https://www.alma.inaf.it/index.php?action=history&feed=atom&title=Galaxy_evolution
Galaxy evolution - Revision history
2026-06-17T03:08:32Z
Revision history for this page on the wiki
MediaWiki 1.39.1
https://www.alma.inaf.it/index.php?title=Galaxy_evolution&diff=3516&oldid=prev
Bonato at 14:17, 15 May 2018
2018-05-15T14:17:21Z
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 16:17, 15 May 2018</td>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>'''References''': •Bonato M., et al., 2014a, MNRAS, 438, 2547. •Bonato M., et al., 2014b, MNRAS, 444, 3446. •Bonato M., et al., 2015, MNRAS, 452, 356. •Bonato M., et al., 2017a, ApJ, 836, 171. •Bonato M., et al., 2017b, MNRAS, 469, 1912. •Massardi M., De Zotti G., 2004, A&A, 424, 409. •Massardi M., et al., 2010a, ApJ, 718, L23. •Massardi M., et al., 2010b, MNRAS, 404, 532. •Massardi M., et al., 2016, MNRAS, 455, 3249. •Massardi M., et al., 2018, A&A, 610, A53</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>'''References''': •Bonato M., et al., 2014a, MNRAS, 438, 2547. •Bonato M., et al., 2014b, MNRAS, 444, 3446. •Bonato M., et al., 2015, MNRAS, 452, 356. •Bonato M., et al., 2017a, ApJ, 836, 171. •Bonato M., et al., 2017b, MNRAS, 469, 1912. •Massardi M., De Zotti G., 2004, A&A, 424, 409. •Massardi M., et al., 2010a, ApJ, 718, L23. •Massardi M., et al., 2010b, MNRAS, 404, 532. •Massardi M., et al., 2016, MNRAS, 455, 3249. •Massardi M., et al., 2018, A&A, 610, A53</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>'''<del style="font-weight: bold; text-decoration: none;">Contacs</del>''': massardi@ira.inaf.it, bonato@ira.inaf.it</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>'''<ins style="font-weight: bold; text-decoration: none;">Contacts</ins>''': massardi@ira.inaf.it, bonato@ira.inaf.it</div></td></tr>
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Bonato
https://www.alma.inaf.it/index.php?title=Galaxy_evolution&diff=3513&oldid=prev
Bonato at 13:30, 15 May 2018
2018-05-15T13:30:27Z
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 15:30, 15 May 2018</td>
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<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>Our expertise includes studies on photometric and IR/sub-mm spectroscopic properties of star forming galaxies and of AGN (Massardi et al. 2016, 2018, Bonato et al. 2014a,b, 2015, 2017a) and on galaxy and AGN (co-)evolution models (Massardi et al. 2010b, Bonato et al. 2014a,b, 2017b). We have developed theoretical galaxy evolution models both in the IR (Bonato et al. 2014a,b<del style="font-weight: bold; text-decoration: none;">, 2018 in prep.</del>) and in the radio regime (Massardi et al. 2010, Bonato et al. 2017b). In the cited papers, we have used our models to work out predictions for observations with future - the SPace IR telescope for Cosmology and Astrophysics (SPICA), the Origins Space Telescope (OST) - or upcoming - the James Webb Space Telescope (JWST) - telescopes. Our expertise is not limited to individual or populations of galaxies, but it also includes analysis of properties and modelling of galaxy clusters (Massardi & De Zotti 2004, Massardi et al. 2010a).</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>Our expertise includes studies on <ins style="font-weight: bold; text-decoration: none;">'''</ins>photometric and IR/sub-mm spectroscopic properties of star forming galaxies and of AGN<ins style="font-weight: bold; text-decoration: none;">''' </ins>(Massardi et al. 2016, 2018, Bonato et al. 2014a,b, 2015, 2017a) and on <ins style="font-weight: bold; text-decoration: none;">'''</ins>galaxy and AGN (co-)evolution models<ins style="font-weight: bold; text-decoration: none;">''' </ins>(Massardi et al. 2010b, Bonato et al. 2014a,b, 2017b). We have developed theoretical galaxy evolution models both in the <ins style="font-weight: bold; text-decoration: none;">'''</ins>IR<ins style="font-weight: bold; text-decoration: none;">''' </ins>(Bonato et al. 2014a,b) and in the <ins style="font-weight: bold; text-decoration: none;">'''</ins>radio regime<ins style="font-weight: bold; text-decoration: none;">''' </ins>(Massardi et al. 2010, Bonato et al. 2017b). In the cited papers, we have used our models to work out <ins style="font-weight: bold; text-decoration: none;">'''</ins>predictions<ins style="font-weight: bold; text-decoration: none;">''' </ins>for observations with future - the SPace IR telescope for Cosmology and Astrophysics (SPICA), the Origins Space Telescope (OST) - or upcoming - the James Webb Space Telescope (JWST) - telescopes. Our expertise is not limited to individual or populations of galaxies, but it also includes analysis of properties and modelling of <ins style="font-weight: bold; text-decoration: none;">'''</ins>galaxy clusters<ins style="font-weight: bold; text-decoration: none;">''' </ins>(Massardi & De Zotti 2004, Massardi et al. 2010a).</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>References<del style="font-weight: bold; text-decoration: none;">.</del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">'''</ins>References<ins style="font-weight: bold; text-decoration: none;">''': •Bonato </ins>M., et al., 2014a, MNRAS, 438, 2547<ins style="font-weight: bold; text-decoration: none;">. •Bonato </ins>M., et al., 2014b, MNRAS, 444, 3446<ins style="font-weight: bold; text-decoration: none;">. •Bonato </ins>M., et al., 2015, MNRAS, 452, 356<ins style="font-weight: bold; text-decoration: none;">. •Bonato </ins>M., et al., 2017a, ApJ, 836, 171<ins style="font-weight: bold; text-decoration: none;">. •Bonato </ins>M., et al., 2017b, MNRAS, 469, 1912. <ins style="font-weight: bold; text-decoration: none;">•Massardi </ins>M., De Zotti G., 2004, A&A, 424, 409<ins style="font-weight: bold; text-decoration: none;">. •Massardi </ins>M., et al., 2010a, ApJ, 718, L23<ins style="font-weight: bold; text-decoration: none;">. •Massardi </ins>M., et al., 2010b, MNRAS, 404, 532<ins style="font-weight: bold; text-decoration: none;">. •Massardi </ins>M., et al., 2016, MNRAS, 455, 3249<ins style="font-weight: bold; text-decoration: none;">. •Massardi </ins>M., et al., 2018, A&A, 610, A53</div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Bonato </del>M., et al., 2014a, MNRAS, 438, 2547</div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Bonato </del>M., et al., 2014b, MNRAS, 444, 3446</div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Bonato </del>M., et al., 2015, MNRAS, 452, 356</div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Bonato </del>M., et al., 2017a, ApJ, 836, 171</div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Bonato </del>M., et al., 2017b, MNRAS, 469, 1912</div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Bonato M</del>.<del style="font-weight: bold; text-decoration: none;">, et al., 2018, in prep.</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Massardi </del>M., De Zotti G., 2004, A&A, 424, 409</div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Massardi </del>M., et al., 2010a, ApJ, 718, L23</div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Massardi </del>M., et al., 2010b, MNRAS, 404, 532</div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Massardi </del>M., et al., 2016, MNRAS, 455, 3249</div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Massardi </del>M., et al., 2018, A&A, 610, A53</div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>Contacs: massardi@ira.inaf.it, bonato@ira.inaf.it</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">'''</ins>Contacs<ins style="font-weight: bold; text-decoration: none;">'''</ins>: massardi@ira.inaf.it, bonato@ira.inaf.it</div></td></tr>
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Bonato
https://www.alma.inaf.it/index.php?title=Galaxy_evolution&diff=3512&oldid=prev
Bonato: Created page with "Our expertise includes studies on photometric and IR/sub-mm spectroscopic properties of star forming galaxies and of AGN (Massardi et al. 2016, 2018, Bonato et al. 2014a,b, 20..."
2018-05-15T13:21:37Z
<p>Created page with "Our expertise includes studies on photometric and IR/sub-mm spectroscopic properties of star forming galaxies and of AGN (Massardi et al. 2016, 2018, Bonato et al. 2014a,b, 20..."</p>
<p><b>New page</b></p><div>Our expertise includes studies on photometric and IR/sub-mm spectroscopic properties of star forming galaxies and of AGN (Massardi et al. 2016, 2018, Bonato et al. 2014a,b, 2015, 2017a) and on galaxy and AGN (co-)evolution models (Massardi et al. 2010b, Bonato et al. 2014a,b, 2017b). We have developed theoretical galaxy evolution models both in the IR (Bonato et al. 2014a,b, 2018 in prep.) and in the radio regime (Massardi et al. 2010, Bonato et al. 2017b). In the cited papers, we have used our models to work out predictions for observations with future - the SPace IR telescope for Cosmology and Astrophysics (SPICA), the Origins Space Telescope (OST) - or upcoming - the James Webb Space Telescope (JWST) - telescopes. Our expertise is not limited to individual or populations of galaxies, but it also includes analysis of properties and modelling of galaxy clusters (Massardi & De Zotti 2004, Massardi et al. 2010a).<br />
<br />
References.<br />
Bonato M., et al., 2014a, MNRAS, 438, 2547<br />
Bonato M., et al., 2014b, MNRAS, 444, 3446<br />
Bonato M., et al., 2015, MNRAS, 452, 356<br />
Bonato M., et al., 2017a, ApJ, 836, 171<br />
Bonato M., et al., 2017b, MNRAS, 469, 1912<br />
Bonato M., et al., 2018, in prep.<br />
Massardi M., De Zotti G., 2004, A&A, 424, 409<br />
Massardi M., et al., 2010a, ApJ, 718, L23<br />
Massardi M., et al., 2010b, MNRAS, 404, 532<br />
Massardi M., et al., 2016, MNRAS, 455, 3249<br />
Massardi M., et al., 2018, A&A, 610, A53<br />
<br />
Contacs: massardi@ira.inaf.it, bonato@ira.inaf.it</div>
Bonato