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Characterization of trace gas emissions at an intermediate port

Wiacek, A.; Li, L.; Tobin, K.; Mitchell, M. (European Geosciences Union Copernicus Publications, 2018)

NLTE Stellar Population Synthesis of Globular Clusters Using Synthetic Integrated Light Spectra. II. Expanded Photometry and Sensitivity of Near-IR Spectral Features to Cluster Age and Metallicity

Young, Mitchell E.; Short, C. Ian (American Astronomical Society, 2019)

Mercury Concentrations in Double-Crested Cormorant Chicks Across Canada

Lavoie, R.A.; Campbell, Linda M. (Springer Netherlands, 2018)

yy Mono- and Bis(imidazolidinium ethynyl) Cations and Reduction of the Latter To Give an Extended Bis-1,4-([3]Cumulene)-p-carboquinoid System

Barry, B.M.; Soper, R.G.; Hurmalainen, J.; Mansikkamaki, A.; Robertson, K.N.; McClennan, W.L.; Veinot, A.J.; Roemmele, T.L.; Clyburne, J.A.C.; Masuda, Jason D. (2018)

STRUCTURE OF Na-26 VIA A NOVEL TECHNIQUE USING (d, p gamma) WITH A RADIOACTIVE Na-25 BEAM

Catford, W.N.; Celik, I.C.; Wilson, G.L.; Matta, A.; Orr, N.; Diget, C.; Adsley, P.; Al-Falou, H.; Austin, R.A.; Kanungo, R. (Jagiellonian University, 2015)

The CFHT large area U-band deep survey (CLAUDS)

Sawicki, Marcin, 1969-; Arnouts, Stephane; Huang, Jiasheng; Coupon, Jean; Golob, Anneya; Gwyn, Stephen; Moutard, Thibaud; Iwata, Ikuru; Chen, Lingjian; Thibert, Nathalie (Oxford University Press on behalf of the Royal Astronomical Society, 2019-09-09)

The Canada–France–Hawaii Telescope (CFHT) Large Area U-band Deep Survey (CLAUDS) uses data taken with the MegaCam mosaic imager on CFHT to produce images of 18.60 de ...

X-ray spectral variability of blazars using principal component analysis

Gallant, D.; Gallo, Luigi C.; Parker, M.L. (Oxford University Press, 2018-07-25)

Principal component analysis (PCA) is applied to a variety of blazars to examine X-ray spectral variability. Data from nine different objects are analysed in two ways: long-term, which examines variability trends across ...

Variable blurred reflection in the narrow-line Seyfert 1 galaxy Mrk 493

Bonson, K.; Gallo, Luigi C.; Wilkins, D.R.; Fabian, A.C. (Oxford University PressOxford University Press on behalf of the Royal Astronomical Society, 2018-04-04)

We examine a 200 ks XMM–Newton observation of the narrow-line Seyfert 1 galaxy Mrk 493. The active galaxy was half as bright as in a previous 2003 snapshot observation ...

The variability of the warm absorber in I Zwicky 1 as seen by XMM-Newton

Silva, C.V.; Costantini, E.; Kriss, G.A.; Brandt, W.N.; Gallo, Luigi C.; Wilkins, D.R. (Oxford University Press on behalf of the Royal Astronomical Society, 2018-07-20)

We present new XMM–Newton observations of the intriguing warm absorber in I Zwicky 1. This luminous and nearby narrow-line Seyfert 1 galaxy shows ionized absorption by two components of outflowing ...

The remarkable X-ray variability of IRAS 13224-3809 - I. The variability process

Alston, W.N.; Fabian, A.C.; Buisson, D.J.K.; Kara, Erin; Parker, M.L.; Lohfink, A.; Uttley, P.; Wilkins, D.R.; Pinto, C.; Gallo, Luigi C. (Oxford University PressOxford University Press on behalf of the Royal Astronomical Society, 2018-09-14)

We present a detailed X-ray timing analysis of the highly variable narrow-line Seyfert 1 (NLS1) galaxy IRAS 13224–3809. The source was recently monitored for 1.5 Ms with XMM–Newton, ...

The Gaia-ESO Survey: matching chemodynamical simulations to observations of the Milky Way

Thompson, B.B.; Few, C.G.; Bergemann, M.; Gibson, B.K.; MacFarlane, B.A.; Serenelli, A.; Gilmore, G.; Randich, S.; Vallenari, A.; Alfaro, E.J. (Oxford University Press on behalf of the Royal Astronomical Society, 2017-09-11)

The typical methodology for comparing simulated galaxies with observational surveys is usually to apply a spatial selection to the simulation to mimic the region of interest covered by a comparable observational survey ...

The 1.5Ms observing campaign on IRAS 13224-3809-I. X-ray spectral analysis

Jiang, J.; Parker, M.L.; Fabian, A.C.; Alston, W.N.; Buisson, D.J.K.; Cackett, E.M.; Chiang, C.Y.; Dauser, T.; Gallo, Luigi C.; Garcia, J.A. (Oxford University Press, 2018)

Spatially unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem

Sorba, Robert; Sawicki, Marcin, 1969- (Oxford University PressRoyal Astronomical Society, 2018-05)

We perform spatially resolved, pixel-by-pixel Spectral Energy Distribution (SED) fitting on galaxies up to z ∼ 2.5 in the Hubble eXtreme Deep Field (XDF). Comparing stellar mass estimates from spatially resolved and ...

Photometric variability of TW Hya from seconds to years as seen from space and the ground during 2013-2017

Siwak, M.; Ogloza, W.; Moffat, A.F.J.; Matthews, J.M.; Rusinski, S.M.; Kallinger, T.; Kushnig, R.; Cameron, C.; Weiss, W.W.; David B. Guenther (Oxford University PressRoyal Astronomical Society, 2018-06-02)

This is the final photometric study of TW Hya based on new MOST satellite observations. During 2014 and 2017, the light curves showed stable 3.75- and 3.69-d quasi-periodic oscillations, respectively. ...

On the lack of correlation between [O III]/[O II] and Lyman continuum escape fraction

Bassett, R.; Ryan-Weber, E.V.; Cooke, J.; DAaz, C.; Nanayakkara, T.; Yuan, T.; Spitler, L.; Mestric, U.; Sawicki, Marcin, 1969-; Golob, Anneya (Oxford University Press, 2018-12-10)

We present the first results of our pilot study of eight photometrically selected Lyman-continuum (LyC) emitting galaxy candidates from the COSMOS field and focus on their optical emission line ratios. Observations were ...

On the fast quenching of young low-mass galaxies up to z similar to 0.6: new spotlight on the lead role of environment

Moutard, Thibaud; Sawicki, Marcin; Arnouts, S.; Golob, Anneya; Malavasi, N.; Adami, C.; Coupon, J.; Ilbert, O. (Oxford University Press, 2018)

Observational constraints on the physical nature of submillimetre source multiplicity: chance projections are common

Hayward, C.C.; Chapman, S.C.; Steidal, C.C.; Golob, A.; Casey, C.M.; Smith, D.J.B.; Zitrin, A.; Blain, A.W.; Bremner, M.N.; Sawicki, Marcin (Oxford University Press, 2018)

Is there a UV/X-ray connection in IRAS 13224-3809?

Buisson, D.J.K.; Lohfink, A.M.; Alton, W.M.; Cackett, E.M.; Chiang, C.Y.; Dauser, T.; De Marco, B.; Fabian, A.C.; Gallo, Luigi C.; Garcia, J.A. (Oxford University Press on behalf of the Royal Astronomical Society, 2018-01-05)

We present results from the optical, ultraviolet, and X-ray monitoring of the NLS1 galaxy IRAS 13224−3809 taken with Swift and XMM–Newton during 2016. IRAS 13224−3809 ...

On stellar mass loss from galaxies in groups and clusters

Tollet, E.; Cattaneo, A.; Mamon, G.A.; Moutard, Thibaud; van den Bosch, F.C. (Oxford University Press, 2017-07-20)

We estimate the stellar mass that satellite galaxies lose once they enter groups (and clusters) by identifying groups in a high-resolution cosmological N-body simulation, assigning entry masses to satellite ...

Eleven years of monitoring the Seyfert 1 Mrk 335 with Swift: Characterizing the X-ray and UV/optical variability

Gallo, Luigi C.; Blue, D.M.; Grupe, D.; Komossa, S.; Wilkins, D.R. (Oxford University Press, 2018)

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