SHELLQs-ALMA (Cycle 4)

Size: px
Start display at page:

Download "SHELLQs-ALMA (Cycle 4)"

Transcription

1 ver Mar. 23, 2017 SHELLQs-ALMA (Cycle 4) Takuma Izumi IoA/UTokyo

2 Cycle 4 Data Delivery Quasar zopt M1450 Deliver (JST) DL (Mpc) LBol (Lsun) BAL J Feb E+12 N J Feb E+13 N J Feb E+12 Y J waiting! E+12 N - From Cycle 4 proposal Three of Four quasar-data targeted in Cycle 4 were delivered recently. Pipeline-reduced visibility data are now being manually CLEANed/analyzed.

3 Quick Look: J beam [CII] 158μm

4 Spatial distribution [CII] Single Gaussian z[cii] = / ~0.18 mjy/beam@dv~50 km/s Double Gaussian θ = 0.54 x 0.43 Color = continuum (1σ = 13.9 μjy/beam) Contour = [CII] mom0 (3,5,7,10σ; 1σ = Jy/beam*km/s) Both (rest) FIR continuum and [CII] line emission are clearly detected! - Peak value; continuum = 97.1μJy/beam (~7σ), [CII] moment 0 = Jy/beam*km/s (~11σ) The [CII] line profile (@center) is skewed. Better to fit with double Gaussians.

5 Channel map The [CII] emission is concentrated to the central 1 = 5.8 kpc region. Elongation to N-S direction? [CII]: Red contour = -3,3,5,7σ; 1σ = mjy/beam@dv~50 km/s Band 6 continuum: Black contour = 3,5,6σ; 1σ = 13.9μJy/beam

6 Integrated values Peak: / mjy Center: / km/s FWHM: / km/s S = / Jy*km/s Peak1: / mjy Center1: / km/s FWHM1: / km/s S1 = / Jy*km/s Peak2: / mjy Center2: / km/s FWHM2: / km/s S2 = / Jy*km/s Flux measurement over the entire emitting region. - [CII]: 1σ = = 50 km/s Double Gaussians are still required. Total [CII]: / Jy*km/s L[CII] = / E9 Lsun (Td = 47 K, β = 1.6; integrated over μm) Total B6 continuum: / mjy LFIR = / E11 Lsun Mdust = / E7 Msun Peak = / μjy/b, Total = / mjy, offset/ = (0.10, 0.00), θm = / , θm = / , PA = deg Beam-deconvolved: θm = 0.50, θm = 0.261, PA = -0.6 deg

7 Quick Look: J beam [CII] 158μm

8 Spatial distribution [CII] z[cii] = / θ = 0.54 x mjy/beam@dv~50 (47) km/s Color = continuum (1σ = 20.2 μjy/beam) Contour = [CII] mom0 (3,4σ; 1σ = Jy/beam*km/s) Peak: / mjy/beam Center: / km/s FWHM: / km/s S = / Jy/beam*km/s The negative feature@~ km/s is due to noise, as the same one is found in the before-continuum-subtracted cube. Both (rest) FIR continuum and [CII] line emission are detected! - Peak value; continuum = 101 μjy/beam (~5σ), [CII] moment 0 = Jy/beam*km/s (4.0σ)

9 Integrated values Peak: / mjy Center: / km/s FWHM: / km/s S = / Jy*km/s 0.29 mjy/beam@dv~50 (47) km/s Flux measurement over the entire emitting region. - [CII]: 1σ = ~ 50 (=47) km/s (Td = 47 K, β = 1.6; integrated over μm) Total [CII]: / Jy*km/s L[CII] = / E8 Lsun Total B6 continuum: / mjy LFIR = / E11 Lsun Mdust = / E7 Msun Peak = / μjy/b, Total = / mjy, offset/ = (0.038, ), θm = / , θm = / , PA = deg Beam-deconvolved: θm = 0.629, θm = 0.462, PA = 35.4 deg

10 Quick Look: J beam 1σ = 0.11 mjy/beam (dv ~ 50 km/s) [CII] 158μm

11 Spatial distribution [CII] z[cii] = / mjy/beam@dv~50 (47) km/s θ = 0.54 x 0.50 Color = continuum (1σ = 10.8 μjy/beam) Contour = [CII] mom0 (3,5,6σ; 1σ = Jy/beam*km/s) Peak: / mjy/beam Center: / km/s FWHM: / km/s S = / Jy/beam*km/s Both (rest) FIR continuum and [CII] line emission are detected! - Peak value; continuum = 124 μjy/beam (~11σ), [CII] moment 0 = Jy/beam*km/s (6.4σ)

12 Integrated values Peak: / mjy Center: / km/s FWHM: / km/s S = / Jy*km/s 0.10 mjy/beam@dv~50 (47) km/s Flux measurement over the entire emitting region. - [CII]: 1σ = 0.10 ~ 50 (=47) km/s (Td = 47 K, β = 1.6; integrated over μm) Total [CII]: / Jy*km/s L[CII] = / E8 Lsun Total B6 continuum: / mjy LFIR = / E11 Lsun Mdust = / E7 Msun Peak = / μjy/b, Total = / mjy, offset/ = (-0.171, ), θm = / , θm = / , PA = / deg Beam-deconvolved: θm = 0.551, θm = 0.402, PA = 78.5 deg

13 Our Quasars log (L[CII] [Lsun]) (b) z > 6 quasars : y = *x From Cycle 4 proposal J M1450 [absolute mag] J (BAL) J Venemans+16 Object log [CII] log FIR log [CII]/FIR M1450 J J J J

14 Other Emitters within FoV Object Line Continuum J0859 N N J1152 N N J2216 N N J Searched for S/N cube (i.e., before primary beam corrections) Other Lines@center Object J0859 J1152 J2216 Line N N N J1202 -

Quick report of the project 123 (submm follow-up)

Quick report of the project 123 (submm follow-up) HSC-AGN f2f meeting Aug. 26, 2016 @IPMU/Tokyo Quick report of the project 123 (submm follow-up) Takuma Izumi IoA/UTokyo 1 #123 Investigation of rest-frame far-ir to submm properties of z = 6-7 QSO-host

More information

High-z QSO (HSC #123)

High-z QSO (HSC #123) Jan. 6 th, 2016 HSC/AGN meeting Next DL = 21 April High-z QSO follow-up @mm/submm (HSC #123) - especially z > 6 objects - Takuma Izumi@IoA/UTokyo takumaizumi@ioa.s.u-tokyo.ac.jp This is a submm follow-up

More information

Can we do this science with SKA1-mid?

Can we do this science with SKA1-mid? Can we do this science with SKA1-mid? Let s start with the baseline design SKA1-mid expected to go up to 3.05 GHz Proposed array configuration: 133 dishes in ~1km core, +64 dishes out to 4 km, +57 antennas

More information

Sequence Obs ID Instrument Exposure uf Exposure f Date Observed Aimpoint (J2000) (ks) (ks) (α, δ)

Sequence Obs ID Instrument Exposure uf Exposure f Date Observed Aimpoint (J2000) (ks) (ks) (α, δ) 1 SUMMARY 1 G120.1+01.4 1 Summary Common Name: Tycho s Distance: 2.4 kpc ( Chevalier et al., 1980 ) Center of X-ray emission (J2000): ( 00 25 19.9, 64 08 18.2 ) X-ray size: 8.7 x8.6 Description: 1.1 Summary

More information

Journal Club Presentation on The BIMA Survey of Nearby Galaxies. I. The Radial Distribution of CO Emission in Spiral Galaxies by Regan et al.

Journal Club Presentation on The BIMA Survey of Nearby Galaxies. I. The Radial Distribution of CO Emission in Spiral Galaxies by Regan et al. Journal Club Presentation on The BIMA Survey of Nearby Galaxies. I. The Radial Distribution of CO Emission in Spiral Galaxies by Regan et al. ApJ, 561:218-237, 2001 Nov 1 1 Fun With Acronyms BIMA Berkely

More information

Feeding and Feedback in U/LIRGs: ALMA Case Studies

Feeding and Feedback in U/LIRGs: ALMA Case Studies Feeding and Feedback in U/LIRGs: ALMA Case Studies Kazushi Sakamoto 2015-06-01, "Galaxies of many colours" @Marstrand, Sweden Feedback in U/LIRGs: ALMA Studies on NGC 3256 and Arp 220 NGC 3256 Dual molecular

More information

Ivan Valtchanov Herschel Science Centre European Space Astronomy Centre (ESAC) ESA. ESAC,20-21 Sep 2007 Ivan Valtchanov, Herschel Science Centre

Ivan Valtchanov Herschel Science Centre European Space Astronomy Centre (ESAC) ESA. ESAC,20-21 Sep 2007 Ivan Valtchanov, Herschel Science Centre SPIRE Observing Strategies Ivan Valtchanov Herschel Science Centre European Space Astronomy Centre (ESAC) ESA Outline SPIRE quick overview Observing with SPIRE Astronomical Observation Templates (AOT)

More information

SUPPLEMENTARY INFORMATION

SUPPLEMENTARY INFORMATION In the format provided by the authors and unedited. VOLUME: 1 ARTICLE NUMBER: 0172 Formation of wide binaries by turbulent fragmentation Jeong-Eun Lee 1, Seokho Lee 1, Michael Dunham 2, Ken ichi Tatematsu

More information

Evolution of the Highest Redshift Quasars

Evolution of the Highest Redshift Quasars Evolution of the Highest Redshift Quasars Xiaohui Fan University of Arizona Collaborators: Becker, Bertoldi, Carilli, Cox, Diamond-Stanic, Hennawi, Ivezic, Jiang, Kelly, Richards, Schneider, Strauss, Vestergaard,

More information

SPIRE In-flight Performance, Status and Plans Matt Griffin on behalf of the SPIRE Consortium Herschel First Results Workshop Madrid, Dec.

SPIRE In-flight Performance, Status and Plans Matt Griffin on behalf of the SPIRE Consortium Herschel First Results Workshop Madrid, Dec. SPIRE In-flight Performance, Status and Plans Matt Griffin on behalf of the SPIRE Consortium Herschel First Results Workshop Madrid, Dec. 17 2009 1 Photometer Herschel First Results Workshop Madrid, Dec.

More information

Lensing & Herschel unveils extreme starformation at z 2

Lensing & Herschel unveils extreme starformation at z 2 Lensing & Herschel unveils extreme starformation at z 2 with Shane Bussmann, Jae Calanog, Alex Conley, Asantha Cooray, Francesco De Bernardis, Rui Marques Chaves, Paloma Martínez Navajas, Ismael Perez

More information

SUPPLEMENTARY INFORMATION

SUPPLEMENTARY INFORMATION doi:10.1038/nature12001 Sample Selection The dusty-spectrum sources targeted for the ALMA observations described here were found in the SPT survey. The full survey comprises 2540 deg 2 of mapped sky, but

More information

Band 4 & 8 Imaging Verification Test Report: 30 May 2014

Band 4 & 8 Imaging Verification Test Report: 30 May 2014 Band 4 & 8 Imaging Verification Test Report: 30 May 2014 ALMA Technical Note Number: 3 Status: FINAL Prepared by: Organization: Date: Takahashi Satoko JAO/NAOJ 30 May 2014 Band 4 Imaging Verification Report

More information

Hughes et al., 1998 ApJ, 505, 732 : ASCA. Westerlund, 1990 A&ARv, 2, 29 : Distance to LMC 1 ) ) (ergs s F X L X. 2 s 1. ) (ergs cm

Hughes et al., 1998 ApJ, 505, 732 : ASCA. Westerlund, 1990 A&ARv, 2, 29 : Distance to LMC 1 ) ) (ergs s F X L X. 2 s 1. ) (ergs cm 1 SUMMARY 1 SNR 0525-66.1 1 Summary Common Name: N 49 Distance: 50 kpc (distance to LMC, Westerlund(1990) ) Position of Central Source (J2000): ( 05 25 59.9, -66 04 50.8 ) X-ray size: 85 x 65 Description:??

More information

e-vlbi observations of the first gamma-ray nova V407 Cyg

e-vlbi observations of the first gamma-ray nova V407 Cyg e-vlbi observations of the first gamma-ray nova V407 Cyg Marcello Giroletti (INAF Istituto di Radioastronomia, Bologna) and E. Koerding, K. Sokolovsky, F. Schinzel, T. Cheung on behalf of the Fermi-LAT

More information

THE LAST SURVEY OF THE OLD WSRT: TOOLS AND RESULTS FOR THE FUTURE HI ABSORPTION SURVEYS

THE LAST SURVEY OF THE OLD WSRT: TOOLS AND RESULTS FOR THE FUTURE HI ABSORPTION SURVEYS F. Maccagni; R. Morganti; T. Oosterloo; K. Geréb; N. Maddox, J. Allison THE LAST SURVEY OF THE OLD WSRT: TOOLS AND RESULTS FOR THE FUTURE HI ABSORPTION SURVEYS A SURVEY BEFORE THE BLIND SURVEYS During

More information

Multiwavelength Study of Distant Galaxies. Toru Yamada (Subaru Telescope, NAOJ)

Multiwavelength Study of Distant Galaxies. Toru Yamada (Subaru Telescope, NAOJ) Multiwavelength Study of Distant Galaxies Toru Yamada (Subaru Telescope, NAOJ) Studying Galaxy Formation with ALMA 1. Studying Galaxy Forming Region with ALMA 2. Multi-wavelength Study of Galaxy Formation/Evolution

More information

Radio Astronomy Project. VLA and VLBA Observations of AGN

Radio Astronomy Project. VLA and VLBA Observations of AGN Astronomy-423: Radio Astronomy Professor: Greg Taylor Spring 2006 Radio Astronomy Project VLA and VLBA Observations of AGN Adam Johnson Cristina Rodríguez Introduction It is important to observe radio

More information

Aperture Synthesis Observations of the Nearby Spiral NGC 6503: Modeling the Thin and Thick HI Disks

Aperture Synthesis Observations of the Nearby Spiral NGC 6503: Modeling the Thin and Thick HI Disks Aperture Synthesis Observations of the Nearby Spiral NGC 653: Modeling the Thin and Thick HI Disks Eric W. Greisen 1, Kristine Spekkens 23, and Gustaaf A. van Moorsel 1 ABSTRACT We present sensitive aperture

More information

Wagg ea. [CII] in ALMA SV 20min, 16 ants. 334GHz. SMA 20hrs

Wagg ea. [CII] in ALMA SV 20min, 16 ants. 334GHz. SMA 20hrs BRI1202-0725 z=4.7 HyLIRG (10 13 L o ) pair SFR ~ few 10 3 M o yr -1 4 + SMG + Salome ea. CO 5-4 + M H2 ~ 10 11 M o QSO + HST 814 Hu ea 96 SMA [CII] 158um 334GHz, 20hrs Iono ea 2007 [CII] in 1202-0725

More information

PACS Spectroscopy performance and calibration PACS Spectroscopy performance and calibration

PACS Spectroscopy performance and calibration PACS Spectroscopy performance and calibration 1 of 18 PACS Spectroscopy performance and PICC-KL-TN-041 Prepared by With inputs by Bart Vandenbussche Joris Blommaert Alessandra Contursi Helmut Feuchtgruber Christophe Jean Albrecht Poglitsch Pierre

More information

Energy Sources of the Far IR Emission of M33

Energy Sources of the Far IR Emission of M33 Energy Sources of the Far IR Emission of M33 Hinz, Reike et al., ApJ 154: S259 265 (2004). Presented by James Ledoux 24 µm 70 µm 160 µm Slide 1 M33 Properties Distance 840kpc = 2.7 Mlyr (1'' ~ 4 pc) Also

More information

Dealing with Noise. Stéphane GUILLOTEAU. Laboratoire d Astrophysique de Bordeaux Observatoire Aquitain des Sciences de l Univers

Dealing with Noise. Stéphane GUILLOTEAU. Laboratoire d Astrophysique de Bordeaux Observatoire Aquitain des Sciences de l Univers Dealing with Noise Stéphane GUILLOTEAU Laboratoire d Astrophysique de Bordeaux Observatoire Aquitain des Sciences de l Univers I - Theory & Practice of noise II Low S/N analysis Outline 1. Basic Theory

More information

Debate on the toroidal structures around hidden- vs non hidden-blr of AGNs

Debate on the toroidal structures around hidden- vs non hidden-blr of AGNs IoA Journal Club Debate on the toroidal structures around hidden- vs non hidden-blr of AGNs 2016/07/08 Reported by T. Izumi Unification scheme of AGNs All AGNs are fundamentally the same (Antonucci 1993)

More information

Probing the Origin of Supermassive Black Hole Seeds with Nearby Dwarf Galaxies. Amy Reines Einstein Fellow NRAO Charlottesville

Probing the Origin of Supermassive Black Hole Seeds with Nearby Dwarf Galaxies. Amy Reines Einstein Fellow NRAO Charlottesville Probing the Origin of Supermassive Black Hole Seeds with Nearby Dwarf Galaxies Amy Reines Einstein Fellow NRAO Charlottesville Motivation: The origin of supermassive BH seeds Motivation: The origin of

More information

arxiv: v1 [astro-ph.ga] 16 Jul 2018

arxiv: v1 [astro-ph.ga] 16 Jul 2018 Draft version November 16, 2018 Preprint typeset using L A TEX style emulateapj v. 12/16/11 CO (7 6), [Ci] 370µm AND [Nii]205µm LINE EMISSION OF THE QSO BRI1335-0417 AT REDSHIFT 4.407 Nanyao Lu 1,2, Tianwen

More information

Multi-wavelength studies of substructures and inhomogeneities in galaxy clusters

Multi-wavelength studies of substructures and inhomogeneities in galaxy clusters Multi-wavelength studies of substructures and inhomogeneities in galaxy clusters SZE (RX J1347) ΔS X (A3667) Tetsu Kitayama Toho University, Japan Infrared (Coma) 1. How can we study ICM physics with the

More information

Extended Molecular Gas Distribution in Mrk 273 and Merger-Luminosity Evolution

Extended Molecular Gas Distribution in Mrk 273 and Merger-Luminosity Evolution University of Massachusetts Amherst From the SelectedWorks of Min S. Yun October 1, 1995 Extended Molecular Gas Distribution in Mrk 273 and Merger-Luminosity Evolution Min S. Yun, University of Massachusetts

More information

PACS Spectroscopy performance and calibration PACS Spectroscopy performance and calibration

PACS Spectroscopy performance and calibration PACS Spectroscopy performance and calibration 1 of 18 PACS Spectroscopy performance and Prepared by Bart Vandenbussche With inputs by Alessandra Contursi Helmut Feuchtgruber Katrina Exter Christophe Jean Albrecht Poglitsch Elena Puga Pierre Royer

More information

Chris J. Willott NRC Herzberg, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada

Chris J. Willott NRC Herzberg, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada Draft version July 5, 218 Preprint typeset using L A TEX style emulateapj v. 12/16/11 A WIDE DISPERSION IN STAR FORMATION RATE AND DYNAMICAL MASS OF 1 8 SOLAR MASS BLACK HOLE HOST GALAXIES AT REDSHIFT

More information

VLA H53 RADIO RECOMBINATION LINE OBSERVATIONS OF THE ULTRALUMINOUS INFRARED GALAXY ARP 220

VLA H53 RADIO RECOMBINATION LINE OBSERVATIONS OF THE ULTRALUMINOUS INFRARED GALAXY ARP 220 The Astrophysical Journal, 633:198 204, 2005 November 1 # 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A. VLA H53 RADIO RECOMBINATION LINE OBSERVATIONS OF THE ULTRALUMINOUS

More information

Next Generation VLA Memo. 41 Initial Imaging Tests of the Spiral Configuration. C.L. Carilli, A. Erickson March 21, 2018

Next Generation VLA Memo. 41 Initial Imaging Tests of the Spiral Configuration. C.L. Carilli, A. Erickson March 21, 2018 Next Generation VLA Memo. 41 Initial Imaging Tests of the Spiral Configuration C.L. Carilli, A. Erickson March 21, 2018 Abstract We investigate the imaging performance of the Spiral214 array in the context

More information

ALMA! Fabian Walter MPIA

ALMA! Fabian Walter MPIA ALMA! Fabian Walter - - - MPIA early science What ALMA will not be: A Survey Machine e.g., LABOCA Survey of the Extended Chandra Deep Field South (LESS) ESO Large Program [Co- PIs: Smail, Walter, Weiss],

More information

Spatially Resolved Kinematics of Binary Quasar Candidates

Spatially Resolved Kinematics of Binary Quasar Candidates Spatially Resolved Kinematics of Binary Quasar Candidates IFU Spectroscopy with VIMOS/VLT Ivana Stoklasová Orlitová Astronomical Institute, Academy of Sciences, Prague, Czech Republic In collaboration

More information

Luminous Infrared Galaxies

Luminous Infrared Galaxies Luminous Infrared Galaxies FIRSED April 3, 2013 The Great Observatories All-sky LIRG Survey (GOALS) IRAS-detected galaxies with f 60μm > 5.24 Jy & b > 5 o 201 galaxies with L IR 10 11.0 L HST, Chandra

More information

Introduction to Interferometry

Introduction to Interferometry Introduction to Interferometry Ciro Pappalardo RadioNet has received funding from the European Union s Horizon 2020 research and innovation programme under grant agreement No 730562 Radioastronomy H.Hertz

More information

ALMA Synergy with ATHENA

ALMA Synergy with ATHENA ALMA Synergy with ATHENA Françoise Combes Observatoire de Paris 9 September 2015 ALMA & Athena: common issues Galaxy formation and evolution, clustering Surveys of galaxies at high and intermediate redshifts

More information

Continuum Observing. Continuum Emission and Single Dishes

Continuum Observing. Continuum Emission and Single Dishes July 11, 2005 NAIC/NRAO Single-dish Summer School Continuum Observing Jim Condon Continuum Emission and Single Dishes Continuum sources produce steady, broadband noise So do receiver noise and drift, atmospheric

More information

Star formation in XMMU J : a massive galaxy cluster at z=1.4

Star formation in XMMU J : a massive galaxy cluster at z=1.4 Star formation in XMMU J2235.3-2557: a massive galaxy cluster at z=1.4 Ruth Grutzbauch University of Nottingham Amanda E. Bauer, University of Nottingham Marcel Bergmann, Gemini Observatory South Inger

More information

Distant galaxies: a future 25-m submm telescope

Distant galaxies: a future 25-m submm telescope Distant galaxies: a future 25-m submm telescope Andrew Blain Caltech 11 th October 2003 Cornell-Caltech Workshop Contents Galaxy populations being probed Modes of investigation Continuum surveys Line surveys

More information

Mock Surveys of the Sub-millimetre Sky

Mock Surveys of the Sub-millimetre Sky Mock Surveys of the Sub-millimetre Sky William Cowley Supervisors: Carlton Baugh, Cedric Lacey, Shaun Cole DEX-X: Thurs 9th Jan Outline Sub-millimetre Galaxies Observational Motivation Angular resolution

More information

arxiv: v1 [astro-ph.ga] 11 Oct 2018

arxiv: v1 [astro-ph.ga] 11 Oct 2018 **Volume Title** ASP Conference Series, Vol. **Volume Number** **Author** c **Copyright Year** Astronomical Society of the Pacific Imaging Molecular Gas at High Redshift arxiv:1810.05053v1 [astro-ph.ga]

More information

, Th. Preibisch ', P. Stee 2, G. Weigelt ' Max-Planck-Institut f ur Radioastronomie, Auf dem H ugel 69, Bonn, Germany

, Th. Preibisch ', P. Stee 2, G. Weigelt ' Max-Planck-Institut f ur Radioastronomie, Auf dem H ugel 69, Bonn, Germany Stars with the B[e] phenomenon ASP Conference Series, Vol. **VOLUME**, Michaela Kraus & Anatoly S. Miroshnichenko The vicinity of the galactic supergiant B [e] star CPD-7 7 from near- and mid-ir long baseline

More information

A2255: the First Detection of Filamentary Polarized Emission in a Radio Halo

A2255: the First Detection of Filamentary Polarized Emission in a Radio Halo SLAC-PUB-10880 astro-ph/0411720 November 2004 A2255: the First Detection of Filamentary Polarized Emission in a Radio Halo F. Govoni 1,2, M. Murgia 1,3, L. Feretti 1, G. Giovannini 1,2, D. Dallacasa 1,2,

More information

Far-infrared Herschel SPIRE spectroscopy reveals physical conditions of ionised gas in high-redshift lensed starbursts

Far-infrared Herschel SPIRE spectroscopy reveals physical conditions of ionised gas in high-redshift lensed starbursts Far-infrared Herschel SPIRE spectroscopy reveals physical conditions of ionised gas in high-redshift lensed starbursts Zhi-Yu (Z-Y) Zhang 张智昱 U. Edinburgh/ESO Outline Background Sample description Herschel

More information

Probing the Molecular Outflows of the Coldest Known Object in the Universe The Boomerang Nebula. R.Sahai (JPL) W. Vlemmings, L-A Nyman & P.

Probing the Molecular Outflows of the Coldest Known Object in the Universe The Boomerang Nebula. R.Sahai (JPL) W. Vlemmings, L-A Nyman & P. Probing the Molecular Outflows of the Coldest Known Object in the Universe The Boomerang Nebula R.Sahai (JPL) W. Vlemmings, L-A Nyman & P. Huggins The Extraordinary Deaths of Ordinary Stars Planetary nebulae

More information

ESO Phase 3 Data Release Description. Data Collection ATLASGAL Release Number 1 Data Provider

ESO Phase 3 Data Release Description. Data Collection ATLASGAL Release Number 1 Data Provider ESO Phase 3 Data Release Description Data Collection ATLASGAL Release Number 1 Data Provider Frederic Schuller, K. Immer, Y. Contreras, T. Csengeri, J. S. Urquhart Date 19.01.2016 Abstract The APEX Telescope

More information

Deconvolving Primary Beam Patterns from SKA Images

Deconvolving Primary Beam Patterns from SKA Images SKA memo 103, 14 aug 2008 Deconvolving Primary Beam Patterns from SKA Images Melvyn Wright & Stuartt Corder University of California, Berkeley, & Caltech, Pasadena, CA. ABSTRACT In this memo we present

More information

ALMA as a Scientific Instrument. Robert Laing

ALMA as a Scientific Instrument. Robert Laing ALMA as a Scientific Instrument Outline What is ALMA? ALMA as it will be ALMA Operations Early Science Planning an ALMA observation Current status Atacama Large Millimetre/ Sub-Millimetre Array Aperture

More information

Tim Rawle. Herschel Lensing Survey (HLS) ESA Research Fellow ESAC, Madrid

Tim Rawle. Herschel Lensing Survey (HLS) ESA Research Fellow ESAC, Madrid Herschel Lensing Survey (HLS) Beyond the Confusion: Enhancing our View of High-z Star Formation via Cluster Lensing Tim Rawle ESA Research Fellow ESAC, Madrid E. Egami (PI; Arizona) B. Altieri (ESAC) L.

More information

PACS spectroscopy Data Analysis

PACS spectroscopy Data Analysis PACS spectroscopy Data Analysis Elena Puga Herschel Science Centre ESA 27/10/2016 Exploiting the Herschel Science Archive E. Puga Exploiting the Herschel Science Archive: PACS Spectrometer Data Analysis

More information

UV/optical spectroscopy of Submilliimeter Galaxies

UV/optical spectroscopy of Submilliimeter Galaxies UV/optical spectroscopy of Submilliimeter Galaxies Scott C. Chapman (Caltech), A. Blain (Caltech), I. Smail (Durham), M. Swinbank (Durham) R. Ivison (Edinburgh) SFR_Hα = SFR_FIR SFR_Hα = 1/10 SFR_FIR Outline:

More information

arxiv: v2 [astro-ph.ga] 17 Oct 2014

arxiv: v2 [astro-ph.ga] 17 Oct 2014 draft version October 20, 2014, accepted for publication in the Astrophysical Journal Preprint typeset using L A TEX style emulateapj v. 05/12/14 ALMA IMAGING OF GAS AND DUST IN A GALAXY PROTOCLUSTER AT

More information

Lecture 2: Molecular Clouds: Galactic Context and Observational Tracers. Corona Australis molecular cloud: Andrew Oreshko

Lecture 2: Molecular Clouds: Galactic Context and Observational Tracers. Corona Australis molecular cloud: Andrew Oreshko Lecture 2: Molecular Clouds: Galactic Context and Observational Tracers Corona Australis molecular cloud: Andrew Oreshko Classification of Young Stellar Objects (YSOs) Spectral Index Hartmann: Accretion

More information

CCAT. Gordon Stacey. Cornell University. Gull

CCAT. Gordon Stacey. Cornell University. Gull CCAT Gordon Stacey Cornell University Gull CCAT Scientific Inspiration Measure the star and characterize the history of star formation in galaxies through cosmic time Photometric surveys to resolve the

More information

X-ray Detection of the Inner Jet in the Radio Galaxy 3C 129

X-ray Detection of the Inner Jet in the Radio Galaxy 3C 129 X-ray Detection of the Inner Jet in the Radio Galaxy 3C 129 D. E. Harris Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138 H. Krawczynski Yale University, P.O. Box 208101, New

More information

Resolving the Steep Spectrum Emission in the Central Radio Source in ZwCl

Resolving the Steep Spectrum Emission in the Central Radio Source in ZwCl Resolving the Steep Spectrum Emission in the Central Radio Source in ZwCl 0735.7+7421 A. S. Cohen 1, T. E. Clarke 1,2, L. Feretti 3 and N. E. Kassim 1 ABSTRACT arxiv:astro-ph/0501564v1 26 Jan 25 It has

More information

Radio relis (and halos) in galaxy clusters

Radio relis (and halos) in galaxy clusters Radio relis (and halos) in galaxy clusters Matthias Hoeft Thüringer Landessternwarte Tautenburg - overall spectrum of relics - relic statistics - an unusual radio halo Radio relic: the textbook example

More information

Methanol masers and their environment at high resolution

Methanol masers and their environment at high resolution Mon. Not. R. Astron. Soc. 300, 1131 1157 (1998) Methanol masers and their environment at high resolution C. J. Phillips, 1 R. P. Norris, 2 S. P. Ellingsen 1 and P. M. McCulloch 1 1 Department of Physics,

More information

Note on OSIRIS Wavelength Calibrations D. Le Mignant, Oct. 5, 2007

Note on OSIRIS Wavelength Calibrations D. Le Mignant, Oct. 5, 2007 Note on OSIRIS Wavelength Calibrations D. Le Mignant, Oct. 5, 2007 1. Observations and data reduction In this short note, we report on some on-going analysis of OSIRIS data in an effort to document our

More information

ASTRO 310: Galac/c & Extragalac/c Astronomy Prof. Jeff Kenney. Class 17 Mar 30, 2016 Starlight Distribu/ons in Disk Galaxies

ASTRO 310: Galac/c & Extragalac/c Astronomy Prof. Jeff Kenney. Class 17 Mar 30, 2016 Starlight Distribu/ons in Disk Galaxies ASTRO 310: Galac/c & Extragalac/c Astronomy Prof. Jeff Kenney Class 17 Mar 30, 2016 Starlight Distribu/ons in Disk Galaxies reminder no class next Monday, April 3!! 3 Color op/cal image of spiral galaxy

More information

Proper motion and apparent contraction in the J

Proper motion and apparent contraction in the J Mem. S.A.It. Vol. 82, 51 c SAIt 2011 Memorie della Proper motion and apparent contraction in the CSO J0650+6001 M. Orienti 1,2 and D. Dallacasa 1,2 1 Dipartimento di Astronomia Università di Bologna, Via

More information

Resolved studies of gas in high-z galaxies

Resolved studies of gas in high-z galaxies Resolved studies of gas in high-z galaxies Jacqueline Hodge Jansky Fellow (NRAO) With Fabian Walter (MPIA), Chris Carilli (NRAO), Erwin de Blok (ASTRON), Dominik Riechers (Cornell), Emanuele Daddi (CEA)

More information

Quasars in the epoch of reioniza1on

Quasars in the epoch of reioniza1on Big Bang Dark Ages Quasars in the epoch of reioniza1on Carnegie-Princeton Fellow Illumina9ng the Dark Ages June 27, Heidelberg, Germany Universe Today Quasars and galaxies in the reioniza1on epoch Quasars

More information

WHAT CAN WE LEARN ABOUT SUBMILLIMETER GALAXIES FROM INTERFEROMETRIC IMAGING? Joshua D. Younger Harvard/CfA

WHAT CAN WE LEARN ABOUT SUBMILLIMETER GALAXIES FROM INTERFEROMETRIC IMAGING? Joshua D. Younger Harvard/CfA WHAT CAN WE LEARN ABOUT SUBMILLIMETER GALAXIES FROM INTERFEROMETRIC IMAGING? Joshua D. Younger Harvard/CfA J. D. Younger, G. G. Fazio, J. Huang (CfA) M. S. Yun, G. Wilson, T. Perera, K. Scott, J. Austermann

More information

within entire molecular cloud complexes

within entire molecular cloud complexes The earliest phases of high-mass stars within entire molecular cloud complexes Frédérique Motte (CEA-Saclay, AIM) Collaborators: S. Bontemps (Obs Bordeaux), N. Schneider, J. Grac (CEA-Saclay), P. Schilke,

More information

Clustering of Star-forming Galaxies and connections with AGN activity

Clustering of Star-forming Galaxies and connections with AGN activity Clustering of Star-forming Galaxies and connections with AGN activity MANUELA MAGLIOCCHETTI IAPS-INAF Collaborators: Herschel PEP team (D.Lutz, P.Popesso, D.Rosario et al.) & A.Lapi, M.Negrello, G.De Zotti.,

More information

Radio and gamma-ray emission in Faint BL Lacs

Radio and gamma-ray emission in Faint BL Lacs AGN X ROMA, 10-13/09/2012 Radio and gamma-ray emission in Faint BL Lacs E. Liuzzo, B. Boccardi, M. Giroletti, G. Giovannini, F. Massaro, M. Orienti, S. Tamburri, C. Casadio 3EG Catalog γ sky EGRET (3EG,

More information

SPIRE Spectrometer data analysis

SPIRE Spectrometer data analysis SPIRE Spectrometer data analysis Rosalind Hopwood SPIRE Instrument and Calibration Scientist 26 th October 2016 Exploiting the Herschel Science Archive Outline Documentation & literature Examining spectra

More information

INTERFEROMETRIC IMAGING OF THE SUNYAEV-ZELDOVICH EFFECT AT 30 GHz

INTERFEROMETRIC IMAGING OF THE SUNYAEV-ZELDOVICH EFFECT AT 30 GHz THE ASTROPHYSICAL JOURNAL, 456 : L75 L78, 1996 January 10 1996. The American Astronomical Society. All rights reserved. Printed in U.S.A. INTERFEROMETRIC IMAGING OF THE SUNYAEV-ZELDOVICH EFFECT AT 30 GHz

More information

THE DISTRIBUTION OF ATOMIC HYDROGEN AROUND TWO IRREGULAR GALAXIES Deidre A. Hunter. and Eric M. Wilcots

THE DISTRIBUTION OF ATOMIC HYDROGEN AROUND TWO IRREGULAR GALAXIES Deidre A. Hunter. and Eric M. Wilcots The Astronomical Journal, 123:2449 2461, 22 May # 22. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE DISTRIBUTION OF ATOMIC HYDROGEN AROUND TWO IRREGULAR GALAXIES Deidre

More information

SZ with ALMA & ACA: a user s perspective. Tetsu Kitayama Toho University, Japan

SZ with ALMA & ACA: a user s perspective. Tetsu Kitayama Toho University, Japan SZ with ALMA & ACA: a user s perspective Tetsu Kitayama Toho University, Japan Collaborators Daisuke Iono Univ. of Tokyo Ryohei Kawabe NAOJ Kotaro Kohno Univ. of Tokyo Eiichiro Komatsu Univ. of Texas Hiroshi

More information

The connection between millimeter and gamma-ray emission in AGNs

The connection between millimeter and gamma-ray emission in AGNs The connection between millimeter and gamma-ray emission in AGNs Marcello Giroletti INAF Istituto di Radioastronomia Secondo Workshop sull'astronomia millimetrica e submillimetrica in Italia Bologna, 2-3

More information

The Cosmic Evolution of Neutral Atomic Hydrogen Gas. Philip Lah. Macquarie University Colloquium 27th March 2015

The Cosmic Evolution of Neutral Atomic Hydrogen Gas. Philip Lah. Macquarie University Colloquium 27th March 2015 The Cosmic Evolution of Neutral Atomic Hydrogen Gas Philip Lah Macquarie University Colloquium 27th March 2015 Collaborators: Frank Briggs (ANU) Jayaram Chengalur (NCRA) Matthew Colless (ANU) Roberto De

More information

Disk+outflow system in G

Disk+outflow system in G EAVW 2018 @ PyeongChang Disk+outflow system in G25.82-0.17 Jungha Kim (D2/SOKENDAI/NAOJ) Tomoya Hirota, Kee-Tae Kim, KaVA SWG for star formation CONTENTS Introduction Observations Results - KaVA imaging

More information

Robert Laing European Instrument Scientist

Robert Laing European Instrument Scientist Kilometre Array Bonn, April 15 2008 Overview What is? Main performance numbers Sensitivity Resolution Spatial scales Spectral-line modes Synergy between and SKA Science Wavelengths, resolutions, surveys

More information

MALATANG THOMAS R. GREVE UNIVERSITY COLLEGE LONDON. MApping the dense molecular gas in The strongest star-forming Galaxies

MALATANG THOMAS R. GREVE UNIVERSITY COLLEGE LONDON. MApping the dense molecular gas in The strongest star-forming Galaxies MALATANG MApping the dense molecular gas in The strongest star-forming Galaxies www.eaobservatory.org/jcmt On behalf of the MALATANG team: THOMAS R. GREVE UNIVERSITY COLLEGE LONDON Seoul National University,

More information

ASTRONOMY AND ASTROPHYSICS. Letter to the Editor VSOP imaging of S : a close-up on plasma instabilities in the jet LETTER

ASTRONOMY AND ASTROPHYSICS. Letter to the Editor VSOP imaging of S : a close-up on plasma instabilities in the jet LETTER Astron. Astrophys. 340, L60 L64 (1998) Letter to the Editor VSOP imaging of S5 0836+710: a close-up on plasma instabilities in the jet ASTRONOMY AND ASTROPHYSICS A.P. Lobanov 1, T.P. Krichbaum 1, A. Witzel

More information

HI Surveys and the xntd Antenna Configuration

HI Surveys and the xntd Antenna Configuration ATNF SKA memo series 006 HI Surveys and the xntd Antenna Configuration Lister Staveley-Smith (ATNF) Date Version Revision 21 August 2006 0.1 Initial draft 31 August 2006 1.0 Released version Abstract Sizes

More information

Multi-frequency study of the TeV blazar Markarian 421 with VLBA observations taken during 2011

Multi-frequency study of the TeV blazar Markarian 421 with VLBA observations taken during 2011 Multi-frequency study of the TeV blazar Markarian 421 with VLBA observations taken during 2011 Presented by: Rocco Lico M.Giroletti, M.Orienti, G.Giovannini, Y.Y.Kovalev, A.Marscher, S.Jorstad, T.P. Krichbaum,

More information

Methanol absorption in PKS B at milliarcsecond scales

Methanol absorption in PKS B at milliarcsecond scales Advance Access publication 2016 December 19 doi:10.1093/mnras/stw3295 Methanol absorption in PKS B1830 211 at milliarcsecond scales M. A. Marshall, 1 S. P. Ellingsen, 1 J. E. J. Lovell, 1 J. M. Dickey,

More information

LOW RADIO FREQUENCY SPECTRAL PROPERTIES OF millijansky RADIO SOURCES

LOW RADIO FREQUENCY SPECTRAL PROPERTIES OF millijansky RADIO SOURCES LOW RADIO FREQUENCY SPECTRAL PROPERTIES OF millijansky RADIO SOURCES Alice Di Vincenzo PhD student at Tautenburg Observatory & LOFAR station TLS Loretta Gregorini Isabella Prandoni Gianni Bernardi Ger

More information

Fragmentation of the Integral Shaped Filament as viewed by ALMA

Fragmentation of the Integral Shaped Filament as viewed by ALMA Fragmentation of the Integral Shaped Filament as viewed by ALMA Jouni Kainulainen Max-Planck-Institute for Astronomy Kainulainen et al. (submitted; arxiv:1603.05688) With: Amelia Stutz, Thomas Stanke,

More information

arxiv: v1 [astro-ph.ga] 10 Apr 2018

arxiv: v1 [astro-ph.ga] 10 Apr 2018 Draft version April 12, 2018 Preprint typeset using L A TEX style AASTeX6 v. 1.0 arxiv:1804.03663v1 [astro-ph.ga] 10 Apr 2018 THE DUST AND [CII] MORPHOLOGIES OF REDSHIFT 4.5 SUB-MILLIMETER GALAXIES AT

More information

GMRT observations of radio halo clusters

GMRT observations of radio halo clusters GMRT observations of radio halo clusters Viral Parekh Raman Research Institute Bangalore Collaborators K.S. Dwarakanath (RRI), Ruta Kale (NCRA), and Huib Intema (Leiden Observatory) SPARCS Meeting, November,

More information

Continuum Submillimetre Astronomy from UKIRT. Ian Robson UK ATC

Continuum Submillimetre Astronomy from UKIRT. Ian Robson UK ATC Continuum Submillimetre Astronomy from UKIRT Ian Robson UK ATC Submillimetre means high - how high can we get? let s s go to Hawaii! (1975,( 76) We need a submillimetre photometer! Lots of lessons learned

More information

Circumnuclear Gaseous Kinematics and Excitation of Four Local Radio Galaxies

Circumnuclear Gaseous Kinematics and Excitation of Four Local Radio Galaxies Circumnuclear Gaseous Kinematics and Excitation of Four Local Radio Galaxies Guilherme S. Couto T. Storchi-Bergmann, A. Robinson, R.A. Riffel, P. Kharb D. Lena, A. Schnorr-Müller UFSC, Florianópolis, Brazil

More information

BLAST: The CIB in a new light. marco viero / university of toronto

BLAST: The CIB in a new light. marco viero / university of toronto BLAST: The CIB in a new light marco viero / university of toronto 1 University of Toronto Peter Martin Barth Netterfield Marco Viero University of Pennsylvania Mark Devlin Marie Rex Chris Semisch Jeff

More information

Peter Teuben (U. Maryland)

Peter Teuben (U. Maryland) ALMA Study Total Power Map to Visibilities (TP2VIS) Joint-Deconvolution of ALMA 12m, 7m & TP Array Data Peter Teuben (U. Maryland) Jin Koda (Stony Brook/NAOJ/JAO); Tsuyoshi Sawada (NAOJ/JAO); Adele Plunkett

More information

Unveiling the nature of z 6 galaxies through [CII] emission studies

Unveiling the nature of z 6 galaxies through [CII] emission studies Unveiling the nature of z 6 galaxies through [CII] emission studies Simona Gallerani in collabora=on with: Livia Vallini, Andrea Ferrara, Andrea PalloMni, Roberto Maiolino, Chiara Feruglio, Dominik Riechers,

More information

SKA Continuum Deep Field Surveys

SKA Continuum Deep Field Surveys SKA Continuum Deep Field Surveys Amit Vishwas April 7, 2010 The Square Kilometer Array The Next Generation Radio Telescope Spread over a long baseline ~1000 kms Large Effective Area: but only a fraction

More information

15m James Clerk Maxwell Telescope (JCMT) Surface accuracy : 24 micron Pointing accuracy : 2 arcsec in Azimuth and Elevation

15m James Clerk Maxwell Telescope (JCMT) Surface accuracy : 24 micron Pointing accuracy : 2 arcsec in Azimuth and Elevation 15m James Clerk Maxwell Telescope (JCMT) Surface accuracy : 24 micron Pointing accuracy : 2 arcsec in Azimuth and Elevation Continuum Instrumentation 5120 bolometers (4 sub arrays x 1280 bolometers) at

More information

Dynamics of starbursting dwarf galaxies. I Zw 18

Dynamics of starbursting dwarf galaxies. I Zw 18 Chapter 2 Dynamics of starbursting dwarf galaxies. I Zw 18 Federico Lelli, Marc Verheijen, Filippo Fraternali, and Renzo Sancisi Astronomy & Astrophysics, 2012, 537, A72 2 Chapter 2. Dynamics of starbursting

More information

PoS(IX EVN Symposium)019

PoS(IX EVN Symposium)019 abc, K.-H. Mack, a C.R. Benn, d R. Carballo, e D. Dallacasa, f a J.I. González-Serrano, g J. Holt h and F. Jiménez-Luján gi a INAF - Istituto di Radioastronomia, Via P. Gobetti 101, I-40129 Bologna, Italy

More information

Ionization Feedback in Massive Star Formation

Ionization Feedback in Massive Star Formation Ionization Feedback in Massive Star Formation Thomas Peters Institut für Theoretische Astrophysik Zentrum für Astronomie der Universität Heidelberg Ralf Klessen, Robi Banerjee (ITA, Heidelberg) Mordecai-Mark

More information

Ay 20 Basic Astronomy and the Galaxy Problem Set 2

Ay 20 Basic Astronomy and the Galaxy Problem Set 2 Ay 20 Basic Astronomy and the Galaxy Problem Set 2 October 19, 2008 1 Angular resolutions of radio and other telescopes Angular resolution for a circular aperture is given by the formula, θ min = 1.22λ

More information

FORCAST: Science Capabili2es and Data Products. William D. Vacca

FORCAST: Science Capabili2es and Data Products. William D. Vacca FORCAST: Science Capabili2es and Data Products William D. Vacca Faint Object infrared Camera for the SOFIA Telescope (FORCAST) SWC (blue) Light from telescope LWC (red) Facility Instrument PI: Terry Herter

More information

Addendum: GLIMPSE Validation Report

Addendum: GLIMPSE Validation Report August 18, 2004 Addendum: GLIMPSE Validation Report The GLIMPSE Team 1. Motivation In our Validation Report of Jan. 30, 2004, we produced reliability calculations and discussed photometric accuracy estimates

More information

ROSAT Roentgen Satellite. Chandra X-ray Observatory

ROSAT Roentgen Satellite. Chandra X-ray Observatory ROSAT Roentgen Satellite Joint facility: US, Germany, UK Operated 1990 1999 All-sky survey + pointed observations Chandra X-ray Observatory US Mission Operating 1999 present Pointed observations How do

More information

arxiv:astro-ph/ v1 20 Apr 2000

arxiv:astro-ph/ v1 20 Apr 2000 Starburst in the Ultra-luminous Galaxy Arp 220 - Constraints from Observations of Radio Recombination Lines and Continuum K.R. Anantharamaiah 1,2, F. Viallefond 3, Niruj R. Mohan 1,2,4, W.M. Goss 1 & J.H.

More information