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41by Cecil, Fogarty, Richards, Bland-Hawthorn, Lange, Moffett, Catinella, Cortese, Ho, Taylor, Bryant, Allen, Sweet, Croom, Driver, Goodwin, Kelvin, Green, Konstantopoulos, Owers, Lawrence, Lorente“... and stars from non-parametric Diskfit fits out to $r\sim2r_e$. For 12/14 with measured H I profiles, ionized...”
Published 2016
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42by Owers, Matt S., Hudson, Michael J., Oman, Kyle A., Bland-Hawthorn, Joss, Brough, S., Bryant, Julia J., Cortese, Luca, Couch, Warrick J., Croom, Scott M., van de Sande, Jesse, Federrath, Christoph, Groves, Brent, Hopkins, A. M., Lawrence, J. S., Lorente, Nuria P. F., McDermid, Richard M., Medling, Anne M., Richards, Samuel N., Scott, Nicholas, Taranu, Dan S., Welker, Charlotte, Yi, Sukyoung K.“.... These $\rm{H}δ$-strong galaxies (HDSGs) are rare, making up only $\sim 2$% (25/1220) of galaxies with stellar...”
Published 2019
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43by Shin, T., Adhikari, S., Baxter, E. J., Chang, C., Jain, B., Battaglia, N., Bleem, L., Bocquet, S., DeRose, J., Gruen, D., Hilton, M., Kravtsov, A., McClintock, T., Rozo, E., Rykoff, E. S., Varga, T. N., Wechsler, R. H., Wu, H., Aiola, S., Allam, S., Bechtol, K., Benson, B. A., Bertin, E., Bond, J. R., Brodwin, M., Brooks, D., Buckley-Geer, E., Burke, D. L., Carlstrom, J. E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F. J., Choi, S. K., Cunha, C. E., Crawford, T. M., da Costa, L. N., De Vicente, J., Desai, S., Devlin, M. J., Dietrich, J. P., Doel, P., Dunkley, J., Eifler, T. F., Evrard, A. E., Flaugher, B., Fosalba, P., Gallardo, P. A., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gralla, M., Gruendl, R. A., Gschwend, J., Gupta, N., Gutierrez, G., Hartley, W. G., Hill, J. C., Ho, S. P., Hollowood, D. L., Honscheid, K., Hoyle, B., Huffenberger, K., Hughes, J. P., James, D. J., Jeltema, T., Kim, A. G., Krause, E., Kuehn, K., Lahav, O., Lima, M., Madhavacheril, M. S., Maia, M. A. G., Marshall, J. L., Maurin, L., McMahon, J., Menanteau, F., Miller, C. J., Miquel, R., Mohr, J. J., Naess, S., Nati, F., Newburgh, L., Niemack, M. D., Ogando, R. L. C., Partridge, L. A. Page B., Patil, S., Plazas, A. A., Rapetti, D., Reichardt, C. L., Romer, A. K., Sanchez, E., Scarpine, V., Schindler, R., Serrano, S., Smith, M., Smith, R. C., Soares-Santos, M., Sobreira, F., Staggs, S. T., Stark, A., Stein, G., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., van Engelen, A., Wollack, E. J., Xu, Z., Zhang, Z.“... selected redMaPPer clusters, $r_{\rm sp}$ is $\sim$ $2σ$ smaller than in the simulations. These results...”
Published 2018
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44by Kirk, D., Omori, Y., Benoit-Lévy, A., Cawthon, R., Chang, C., Larsen, P., Amara, A., Bacon, D., Crawford, T. M., Dodelson, S., Fosalba, P., Giannantonio, T., Holder, G., Jain, B., Kacprzak, T., Lahav, O., MacCrann, N., Nicola, A., Refregier, A., Sheldon, E., Story, K. T., Troxel, M. A., Vieira, J. D., Vikram, V., Zuntz, J., Abbott, T. M. C., Abdalla, F. B., Becker, M. R., Benson, B. A., Bernstein, G. M., Bernstein, R. A., Bleem, L. E., Bonnett, C., Bridle, S. L., Brooks, D., Buckley-Geer, E., Burke, D. L., Capozzi, D., Carlstrom, J. E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Crocce, M., Cunha, C. E., D'Andrea, C. B., da Costa, L. N., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Eifler, T. F., Evrard, A. E., Flaugher, B., Frieman, J., Gerdes, D. W., Goldstein, D. A., Gruen, D., Gruendl, R. A., Honscheid, K., James, D. J., Jarvis, M., Kent, S., Kuehn, K., Kuropatkin, N., Lima, M., March, M., Martini, P., Melchior, P., Miller, C. J., Miquel, R., Nichol, R. C., Ogando, R., Plazas, A. A., Reichardt, C. L., Roodman, A., Rozo, E., Rykoff, E. S., Sako, M., Sanchez, E., Scarpine, V., Schubnell, M., Sevilla-Noarbe, I., Simard, G., Smith, R. C., Soares-Santos, M., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Wechsler, R. H., Weller, J.“... the CMB lensing kernel is broad and peaks at $z{\sim}2$. The resulting cross-correlation is maximally...”
Published 2015
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45by Jarugula, Sreevani“... in early universe. A bulk of star formation at $z sim 2-3$ takes place in DSFGs but are obscured by dust...”
Published in Proceedings of the 72nd International Symposium on Molecular Spectroscopy (2017)
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46by Bothwell, M. S., Aguirre, J. E., Aravena, M., Bethermin, M., Bisbas, T. G., Chapman, S. C., De Breuck, C., Gonzalez, A. H., Greve, T. R., Hezaveh, Y., Ma, J., Malkan, M., Marrone, D. P., Murphy, E. J., Spilker, J. S., Strandet, M., Vieira, J. D., Weiss, A.“...) an elevated CO-to-H$_2$ conversion factor for our sample of $α_{\rm CO} \sim 2.5$ and a gas-to-dust ratio...”
Published 2016
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47by Bothwell, MS, Aguirre, JE, Aravena, M, Bethermin, M, Bisbas, TG, Chapman, SC, De Breuck, C, Gonzalez, AH, Greve, TR, Hezaveh, Y, Ma, J, Malkan, M, Marrone, DP, Murphy, EJ, Spilker, JS, Strandet, M, Vieira, JD, Weiss, A“...) an elevated CO-to-H$_2$ conversion factor for our sample of $\alpha_{\rm CO} \sim 2.5$ and a gas-to-dust ratio...”
Published 2017
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48by Kirk, D., Omori, Y., Benoit-Lévy, A., Cawthon, R., Chang, C., Larsen, P., Amara, A., Bacon, D., Crawford, T. M., Dodelson, S., Fosalba, P., Giannantonio, T., Holder, G., Jain, B., Kacprzak, T., Lahav, O., MacCrann, N., Nicola, A., Refregier, A., Sheldon, E., Story, K. T., Troxel, M. A., Vieira, J. D., Vikram, V., Zuntz, J., Abbott, T. M. C., Abdalla, F. B., Becker, M. R., Benson, B. A., Bernstein, G. M., Bernstein, R. A., Bleem, L. E., Bonnett, C., Bridle, S. L., Brooks, D., Buckley-Geer, E., Burke, D. L., Capozzi, D., Carlstrom, J. E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Crocce, M., Cunha, C. E., D'Andrea, C. B., da Costa, L. N., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Eifler, T. F., Evrard, A. E., Flaugher, B., Frieman, J., Gerdes, D. W., Goldstein, D. A., Gruen, D., Gruendl, R. A., Honscheid, K., James, D. J., Jarvis, M., Kent, S., Kuehn, K., Kuropatkin, N., Lima, M., March, M., Martini, P., Melchior, P., Miller, C. J., Miquel, R., Nichol, R. C., Ogando, R., Plazas, A. A., Reichardt, C. L., Roodman, A., Rozo, E., Rykoff, E. S., Sako, M., Sanchez, E., Scarpine, V., Schubnell, M., Sevilla-Noarbe, I., Simard, G., Smith, R. C., Soares-Santos, M., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Wechsler, R. H., Weller, J.“... the CMB lensing kernel is broad and peaks at $z{\sim}2$. The resulting cross-correlation is maximally...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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49by Bothwell, MS, Aguirre, JE, Aravena, M, Bethermin, M, Bisbas, TG, Chapman, SC, De Breuck, C, Gonzalez, AH, Greve, TR, Hezaveh, Y, Ma, J, Malkan, M, Marrone, DP, Murphy, EJ, Spilker, JS, Strandet, M, Vieira, JD, Weiß, A“...) an elevated CO-to-H$_2$ conversion factor for our sample of $\alpha_{\rm CO} \sim 2.5$ and a gas-to-dust ratio...”
Published 2017
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50by Owers, Matt S., Hudson, Michael J., Oman, Kyle A., Bland-Hawthorn, Joss, Brough, S., Bryant, Julia J., Cortese, Luca, Couch, Warrick J., Croom, Scott M., van de Sande, Jesse, Federrath, Christoph, Groves, Brent, Hopkins, A. M., Lawrence, J. S., Lorente, Nuria P. F., McDermid, Richard M., Medling, Anne M., Richards, Samuel N., Scott, Nicholas, Taranu, Dan S., Welker, Charlotte, Yi, Sukyoung K.“.... These $\rm{H}{\delta}$-strong galaxies (HDSGs) are rare, making up only $\sim 2$% (25/1220) of galaxies...”
Published in The Astrophysical Journal (2019)
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51by Shin, T., Adhikari, S., Baxter, E. J., Chang, C., Jain, B., Battaglia, N., Bleem, L., Bocquet, S., DeRose, J., Gruen, D., Hilton, M., Kravtsov, A., McClintock, T., Rozo, E., Rykoff, E. S., Varga, T. N., Wechsler, R. H., Wu, H., Aiola, S., Allam, S., Bechtol, K., Benson, B. A., Bertin, E., Bond, J. R., Brodwin, M., Brooks, D., Buckley-Geer, E., Burke, D. L., Carlstrom, J. E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F. J., Choi, S. K., Cunha, C. E., Crawford, T. M., da Costa, L. N., De Vicente, J., Desai, S., Devlin, M. J., Dietrich, J. P., Doel, P., Dunkley, J., Eifler, T. F., Evrard, A. E., Flaugher, B., Fosalba, P., Gallardo, P. A., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gralla, M., Gruendl, R. A., Gschwend, J., Gupta, N., Gutierrez, G., Hartley, W. G., Hill, J. C., Ho, S. P., Hollowood, D. L., Honscheid, K., Hoyle, B., Huffenberger, K., Hughes, J. P., James, D. J., Jeltema, T., Kim, A. G., Krause, E., Kuehn, K., Lahav, O., Lima, M., Madhavacheril, M. S., Maia, M. A. G., Marshall, J. L., Maurin, L., McMahon, J., Menanteau, F., Miller, C. J., Miquel, R., Mohr, J. J., Naess, S., Nati, F., Newburgh, L., Niemack, M. D., Ogando, R. L. C., Partridge, L. A. Page B., Patil, S., Plazas, A. A., Rapetti, D., Reichardt, C. L., Romer, A. K., Sanchez, E., Scarpine, V., Schindler, R., Serrano, S., Smith, M., Smith, R. C., Soares-Santos, M., Sobreira, F., Staggs, S. T., Stark, A., Stein, G., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., van Engelen, A., Wollack, E. J., Xu, Z., Zhang, Z.“... selected redMaPPer clusters, $r_{\rm sp}$ is $\sim$ $2\sigma$ smaller than in the simulations...”
Published in Monthly Notices of the Royal Astronomical Society (2018)
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52by Cecil, G., Fogarty, L. M. R., Richards, S., Bland-Hawthorn, J., Lange, R., Moffett, A., Catinella, B., Cortese, L., Ho, I. -T., Taylor, E. N., Bryant, J. J., Allen, J. T., Sweet, S. M., Croom, S. M., Driver, S. P., Goodwin, M., Kelvin, L., Green, A. W., Konstantopoulos, I. S., Owers, M. S., Lawrence, J. S., Lorente, N. P. F.“... and stars from non-parametric Diskfit fits out to $r\sim2r_e$. For 12/14 with measured H I profiles, ionized...”
Published in Monthly Notices of the Royal Astronomical Society (2015)
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53by Bothwell, M. S., Aguirre, J. E., Aravena, M., Bethermin, M., Bisbas, T. G., Chapman, S. C., De Breuck, C., Gonzalez, A. H., Greve, T. R., Hezaveh, Y., Ma, J., Malkan, M., Marrone, D. P., Murphy, E. J., Spilker, J. S., Strandet, M., Vieira, J. D., Weiss, A.“...) an elevated CO-to-H$_2$ conversion factor for our sample of $\alpha_{\rm CO} \sim 2.5$ and a gas-to-dust ratio...”
Published in Monthly Notices of the Royal Astronomical Society (2016)
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54“... decrease the current uncertainties on the timing of the EoR by factors of $\sim$2 - 3. Comment: 14 pages, 6...”
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55“... to the west of the Kamchatka peninsula, which is $$\sim$$ ∼ 2.5% slower than PREM, immediately above the CMB...”
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56“... to the west of the Kamchatka peninsula, which is $$\sim$$ ∼ 2.5% slower than PREM, immediately above the CMB...”
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57“... of their number density. This effect vanishes at high redshift $z\sim2$ and for high masses $M_{200\textrm m...”
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58by Jones, Amy P.“... the late Neogene. The first is a compilation of \(\sim\)2.5 Ma time-slice data from ocean sediments...”
Published 2021
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59by Wang, Di, Lagos, Claudia D. P., Croom, Scott M., Wright, Ruby J., Bahé, Yannick M., Bryant, Julia J., van de Sande, Jesse, Vaughan, Sam P.“... timescale (median $t_{\rm quench}$ > 2 Gyr). The simulated galaxies at higher redshift ($z=0.7\sim2...”
Published in Monthly Notices of the Royal Astronomical Society (2023)
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60by Kirk, D., Omori, Y., Benoit-Lévy, A., Cawthon, R., Chang, C., Larsen, P., Amara, A., Bacon, D., Crawford, T. M., Dodelson, S., Fosalba, P., Giannantonio, T., Holder, G., Jain, B., Kacprzak, T., Lahav, O., MacCrann, N., Nicola, A., Refregier, A., Sheldon, E., Story, K. T., Troxel, M. A., Vieira, J. D., Vikram, V., Zuntz, J., Abbott, T. M. C., Abdalla, F. B., Becker, M. R., Benson, B. A., Bernstein, G. M., Bernstein, R. A., Bleem, L. E., Bonnett, C., Bridle, S. L., Brooks, D., Buckley-Geer, E., Burke, D. L., Capozzi, D., Carlstrom, J. E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Crocce, M., Cunha, C. E., D'Andrea, C. B., da Costa, L. N., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Eifler, T. F., Evrard, A. E., Flaugher, B., Frieman, J., Gerdes, D. W., Goldstein, D. A., Gruen, D., Gruendl, R. A., Honscheid, K., James, D. J., Jarvis, M., Kent, S., Kuehn, K., Kuropatkin, N., Lima, M., March, M., Martini, P., Melchior, P., Miller, C. J., Miquel, R., Nichol, R. C., Ogando, R., Plazas, A. A., Reichardt, C. L., Roodman, A., Rozo, E., Rykoff, E. S., Sako, M., Sanchez, E., Scarpine, V., Schubnell, M., Sevilla-Noarbe, I., Simard, G., Smith, R. C., Soares-Santos, M., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Wechsler, R. H., Weller, J.“... the CMB lensing kernel is broad and peaks at $z{\sim}2$. The resulting cross-correlation is maximally...”
Published in Monthly Notices of the Royal Astronomical Society (2015)
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