19
1 / 19 Three Years of AstroSat V Girish ISRO, Bangalore

Three Years of AstroSat - events.spacepole.be

  • Upload
    others

  • View
    12

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Three Years of AstroSat - events.spacepole.be

1 / 19

Three Years of AstroSat

V GirishISRO, Bangalore

Page 2: Three Years of AstroSat - events.spacepole.be

2 / 19

AstroSat

● India's first multi-wavelength Astronomy satellite

● Launched from Sriharikota on 28th sept 2015

● Low earth, low inclination angle

Page 3: Three Years of AstroSat - events.spacepole.be

3 / 19

IntroductionFive Scientific payloads and one auxiliary

● Ultra Violet Imaging Telescope (UVIT)

● Soft X-ray Telescope (SXT)

● Large Area X-ray proportional Counter (LAXPC)

● Cadmium Zinc Telluride Imager (CZTi)

● Scanning Sky Monitor (SSM)

● Charge Particle Monitor (CPM)

From NUV to high energy X-rays

Imaging, timing and Polarimetry (!!!)

Page 4: Three Years of AstroSat - events.spacepole.be

4 / 19

Results till now

● Initial six months P&V phase

● Six months GTO

● Nearing 100 refereed publications

– X-ray polarization from off pulse region– Solving the puzzle of faint red star bright in

UV

● Data is made public now

Page 5: Three Years of AstroSat - events.spacepole.be

5 / 19

UVIT● Two 40 cm RC telescopes

FUV-Alignment Cube

NUV/VIS-Alignment Cube

FUV-Optical Axis

NUV/VIS- Optical Axis

Page 6: Three Years of AstroSat - events.spacepole.be

6 / 19

UVIT● Two 40 cm RC telescopes

● Astrometry 1.2 – 1.4'

● Multiple filters

Rahna et al., 2018

Page 7: Three Years of AstroSat - events.spacepole.be

7 / 19

Soft X-ray Telescope (SXT)

● Gold plated foils; Wolter I configuration

● 600 x 600 pixels

● 0.8 – 8.0 keV range

● Energy Resolution: 90 eV at 1.5 keV 136 eV at 5.9 keV

● Time resolution ~ 2.4 s (full frame) ~ 0.278 s (window mode)

● Effective Area ~90 cm 2 at 1.5 keV

Page 8: Three Years of AstroSat - events.spacepole.be

8 / 19

Soft X-ray Telescope (SXT)

Singh et al., 2017

Page 9: Three Years of AstroSat - events.spacepole.be

9 / 19

LAXPC

● Highest collecting areain 3 - 60 keV

● Three proportional counters

Page 10: Three Years of AstroSat - events.spacepole.be

10 / 19

LAXPCms phenomena in 4U 1728-34

QPO in high energies and measuring delay between energy bands

● Changing frequency 820 – 850 Hz

● Time lag :with-in 2500 s observations

● Type-1 burst too

Chauhan et al., 2017

Page 11: Three Years of AstroSat - events.spacepole.be

11 / 19

LAXPC multi-wavelength/Co-ord

4U 1630-47 Evidence of rapid spin/disk wind(Mayukh et al., 2018)

SXP 15.3: Cyclotron

(Maitra et al., 2018)

Page 12: Three Years of AstroSat - events.spacepole.be

12 / 19

CZTi● 64 Cd Zn Te modules → 960 cm2

● Each CZT module = 16x16 = 256 pixels => 16384 pixels (total)

● 10 – 100 keV, 8% at 100 keV

● Coded Aperture Mask, Open beyond 100 keV

Page 13: Three Years of AstroSat - events.spacepole.be

13 / 19

CZTi

Page 14: Three Years of AstroSat - events.spacepole.be

14 / 19

CZTi

Page 15: Three Years of AstroSat - events.spacepole.be

15 / 19

SSM

Page 16: Three Years of AstroSat - events.spacepole.be

16 / 19

SSMhttps://issdc.gov.in/SSM_Web/index.jsp

Page 17: Three Years of AstroSat - events.spacepole.be

17 / 19

On 26th Chairman, ISRO opened AstroSat data open for public

https://astrobrowse.issdc.gov.in/astrohtml

Page 18: Three Years of AstroSat - events.spacepole.be

18 / 19

AstroSat Support Cell

http://astrosat-ssc.iucaa.in

Page 19: Three Years of AstroSat - events.spacepole.be

19 / 19

Future● AO for next Astronomy mission

– Short listing stage– X-ray polarization priority for X-ray

proposals– Gamma ray detection

● AO for Venus mission

– Orbiter + Balloon (~ 5kg scientific payload)

...

Thanks