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+---
+title: "IVOA Newsletter - May 2014"
+date: 2014-05-01T00:01:00+02:00
+tags:
+- news
+---
+
+[Subscribe](http://www.ivoa.net/mailman/listinfo/ivoa-news) | [Newsletter archives](http://www.ivoa.net/newsletter/) | [Write to the editors](mailto:ivoa-news-editors@ivoa.net)
+**IVOA Newsletter Editors:** Mark G. Allen, Deborah Baines, Sarah Emery Bunn,
+Chenzou Cui, August Muench, Mark Taylor, & Ivan Zolotukhin.
+
+** The International Virtual Observatory Alliance (IVOA) was formed in June 2002
+with a mission to facilitate the international coordination and collaboration
+necessary for the development and deployment of the tools, systems and
+organizational structures necessary to enable the international utilization of
+astronomical archives as an integrated and interoperating virtual observatory.
+The IVOA now comprises 20 VO programs from Argentina, Armenia, Australia,
+Brazil, Canada, Chile, China, Europe, France, Germany, Hungary, India, Italy,
+Japan, Russia, South Africa, Spain, Ukraine, the United Kingdom, and the United
+States and an inter-governmental organization (ESA). Membership is open to other
+national and international programs according to the
+[IVOA Guidelines for Participation](http://ivoa.net/Documents/latest/IVOAParticipation.html).
+You can read more about the IVOA and what we do at .**
+
+### What is the VO?
+
+The Virtual Observatory (VO) aims to provide a research environment that will
+open up new possibilities for scientific research based on data discovery,
+efficient data access, and interoperability. The vision is of global astronomy
+archives connected via the VO to form a multiwavelength digital sky that can be
+searched, visualized, and analyzed in new and innovative ways. VO projects
+worldwide working toward this vision are already providing science capabilities
+with new tools and services. This newsletter, aimed at astronomers, highlights
+VO tools and technologies for doing astronomy research, recent papers, and
+upcoming events.
+
+---
+
+# IVOA news
+
+{{< side-image image="ChiVO.png" position="left" >}}
+
+### Chilean Virtual Observatory (ChiVO) joins the IVOA
+
+The Chilean VO, which is supported by five Chilean universities, ALMA, and the
+REUNA research consortium, was welcomed into the IVOA at the September 2013 IVOA
+meeting. ChiVO will focus on building the tools and technology infrastructure
+necessary for Chilean researchers to take advantage of the terabytes of data
+that will be produced by ALMA. More information can be found at
+.
+
+{{ side-image >}}
+
+{{< side-image image="ProcessDiagram_crop2.png" position="right" >}}
+
+### Moving forward with Data Standards
+
+The past six months have seen the recommendation of three new data standards. These include a [Photometry Data Model](http://ivoa.net/documents/PHOTDM/index.html) for describing photometric systems, and two specifications for data access services ([Data Access Layer Interface](http://ivoa.net/documents/DALI/index.html), [Describing Simple Data Access Services](http://ivoa.net/documents/SimpleDALRegExt/index.html)). The VOTable standard, which is an XML standard for the interchange of tables of data and metadata, moved to [version 1.3](http://www.ivoa.net/documents/VOTable/).
+
+{{ side-image >}}
+
+---
+
+# VO applications and implementation highlights
+
+{{< side-image image="TAO_illust.png" thumbnail="TAO_illust.png" position="right" >}}
+
+### Theoretical Astrophysical Observatory (TAO)
+
+The Australian VO is happy to announce the launch of the TAO, which houses
+queryable data from multiple popular cosmological simulations and galaxy
+formation models. Results can be funnelled through higher-level modules to build
+custom mock galaxy catalogues and images. TAO is accessible from anywhere you
+can access the internet. TAO is part of the All-Sky Virtual Observatory (ASVO)
+and is funded and supported by Astronomy Australia Limited, the National
+eResearch Collaboration Tools and Resources (NeCTAR), and Swinburne University
+of Technology.
+
+**More Information:**
+
+{{ side-image >}}
+
+{{< side-image image="voclient.png" thumbnail="voclient.png" position="left" >}}
+
+### VO Client Release - Access the VO from your desktop
+
+The US Virtual Astronomical Observatory (VAO) has released VOClient - a software
+package that enables direct access to services in the VO from a Unix terminal or
+scripting environment. The VOClient command-line tools allow you to discover
+archives and catalogs through queries to the VAO Registry, search-for and
+download images, spectra, and catalogs, and interoperate with other
+VO-compatible tools. These tools can be used to create customized access to VO
+services, new VO tools or enhancements to existing software by adding VO
+capabilities.
+
+**More Information:**
+
+{{ side-image >}}
+
+{{< side-image image="vtp.png" thumbnail="vtp.png" position="right" >}}
+
+### Comet, a Python implementation of the VOEvent Transport Protocol
+
+VOEvent is the IVOA system for describing transient celestial events. Details of
+transients detected by many projects, including Fermi, Swift, and the Catalina
+Sky Survey, are currently made available as VOEvents, and it has been selected
+as the standard alert format by future facilities such as LSST and SKA. Comet is
+an implementation of the VOEvent Transport Protocol, which makes the fast and
+reliable distribution of VOEvents to the community possible. Comet enables you
+to subscribe to real-time streams of ongoing events, to use filters to select
+only events relevant to your science case and to publish your own events to the
+global VOEvent backbone. Comet is written in Python, is open source and is
+freely available from .
+
+**More Information:** ,
+
+
+{{ side-image >}}
+
+{{< side-image image="tcviz_news.png" thumbnail="tcviz_news_thumb.png" position="left" >}}
+
+### TOPCAT Visualisation
+
+TOPCAT has recently had an overhaul of its visualisation capabilities. New
+features include sky axes, the ability to plot vectors, ellipses, contours and
+analytic functions, hybrid scatter/density plots, improved 3d navigation, better
+interactive response, LaTeX labelling of axes, more configurability, and better
+performance for large (multi-million-row) tables. As well as visualisation,
+TOPCAT continues to provide a wide range of other analysis capabilities for
+tabular data including VO access, crossmatching and row selections.
+
+**More Information:**
+
+{{ side-image >}}
+
+
+{{< side-image image="ssap_vamdc.jpg" thumbnail="ssap_vamdc.jpg" position="right" >}}
+
+### CASSIS: Version 3.6.1 released
+
+The latest release of CASSIS (Centre d'Analyse Scientifique de Spectres
+Instrumentaux et Synthétiques), version 3.6.1, is available for download since
+March 4, 2014. CASSIS provides tools to visualize and analyze spectra, in
+particular to perform line identification. A number of changes have been and are
+being implemented to make CASSIS VO-compatible. CASSIS now includes a Simple
+Spectral Access (SSA) module and also allows the user to interrogate the VAMDC
+online database (http://www.vamdc.eu/access-data/portal), rather than a local
+database. Both of these features are illustrated in the accompanying figure: the
+top panel shows a SSA query on Orion with the responses from different services
+being displayed in different tabs, while the bottom panel shows the display of
+the selected ISO-LWS spectrum, overlaid with all CO transitions found in the
+VAMDC/CDMS database and potentially present in the spectrum (green lines);
+clicking on any of these lines displays the associated spectroscopic parameters.
+
+**More Information:**
+
+{{ side-image >}}
+
+{{< side-image image="ETC-Logo-125.png" thumbnail="ETC-Logo-125.png" position="left" >}}
+
+### ETC-42
+
+ETC-42 is a Generic Exposure Time Calculator developed by CeSAM/LAM. Unlike
+usual existing ETCs, it can calculate the Signal to Noise Ratio (SNR) for any
+site and instrumentation type and perform simulations for a wide range of
+existing or future telescopes. It can simulate objects using theoretical
+spectral distributions (black bodies, flat energy flux, etc) or with user
+defined (or imported via SAMP) spectra. Simulation results can be saved,
+exported or broadcast in VOTable format. A plugin framework is also available
+for pre and post process of simulations. ETC-42 provides a user friendly
+Graphical User Interface (GUI) as well as a command line mode supporting script
+execution.
+
+**More Information:**
+
+{{ side-image >}}
+
+---
+
+# Some recent papers about VO-enabled science
+
+### Featured Paper
+
+[A Cross-correlation Analysis of Active Galactic Nuclei and Galaxies Using Virtual Observatory: Dependence on Virial Mass of Supermassive Black Hole](http://adsabs.harvard.edu/abs/2013ApJ...775...43K)
+**Komiya, Yutaka; Shirasaki, Yuji; Ohishi, Masatoshi; Mizumoto, Yoshihiko**
+_The Astrophysical Journal, Volume 775, Issue 1, article id. 43, 12 pp. (2_013)._
+
+We present results of the cross-correlation analysis between active galactic
+nuclei (AGNs) and galaxies at redshift 0.1-1. We obtain data of ~10, 000 Sloan
+Digital Sky Survey AGNs in which their virial masses with a supermassive black
+hole (SMBH) were estimated. The UKIDSS galaxy samples around the AGNs were
+obtained using the virtual observatory. The scale length of AGN-galaxy
+cross-correlation for all of the samples is measured to be r_0=
+5.8^{+0.8}_{-0.6}\,h^{-1}\,Mpc (for the fixed slope parameter γ = 1.8). We also
+derived a dependence of r0 on the BH mass, MBH, and found an indication of an
+increasing trend of r0 at MBH > 108 M⊙. It is suggested that the growth of SMBHs
+is mainly driven by interactions with the surrounding environment for MBH > 108
+M⊙. On the other hand, at MBH <~ 108 M⊙, we did not find the BH mass dependence.
+This would imply that for less massive BHs, the mass growth process can be
+different from that for massive BHs.
+
+### Refereed Publications
+
+* [Astropy: A community Python package for astronomy](http://adsabs.harvard.edu/abs/2013A%26A...558A..33A)
+ _Astropy Collaboration
+ Astronomy & Astrophysics, Volume 558, id.A33, 9 pp. (2013)._
+
+* [Characterization of the gaseous companion κ Andromedae b. New Keck and LBTI high-contrast observations](http://adsabs.harvard.edu/abs/2014A%26A...562A.111B)
+ _Bonnefoy, M.; Currie, T.; Marleau, G.-D.; et al.
+ Astronomy & Astrophysics, Volume 562, id.A111, 20 pp. (2014)._
+
+* [The green valley is a red herring: Galaxy Zoo reveals two evolutionary pathways towards quenching of star formation in early- and late-type galaxies](http://adsabs.harvard.edu/abs/2014MNRAS.440..889S)
+ _Schawinski, Kevin; Urry, C. Megan; Simmons, Brooke D.; Fortson, Lucy; Kaviraj, Sugata; Keel, William C.; Lintott, Chris J.; Masters, Karen L.; Nichol, Robert C.; Sarzi, Marc; Skibba, Ramin; Treister, Ezequiel; Willett, Kyle W.; Wong, O. Ivy; Yi, Sukyoung K.
+ Monthly Notices of the Royal Astronomical Society, Volume 440, Issue 1, p.889-907. (2014)_
+
+* [Empirical Links between XRB and AGN Accretion Using the Complete z < 0.4 Spectroscopic CSC/SDSS Catalog](http://adsabs.harvard.edu/abs/2013ApJ...778..188T)
+ _Trichas, Markos; Green, Paul J.; Constantin, Anca; Aldcroft, Tom; Kalfountzou, Eleni; Sobolewska, Malgosia; Hyde, Ashley K.; Zhou, Hongyan; Kim, Dong-Woo; Haggard, Daryl; Kelly, Brandon C.
+ The Astrophysical Journal, Volume 778, Issue 2, article id. 188, 12 pp. (2013)._
+
+* [Cepheids in open clusters: an 8D all-sky census](http://adsabs.harvard.edu/abs/2013MNRAS.434.2238A)
+ _Anderson, Richard I.; Eyer, Laurent; Mowlavi, Nami
+ Monthly Notices of the Royal Astronomical Society, Volume 434, Issue 3, p.2238-2261 (2013)._
+
+* [Kepler-91b: a planet at the end of its life. Planet and giant host star properties via light-curve variations](http://adsabs.harvard.edu/abs/2014A%26A...562A.109L)
+ _Lillo-Box, J.; Barrado, D.; Moya, A.; Montesinos, B.; Montalbán, J.; Bayo, A.; Barbieri, M.; Régulo, C.; Mancini, L.; Bouy, H.; Henning, T.
+ Astronomy & Astrophysics, Volume 562, id.A109, 19 pp. (2013)._
+
+* [X-shooter spectroscopy of young stellar objects. III. Photospheric and chromospheric properties of Class III objects](http://adsabs.harvard.edu/abs/2013A%26A...558A.141S)
+ _Stelzer, B.; Frasca, A.; Alcalá, J. M.; Manara, C. F.; Biazzo, K.; Covino, E.; Rigliaco, E.; Testi, L.; Covino, S.; D'Elia, V.
+ Astronomy & Astrophysics, Volume 558, id.A141, 16 pp. (2013)._
+
+* [An in-depth study of HD 174966 with CoRoT photometry and HARPS spectroscopy. Large separation as a new observable for δ Scuti stars](http://adsabs.harvard.edu/abs/2013A%26A...559A..63G)
+ _García Hernández, A.; Moya, A.; Michel, E.; Suárez, J. C.; Poretti, E.; Martín-Ruíz, S.; Amado, P. J.; Garrido, R.; Rodríguez, E.; Rainer, M.; Uytterhoeven, K.; Rodrigo, C.; Solano, E.; Rodón, J. R.; Mathias, P.; Rolland, A.; Auvergne, M.; Baglin, A.; Baudin, F.; Catala, C.; Samadi, R.
+ Astronomy & Astrophysics, Volume 559, id.A63, 14 pp. (2013)._
+
+* [The stellar mass-size relation for the most isolated galaxies in the local Universe](http://adsabs.harvard.edu/abs/2013MNRAS.434..325F)
+ _Fernández Lorenzo, M.; Sulentic, J.; Verdes-Montenegro, L.; Argudo-Fernández, M.
+ Monthly Notices of the Royal Astronomical Society, Volume 434, Issue 1, p.325-335 (2013)._
+
+* [Red bulgeless galaxies in SDSS DR7. Are there any AGN hosts?](http://adsabs.harvard.edu/abs/2013MNRAS.436.2426C)
+ _Coelho, B.; Antón, S.; Lobo, C.; Ribeiro, B.
+ Monthly Notices of the Royal Astronomical Society, Volume 436, Issue 3, p.2426-2434 (2013)._
+
+* [KIC 3858884: a hybrid δ Scuti pulsator in a highly eccentric eclipsing binary](http://adsabs.harvard.edu/abs/2014A%26A...563A..59M)
+ _Maceroni, C.; Lehmann, H.; da Silva, R.; Montalbán, J.; Lee, C.-U.; Ak, H.; Deshpande, R.; Yakut, K.; Debosscher, J.; Guo, Z.; Kim, S.-L.; Lee, J. W.; Southworth, J.
+ Astronomy & Astrophysics, Volume 563, id.A59, 17 pp. (2014)._
+
+* [The Millennium Run Observatory: first light](http://adsabs.harvard.edu/abs/2013MNRAS.428..778O)
+ _Overzier, R.; Lemson, G.; Angulo, R. E.; Bertin, E.; Blaizot, J.; Henriques, B. M. B.; Marleau, G.-D.; White, S. D. M.
+ Monthly Notices of the Royal Astronomical Society, Volume 428, Issue 1, p.778-803 (2013)._
+ **Note:** There are a [number of papers](http://labs.adsabs.harvard.edu/adsabs/search/?month_to=&db_f=%28astronomy+OR+physics%29&year_from=&bigquery=&month_from=&q=gavo+millennium&article=1&nr=&prop_f=refereed&year_to=) that cite the [GAVO interface for Millenium](http://gavo.mpa-garching.mpg.de/Millennium/).
+
+* [WINGS Data Release: a database of galaxies in nearby clusters](http://adsabs.harvard.edu/abs/2014A%26A...564A.138M)
+ _Moretti, A.; Poggianti, B. M.; Fasano, G.; Bettoni, D.; D'Onofrio, M.; Fritz, J.; Cava, A.; Varela, J.; Vulcani, B.; Gullieuszik, M.; Couch, W. J.; Omizzolo, A.; Valentinuzzi, T.; Dressler, A.; Moles, M.; Kjærgaard, P.; Smareglia, R.; Molinaro, M.
+ Astronomy & Astrophysics, Volume 564, id.A138, 11 pp. (2014)._
+
+* [Measuring mean densities of δ Scuti stars with asteroseismology. Theoretical properties of large separations using TOUCAN](http://adsabs.harvard.edu/abs/2014A%26A...563A...7S)
+ _Suárez, J. C.; García Hernández, A.; Moya, A.; Rodrigo, C.; Solano, E.; Garrido, R.; Rodón, J. R.
+ Astronomy & Astrophysics, Volume 563, id.A7, 11 pp. (2014)._
+
+* [Proper motions of young stars in Chamaeleon. II. New kinematical candidate members of Chamaeleon I and II](http://adsabs.harvard.edu/abs/2013A%26A...556A.144L)
+ _López Martí, Belén; Jiménez-Esteban, Francisco; Bayo, Amelia; Barrado, David; Solano, Enrique; Bouy, Hervé; Rodrigo, Carlos
+ Astronomy & Astrophysics, Volume 556, id.A144, 11 pp. (2013)._
+
+* [Kepler observations of very low-mass stars](http://adsabs.harvard.edu/abs/2013A%26A...555A.108M)
+ _Martín, E. L.; Cabrera, J.; Martioli, E.; Solano, E.; Tata, R.
+ Astronomy & Astrophysics, Volume 555, id.A108, 11 pp. (2013)._
+
+### More Ways to Find VO-related Publications
+
+[All ADS links](http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?db_key=AST&db_key=PRE&qform=AST&arxiv_sel=astro-ph&arxiv_sel=cond-mat&arxiv_sel=cs&arxiv_sel=gr-qc&arxiv_sel=hep-ex&arxiv_sel=hep-lat&arxiv_sel=hep-ph&arxiv_sel=hep-th&arxiv_sel=math&arxiv_sel=math-ph&arxiv_sel=nlin&arxiv_sel=nucl-ex&arxiv_sel=nucl-th&arxiv_sel=physics&arxiv_sel=quant-ph&arxiv_sel=q-bio&sim_query=YES&ned_query=YES&aut_logic=OR&obj_logic=OR&author=&object=&start_mon=&start_year=&end_mon=&end_year=&ttl_logic=OR&title=&txt_logic=OR&text=%22virtual+observatory%22&nr_to_return=200&start_nr=1&jou_pick=ALL&ref_stems=&data_and=ALL&group_and=ALL&start_entry_day=&start_entry_mon=&start_entry_year=&end_entry_day=&end_entry_mon=&end_entry_year=&min_score=&sort=SCORE&data_type=SHORT&aut_syn=YES&ttl_syn=YES&txt_syn=YES&aut_wt=1.0&obj_wt=1.0&ttl_wt=0.3&txt_wt=3.0&aut_wgt=YES&obj_wgt=YES&ttl_wgt=YES&txt_wgt=YES&ttl_sco=YES&txt_sco=YES&version=1) mentioning the "virtual observatory" in the abstract
+
+[All refereed publications](http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?db_key=AST&qform=AST&arxiv_sel=astro-ph&arxiv_sel=cond-mat&arxiv_sel=cs&arxiv_sel=gr-qc&arxiv_sel=hep-ex&arxiv_sel=hep-lat&arxiv_sel=hep-ph&arxiv_sel=hep-th&arxiv_sel=math&arxiv_sel=math-ph&arxiv_sel=nlin&arxiv_sel=nucl-ex&arxiv_sel=nucl-th&arxiv_sel=physics&arxiv_sel=quant-ph&arxiv_sel=q-bio&sim_query=YES&ned_query=YES&aut_logic=OR&obj_logic=OR&author=&object=&start_mon=&start_year=&end_mon=&end_year=&ttl_logic=OR&title=&txt_logic=OR&text=%22virtual+observatory%22&nr_to_return=200&start_nr=1&jou_pick=NO&ref_stems=&data_and=ALL&group_and=ALL&start_entry_day=&start_entry_mon=&start_entry_year=&end_entry_day=&end_entry_mon=&end_entry_year=&min_score=&sort=SCORE&data_type=SHORT&aut_syn=YES&ttl_syn=YES&txt_syn=YES&aut_wt=1.0&obj_wt=1.0&ttl_wt=0.3&txt_wt=3.0&aut_wgt=YES&obj_wgt=YES&ttl_wgt=YES&txt_wgt=YES&ttl_sco=YES&txt_sco=YES&version=1) mentioning the "virtual observatory" in the abstract
+
+---
+
+# VO calendar
+
+* **18-23 May 2014 - [IVOA Interoperability Meeting](http://www.sciops.esa.int/index.php?project=CONF2014&page=IVOA2014)**
+
+ (ESAC, Villanueva de la Cañada, Madrid, Spain)
+
+ The IVOA Interop Meetings are aimed at making significant progress in defining
+ standards and sharing best practices in the development of the world wide
+ Virtual Observatory initiatives.
+
+* **9-11 July 2014 - [Gaia data visualization workshop](http://gaiaviz.univie.ac.at/home/)**
+
+ (University Observatory, Vienna, Austria)
+
+ The main goal of the Gaia data visualization workshop is to bring together
+ astronomers, experts in data visualization, and researchers in other fields
+ dealing with the visualization of large data bases and discuss how to tackle
+ some of the challenging issues faced by Gaia data visualization.
+
+* **25-29 Aug 2014- [Astroinformatics 2014](http://eventos.cmm.uchile.cl/astro2014/)**
+
+ (Center for Mathematical Modeling (CMM), University of Chile, Valparaiso, Chile)
+
+* **5-9 October 2014 - [ADASS XXIV](http://www.adass.org/futureven.html)**
+
+ (Calgary, Canada)
+
+* **10-12 October 2014 - [IVOA Interoperability Meeting](http://wiki.ivoa.net/twiki/bin/view/IVOA/IvoaEvents)**
+
+ (Banff, Alberta, Canada)
+
+* **12-14 November 2014 - [2014 Conference on Big Data from Space (BiDS '14)](http://congrexprojects.com/2014-events/BigDatafromSpace/introduction)**
+
+ (ESRIN, Frascati, Italy)
+
+ This conference aims to bring together researchers, engineers, users in the
+ area of Big Data in the Space sector. The focus is on the whole data
+ lifecycle, ranging from data acquisition by spaceborne and ground-based
+ sensors to data management, analysis and exploitation in the domains of Earth
+ Observation, Space Science, Space Engineering, Space Weather, etc.
+
+* **8-10 December 2014 - [.Astronomy 6](http://dotastronomy.com/six/)**
+
+ (Adler Planetarium, Chicago, Illinois, USA)
+
+ .Astronomy (pronounced 'dot-astronomy') aims to bring together an
+ international community of astronomy researchers, developers, educators and
+ communicators to showcase and build web-based projects, from outreach and
+ education to research tools and data analysis.
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