Reanalyzing Jupiter ISO/SWS data through a more recent atmospheric model by Ribeiro, J, Machado, P, Perez-Hoyos, S, Dias, JA, Irwin, P

“…To help in this endeavour, we used Infrared Space Observatory Short Wavelength Spectrometer (ISO/SWS) Jupiter observations in the 793–1500 cm (Formula presented.) region together with the Nonlinear Optimal Estimator for MultivariatE Spectral analySIS (NEMESIS) radiative transfer suite to retrieve the temperature–pressure profile and the chemical abundances for various chemical species. …”

Fifteen Years of Continuous High-Resolution Borehole Strainmeter Measurements in Eastern Taiwan: An Overview and Perspectives by Alexandre Canitano, Maxime Mouyen, Ya-Ju Hsu, Alan Linde, Selwyn Sacks, Hsin-Ming Lee

Get full text

EUSO: using high energy cosmic rays and neutrinos as messengers from the unknown universe by L. Scarsi

“…Exploiting the earth atmosphere as a giant detector for the incoming extraterrestrial fl ux of high energy cosmic rays
 and cosmic neutrinos, the mission «EUSO-Extreme Universe Space Observatory» is devoted to the exploration
 of the domain of the highest energy processes occurring in the universe up to its accessible boundaries. …”
Get full text

Constraining a Thin Dark Matter Disk with Gaia by Schutz, Katelin, Lin, Tongyan, Safdi, Benjamin R., Wu, Chih-Liang

“…Using the first data release from the Gaia space observatory, we search for a dark disk via its effect on stellar kinematics in the Milky Way. …”
Get full text

Herschel-ATLAS: Extragalactic number counts from 250 to 500 microns by Clements, D, Rigby, E, Maddox, S, Dunne, L, Mortier, A, Pearson, C, Amblard, A, Auld, R, Baes, M, Bonfield, D, Burgarella, D, Buttiglione, S, Cava, A, Cooray, A, Dariush, A, de Zotti, G, Dye, S, Eales, S, Frayer, D, Fritz, J, Gardner, J, Gonzalez-Nuevo, J, Herranz, D, Ibar, E, Ivison, R

“…The Herschel-ATLAS survey (H-ATLAS) will be the largest area survey to be undertaken by the Herschel Space Observatory. It will cover 550 sq. deg. of extragalactic sky at wavelengths of 100, 160, 250, 350 and 500 μm when completed, reaching flux limits (5σ) from 32 to 145 mJy. …”

Cold dust and young starbursts: spectral energy distributions of Herschel SPIRE sources from the HerMES survey by Rowan-Robinson, M, Roseboom, I, Vaccari, M, Amblard, A, Arumugam, V, Auld, R, Aussel, H, Babbedge, T, Blain, A, Bock, J, Boselli, A, Brisbin, D, Buat, V, Burgarella, D, Castro-Rodriguez, N, Cava, A, Chanial, P, Clements, D, Conley, A, Conversi, L, Cooray, A, Dowell, C, Dwek, E, Dye, S, Eales, S

“…We find that while many galaxies ( 56 per cent) are well fitted with the templates used to fit IRAS, Infrared Space Observatory (ISO) and Spitzer sources, for about half the galaxies two new templates are required: quiescent ('cirrus') models with colder (10-20 K) dust and a young starburst model with higher optical depth than Arp 220. …”

Herschel -ATLAS: Extragalactic number counts from 250 to 500 microns by Clements, D, Rigby, E, Maddox, S, Dunne, L, Mortier, A, Pearson, C, Amblard, A, Auld, R, Baes, M, Bonfield, D, Burgarella, D, Buttiglione, S, Cava, A, Cooray, A, Dariush, A, De Zotti, G, Dye, S, Eales, S, Frayer, D, Fritz, J, Gardner, J, Gonzalez-Nuevo, J, Herranz, D, Ibar, E, Ivison, R

“…The Herschel-ATLAS survey (H-ATLAS) will be the largest area survey to be undertaken by the Herschel Space Observatory. It will cover 550 sq. deg. of extragalactic sky at wavelengths of 100, 160, 250, 350 and 500 μm when completed, reaching flux limits (5σ) from 32 to 145 mJy. …”

A comparison of two different techniques for deriving the quiet day curve from SARINET riometer data by J. Moro, C. M. Denardini, E. Correia, E. Correia, M. A. Abdu, N. J. Schuch, K. Makita

“…To validate our approach, the QDC is estimated from data acquired by the Imaging Riometer for Ionospheric Studies (IRIS) installed at the Southern Space Observatory (SSO/CRS/CCR/INPE – MCT, 29°4´ S, 53°8´ W, 480 m a.s.l.), São Martinho da Serra – Brazil. …”
Get full text

An infrared-radio simulation of the extragalactic sky: from the Square Kilometer Array to Herschel by Wilman, R, Jarvis, M, Mauch, T, Rawlings, S, Hickey, S

“…To exploit synergies between the Herschel Space Observatory and next generation radio facilities, we have extended the semi-empirical extragalactic radio continuum simulation of Wilman et al. (2008) to the mid- and far-infrared. …”

In-flight calibration of the Herschel -SPIRE instrument by Swinyard, B, Ade, P, Baluteau, J, Aussel, H, Barlow, M, Bendo, G, Benielli, D, Bock, J, Brisbin, D, Conley, A, Conversi, L, Dowell, A, Dowell, D, Ferlet, M, Fulton, T, Glenn, J, Glauser, A, Griffin, D, Griffin, M, Guest, S, Imhof, P, Isaak, K, Jones, S, King, K, Leeks, S

“…SPIRE, the Spectral and Photometric Imaging REceiver, is the Herschel Space Observatory's submillimetre camera and spectrometer. …”

ISO photometry of hyperluminous infrared galaxies: Implications for the origin of their extreme luminosities by Verma, A, Rowan-Robinson, M, McMahon, R, Efstathiou, A

“…We present 7-180μm photometry of a sample of hyperluminous infrared galaxies (HyLIGs) obtained with the photometer and camera mounted on the Infrared Space Observatory (ISO). We have used state-of-the-art' radiative transfer models of obscured starbursts and dusty tori to model their broadband spectral energy distributions (SEDs). …”

In-flight calibration of the Herschel-SPIRE instrument by Swinyard, B, Ade, P, Baluteau, J, Aussel, H, Barlow, M, Bendo, G, Benielli, D, Bock, J, Brisbin, D, Conley, A, Conversi, L, Dowell, A, Dowell, D, Ferlet, M, Fulton, T, Glenn, J, Glauser, A, Griffin, D, Griffin, M, Guest, S, Imhof, P, Isaak, K, Jones, S, King, K, Leeks, S

“…SPIRE, the Spectral and Photometric Imaging REceiver, is the Herschel Space Observatory's submillimetre camera and spectrometer. …”

Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913 by M. Ginolfi, E. Piconcelli, L. Zappacosta, G. C. Jones, L. Pentericci, R. Maiolino, A. Travascio, N. Menci, S. Carniani, F. Rizzo, F. Arrigoni Battaia, S. Cantalupo, C. De Breuck, L. Graziani, K. Knudsen, P. Laursen, V. Mainieri, R. Schneider, F. Stanley, R. Valiante, A. Verhamme

Get full text

X-RAY EMISSION OF ICRF SOURCES by V. V. Voitsekhovskiy, A. Tugay, V. V. Tkachuk, S. Yu. Shevchenko

“…Among 295 selected reference frames of the system we identified 54 X-ray sources which were observed by space observatory XMM Newton and noticed rapid variability of the blazars 2E 2673 (W Com) and 2E 1802 which enables to conclude that they have some very active processes in the sources centers . …”
Get full text

HerMES: SPIRE detection of high-redshift massive compact galaxies in GOODS-N field by Cava, A, Rodighiero, G, Perez-Fournon, I, Buitrago, F, Trujillo, I, Altieri, B, Amblard, A, Auld, R, Bock, J, Brisbin, D, Burgarella, D, Castro-Rodriguez, N, Chanial, P, Cirasuolo, M, Clements, D, Conselice, C, Cooray, A, Eales, S, Elbaz, D, Ferrero, P, Franceschini, A, Glenn, J, Gonzalez Solares, E, Griffin, M, Ibar, E

“…Wehave analysed the rest-frame far-infrared properties ofa sample of massive (M* > 1011 M⊙) galaxies at 2 ≲ z ≲ 3 in the Great Observatories Origins Deep Survey-North (GOODS-N) field using the Spectral and Photometric Imaging Receiver (SPIRE) instrument aboard the Herschel Space Observatory. To conduct this analysis we take advantage of the data from the Herschel Multi-tiered Extragalactic Survey (HerMES) key programme. …”

FORS spectroscopy of galaxies in the Hubble Deep Field-South by Rigopoulou, D, Vacca, W, Berta, S, Franceschini, A, Aussel, H

“…Thirty-two primary spectroscopic targets in the HST-WFPC2 HDFS were supplemented with galaxies detected in the Infrared Space Observatory's survey of the HDFS and the ESO Imaging Deep Survey to comprise a sample of 100 galaxies for spectroscopic observations. …”

The new galaxy evolution paradigm revealed by the Herschel surveys by Eales, S, Smith, D, Bourne, N, Loveday, J, Rowlands, K, Werf, P, Driver, S, Dunne, L, Dye, S, Furlanetto, C, Ivison, R, Maddox, S, Robotham, A, Smith, M, Taylor, E, Valiante, E, Wright, A, Cigan, P, De Zotti, G, Jarvis, M, Marchetti, L, Michałowski, M, Phillipps, S, Viaene, S, Vlahakis, C

“…The Herschel Space Observatory has revealed a very different galaxyscape from that shown by optical surveys which presents a challenge for galaxy-evolution models. …”

The far-infrared/radio correlation and radio spectral index of galaxies in the SFR-M∗ plane up to z~2 by Magnelli, B, Ivison, R, Lutz, D, Valtchanov, I, Farrah, D, Berta, S, Bertoldi, F, Bock, J, Cooray, A, Ibar, E, Karim, A, Le Floc'h, E, Nordon, R, Oliver, S, Page, M, Popesso, P, Pozzi, F, Rigopoulou, D, Riguccini, L, Rodighiero, G, Rosario, D, Roseboom, I, Wang, L, Wuyts, S

“…The infrared luminosities of our SFR-M∗-z bins are estimated using their stacked far-infrared flux densities inferred from observations obtained with the Herschel Space Observatory. Their radio luminosities and radio spectral indices (i.e. α, where Sν ∝ ν-α) are estimated using their stacked 1.4 GHz and 610 MHz flux densities from the Very Large Array and Giant Metre-wave Radio Telescope, respectively. …”

A first glimpse into the far-IR properties of high-z UV-selected galaxies: Herschel/PACS observations of z ∼ 3 LBGS by Magdis, G, Elbaz, D, Hwang, H, Daddi, E, Rigopoulou, D, Altieri, B, Andreani, P, Aussel, H, Berta, S, Cava, A, Bongiovanni, A, Cepa, J, Cimatti, A, Dickinson, M, Dominguez, H, Förster Schreiber, N, Genzel, R, Huang, J, Lutz, D, Maiolino, R, Magnelli, B, Morrison, G, Nordon, R, Pérez García, A, Poglitsch, A

“…We present first insights into the far-IR properties for a sample of IRAC and MIPS 24 μm detected Lyman break galaxies (LBGs) at z ∼ 3, as derived from observations in the northern field of the Great Observatories Origins Survey (GOODS-N) carried out with the PACS instrument on board the Herschel Space Observatory. Although none of our galaxies are detected by Herschel, we employ a stacking technique to construct, for the first time, the average spectral energy distribution (SED) of infrared luminous LBGs from UV to radio wavelengths. …”

Herschel Observations of Far-Infrared Cooling Lines in intermediate Redshift (Ultra)-luminous Infrared Galaxies by Rigopoulou, D, Hopwood, R, Magdis, G, Thatte, N, Swinyard, B, Farrah, D, Huang, J, Alonso-Herrero, A, Bock, J, Clements, D, Cooray, A, Griffin, M, Oliver, S, Pearson, C, Riechers, D, Scott, D, Smith, A, Vaccari, M, Valtchanov, I, Wang, L

“…We report the first results from a spectroscopic survey of the [CII] 158um line from a sample of intermediate redshift (0.2<z<0.8) (lir="" (u)lirgs="" (ultra)-luminous="" galaxies,="" infrared="">10^11.5 Lsun), using the SPIRE-Fourier Transform Spectrometer (FTS) on board the Herschel Space Observatory. This is the first survey of [CII] emission, an important tracer of star-formation, at a redshift range where the star-formation rate density of the Universe increases rapidly. …”