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    The UKIRT Hemisphere Survey: definition and J-band data release by Dye, S., Lawrence, A., Read, M.A., Fan, X., Kerr, T., Varricatt, W., Furnell, K.E., Edge, A.C., Irwin, M., Hambly, N., Lucas, P., Almaini, O., Chambers, K., Green, R., Hewett, P., Liu, M.C., McGreer, I., Best, W., Zhang, Z., Sutorius, E., Froebrich, D., Magnier, E., Hasinger, G., Lederer, S.M., Bold, M., Tedds, J.A.

    Published 2018
    “…This paper defines the UK Infra-Red Telescope (UKIRT) Hemisphere Survey (UHS) and release of the remaining ∼12 700 deg2 of J-band survey data products. The UHS will provide continuous J- and K-band coverage in the Northern hemisphere from a declination of 0◦ to 60◦ by combining the existing Large Area Survey, Galactic Plane Survey and Galactic Clusters Survey conducted under the UKIRT Infra-red Deep Sky Survey (UKIDSS) programme with this new additional area not covered by UKIDSS. …”
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    Seafloor silicification and hardground development during deposition of 2.5 Ga banded iron formations by Rasmussen, Birger, Krapež, Bryan, Muhling, Janet

    Published 2015
    “…Banded iron formations (BIFs) are important archives of the ancient oceans, atmosphere, and biosphere, but fundamental questions remain about their origin. …”
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    Comprehensive view of a z ∼ 6.5 radio-loud quasi-stellar object: From the radio to the optical/NIR to the X-ray band by Ighina, Luca, Caccianiga, A., Moretti, A., Broderick, Jess, Leung, J.K., Paterson, Sean, Rigamonti, F., Seymour, Nick, Belladitta, S., Drouart, G., Galvin, T.J., Hurley-Walker, Natasha

    Published 2024
    “…We present a multi-wavelength analysis, from the radio to the X-ray band, of the redshift z=6.44 VIK J2318-31 radio-loud quasi-stellar object, one of the most distant currently known of this class. …”
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    Development of suspended particulate matter empirical equation for tropics estuary from landsat ETM+ data by Zakariya, razak, Ahmad, Zuhairi, Saad, Shahbudin, Rosnan, Y.

    Published 2015
    “…In this study, we have developed empirical relationship based on a strong relationship between Landsat near infrared (NIR) band and archived SPM data. The following were the power equations: SPM NE (mg/l) = 11.68x^0.666 SPM SW (mg/l) = 18.61x^0.493 where, x (TM4) is radiance of ETM+ NIR band 4 was developed under tropical atmospheric conditions. …”
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    Solar Radio Burst Statistics and Implications for Space Weather Effects by Giersch, O., Kennewell, J., Lynch, Mervyn

    Published 2017
    “…However, over the last decade a series of extreme L band solar radio bursts in December 2006 have renewed interest in these effects. …”
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    The VISTA deep extragalactic observations (VIDEO) survey by Jarvis, M., Bonfield, D., Bruce, V., Geach, J., McAlpine, K., McLure, R., González-Solares, E., Irwin, M., Lewis, J., Yoldas, A., Andreon, S., Cross, N., Emerson, J., Dalton, G., Dunlop, J., Hodgkin, S., Le Févre, O., Karouzos, M., Meisenheimer, K., Oliver, S., Rawlings, S., Simpson, C., Smail, I., Smith, D., Sullivan, M., Sutherland, W., White, Sarah, Zwart, J.

    Published 2013
    “…All images and catalogues presented in this paper are publicly available through ESO's phase 3 archive and the VISTA Science Archive. © 2012 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.…”
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    Breakthrough Listen follow-up of the reported transient signal observed at the Arecibo Telescope in the direction of Ross 128 by Enriquez, J., Siemion, A., Dana, R., Croft, S., Méndez, A., Xu, A., DeBoer, D., Gajjar, V., Hellbourg, Gregory, Isaacson, H., others

    Published 2017
    “…We report here the non-detections from the GBT observations in C band (4–8 GHz), as well as non-detections in archival data at L band (1.1–1.9 GHz). …”
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    The Nature of the Bright ULX X-2 in NGC 3921: A Chandra Position and HST Candidate Counterpart by Jonker, P., Heida, M., Torres, M., Miller-Jones, James, Fabian, A., Ratti, E., Miniutti, G., Walton, D., Roberts, T.

    Published 2012
    “…Furthermore, converting the 1994 F336W and 2000 F300W WFPC2 and the 2010 F336W WFC3 observations to the Johnson U-band filter assuming a spectral type of O7I, we find evidence for a brightening of the U-band light in 2000. …”
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    A study of diffuse radio sources and X-ray emission in six massive clusters by Parekh, V., Dwarakanath, K., Kale, R., Intema, Hubertus

    Published 2017
    “…Here, we report GMRT and EVLA radio observations of six galaxy clusters taken from the MAssive Cluster Survey (MACS) catalogue to detect diffuse radio emission. We used archival GMRT (150, 235, and 610 MHz) and EVLA (L band) data and made images at multiple radio frequencies of the following six clusters – MACSJ0417.5−1154, MACSJ1131.8−1955, MACSJ0308.9+2645, MACSJ2243.3−0935, MACSJ2228.5+2036, and MACSJ0358.8−2955. …”
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    Revisiting the ultraluminous supersoft source in M 101: An optically thick outflow model by Soria, Roberto, Kong, A.

    Published 2016
    “…The origin of the thermal component and the relation between ULSs and standard (broad-band spectrum) ultraluminous X-ray sources are still controversial. …”
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