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14 results on '"Namumba, B."'

1. MHONGOOSE -- A MeerKAT Nearby Galaxy HI Survey

Author

de Blok, W. J. G., Healy, J., Maccagni, F. M., Pisano, D. J., Bosma, A., English, J., Jarrett, T., Marasco, A., Meurer, G. R., Veronese, S., Bigiel, F., Chemin, L., Fraternali, F., Holwerda, B. W., Kamphuis, P., Klöckner, H. R., Kleiner, D., Leroy, A. K., Mogotsi, M., Oman, K. A., Schinnerer, E., Verdes-Montenegro, L., Westmeier, T., Wong, O. I., Zabel, N., Amram, P., Carignan, C., Combes, F., Brinks, E., Dettmar, R. J., Gibson, B. K., Jozsa, G. I. G., Koribalski, B. S., McGaugh, S. S., Oosterloo, T. A., Spekkens, K., Schröder, A. C., Adams, E. A. K., Athanassoula, E., Bershady, M. A., Beswick, R. J., Blyth, S., Elson, E. C., Frank, B. S., Heald, G., Henning, P. A., Kurapati, S., Loubser, S. I., Lucero, D., Meyer, M., Namumba, B., Oh, S. -H., Sardone, A., Sheth, K., Smith, M. W. L., Sorgho, A., Walter, F., Williams, T., Woudt, P. A., and Zijlstra, A.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

The MHONGOOSE (MeerKAT HI Observations of Nearby Galactic Objects: Observing Southern Emitters) survey maps the distribution and kinematics of the neutral atomic hydrogen (HI) gas in and around 30 nearby star-forming spiral and dwarf galaxies to extremely low HI column densities. The HI column density sensitivity (3 sigma over 16 km/s) ranges from ~ 5 x 10^{17} cm^{-2} at 90'' resolution to ~4 x 10^{19} cm^{-2} at the highest resolution of 7''. The HI mass sensitivity (3 sigma over 50 km/s) is ~5.5 X 10^5 M_sun at a distance of 10 Mpc (the median distance of the sample galaxies). The velocity resolution of the data is 1.4 km/s. One of the main science goals of the survey is the detection of cold, accreting gas in the outskirts of the sample galaxies. The sample was selected to cover a range in HI masses, from 10^7 M_sun to almost 10^{11} M_sun, to optimally sample possible accretion scenarios and environments. The distance to the sample galaxies ranges from 3 to 23 Mpc. In this paper, we present the sample selection, survey design, and observation and reduction procedures. We compare the integrated HI fluxes based on the MeerKAT data with those derived from single-dish measurement and find good agreement, indicating that our MeerKAT observations are recovering all flux. We present HI moment maps of the entire sample based on the first ten percent of the survey data, and find that a comparison of the zeroth- and second-moment values shows a clear separation between the physical properties of the HI in areas with star formation and areas without, related to the formation of a cold neutral medium. Finally, we give an overview of the HI-detected companion and satellite galaxies in the 30 fields, five of which have not previously been catalogued. We find a clear relation between the number of companion galaxies and the mass of the main target galaxy., Comment: Accepted for publication in Astronomy & Astrophysics

Published
2024
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2. The MeerKAT Galaxy Cluster Legacy Survey I. Survey Overview and Highlights

Author

Knowles, K., Cotton, W. D., Rudnick, L., Camilo, F., Goedhart, S., Deane, R., Ramatsoku, M., Bietenholz, M. F., Brüggen, M., Button, C., Chen, H., Chibueze, J. O., Clarke, T. E., de Gasperin, F., Ianjamasimanana, R., Józsa, G. I. G., Hilton, M., Kesebonye, K. C., Kolokythas, K., Kraan-Korteweg, R. C., Lawrie, G., Lochner, M., Loubser, S. I., Marchegiani, P., Mhlahlo, N., Moodley, K., Murphy, E., Namumba, B., Oozeer, N., Parekh, V., Pillay, D. S., Passmoor, S. S., Ramaila, A. J. T., Ranchod, S., Retana-Montenegro, E., Sebokolodi, L., Sikhosana, S. P., Smirnov, O., Thorat, K., Venturi, T., Abbott, T. D., Adam, R. M., Adams, G., Aldera, M. A., Bauermeister, E. F., Bennett, T. G. H., Bode, W. A., Botha, D. H., Botha, A. G., Brederode, L. R. S., Buchner, S., Burger, J. P., Cheetham, T., de Villiers, D. I. L., Dikgale-Mahlakoana, M. A., Toit, L. J. du, Esterhuyse, S. W. P., Fadana, G., Fanaroff, B. L., Fataar, S., Foley, A. R., Fourie, D. J., Frank, B. S., Gamatham, R. R. G., Gatsi, T. G., Geyer, M., Gouws, M., Gumede, S. C., Heywood, I., Hlakola, M. J., Hokwana, A., Hoosen, S. W., Horn, D. M., Horrell, J. M. G., Hugo, B. V., Isaacson, A. R., Jonas, J. L., Jordaan, J. D. B., Joubert, A. F., Julie, R. P. M., Kapp, F. B., Kasper, V. A., Kenyon, J. S., Kotzé, P. P. A., Kotze, A. G., Kriek, N., Kriel, H., Krishnan, V. K., Kusel, T. W., Legodi, L. S., Lehmensiek, R., Liebenberg, D., Lord, R. T., Lunsky, B. M., Madisa, K., Magnus, L. G., Main, J. P. L., Makhaba, A., Makhathini, S., Malan, J. A., Manley, J. R., Marais, S. J., Maree, M. D. J., Martens, A., Mauch, T., McAlpine, K., Merry, B. C., Millenaar, R. P., Mokone, O. J., Monama, T. E., Mphego, M. C., New, W. S., Ngcebetsha, B., Ngoasheng, K. J., Ockards, M. T., Otto, A. J., Patel, A. A., Peens-Hough, A., Perkins, S. J., Ramanujam, N. M., Ramudzuli, Z. R., Ratcliffe, S. M., Renil, R., Robyntjies, A., Rust, A. N., Salie, S., Sambu, N., Schollar, C. T. G., Schwardt, L. C., Schwartz, R. L., Serylak, M., Siebrits, R., Sirothia, S. K., Slabber, M., Sofeya, L., Taljaard, B., Tasse, C., Tiplady, A. J., Toruvanda, O., Twum, S. N., van Balla, T. J., van der Byl, A., van der Merwe, C., van Dyk, C. L., Van Tonder, V., Van Wyk, R., Venter, A. J., Venter, M., Welz, M. G., Williams, L. P., and Xaia, B.

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

MeerKAT's large number of antennas, spanning 8 km with a densely packed 1 km core, create a powerful instrument for wide-area surveys, with high sensitivity over a wide range of angular scales. The MeerKAT Galaxy Cluster Legacy Survey (MGCLS) is a programme of long-track MeerKAT L-band (900-1670 MHz) observations of 115 galaxy clusters, observed for $\sim$6-10 hours each in full polarisation. The first legacy product data release (DR1), made available with this paper, includes the MeerKAT visibilities, basic image cubes at $\sim$8" resolution, and enhanced spectral and polarisation image cubes at $\sim$8" and 15" resolutions. Typical sensitivities for the full-resolution MGCLS image products are $\sim$3-5 {\mu}Jy/beam. The basic cubes are full-field and span 4 deg^2. The enhanced products consist of the inner 1.44 deg^2 field of view, corrected for the primary beam. The survey is fully sensitive to structures up to $\sim$10' scales and the wide bandwidth allows spectral and Faraday rotation mapping. HI mapping at 209 kHz resolution can be done at $0

Published
2021
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3. MIGHTEE-HI: The HI emission project of the MeerKAT MIGHTEE survey

Author

Maddox, Natasha, Frank, Bradley S., Ponomareva, A. A., Jarvis, M. J., Adams, E. A. K., Davé, R., Oosterloo, T. A., Santos, M. G., Blyth, S. L., Glowacki, M., Kraan-Korteweg, R. C., Mulaudzi, W., Namumba, B., Prandoni, I., Rajohnson, S. H. A., Spekkens, K., Adams, N. J., Bowler, R. A. A., Collier, J. D., Heywood, I., Sekhar, S., and Taylor, A. R.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

We present the HI emission project within the MIGHTEE survey, currently being carried out with the newly commissioned MeerKAT radio telescope. This is one of the first deep, blind, medium-wide interferometric surveys for neutral hydrogen (HI) ever undertaken, extending our knowledge of HI emission to z=0.6. The science goals of this medium-deep, medium-wide survey are extensive, including the evolution of the neutral gas content of galaxies over the past 5 billion years. Simulations predict nearly 3000 galaxies over 0

Published
2020
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4. An Overview of the MHONGOOSE Survey: Observing Nearby Galaxies with MeerKAT

Author

de Blok, W. J. G., Adams, E. A. K., Amram, P., Athanassoula, E., Bagetakos, I., Balkowski, C., Bershady, M. A., Beswick, R., Bigiel, F., Blyth, S. -L., Bosma, A., Booth, R. S., Bouchard, A., Brinks, E., Carignan, C., Chemin, L., Combes, F., Conway, J., Elson, E. C., English, J., Epinat, B., Frank, B. S., Fiege, J., Fraternali, F., Gallagher, J. S., Gibson, B. K., Heald, G., Henning, P. A., Holwerda, B. W., Jarrett, T. H., Jerjen, H., Józsa, G. I., Kapala, M., Klöckner, H. -R., Koribalski, B. S., Kraan-Korteweg, R. C., Leon, S., Leroy, A., Loubser, S. I., Lucero, D. M., McGaugh, S. S., Meurer, G. R., Meyer, M., Mogotsi, M., Namumba, B., Oh, S-H., Oosterloo, T. A., Pisano, D. J., Popping, A., Ratcliffe, S., Sellwood, J. A., Schinnerer, E., Schröder, A. C., Sheth, K., Smith, M. W. L., Sorgho, A., Spekkens, K., Stanimirovic, S., van der Heyden, K., van Driel, W., Verdes-Montenegro, L., Walter, F., Westmeier, T., Wilcots, E., Williams, T., Wong, O. I., Woudt, P. A., and Zijlstra, A.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

MHONGOOSE is a deep survey of the neutral hydrogen distribution in a representative sample of 30 nearby disk and dwarf galaxies with HI masses from 10^6 to ~10^{11} M_sun, and luminosities from M_R ~ -12 to M_R ~ -22. The sample is selected to uniformly cover the available range in log(M_HI). Our extremely deep observations, down to HI column density limits of well below 10^{18} cm^{-2} - or a few hundred times fainter than the typical HI disks in galaxies - will directly detect the effects of cold accretion from the intergalactic medium and the links with the cosmic web. These observations will be the first ever to probe the very low-column density neutral gas in galaxies at these high resolutions. Combination with data at other wavelengths, most of it already available, will enable accurate modelling of the properties and evolution of the mass components in these galaxies and link these with the effects of environment, dark matter distribution, and other fundamental properties such as halo mass and angular momentum. MHONGOOSE can already start addressing some of the SKA-1 science goals and will provide a comprehensive inventory of the processes driving the transformation and evolution of galaxies in the nearby universe at high resolution and over 5 orders of magnitude in column density. It will be a Nearby Galaxies Legacy Survey that will be unsurpassed until the advent of the SKA, and can serve as a highly visible, lasting statement of MeerKAT's capabilities., Comment: To be published in "MeerKAT Science: On the Pathway to the SKA". Proceedings of Science. Workshop held 25-27 May, 2016 Stellenbosch, South Africa

Published
2017

5. MIGHTEE-H i: possible interactions with the galaxy NGC 895

Author

Namumba, B, primary, Román, J, additional, Falcón-Barroso, J, additional, Knapen, J H, additional, Ianjamasimanana, R, additional, Naluminsa, E, additional, Józsa, G I G, additional, Korsaga, M, additional, Maddox, N, additional, Frank, B, additional, Sikhosana, S, additional, Legodi, S, additional, Carignan, C, additional, Ponomareva, A A, additional, Jarrett, T, additional, Lucero, D, additional, Smirnov, O M, additional, van der Hulst, J M, additional, Pisano, D J, additional, Malek, K, additional, Marchetti, L, additional, Vaccari, M, additional, Jarvis, M, additional, Baes, M, additional, Meyer, M, additional, Adams, E A K, additional, Chen, H, additional, Delhaize, J, additional, Rajohnson, S H A, additional, Kurapati, S, additional, Heywood, I, additional, and Verdes-Montenegro, L, additional

Published
2023
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6. MIGHTEE-H I: possible interactions with the galaxy NGC 895

Author

Ministerio de Ciencia e Innovación (España), Gobierno de Canarias, European Commission, Namumba, B., Román, J., Falcón-Barroso, J., Knapen, J. H., Ianjamasimanana, Roger, Naluminsa, E., Józsa, G. I. G., Korsaga, M., Maddox, N., Frank, B., Sikhosana, S., Legodi, S., Carignan, C., Ponomareva, A. A., Jarrett, T., Lucero, D., Smirnov, O. M., van der Hulst, J. M., Pisano, D. J., Malek, K., Marchetti, L., Vaccari, M., Jarvis, M., Baes, M., Meyer, M., Adams, E. A. K., Chen, H., Delhaize, J., Rajohnson, S. H. A., Kurapati, S., Heywood, I., Verdes-Montenegro, Lourdes, Ministerio de Ciencia e Innovación (España), Gobierno de Canarias, European Commission, Namumba, B., Román, J., Falcón-Barroso, J., Knapen, J. H., Ianjamasimanana, Roger, Naluminsa, E., Józsa, G. I. G., Korsaga, M., Maddox, N., Frank, B., Sikhosana, S., Legodi, S., Carignan, C., Ponomareva, A. A., Jarrett, T., Lucero, D., Smirnov, O. M., van der Hulst, J. M., Pisano, D. J., Malek, K., Marchetti, L., Vaccari, M., Jarvis, M., Baes, M., Meyer, M., Adams, E. A. K., Chen, H., Delhaize, J., Rajohnson, S. H. A., Kurapati, S., Heywood, I., and Verdes-Montenegro, Lourdes

Abstract

The transformation and evolution of a galaxy is strongly influenced by interactions with its environment. Neutral hydrogen (H I) is an excellent way to trace these interactions. Here, we present H I observations of the spiral galaxy NGC 895, which was previously thought to be isolated. High-sensitivity H I observations from the MeerKAT large survey project MIGHTEE reveal possible interaction features, such as extended spiral arms and the two newly discovered H I companions, that drive us to change the narrative that it is an isolated galaxy. We combine these observations with deep optical images from the Hyper Suprime Camera to show an absence of tidal debris between NGC 895 and its companions. We do find an excess of light in the outer parts of the companion galaxy MGTH_J022138.1-052631, which could be an indication of external perturbation and thus possible sign of interactions. Our analysis shows that NGC 895 is an actively star-forming galaxy with a SFR of 1.75 ± 0.09[M⊙/yr], a value typical for high-stellar mass galaxies on the star-forming main sequence. It is reasonable to state that different mechanisms may have contributed to the observed features in NGC 895, and this emphasizes the need to revisit the target with more detailed observations. Our work shows the high potential and synergy of using state-of-the-art data in both H I and optical to reveal a more complete picture of galaxy environments. © 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Published
2023

7. The MeerKAT Galaxy Cluster Legacy Survey

Author

Knowles, K., primary, Cotton, W. D., additional, Rudnick, L., additional, Camilo, F., additional, Goedhart, S., additional, Deane, R., additional, Ramatsoku, M., additional, Bietenholz, M. F., additional, Brüggen, M., additional, Button, C., additional, Chen, H., additional, Chibueze, J. O., additional, Clarke, T. E., additional, de Gasperin, F., additional, Ianjamasimanana, R., additional, Józsa, G. I. G., additional, Hilton, M., additional, Kesebonye, K. C., additional, Kolokythas, K., additional, Kraan-Korteweg, R. C., additional, Lawrie, G., additional, Lochner, M., additional, Loubser, S. I., additional, Marchegiani, P., additional, Mhlahlo, N., additional, Moodley, K., additional, Murphy, E., additional, Namumba, B., additional, Oozeer, N., additional, Parekh, V., additional, Pillay, D. S., additional, Passmoor, S. S., additional, Ramaila, A. J. T., additional, Ranchod, S., additional, Retana-Montenegro, E., additional, Sebokolodi, L., additional, Sikhosana, S. P., additional, Smirnov, O., additional, Thorat, K., additional, Venturi, T., additional, Abbott, T. D., additional, Adam, R. M., additional, Adams, G., additional, Aldera, M. A., additional, Bauermeister, E. F., additional, Bennett, T. G. H., additional, Bode, W. A., additional, Botha, D. H., additional, Botha, A. G., additional, Brederode, L. R. S., additional, Buchner, S., additional, Burger, J. P., additional, Cheetham, T., additional, de Villiers, D. I. L., additional, Dikgale-Mahlakoana, M. A., additional, du Toit, L. J., additional, Esterhuyse, S. W. P., additional, Fadana, G., additional, Fanaroff, B. L., additional, Fataar, S., additional, Foley, A. R., additional, Fourie, D. J., additional, Frank, B. S., additional, Gamatham, R. R. G., additional, Gatsi, T. G., additional, Geyer, M., additional, Gouws, M., additional, Gumede, S. C., additional, Heywood, I., additional, Hlakola, M. J., additional, Hokwana, A., additional, Hoosen, S. W., additional, Horn, D. M., additional, Horrell, J. M. G., additional, Hugo, B. V., additional, Isaacson, A. R., additional, Jonas, J. L., additional, Jordaan, J. D. B., additional, Joubert, A. F., additional, Julie, R. P. M., additional, Kapp, F. B., additional, Kasper, V. A., additional, Kenyon, J. S., additional, Kotzé, P. P. A., additional, Kotze, A. G., additional, Kriek, N., additional, Kriel, H., additional, Krishnan, V. K., additional, Kusel, T. W., additional, Legodi, L. S., additional, Lehmensiek, R., additional, Liebenberg, D., additional, Lord, R. T., additional, Lunsky, B. M., additional, Madisa, K., additional, Magnus, L. G., additional, Main, J. P. L., additional, Makhaba, A., additional, Makhathini, S., additional, Malan, J. A., additional, Manley, J. R., additional, Marais, S. J., additional, Maree, M. D. J., additional, Martens, A., additional, Mauch, T., additional, McAlpine, K., additional, Merry, B. C., additional, Millenaar, R. P., additional, Mokone, O. J., additional, Monama, T. E., additional, Mphego, M. C., additional, New, W. S., additional, Ngcebetsha, B., additional, Ngoasheng, K. J., additional, Ockards, M. T., additional, Otto, A. J., additional, Patel, A. A., additional, Peens-Hough, A., additional, Perkins, S. J., additional, Ramanujam, N. M., additional, Ramudzuli, Z. R., additional, Ratcliffe, S. M., additional, Renil, R., additional, Robyntjies, A., additional, Rust, A. N., additional, Salie, S., additional, Sambu, N., additional, Schollar, C. T. G., additional, Schwardt, L. C., additional, Schwartz, R. L., additional, Serylak, M., additional, Siebrits, R., additional, Sirothia, S. K., additional, Slabber, M., additional, Sofeya, L., additional, Taljaard, B., additional, Tasse, C., additional, Tiplady, A. J., additional, Toruvanda, O., additional, Twum, S. N., additional, van Balla, T. J., additional, van der Byl, A., additional, van der Merwe, C., additional, van Dyk, C. L., additional, Van Tonder, V., additional, Van Wyk, R., additional, Venter, A. J., additional, Venter, M., additional, Welz, M. G., additional, Williams, L. P., additional, and Xaia, B., additional

Published
2022
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8. MeerKAT-64 discovers wide-spread tidal debris in the nearby NGC 7232 galaxy group

Author

Namumba, B, primary, Koribalski, B S, additional, Józsa, G I G, additional, Lee-Waddell, K, additional, Jones, M G, additional, Carignan, C, additional, Verdes-Montenegro, L, additional, Ianjamasimanana, R, additional, de Blok, W J G, additional, Cluver, M, additional, Garrido, J, additional, Sánchez-Expósito, S, additional, Ramaila, A J T, additional, Thorat, K, additional, Andati, L A L, additional, Hugo, B V, additional, Kleiner, D, additional, Kamphuis, P, additional, Serra, P, additional, Smirnov, O M, additional, Maccagni, F M, additional, Makhathini, S, additional, Molnár, D Cs, additional, Perkins, S, additional, Ramatsoku, M, additional, White, S V, additional, and Loi, F, additional

Published
2021
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9. MIGHTEE-HI: The H I emission project of the MeerKAT MIGHTEE survey

Author

Maddox, N., primary, Frank, B. S., additional, Ponomareva, A. A., additional, Jarvis, M. J., additional, Adams, E. A. K., additional, Davé, R., additional, Oosterloo, T. A., additional, Santos, M. G., additional, Blyth, S. L., additional, Glowacki, M., additional, Kraan-Korteweg, R. C., additional, Mulaudzi, W., additional, Namumba, B., additional, Prandoni, I., additional, Rajohnson, S. H. A., additional, Spekkens, K., additional, Adams, N. J., additional, Bowler, R. A. A., additional, Collier, J. D., additional, Heywood, I., additional, Sekhar, S., additional, and Taylor, A. R., additional

Published
2021
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12. An Overview of the MHONGOOSE Survey: Observing Nearby Galaxies with MeerKAT

Author

de Blok, W.J.G., primary, Adams, E.A.K., additional, Amram, P., additional, Athanassoula, E., additional, Bagetakos, I., additional, Balkowski, C., additional, Bershady, M.A., additional, Beswick, Rob J., additional, Bigiel, F., additional, Blyth, S.-L., additional, Bosma, A., additional, Booth, R.S., additional, Bouchard, A., additional, Brinks, E., additional, Carignan, C., additional, Chemin, L., additional, Combes, F., additional, Conway, J., additional, Elson, E.C., additional, English, J., additional, Epinat, B., additional, Frank, B.S., additional, Fiege, J., additional, Fraternali, F., additional, Gallagher, J.S., additional, Gibson, B.K., additional, Heald, G., additional, Henning, P.A., additional, Holwerda, B.W., additional, Jarrett, T.H., additional, Jerjen, H., additional, Józsa, G.I., additional, Kapala, M., additional, Klöckner, H.-R., additional, Koribalski, B.S., additional, Kraan-Korteweg, R.C., additional, Leon, S., additional, Leroy, A., additional, Loubser, S.I., additional, Lucero, D.M., additional, McGaugh, S.S., additional, Meurer, G.R., additional, Meyer, M., additional, Mogotsi, M., additional, Namumba, B., additional, Oh, S-H., additional, Oosterloo, T.A., additional, Pisano, D.J., additional, Popping, A., additional, Ratcliffe, S., additional, Sellwood, J.A., additional, Schinnerer, E., additional, Schröder, A.C., additional, Sheth, K., additional, Smith, M.W.L., additional, Sorgho, A., additional, Spekkens, K., additional, Stanimirovic, S., additional, van der Heyden, K. J., additional, Verdes-Montenegro, L., additional, van Driel, W., additional, Walter, F., additional, Westmeier, T., additional, Wilcots, E., additional, Williams, T., additional, Wong, O.I., additional, Woudt, P.A., additional, and Zijlstra, A., additional

Published
2018
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14. an overview of the MHONGOOSE survey

Author

MHONGOOSE, Blok, W. J. G., Adams, E. A. K., Amram, P., Athanassoula, E., Bagetakos, I., Balkowski, C., Bershady, M. A., Beswick, R., Bigiel, F., Blyth, S. L., Bosma, A., Booth, R. S., Bouchard, A., Brinks, E., Carignan, C., Chemin, L., Combes, F., Conway, J., Elson, E. C., English, J., Epinat, B., Frank, B. S., Fiege, J., Fraternali, F., Gallagher, J. S., Gibson, B. K., Heald, G., Henning, P. A., Holwerda, B. W., Jarrett, T. H., Jerjen, H., Józsa, G. I., Kapala, M., Klöckner, H. R., Koribalski, B. S., Kraan-Korteweg, R. C., Leon, S., Leroy, A., Loubser, S. I., Lucero, D. M., Mcgaugh, S. S., Meurer, Gerhardt R., Martin Meyer, Mogotsi, M., Namumba, B., Oh, S. H., Oosterloo, T. A., Pisano, D. J., Popping, A., Ratcliffe, S., Sellwood, J. A., Schinnerer, E., Schröder, A. C., Sheth, K., Smith, M. W. L., Sorgho, A., Spekkens, K., Stanimirovic, S., Heyden, K., Driel, W., Verdes-Montenegro, L., Walter, F., Westmeier, T., Wilcots, E., Williams, T., O. Ivy Wong, Woudt, P. A., and Zijlstra, A.

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