Latest Space News
Fri, 20 Oct 2017 00:00:00 +0100
"Using a model that more realistically simulates atmospheric conditions, we discovered a new process that controls the habitability of exoplanets and will guide us in identifying candidates for further study," said Yuka Fujii of NASA's Goddard Institute for Space Studies (GISS), New York, New York and the Earth-Life Science Institute at the Tokyo Institute of Technology, Japan, lead author of a paper on the research published in the Astrophysical Journal Oct. 17. Previous models simulated atm...
Thu, 19 Oct 2017 22:40:00 +0100
NASA has selected Space Exploration Technologies (SpaceX) of Hawthorne, California, to provide launch services for the Sentinel-6A mission. Launch is currently targeted for November 2020, on a SpaceX Falcon 9 Full Thrust rocket from Space Launch Complex 4E at Vandenberg Air Force Base in California. The total cost for NASA to launch Sentinel-6A is approximately $97 million, which includes the launch service and other mission related costs. The Sentinel-6A mission, also known as Jason Conti...
Thu, 19 Oct 2017 00:00:00 +0100
NASA Team Finds Noxious Ice Cloud on Saturn's Moon Titan Researchers with NASA's Cassini mission found evidence of a toxic hybrid ice in a wispy cloud high above the south pole of Saturn's largest moon, Titan. The finding is a new demonstration of the complex chemistry occurring in Titan's atmosphere-in this case, cloud formation in the giant moon's stratosphere-and part of a collection of processes that ultimately helps deliver a smorgasbord of organic molecules to Titan's surface. Inv...
Tue, 17 Oct 2017 00:00:00 +0100
ESO's fleet of telescopes in Chile have detected the first visible counterpart to a gravitational wave source. These historic observations suggest that this unique object is the result of the merger of two neutron stars. The cataclysmic aftermaths of this kind of merger - long-predicted events called kilonovae - disperse heavy elements such as gold and platinum throughout the Universe. This discovery, published in several papers in the journal Nature and elsewhere, also provides the strongest ev...
Tue, 17 Oct 2017 00:00:00 +0100
For the first time, NASA scientists have detected light tied to a gravitational-wave event, thanks to two merging neutron stars in the galaxy NGC 4993, located about 130 million light-years from Earth in the constellation Hydra. Shortly after 8:41 a.m. EDT on Aug. 17, NASA's Fermi Gamma-ray Space Telescope picked up a pulse of high-energy light from a powerful explosion, which was immediately reported to astronomers around the globe as a short gamma-ray burst. The scientists at the National S...
Mon, 16 Oct 2017 18:43:00 +0100
Thales Alenia Space has signed a contract with Airbus Defence and Space GmbH to develop the feed array system for the antenna on the European Space Agency's Biomass spacecraft. This equipment is essential to guarantee the full satellite performance. One of ESA's Earth Explorer missions dedicated to protect our planet, Biomass will help us understand the quantity of carbon stored in the world's forests within the global carbon cycle. Due for launch in 2021, Biomass is primarily designed to d...
Sun, 15 Oct 2017 08:00:00 +0100
A United Launch Alliance (ULA) Atlas V rocket carrying a payload for the National Reconnaissance Office lifted off from Space Launch Complex-41 on Oct. 15 at 3:28 a.m. EDT. Designated NROL-52, the mission is in support of national security. "Today's launch is a testament to the tireless dedication of the ULA team, demonstrating why ULA continues to serve as our nation's most dependable and successful launch provider," said Laura Maginnis, ULA vice president of Government Satellite Launch. "Af...
Fri, 13 Oct 2017 13:05:00 +0100
The first Copernicus mission dedicated to monitoring our atmosphere, Sentinel-5P, has been launched from the Plesetsk Cosmodrome in northern Russia. The 820 kg satellite was carried into orbit on a Rockot launcher at 09:27 GMT (11:27 CEST) today. The first stage separated 2 min 16 sec after liftoff, followed by the fairing and second stage at 3 min 3 sec and 5 min 19 sec, respectively. The upper stage then fired twice, delivering Sentinel-5P to its final orbit 79 min after liftoff. ...
Fri, 13 Oct 2017 10:55:00 +0100
The first full-scale model of the rocket motor that will propel Ariane 6 and Vega-C into orbit has been cast and filled with inert propellant for testing at Europe's Spaceport in French Guiana. The P120C is the largest solid-propellant rocket motor ever built in one segment. Each P120C will hold over 140 tonnes of propellant in a carbon fibre casing almost 11.5 m long and about 3.4 m in diameter. It is derived from Vega's current first stage motor, the P80, which holds 88 tonnes of propell...
Fri, 13 Oct 2017 00:00:00 +0100
There's no map showing all the billions of exoplanets hiding in our galaxy -- they're so distant and faint compared to their stars, it's hard to find them. Now, astronomers hunting for new worlds have established a possible signpost for giant exoplanets. A new study finds that giant exoplanets that orbit far from their stars are more likely to be found around young stars that have a disk of dust and debris than those without disks. The study, published in The Astronomical Journal, focused on ...
Fri, 13 Oct 2017 00:00:00 +0100
Our 4th Space Resiliency Summit is designed as an educational and training ''Town Hall'' forum, where thought leaders and key policy-makers across military services, defense agencies, and civilian organizations can come together for actionable discussions and debate. This year's summit will focus on technology and innovation needed to defend critical space assets against increasing and new threats. Download Conference Agenda | Register to attend this Conference 2017 Summit Topics to Includ...
Thu, 12 Oct 2017 08:50:00 +0100
EchoStar Corp. (NASDAQ: SATS) announced today that the EchoStar 105/SES-11 satellite was successfully launched on October 11 at 6:53 PM EDT on a SpaceX Falcon 9 vehicle from NASA's Kennedy Space Center in Florida. EchoStar 105/SES-11, a dual-mission satellite for EchoStar and SES, is a hybrid Ku and C-band communications satellite that provides EchoStar with 24 Ku-band transponders of 36 MHz, marketed as EchoStar 105, and SES with a C-band payload of 24 transponders, marketed under the name S...
Tue, 10 Oct 2017 14:00:00 +0100
Raytheon Company (NYSE: RTN) was recently selected by DigitalGlobe, Inc. as the next-generation WorldView Legion satellite imaging constellation payload provider. Under the contract, Raytheon will deliver the telescopes, detectors and combined electronics to Space Systems Loral, the WorldView Legion space vehicle integrator. Raytheon's new payload doubles DigitalGlobe's capacity to capture multispectral and 30 cm imagery, while tripling to quadrupling the company's capacity to image high-dema...
Tue, 10 Oct 2017 13:32:00 +0100
Mission controllers completed a critical final rehearsal today, confirming that everything and everyone on ground are ready to take over control of Sentinel-5P in the harsh environment of space. A 'team of teams' working at ESA's control centre in Darmstadt, Germany, today conducted a final rehearsal for this week's launch of Sentinel-5P. They were joined by engineers working at ground stations on three continents and by teams responsible for the launcher and its payload in Plesetsk, Russ...
Tue, 10 Oct 2017 13:00:00 +0100
Ushering in a new era of advanced Global Positioning System (GPS) technology, the U.S. Air Force declared the first Lockheed Martin (NYSE: LMT)-built GPS III satellite "Available for Launch." The Air Force's "AFL" declaration is the final acceptance of Lockheed Martin's first GPS III Space Vehicle (GPS III SV01) prior to its expected 2018 launch. GPS III SV01 will bring new capabilities to U.S. and allied military forces, and a new civil signal that will improve future connectivity worldwide ...
Mon, 9 Oct 2017 16:30:00 +0100
With four days to liftoff, the next Sentinel satellite is now on the launch pad at the Plesetsk Cosmodrome in northern Russia. The rocket will be fuelled two days before launch, set for Friday at 09:27 GMT (11:27 CEST). The Sentinel-5P satellite has been at the cosmodrome since early September going through a series of tests and being readied for the big day. After being sealed from view in the rocket fairing last week, it was rolled out to the launch pad on Saturday. "This point in any...
Mon, 9 Oct 2017 15:00:00 +0100
L3 Technologies (NYSE:LLL) announced today that it has been awarded a contract to provide Hawkeye(tm) III Lite VSAT satellite communications terminals and on-site training to the U.S. Air National Guard's Joint Incident Site Communications Capability (JISCC) teams. These terminals will facilitate direct communication from remote locations in all 50 states and U.S. territories. Additionally, these Army Strategic Command (ARSTRAT)-certified terminals will enable access to the Wideband Global SATCO...
Mon, 9 Oct 2017 12:03:00 +0100
The third batch of Iridium(r) NEXT satellites built by Thales Alenia Space has been successfully launched by SpaceX from Vandenberg Air Force Base in California. After the perfect commissioning of the first 20 satellites launched in January and June, thirteen of which are now interconnected and operating in full compatibility with the initial Block One Constellation, with seven being maneuvered to an adjacent plane, this new milestone allows to continue the fantastic Iridium(r) NEXT adventure. ...
Thu, 5 Oct 2017 00:00:00 +0100
Astronomers have identified a bumper crop of dual supermassive black holes in the centers of galaxies. This discovery could help astronomers better understand how giant black holes grow and how they may produce the strongest gravitational wave signals in the Universe. The new evidence reveals five pairs of supermassive black holes, each containing millions of times the mass of the Sun. These black hole couples formed when two galaxies collided and merged with each other, forcing their superma...
Wed, 4 Oct 2017 14:30:00 +0100
As preparations for the launch of Sentinel-5P continue on track, the team at Russia's Plesetsk site has bid farewell to the satellite as it was sealed from view in the Rockot fairing. Liftoff is set for 13 October at 09:27 GMT (11:27 CEST). Since its arrival at the launch site at the beginning of September, Sentinel-5P has been through a series of stringent tests to confirm there was no damage during the flight from the UK. These tests have made sure that everything is in good working orde...
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  • CV: Astronomy Researcher

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    Personal information
     Name:<withheld>
     Age:<withheld>
     Country:<withheld>
     Location:<withheld>
    Contact information
     Email:<withheld>
     Phone:<withheld>
     Mobile:<withheld>
    Candidate Profile
     Date Submitted:14-07-2014
     Last Modified:14-07-2014 (08:04)
    Job information
     Current job:Astronomy Researcher
     Employment Term:Either
     Job location:Europe only
     Date available:within 3months
     Industry:Business Services, Consulting/Engineering Services, Space Tourism
     KeywordsphD Spectroscopy
    CV

    Nationality:  Italy

    Country of Birth:  Italy

    Date of Birth: 30/01/1984

    City of Birth: Cento (Ferrara), Italy

     

    Current Professional Situation: 

    Studentship at the  University of Cambridge

     

    Institution: Cambridge University (Cambridge, UK)

    Modality of the contract: Temporary 

    Dates: 1 year (January 2014 - January 2015)

    Professional Activity:

    I am carrying out a research project on the study of  the 2D kinematic properties of the neutral gas (NaD 5890,5896 A) in a sample of 38 local Luminous and Ultra-Luminous Infrared Galaxies ([U]LIRGs, 31 LIRGs and 7 ULIRGs, 51 individual galaxies) observed with VIMOS/VLT. This sample covers well the less studied LIRG luminosity range, and it includes the morphological types corresponding to the different phases along the merging process (i.e., isolated disks, interacting systems, and mergers). This work differs from other  recent studies of galactic winds (e.g., Westmoquette et al. (2012)) by the comparison of the kinematics of the neutral gas and that of the ionized gas on spaxel-by-spaxel basis (0.6’’ spatial sampling) and by the ability to probe simultaneously multiple gas phases (neutral and ionized).

    Later, I will extend this study to other kind of feedback mechanisms (e.g., SF occurring in outflows) in a small sample of three galaxies (hosting an AGN) by using near-IR spectroscopy data taken with Near Infrared Camera Spectrometer (NICS) mounted on the Telescopio Nazionale Galileo (La Palma, Islas Canarias/España).

     

    Context:

    It is crucial to understand the forces central to galaxy evolution, including physical feedback processes during the lifetime of a galaxy, such as winds. Multiphase galactic winds are ever present in starburst galaxies, and their main properties can directly be probed by the NaD lines produced by the neutral phase of the outflowing gas. The results for local wind could be used for a direct comparison other feedback mechanisms.

     

    Position held before current job

     

    CSIC-Contract

    Institution: CSIC-CAB (Torrejon de Ardoz, Madrid)

    Modality of the contract: Temporary 

    Dates: 1 year (January 2013 - December 2013)

    Professional Activity:

    I have carried out a research training project on the study of the neutral gas kinematics of [U]LIRGs using VIMOS/VLT Integral Field Spectroscopy (IFS) data. I have investigated the presence of outflows in these galaxies using the Sodium absorption line feature (NaD 5890,5896 A). I have studied the kinematics of the neutral gas using 2-D (spatially resolved) IFS data. 

     

    Paper: Spatially resolved kinematics, galactic wind, and quenching of star formation in the luminous infrared galaxy IRAS F11506-3851. Cazzoli et al. 2014 - accepted: A&A

     

    Marie Curie Contract

    Institution: CSIC-CAB (Torrejon de Ardoz, Madrid)

    Modality of the contract: Temporary 

    Dates: 2 years (September 2010 - September 2012)

    Professional Activity:

    I have carried out a research training project on the study of the neutral gas kinematics of [U]LIRGs using VIMOS/VLT Integral Field Spectroscopy (IFS) data. I have investigated the presence of outflows in these galaxies using the Sodium absorption line feature (NaD 5890,5896 A). I have studied the kinematics of the neutral gas using 1-D (spatially integrated spectra).

     

    Keywords. galaxies: starburst — ISM: jets and outflows — ISM: kinematics and dynamics

    This work  was funded by the Marie Curie Initial Training Network ELIXIR (EarLy UnIverse eXploration with nIRspec) of the European Commission under contract PITN-GA-2008-214227.

     

     

    Stage at  Alma Mater Studiorum Bologna

    Institution: University,  Alma Mater Studiorum Bologna 

    Modality of the contract: Temporary 

    Dates: 8 months (starting: 01/2010)

    Professional Activity:

    After my graduation, I was in Bologna to extend my project characterizing with multi wavelength data the X-Ray Sources around the galaxy cluster Abells1995 (e.g. looking for the optical counterparts of these sources). I studied the source-counts in the very deep and wide surveys that have been recently  performed with XMM-Newton and Chandra Observatory (e.g. C-COSMOS and XMM-COSMOS) to reveal AGN overdensities and to study the phenomenology and evolution of the galaxy/AGN population as a function of the environment. I showed my results during seminars and conferences.

     

    Keywords: Large Scale Structures, Cosmology, Multi-band Photometry, Surveys

     

    Training Received

    My University education consisted of two levels, for a total of 5 years (3 years Bachelor, 2 years Master).

    First Level Degree (Bachelor Degree)

    Official University Qualification: “Laurea in Fisica e Astrofisica” / Degree in Physics and Astrophysics (with a grade of 102 in a scale with a maximum grade of 110)

    Entity issuing the qualification: University of Ferrara

    Date of qualification: 26/03/2007

    Master Degree 

    Official University Qualification: “Laurea Specialistica in Astrofisica e cosmologia” / Master Degree in Astrophysics and Cosmology (with a grade of 106 in a scale with a maximum grade of 110)

    Entity issuing the qualification:  Alma Mater Studiorum Bologna

    Date of qualification: 09/10/2009

     

    Language Skills

    Italian: Mother tongue

    English: Good [Speech, Reading and Writing]

    Spanish: Good [Speech, Reading and Writing]

    French: Sufficient [Speech, Reading and Writing]

     

    Scientific Activities

     

    Schools

    Titile: The complex physics of dusty star-forming galaxies and AGN

    Institution:  Universita’ di Bologna, Bologna, Italy

    Dates: 4 days  (starting: 19/05/014) 

     

    Titile: Simulations of NIRSpec observations

    Institution:  European Space Agency (ESA-ESTEC), Noordwijk, Holland

    Dates: 2 days  (26-27/09/2012)

     

    Title: International School for Advanced Instrumentation (IScAI)

    Institution:  Istituto de Astrofisica de Canarias (IAC)

    Dates: 1 week (starting: 14/05/2012)

     

    Title: How a Space Project Works ?

    Institution: European Space Agency (ESA-ESTEC), Noordwijk, Holland

    Dates: 4 days, (starting from: 10/05/2011)

    Type of participation: Attending, and I also chair the session about the JWST management)

     

    Title: Physical properties of Active Galactic Nuclei

    Institution: Alma Mater Studiorum, Universita di Bologna (Italy)

    Dates: 1 week (starting: 20/10/2010)

     

    Title: Gravitational lenses and dark matter – Black holes in astrophysics

    Institution: University, Madonna di Campiglio, Trento (Italy)

    Dates: 1 week (starting: 27/06/2010)

     

     

     

     

    Conferences, Workshops, Seminars and ELIXIR Meetings

    Conference: "3D2014: Gas and stars in galaxies: A multi-wavelength 3D perspective"

    Institution: ESO, Garching (Germany)

    Dates: 5 days (starting: 10/03/2014)

    Type of participation: Poster 

    Title of the poster: A search of neutral gas outflows in nearby [U]LIRGs via optical IFS of the NaD feature

    Authors: Sara Cazzoli,  Santiago Arribas, Roberto Maiolino and Luis Colina

     

    Conference: 2012 STScI May Symposium: Gas Flows in Galaxies

    Institution: Space Telescope Science Institute (Baltimore, USA)

    Dates: 5 days (starting: 06/05/2012)

    Type of participation: Poster 

    Title of the poster: Neutral gas kinematics of Luminous and Ultra-Luminous Infrared Galaxies([U]LIRGs) using Very Large Telescope (VLT)-VIMOS Integral Field Spectroscopy (IFS) Data

    Authors: Sara Cazzoli,  Santiago Arribas

     

    Conference: Metals in 3D: New Insights from Integral Field Spectroscopy

    Institution: Instituto de Astrofísica de Andalucía - CSIC and AIP (Granada, Spain)

    Dates: 3 days (starting: 18/04/2012)

    Type of participation: attending

     

    Conference: IX° Congresso Nazionale sui Nuclei Galattici Attivi (AGN 9)

    Institution: University of Ferrara (Italy)

    Dates: 5 days (starting: 24/05/2010)

    Type of participation: Poster

    Title: Analysis of a Large Scale Structure at redshift~0.3 with the Chandra Observatory

    Authors: Sara Cazzoli; Cristian Vignali; Roberto Gilli; Andrea Comastri

     

    Conference: X-Ray Astronomy 2009 (present status multi wavelength approach and future perspectives)

    Institution: Alma Mater Studiorum, Universita di Bologna (Italy)

    Dates: 4 days (starting: 07/09/2009)

    Type of participation: attending

     

     

     

    Workshop: OSIRIS pipeline

    Date: 21/01/2013

    Institution: Universidad Complutense de Madrid

    Type of participation: attending

     

     

     

    Seminar:   “Young Researcher’s Day” 

    dates: 23-24/10/2012

    Institution: CSIC -CAB Torrejon de Ardoz

    Type of participation:  talk 

     

    Seminar:  “Reuniones de Formación y Evolución de Galaxias" 

    Dates: 17/10/2012

    Institution: CSIC -CAB Torrejon de Ardoz

    (in collaboration with CAB (VillaFranca) and OAN)

    Type of participation:  talk 

    Title: VIMOS/VLT Spectroscopy for a sample of low redshift (U)LIRGs: 2-D neutral gas kinematics and galactic winds

     

    Seminar

    Institution: Fondazione Galileo, La Palma, Canary Islands, Spain

    Dates: 25/03/2011

    Type of participation: Talk

    Title: Neutral gas kinematics in Luminous and Ultra-Luminous Infrared Galaxies

     

     

     

     

    Meeting: ELIXIR Meting

    Institution: Leiden Observatory, Holland

    Dates: 2 days (12-13/11/2012)

    Type of participation: Talk

     

    Meeting: ELIXIR annual Meeting

    Institution: Consejo Superior de Investigacion Cientificas (CSIC), Madrid

    Dates: 3 days (starting: 04/10/2011)

    Type of participation: Talk

    Title:  2-D Neutral gas kinematics of Luminous and Ultra-Luminous Infrared Galaxies using VLT-VIMOS Integral Field Spectroscopy

    Authors: Sara Cazzoli,  Santiago Arribas

     

    Meeting: ELIXIR Mid Term Review

    Institution: Institut Astrophysique de Paris (IAP), France

    Dates: 3days (starting from: 02/11/2010)

    Type of participation: Talk

    Title:  2-D Neutral gas kinematics of Luminous and Ultra-Luminous Infrared Galaxies

    Authors: Sara Cazzoli,  Santiago Arribas

     

     

     

    Experiences in organising scientific events

    Conference: ELIXIR annual Meeting and NIRSpec Instrument Science Team Meeting

    Institution: CSIC, Madrid

    Dates: 4 days (starting: 04/10/2011)

    Type of participation: Logistic and Organizing 

     

    Conference: X-Ray Astronomy 2009 (present status multi wavelength approach and future perspectives)

    Institution: Alma Mater Studiorum, Universita di Bologna (Italy)

    Dates: 4 days (starting: 07/09/2009)

    Type of participation: Logistic help during the conference

     

    Seminars: “Reuniones de Formación y Evolución de Galaxias" 

    (in collaboration with CAB (VillaFranca) and OAN)

    Institution: CSIC -CAB Torrejon de Ardoz

    Type of participation:  Logistic and Organizing

     

     

     

    Other Activities 

    Observing Program: SFR tracers in dusty galaxies: Narrow-band imaging in Halpha of local LIRGs

    Telescope: North Optical Telescope (NOT, Observatorio del Roque de los Muchachos)

    Dates: 3 nights (11/2011) 

    Type of participation: Observer.

     

     

     

    Observing Program: Studying the AGN triggering mechanism in the medium-high density environments

    Telescope: Telescopio Nazionale Galileo (TNG, Observatorio del Roque de los Muchachos) 

    Dates: 2 nights (11/2011) 

    Type of participation: Observer.

     

     

     

    Observational Proposal (Accepted):

    Title: Sub-kpc Kenicutt-Schmidt star formation law in luminous infrared disks

    PI: Luis colina

     

     

     


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