak, P., additional, Carollo, M., additional, Civano, F., additional, Dunlop, J., additional, Elvis, M., additional, Faisst, A., additional, Finoguenov, A., additional, Fu, Hai, additional, Giavalisco, M., additional, Guo, Q., additional, Ilbert, O., additional, Iovino, A., additional, Kajisawa, M., additional, Kartaltepe, J., additional, Leauthaud, A., additional, Le Fèvre, O., additional, LeFloch, E., additional, Lilly, S. J., additional, Liu, C. T.-C., additional, Manohar, S., additional, Massey, R., additional, Masters, D., additional, McCracken, H. J., additional, Mobasher, B., additional, Peng, Y.-J., additional, Renzini, A., additional, Rhodes, J., additional, Salvato, M., additional, Sanders, D. B., additional, Sarvestani, B. D., additional, Scarlata, C., additional, Schinnerer, E., additional, Sheth, K., additional, Shopbell, P. L., additional, Smolčić, V., additional, Taniguchi, Y., additional, Taylor, J. E., additional, White, S. D. M., additional, and Yan, L., additional

Published
2013
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49. MID-INFRARED PROPERTIES OF NEARBY LUMINOUS INFRARED GALAXIES. I. SPITZER INFRARED SPECTROGRAPH SPECTRA FOR THE GOALS SAMPLE

Author

Stierwalt, S., primary, Armus, L., additional, Surace, J. A., additional, Inami, H., additional, Petric, A. O., additional, Diaz-Santos, T., additional, Haan, S., additional, Charmandaris, V., additional, Howell, J., additional, Kim, D. C., additional, Marshall, J., additional, Mazzarella, J. M., additional, Spoon, H. W. W., additional, Veilleux, S., additional, Evans, A., additional, Sanders, D. B., additional, Appleton, P., additional, Bothun, G., additional, Bridge, C. R., additional, Chan, B., additional, Frayer, D., additional, Iwasawa, K., additional, Kewley, L. J., additional, Lord, S., additional, Madore, B. F., additional, Melbourne, J. E., additional, Murphy, E. J., additional, Rich, J. A., additional, Schulz, B., additional, Sturm, E., additional, U, V., additional, Vavilkin, T., additional, and Xu, K., additional

Published
2013
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