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Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10(11) solar masses.

Nature

Amblard A, Cooray A, Serra P, Altieri B, Arumugam V, Aussel H, Blain A, Bock J, Boselli A, Buat V, Castro-Rodríguez N, Cava A, Chanial P, Chapin E, Clements DL, Conley A, Conversi L, Dowell CD, Dwek E, Eales S, Elbaz D, Farrah D, Franceschini A, Gear W, Glenn J, Griffin M, Halpern M, Hatziminaoglou E, Ibar E, Isaak K, Ivison RJ, Khostovan AA, Lagache G, Levenson L, Lu N, Madden S, Maffei B, Mainetti G, Marchetti L, Marsden G, Mitchell-Wynne K, Nguyen HT, O'Halloran B, Oliver SJ, Omont A, Page MJ, Panuzzo P, Papageorgiou A, Pearson CP, Pérez-Fournon I, Pohlen M, Rangwala N, Roseboom IG, Rowan-Robinson M, Portal MS, Schulz B, Scott D, Seymour N, Shupe DL, Smith AJ, Stevens JA, Symeonidis M, Trichas M, Tugwell K, Vaccari M, Valiante E, Valtchanov I, Vieira JD, Vigroux L, Wang L, Ward R, Wright G, Xu CK, Zemcov M.
PMID: 21326201
Nature. 2011 Feb 24;470(7335):510-2. doi: 10.1038/nature09771. Epub 2011 Feb 16.

The extragalactic background light at far-infrared wavelengths comes from optically faint, dusty, star-forming galaxies in the Universe with star formation rates of a few hundred solar masses per year. These faint, submillimetre galaxies are challenging to study individually because...

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Amblard A, Cooray A, Serra P, et al. Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10(11) solar masses. Nature. 2011;470(7335):510-2doi: 10.1038/nature09771.
Amblard, A., Cooray, A., Serra, P., Altieri, B., Arumugam, V., Aussel, H., Blain, A., Bock, J., Boselli, A., Buat, V., Castro-Rodríguez, N., Cava, A., Chanial, P., Chapin, E., Clements, D. L., Conley, A., Conversi, L., Dowell, C. D., Dwek, E., Eales, S., Elbaz, D., Farrah, D., Franceschini, A., Gear, W., Glenn, J., Griffin, M., Halpern, M., Hatziminaoglou, E., Ibar, E., Isaak, K., Ivison, R. J., Khostovan, A. A., Lagache, G., Levenson, L., Lu, N., Madden, S., Maffei, B., Mainetti, G., Marchetti, L., Marsden, G., Mitchell-Wynne, K., Nguyen, H. T., O'Halloran, B., Oliver, S. J., Omont, A., Page, M. J., Panuzzo, P., Papageorgiou, A., Pearson, C. P., Pérez-Fournon, I., Pohlen, M., Rangwala, N., Roseboom, I. G., Rowan-Robinson, M., Portal, M. S., Schulz, B., Scott, D., Seymour, N., Shupe, D. L., Smith, A. J., Stevens, J. A., Symeonidis, M., Trichas, M., Tugwell, K., Vaccari, M., Valiante, E., Valtchanov, I., Vieira, J. D., Vigroux, L., Wang, L., Ward, R., Wright, G., Xu, C. K., & Zemcov, M. (2011). Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10(11) solar masses. Nature, 470(7335), 510-2. https://doi.org/10.1038/nature09771
Amblard, Alexandre, et al. "Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10(11) solar masses." Nature vol. 470,7335 (2011): 510-2. doi: https://doi.org/10.1038/nature09771
Amblard A, Cooray A, Serra P, Altieri B, Arumugam V, Aussel H, Blain A, Bock J, Boselli A, Buat V, Castro-Rodríguez N, Cava A, Chanial P, Chapin E, Clements DL, Conley A, Conversi L, Dowell CD, Dwek E, Eales S, Elbaz D, Farrah D, Franceschini A, Gear W, Glenn J, Griffin M, Halpern M, Hatziminaoglou E, Ibar E, Isaak K, Ivison RJ, Khostovan AA, Lagache G, Levenson L, Lu N, Madden S, Maffei B, Mainetti G, Marchetti L, Marsden G, Mitchell-Wynne K, Nguyen HT, O'Halloran B, Oliver SJ, Omont A, Page MJ, Panuzzo P, Papageorgiou A, Pearson CP, Pérez-Fournon I, Pohlen M, Rangwala N, Roseboom IG, Rowan-Robinson M, Portal MS, Schulz B, Scott D, Seymour N, Shupe DL, Smith AJ, Stevens JA, Symeonidis M, Trichas M, Tugwell K, Vaccari M, Valiante E, Valtchanov I, Vieira JD, Vigroux L, Wang L, Ward R, Wright G, Xu CK, Zemcov M. Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10(11) solar masses. Nature. 2011 Feb 24;470(7335):510-2. doi: 10.1038/nature09771. Epub 2011 Feb 16. PMID: 21326201.
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Cerebral air embolism following transbronchial lung biopsy during flexible bronchoscopy.

Respiratory medicine case reports

Evison M, Crosbie PA, Bright-Thomas R, Alaloul M, Booton R.
PMID: 26029537
Respir Med Case Rep. 2014 Mar 28;12:39-40. doi: 10.1016/j.rmcr.2013.10.005. eCollection 2014.

During a diagnostic flexible bronchoscopy an 84 year old patient suffered a sudden reduction in conscious level following a transbronchial lung biopsy. A subsequent computed tomography brain scan confirmed cerebral air emboli. The patient survived following a period of...

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Evison M, Crosbie PA, Bright-Thomas R, et al. Cerebral air embolism following transbronchial lung biopsy during flexible bronchoscopy. Respir Med Case Rep. 2014;12:39-40doi: 10.1016/j.rmcr.2013.10.005.
Evison, M., Crosbie, P. A., Bright-Thomas, R., Alaloul, M., & Booton, R. (2014). Cerebral air embolism following transbronchial lung biopsy during flexible bronchoscopy. Respiratory medicine case reports, 1239-40. https://doi.org/10.1016/j.rmcr.2013.10.005
Evison, Matthew, et al. "Cerebral air embolism following transbronchial lung biopsy during flexible bronchoscopy." Respiratory medicine case reports vol. 12 (2014): 39-40. doi: https://doi.org/10.1016/j.rmcr.2013.10.005
Evison M, Crosbie PA, Bright-Thomas R, Alaloul M, Booton R. Cerebral air embolism following transbronchial lung biopsy during flexible bronchoscopy. Respir Med Case Rep. 2014 Mar 28;12:39-40. doi: 10.1016/j.rmcr.2013.10.005. eCollection 2014. PMID: 26029537; PMCID: PMC4061444.
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Logical memory in the wechsler memory scales - does the order of passages affect difficulty in an university sample?.

The Clinical neuropsychologist

Ivison D.
PMID: 29022475
Clin Neuropsychol. 1993 Apr;7(2):215-218. doi: 10.1080/13854049308401525.

The relative difficulty of the logical memory passages on WMS-1, WMS-2, and WMS-R were investigated in different orders of presentation within and between test forms. No evidence of order effects on difficulty level was obtained though, as expected, the...

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Ivison D. Logical memory in the wechsler memory scales - does the order of passages affect difficulty in an university sample?. Clin Neuropsychol. 1993;7(2):215-218doi: 10.1080/13854049308401525.
Ivison, D. (1993). Logical memory in the wechsler memory scales - does the order of passages affect difficulty in an university sample?. The Clinical neuropsychologist, 7(2), 215-218. https://doi.org/10.1080/13854049308401525
Ivison, David. "Logical memory in the wechsler memory scales - does the order of passages affect difficulty in an university sample?." The Clinical neuropsychologist vol. 7,2 (1993): 215-218. doi: https://doi.org/10.1080/13854049308401525
Ivison D. Logical memory in the wechsler memory scales - does the order of passages affect difficulty in an university sample?. Clin Neuropsychol. 1993 Apr;7(2):215-218. doi: 10.1080/13854049308401525. PMID: 29022475.
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Gone with the heat: a fundamental constraint on the imaging of dust and molecular gas in the early Universe.

Royal Society open science

Zhang ZY, Papadopoulos PP, Ivison RJ, Galametz M, Smith MW, Xilouris EM.
PMID: 27429763
R Soc Open Sci. 2016 Jun 08;3(6):160025. doi: 10.1098/rsos.160025. eCollection 2016 Jun.

Images of dust continuum and carbon monoxide (CO) line emission are powerful tools for deducing structural characteristics of galaxies, such as disc sizes, H2 gas velocity fields and enclosed H2 and dynamical masses. We report on a fundamental constraint...

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Zhang ZY, Papadopoulos PP, Ivison RJ, et al. Gone with the heat: a fundamental constraint on the imaging of dust and molecular gas in the early Universe. R Soc Open Sci. 2016;3(6):160025doi: 10.1098/rsos.160025.
Zhang, Z. Y., Papadopoulos, P. P., Ivison, R. J., Galametz, M., Smith, M. W., & Xilouris, E. M. (2016). Gone with the heat: a fundamental constraint on the imaging of dust and molecular gas in the early Universe. Royal Society open science, 3(6), 160025. https://doi.org/10.1098/rsos.160025
Zhang, Zhi-Yu, et al. "Gone with the heat: a fundamental constraint on the imaging of dust and molecular gas in the early Universe." Royal Society open science vol. 3,6 (2016): 160025. doi: https://doi.org/10.1098/rsos.160025
Zhang ZY, Papadopoulos PP, Ivison RJ, Galametz M, Smith MW, Xilouris EM. Gone with the heat: a fundamental constraint on the imaging of dust and molecular gas in the early Universe. R Soc Open Sci. 2016 Jun 08;3(6):160025. doi: 10.1098/rsos.160025. eCollection 2016 Jun. PMID: 27429763; PMCID: PMC4929898.
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A study of patients with isolated mediastinal and hilar lymphadenopathy undergoing EBUS-TBNA.

BMJ open respiratory research

Evison M, Crosbie PA, Morris J, Martin J, Barber PV, Booton R.
PMID: 25478187
BMJ Open Respir Res. 2014 May 31;1(1):e000040. doi: 10.1136/bmjresp-2014-000040. eCollection 2014.

BACKGROUND: Isolated mediastinal and/or hilar lymphadenopathy (IMHL) may be caused by benign and malignant disorders or be 'reactive'. Endobronchial ultrasound-guided transbronchial needle aspiration (EBUS-TBNA) has a reported low negative predictive value (NPV) in IMHL, necessitating mediastinoscopy in selected patients....

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Evison M, Crosbie PA, Morris J, et al. A study of patients with isolated mediastinal and hilar lymphadenopathy undergoing EBUS-TBNA. BMJ Open Respir Res. 2014;1(1):e000040doi: 10.1136/bmjresp-2014-000040.
Evison, M., Crosbie, P. A., Morris, J., Martin, J., Barber, P. V., & Booton, R. (2014). A study of patients with isolated mediastinal and hilar lymphadenopathy undergoing EBUS-TBNA. BMJ open respiratory research, 1(1), e000040. https://doi.org/10.1136/bmjresp-2014-000040
Evison, Matthew, et al. "A study of patients with isolated mediastinal and hilar lymphadenopathy undergoing EBUS-TBNA." BMJ open respiratory research vol. 1,1 (2014): e000040. doi: https://doi.org/10.1136/bmjresp-2014-000040
Evison M, Crosbie PA, Morris J, Martin J, Barber PV, Booton R. A study of patients with isolated mediastinal and hilar lymphadenopathy undergoing EBUS-TBNA. BMJ Open Respir Res. 2014 May 31;1(1):e000040. doi: 10.1136/bmjresp-2014-000040. eCollection 2014. PMID: 25478187; PMCID: PMC4212715.
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Type II supernovae as a significant source of interstellar dust.

Nature

Dunne L, Eales S, Ivison R, Morgan H, Edmunds M.
PMID: 12867973
Nature. 2003 Jul 17;424(6946):285-7. doi: 10.1038/nature01792.

Large amounts of dust (>10(8)M(o)) have recently been discovered in high-redshift quasars and galaxies corresponding to a time when the Universe was less than one-tenth of its present age. The stellar winds produced by stars in the late stages...

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Dunne L, Eales S, Ivison R, et al. Type II supernovae as a significant source of interstellar dust. Nature. 2003;424(6946):285-7doi: 10.1038/nature01792.
Dunne, L., Eales, S., Ivison, R., Morgan, H., & Edmunds, M. (2003). Type II supernovae as a significant source of interstellar dust. Nature, 424(6946), 285-7. https://doi.org/10.1038/nature01792
Dunne, Loretta, et al. "Type II supernovae as a significant source of interstellar dust." Nature vol. 424,6946 (2003): 285-7. doi: https://doi.org/10.1038/nature01792
Dunne L, Eales S, Ivison R, Morgan H, Edmunds M. Type II supernovae as a significant source of interstellar dust. Nature. 2003 Jul 17;424(6946):285-7. doi: 10.1038/nature01792. PMID: 12867973.
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Modeling the Evolution and Rupture of Pendular Liquid Bridges in the Presence of Large Wetting Hysteresis.

Journal of colloid and interface science

Pepin X, Rossetti D, Iveson SM, Simons SJ.
PMID: 11097763
J Colloid Interface Sci. 2000 Dec 15;232(2):289-297. doi: 10.1006/jcis.2000.7182.

A model has been developed to predict the shape evolution, rupture distance and postrupture liquid distribution of a pendular liquid bridge between two unequally sized spherical particles in the presence of wetting hysteresis. Two different simplifications of the bridge...

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Pepin X, Rossetti D, Iveson SM, et al. Modeling the Evolution and Rupture of Pendular Liquid Bridges in the Presence of Large Wetting Hysteresis. J Colloid Interface Sci. 2000;232(2):289-297doi: 10.1006/jcis.2000.7182.
Pepin, X., Rossetti, D., Iveson, S. M., & Simons, S. J. (2000). Modeling the Evolution and Rupture of Pendular Liquid Bridges in the Presence of Large Wetting Hysteresis. Journal of colloid and interface science, 232(2), 289-297. https://doi.org/10.1006/jcis.2000.7182
Pepin, et al. "Modeling the Evolution and Rupture of Pendular Liquid Bridges in the Presence of Large Wetting Hysteresis." Journal of colloid and interface science vol. 232,2 (2000): 289-297. doi: https://doi.org/10.1006/jcis.2000.7182
Pepin X, Rossetti D, Iveson SM, Simons SJ. Modeling the Evolution and Rupture of Pendular Liquid Bridges in the Presence of Large Wetting Hysteresis. J Colloid Interface Sci. 2000 Dec 15;232(2):289-297. doi: 10.1006/jcis.2000.7182. PMID: 11097763.
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The formation of cluster elliptical galaxies as revealed by extensive star formation.

Nature

Stevens JA, Ivison RJ, Dunlop JS, Smail IR, Percival WJ, Hughes DH, Röttgering HJ, Van Breugel WJ, Reuland M.
PMID: 13679908
Nature. 2003 Sep 18;425(6955):264-7. doi: 10.1038/nature01976.

The most massive galaxies in the present-day Universe are found to lie in the centres of rich clusters. They have old, coeval stellar populations suggesting that the bulk of their stars must have formed at early epochs in spectacular...

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Stevens JA, Ivison RJ, Dunlop JS, et al. The formation of cluster elliptical galaxies as revealed by extensive star formation. Nature. 2003;425(6955):264-7doi: 10.1038/nature01976.
Stevens, J. A., Ivison, R. J., Dunlop, J. S., Smail, I. R., Percival, W. J., Hughes, D. H., Röttgering, H. J., Van Breugel, W. J., & Reuland, M. (2003). The formation of cluster elliptical galaxies as revealed by extensive star formation. Nature, 425(6955), 264-7. https://doi.org/10.1038/nature01976
Stevens, J A, et al. "The formation of cluster elliptical galaxies as revealed by extensive star formation." Nature vol. 425,6955 (2003): 264-7. doi: https://doi.org/10.1038/nature01976
Stevens JA, Ivison RJ, Dunlop JS, Smail IR, Percival WJ, Hughes DH, Röttgering HJ, Van Breugel WJ, Reuland M. The formation of cluster elliptical galaxies as revealed by extensive star formation. Nature. 2003 Sep 18;425(6955):264-7. doi: 10.1038/nature01976. PMID: 13679908.
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Intense star formation within resolved compact regions in a galaxy at z = 2.3.

Nature

Swinbank AM, Smail I, Longmore S, Harris AI, Baker AJ, De Breuck C, Richard J, Edge AC, Ivison RJ, Blundell R, Coppin KE, Cox P, Gurwell M, Hainline LJ, Krips M, Lundgren A, Neri R, Siana B, Siringo G, Stark DP, Wilner D, Younger JD.
PMID: 20305639
Nature. 2010 Apr 01;464(7289):733-6. doi: 10.1038/nature08880. Epub 2010 Mar 21.

Massive galaxies in the early Universe have been shown to be forming stars at surprisingly high rates. Prominent examples are dust-obscured galaxies which are luminous when observed at sub-millimetre wavelengths and which may be forming stars at a rate...

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Swinbank AM, Smail I, Longmore S, et al. Intense star formation within resolved compact regions in a galaxy at z = 2.3. Nature. 2010;464(7289):733-6doi: 10.1038/nature08880.
Swinbank, A. M., Smail, I., Longmore, S., Harris, A. I., Baker, A. J., De Breuck, C., Richard, J., Edge, A. C., Ivison, R. J., Blundell, R., Coppin, K. E., Cox, P., Gurwell, M., Hainline, L. J., Krips, M., Lundgren, A., Neri, R., Siana, B., Siringo, G., Stark, D. P., Wilner, D., & Younger, J. D. (2010). Intense star formation within resolved compact regions in a galaxy at z = 2.3. Nature, 464(7289), 733-6. https://doi.org/10.1038/nature08880
Swinbank, A M, et al. "Intense star formation within resolved compact regions in a galaxy at z = 2.3." Nature vol. 464,7289 (2010): 733-6. doi: https://doi.org/10.1038/nature08880
Swinbank AM, Smail I, Longmore S, Harris AI, Baker AJ, De Breuck C, Richard J, Edge AC, Ivison RJ, Blundell R, Coppin KE, Cox P, Gurwell M, Hainline LJ, Krips M, Lundgren A, Neri R, Siana B, Siringo G, Stark DP, Wilner D, Younger JD. Intense star formation within resolved compact regions in a galaxy at z = 2.3. Nature. 2010 Apr 01;464(7289):733-6. doi: 10.1038/nature08880. Epub 2010 Mar 21. PMID: 20305639.
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Detection of a noble gas molecular ion, 36ArH+, in the Crab Nebula.

Science (New York, N.Y.)

Barlow MJ, Swinyard BM, Owen PJ, Cernicharo J, Gomez HL, Ivison RJ, Krause O, Lim TL, Matsuura M, Miller S, Olofsson G, Polehampton ET.
PMID: 24337290
Science. 2013 Dec 13;342(6164):1343-5. doi: 10.1126/science.1243582.

Noble gas molecules have not hitherto been detected in space. From spectra obtained with the Herschel Space Observatory, we report the detection of emission in the 617.5- and 1234.6-gigahertz J = 1-0 and 2-1 rotational lines of (36)ArH(+) at...

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Barlow MJ, Swinyard BM, Owen PJ, et al. Detection of a noble gas molecular ion, 36ArH+, in the Crab Nebula. Science. 2013;342(6164):1343-5doi: 10.1126/science.1243582.
Barlow, M. J., Swinyard, B. M., Owen, P. J., Cernicharo, J., Gomez, H. L., Ivison, R. J., Krause, O., Lim, T. L., Matsuura, M., Miller, S., Olofsson, G., & Polehampton, E. T. (2013). Detection of a noble gas molecular ion, 36ArH+, in the Crab Nebula. Science (New York, N.Y.), 342(6164), 1343-5. https://doi.org/10.1126/science.1243582
Barlow, M J, et al. "Detection of a noble gas molecular ion, 36ArH+, in the Crab Nebula." Science (New York, N.Y.) vol. 342,6164 (2013): 1343-5. doi: https://doi.org/10.1126/science.1243582
Barlow MJ, Swinyard BM, Owen PJ, Cernicharo J, Gomez HL, Ivison RJ, Krause O, Lim TL, Matsuura M, Miller S, Olofsson G, Polehampton ET. Detection of a noble gas molecular ion, 36ArH+, in the Crab Nebula. Science. 2013 Dec 13;342(6164):1343-5. doi: 10.1126/science.1243582. PMID: 24337290.
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Glaucoma Diagnosis and Monitoring Using Advanced Imaging Technologies.

US ophthalmic review

Sehi M, Iverson SM.
PMID: 24470807
US Ophthalmic Rev. 2013;6(1):15-25.

Advanced ocular imaging technologies facilitate objective and reproducible quantification of change in glaucoma but at the same time, impose new challenges on scientists and clinicians for separating true structural change from imaging noise. This review examines time-domain and spectral-domain...

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Sehi M, Iverson SM. Glaucoma Diagnosis and Monitoring Using Advanced Imaging Technologies. US Ophthalmic Rev. 2013;6(1):15-25
Sehi, M., & Iverson, S. M. (2013). Glaucoma Diagnosis and Monitoring Using Advanced Imaging Technologies. US ophthalmic review, 6(1), 15-25.
Sehi, Mitra, and Iverson, Shawn M. "Glaucoma Diagnosis and Monitoring Using Advanced Imaging Technologies." US ophthalmic review vol. 6,1 (2013): 15-25.
Sehi M, Iverson SM. Glaucoma Diagnosis and Monitoring Using Advanced Imaging Technologies. US Ophthalmic Rev. 2013;6(1):15-25. PMID: 24470807; PMCID: PMC3901957.
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Comet-like mineralogy of olivine crystals in an extrasolar proto-Kuiper belt.

Nature

de Vries BL, Acke B, Blommaert JA, Waelkens C, Waters LB, Vandenbussche B, Min M, Olofsson G, Dominik C, Decin L, Barlow MJ, Brandeker A, Di Francesco J, Glauser AM, Greaves J, Harvey PM, Holland WS, Ivison RJ, Liseau R, Pantin EE, Pilbratt GL, Royer P, Sibthorpe B.
PMID: 23038467
Nature. 2012 Oct 04;490(7418):74-6. doi: 10.1038/nature11469.

Some planetary systems harbour debris disks containing planetesimals such as asteroids and comets. Collisions between such bodies produce small dust particles, the spectral features of which reveal their composition and, hence, that of their parent bodies. A measurement of...

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de Vries BL, Acke B, Blommaert JA, et al. Comet-like mineralogy of olivine crystals in an extrasolar proto-Kuiper belt. Nature. 2012;490(7418):74-6doi: 10.1038/nature11469.
de Vries, B. L., Acke, B., Blommaert, J. A., Waelkens, C., Waters, L. B., Vandenbussche, B., Min, M., Olofsson, G., Dominik, C., Decin, L., Barlow, M. J., Brandeker, A., Di Francesco, J., Glauser, A. M., Greaves, J., Harvey, P. M., Holland, W. S., Ivison, R. J., Liseau, R., Pantin, E. E., Pilbratt, G. L., Royer, P., & Sibthorpe, B. (2012). Comet-like mineralogy of olivine crystals in an extrasolar proto-Kuiper belt. Nature, 490(7418), 74-6. https://doi.org/10.1038/nature11469
de Vries, B L, et al. "Comet-like mineralogy of olivine crystals in an extrasolar proto-Kuiper belt." Nature vol. 490,7418 (2012): 74-6. doi: https://doi.org/10.1038/nature11469
de Vries BL, Acke B, Blommaert JA, Waelkens C, Waters LB, Vandenbussche B, Min M, Olofsson G, Dominik C, Decin L, Barlow MJ, Brandeker A, Di Francesco J, Glauser AM, Greaves J, Harvey PM, Holland WS, Ivison RJ, Liseau R, Pantin EE, Pilbratt GL, Royer P, Sibthorpe B. Comet-like mineralogy of olivine crystals in an extrasolar proto-Kuiper belt. Nature. 2012 Oct 04;490(7418):74-6. doi: 10.1038/nature11469. PMID: 23038467.
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