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	<title>Distant Galaxies Archives - GUAIX GROUP</title>
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		<title>Jesús Gallego gives the inaugural invited talk at the II International Astronomy Congress in Guatemala</title>
		<link>https://guaix.ucm.es/2021/12/gallego_guatemala_talk</link>
		
		<dc:creator><![CDATA[admin]]></dc:creator>
		<pubDate>Thu, 16 Dec 2021 11:38:40 +0000</pubDate>
				<category><![CDATA[Distant Galaxies]]></category>
		<category><![CDATA[General]]></category>
		<category><![CDATA[Uncategorized]]></category>
		<guid isPermaLink="false">https://guaix.ucm.es/?p=58529</guid>

					<description><![CDATA[<p>The post <a href="https://guaix.ucm.es/2021/12/gallego_guatemala_talk">Jesús Gallego gives the inaugural invited talk at the II International Astronomy Congress in Guatemala</a> appeared first on <a href="https://guaix.ucm.es">GUAIX GROUP</a>.</p>
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			<p><strong>This invited talk was the one that opened the congress, that was held at the Universidad Galileo in Guatemala City.</strong></p>
<p>Jesús Gallego reviewed our conception of the cosmos, since the beginning of humanity, the firmament has always attracted us as something distant and unreachable. From the sphere of fixed stars in the book &#8220;Del saber de la Astronomía&#8221; by Alfonso X, &#8220;the Wise&#8221;, to the large astronomical telescopes of today, the history of astronomy is based on the constant effort to know the nature of the increasingly remote universe that our instruments reveal to us. Jesús concluded by explaining what is currently known about the most remote universe.</p>

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</div><p>The post <a href="https://guaix.ucm.es/2021/12/gallego_guatemala_talk">Jesús Gallego gives the inaugural invited talk at the II International Astronomy Congress in Guatemala</a> appeared first on <a href="https://guaix.ucm.es">GUAIX GROUP</a>.</p>
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		<title>The Gran Telescopio Canarias finds the farthest black hole that belongs to a rare family of galaxies</title>
		<link>https://guaix.ucm.es/2020/10/blackhole/</link>
		
		<dc:creator><![CDATA[admin]]></dc:creator>
		<pubDate>Tue, 27 Oct 2020 20:42:26 +0000</pubDate>
				<category><![CDATA[Distant Galaxies]]></category>
		<category><![CDATA[General]]></category>
		<guid isPermaLink="false">https://guaix.ucm.es/?p=58291</guid>

					<description><![CDATA[<p>The post <a href="https://guaix.ucm.es/2020/10/blackhole/">The Gran Telescopio Canarias finds the farthest black hole that belongs to a rare family of galaxies</a> appeared first on <a href="https://guaix.ucm.es">GUAIX GROUP</a>.</p>
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			<p style="text-align: left;"><strong><span lang="EN-GB" xml:lang="EN-GB">An international team of astronomers has identified one of the rarest known classes of gamma-ray emitting galaxies, called BL Lacertae, within the first 2 billion years of the age of the Universe. The team, that has used one of the largest optical telescope in the world, Gran Telescopio Canarias (GTC), located at the Observatorio del Roque de los Muchachos (Garafía, La Palma), consists of researchers from the Universidad Complutense de Madrid (UCM, Spain), DESY (Germany), University of California Riverside and Clemson University (USA). The finding is published in <em>The Astrophysical Journal Letters</em>.</span></strong></p>
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			<p><span lang="EN-GB" xml:lang="EN-GB">Only a small fraction of the galaxies emits gamma rays, which is the most extreme form of light. Astronomers believe that these highly energetic photons originate from the vicinity of a supermassive black hole residing at the centers of these galaxies. When this happens, they are known as <em>active galaxies</em>. The black hole swallows matter from its surroundings and emits jets or, in other words, collimated streams of matter and radiation. Few of these active galaxies (less than 1%) have their jets pointing by chance toward Earth. Scientists call them <em>blazars</em> and are one of the most powerful sources of radiation in the universe.</span></p>
<p><span lang="EN-GB" xml:lang="EN-GB">Blazars come in two flavors: BL Lacertae (BL Lac) and flat-spectrum radio-quasars (FSRQs). Our current understanding about these mysterious astronomical objects is that FSRQs are relatively young active galaxies, rich in dust and gas that surround the central black hole. As time passes, the amount of matter available to feed the black hole is consumed and the FSRQ evolves to become a BL Lac object. &#8220;In other words, BL Lacs may represent the elderly and evolved phase of a blazar&#8217;s life, while FSRQs resemble an adult,&#8221; explains <strong>Vaidehi Paliya</strong>, a DESY researcher who participated in this program.</span></p>
<p>“Since the speed of light is limited, the farther we look, the earlier in the age of the Universe we investigate,” says <strong>Alberto Domínguez</strong> of the Institute of Physics of Particles and the Cosmos (IPARCOS) at UCM and co-author of the study. Astronomers believe that the current age of the Universe is around 13.8 billion years. The most distant FSRQ was identified at a distance when the age of the universe was merely 1 billion years. For a comparison, the farthest BL Lac that is known was found when the age of the Universe was around 2.5 billion years. Therefore, the hypothesis of the evolution from FSRQ to BL Lacs appears to be valid.</p>

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			<div class="vc_single_image-wrapper   vc_box_border_grey"><img decoding="async" width="1019" height="573" src="https://guaix.ucm.es/wp-content/uploads/2020/10/Captura-de-pantalla-2020-10-27-a-las-21.38.05.png" class="vc_single_image-img attachment-full" alt="" title="UCM Team" srcset="https://guaix.ucm.es/wp-content/uploads/2020/10/Captura-de-pantalla-2020-10-27-a-las-21.38.05.png 1019w, https://guaix.ucm.es/wp-content/uploads/2020/10/Captura-de-pantalla-2020-10-27-a-las-21.38.05-300x169.png 300w, https://guaix.ucm.es/wp-content/uploads/2020/10/Captura-de-pantalla-2020-10-27-a-las-21.38.05-768x432.png 768w, https://guaix.ucm.es/wp-content/uploads/2020/10/Captura-de-pantalla-2020-10-27-a-las-21.38.05-600x337.png 600w" sizes="(max-width: 1019px) 100vw, 1019px"  data-dt-location="https://guaix.ucm.es/2020/10/blackhole/captura-de-pantalla-2020-10-27-a-las-21-38-05/" /></div><figcaption class="vc_figure-caption">On the left, Vaidehi S. Paliya. In the photo on the right: Cristina Cabello, Jesús Gallego, Alberto Domínguez, Armando Gil de Paz y Nicolás Cardiel.</figcaption>
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			<p>Now, the team of international scientists has discovered a new BL Lac object, named 4FGL J1219.0+3653, much farther away than the previous record holder. &#8220;We have discovered a BL Lac existing even 800 million years earlier, this is when the Universe was less than 2 billion years old,&#8221; states <strong>Cristina Cabello</strong>, a graduate student at IPARCOS-UCM. &#8220;This finding challenges the current scenario that BL Lacs are actually an evolved phase of FSRQ,&#8221; adds <strong>Nicolás Cardiel</strong>, a professor at IPARCOS-UCM. <strong>Jesús Gallego</strong>, also a professor at the same institution and a co-author of the study concludes: “This discovery has challenged our knowledge of the cosmic evolution of blazars and active galaxies in general.”</p>
<p><span lang="EN-GB" xml:lang="EN-GB">The researchers have used the OSIRIS and EMIR instruments, designed and built by the Instituto de Astrofísica de Canarias (IAC) and mounted on GTC, also known as Grantecan. &#8220;These results are a clear example of how the combination of the large collecting area of ​​GTC, the world&#8217;s largest optical-infrared telescope, together with the unique capabilities of complementary instruments installed in the telescope are providing breakthrough results to improve our understanding of the Universe,” underlines <strong>Romano Corradi</strong>, director of Grantecan. </span></p>
<p><span lang="EN-GB" xml:lang="EN-GB">The Observatories of the Instituto de Astrofísica de Canarias (IAC) are part of the network of Singular Scientific and Technical Infrastructures (ICTS) of Spain.</span></p>
<p><strong>Article:</strong></p>
<p>Vaidehi S. Paliya, A. Domínguez, C. Cabello, et al. <span lang="EN-GB" xml:lang="EN-GB">&#8220;The First Gamma-ray Emitting BL Lacertae Object at the Cosmic Dawn&#8221;, The Astrophysical Journal Letters, Oct. 2020 DOI: <a href="https://iopscience.iop.org/article/10.3847/2041-8213/abbc06" target="_blank" rel="noopener noreferrer">10.3847/2041-8213/abbc06</a></span>  <a href="https://arxiv.org/abs/2010.12907" target="_blank" rel="noopener noreferrer">arXiv:2010.12907</a></p>

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</div><p>The post <a href="https://guaix.ucm.es/2020/10/blackhole/">The Gran Telescopio Canarias finds the farthest black hole that belongs to a rare family of galaxies</a> appeared first on <a href="https://guaix.ucm.es">GUAIX GROUP</a>.</p>
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		<title>Cristina Cabello gives a talk at the J-PAS RIA Workshop</title>
		<link>https://guaix.ucm.es/2019/12/jpas/</link>
		
		<dc:creator><![CDATA[admin]]></dc:creator>
		<pubDate>Wed, 18 Dec 2019 16:01:23 +0000</pubDate>
				<category><![CDATA[Distant Galaxies]]></category>
		<category><![CDATA[General]]></category>
		<guid isPermaLink="false">https://guaix.ucm.es/?p=55481</guid>

					<description><![CDATA[<p>The post <a href="https://guaix.ucm.es/2019/12/jpas/">Cristina Cabello gives a talk at the J-PAS RIA Workshop</a> appeared first on <a href="https://guaix.ucm.es">GUAIX GROUP</a>.</p>
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<div>GUAIX member Cristina Cabello attended the J-PAS RIA Workshop: &#8216;The Universe in 56 colours: science with the first J-PAS data&#8217; held in Teruel from 2 to 4 December, and gave a talk entitled <i>Studying the properties of low-mass galaxies at z ∼1. How can J-PAS be useful here?</i></div>
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<div>This research surveys the Extended Groth Strip (EGS) field exploiting the Guaranteed Time (GT) of the EMIR instrument at Gran Telescopio Canarias (GTC) to obtain near-IR spectra of low-mass galaxies at z ∼1. This multi-object spectrograph is capable of observing multiple sources at the same time. However, due to the limited spectral range covered by the grism, spectroscopic or accurate photometric redshifts are crucial to secure detection and to not miss emission lines of interest. Fortunately, the J-PAS survey provides high quality photometric redshifts and low-resolution spectra for million of galaxies. In particular, the data taken with the camera Pathfinder in the EGS field would improve the candidate selection and therefore enhancing the success rate of H-alpha detections in the J band with EMIR. Moreover, the 56 narrow-band filters of JPAS are essential for the detection of different emission lines in the optical range and hence for a detailed study of the sources. This synergy between both projects is key to determine the properties of low-mass sources and to understand the evolution of the star-forming galaxy population at z ∼1.</div>
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</div><p>The post <a href="https://guaix.ucm.es/2019/12/jpas/">Cristina Cabello gives a talk at the J-PAS RIA Workshop</a> appeared first on <a href="https://guaix.ucm.es">GUAIX GROUP</a>.</p>
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		<title>CM research projects awarded to Dr. Bililign T. Dullo &#038; Dr. Santi Roca-Fàbrega</title>
		<link>https://guaix.ucm.es/2019/12/proyectos_jovenes_cm_2019/</link>
		
		<dc:creator><![CDATA[admin]]></dc:creator>
		<pubDate>Wed, 18 Dec 2019 10:05:25 +0000</pubDate>
				<category><![CDATA[Distant Galaxies]]></category>
		<category><![CDATA[Galaxy Simulations]]></category>
		<category><![CDATA[General]]></category>
		<guid isPermaLink="false">https://guaix.ucm.es/?p=55450</guid>

					<description><![CDATA[<p>The post <a href="https://guaix.ucm.es/2019/12/proyectos_jovenes_cm_2019/">CM research projects awarded to Dr. Bililign T. Dullo &#038; Dr. Santi Roca-Fàbrega</a> appeared first on <a href="https://guaix.ucm.es">GUAIX GROUP</a>.</p>
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<p>The regional government of the Comunidad de Madrid has awarded two research projects for Young Researchers to GUAIX members Dr. Bililign T. Dullo and Dr. Santi Roca-Fàbrega, both Captación de Talento fellows in the group.</p>
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<p>The amount awarded is over 90 k€ to support their research on the process that drive galaxy formation, from the properties and impact of Supermassive Black Holes to the understanding of the gas around galaxies (circum-galactic medium) throughout the history of the Universe.</p>
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</div><p>The post <a href="https://guaix.ucm.es/2019/12/proyectos_jovenes_cm_2019/">CM research projects awarded to Dr. Bililign T. Dullo &#038; Dr. Santi Roca-Fàbrega</a> appeared first on <a href="https://guaix.ucm.es">GUAIX GROUP</a>.</p>
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		<title>Bil Dullo gave a talk at the &#8220;Spain in SKA&#8221; meeting</title>
		<link>https://guaix.ucm.es/eso-director-general-visits-the-ucm-2-2-2/</link>
		
		<dc:creator><![CDATA[admin]]></dc:creator>
		<pubDate>Thu, 13 Jun 2019 10:39:25 +0000</pubDate>
				<category><![CDATA[Distant Galaxies]]></category>
		<category><![CDATA[General]]></category>
		<guid isPermaLink="false">https://guaix.ucm.es/?p=55163</guid>

					<description><![CDATA[<p>The post <a href="https://guaix.ucm.es/eso-director-general-visits-the-ucm-2-2-2/">Bil Dullo gave a talk at the &#8220;Spain in SKA&#8221; meeting</a> appeared first on <a href="https://guaix.ucm.es">GUAIX GROUP</a>.</p>
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			<h3><strong>&#8220;The nuclear activity and central structure of the elliptical galaxy NGC 5322&#8221;</strong></h3>
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			<div>Bil Dullo attended the &#8216;SKA in Spain&#8217; meeting at Granada this week with a talk about &#8220;The nuclear activity and central structure of the elliptical galaxy NGC 5322&#8221;. His contribution showcased best strategies to exploit synergies from a large sample of high-resolution, multi-<wbr />wavelength data, including from HST (optical and infrared) and e-MERLIN (radio continuum observations).</div>
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<div>He gave particular emphasise to an extraordinary elliptical galaxy NGC 5322 with radio jet, diffuse core, counter rotating stellar disk and outer stellar halo, where the high-resolution optical and radio structural analyses taken together allowed to firmly constrain the three-phase assembly of the galaxy.</div>
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<div>His conclusions highlighted that similar approaches could be adopted to exploit high-resolution <wbr />and high-sensitivity radio observations of radio sources from the next generation radio telescope (SKA).</div>
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			<p>Other GUAIX members attended the RIA SKA meeting in Granada, including África Castillo-Morales, Mario Chamorro-Cazorla and Armando Gil de Paz (SOC member).</p>

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</div><p>The post <a href="https://guaix.ucm.es/eso-director-general-visits-the-ucm-2-2-2/">Bil Dullo gave a talk at the &#8220;Spain in SKA&#8221; meeting</a> appeared first on <a href="https://guaix.ucm.es">GUAIX GROUP</a>.</p>
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