observing psr b1749-28
TRANSCRIPT
![Page 1: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/1.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
PSR B1749-28 - Observations & PropertiesExperiment during POS - 2013
Poruri Sai Rahul
Department of PhysicsIIT Madras
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PSRB1749-28 -POS 2013
Poruri SaiRahul
Pulsar Properties
Some properties of the pulsar, from ATNF Pulsar Catalogue1
and VizieR are2
• Strength S400 = 1.1Jy
• Dispersion Measure - DM = 50.88000kpc/cm3
• Highly Polarized Flux
• Barycentric period of PulsarP = 562.5578578340000ms
• Profile Width at 50% of peakW 50 = 9.1ms
1http://goo.gl/Xuo4c2http://goo.gl/maeGC
![Page 3: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/3.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Pulsar Properties
Some properties of the pulsar, from ATNF Pulsar Catalogue1
and VizieR are2
• Strength S400 = 1.1Jy
• Dispersion Measure - DM = 50.88000kpc/cm3
• Highly Polarized Flux
• Barycentric period of PulsarP = 562.5578578340000ms
• Profile Width at 50% of peakW 50 = 9.1ms
1http://goo.gl/Xuo4c2http://goo.gl/maeGC
![Page 4: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/4.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Pulsar Spectrum
The spectrum of a pulsar can be modelled using a power lawspectrum -
fν = να
where the average spectral index is −1.6 ± 0.3 3
3arXiv:1302.2053
![Page 5: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/5.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Pulsar Spectrum
The spectrum of a pulsar can be modelled using a power lawspectrum -
fν = να
where the average spectral index is −1.6 ± 0.3 3
3arXiv:1302.2053
![Page 6: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/6.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Pulsar Spectrum
the strength of the pulsar is known at 3 different frequencies -
• S400 = 1100.00 mJy
• S600 = 335.00 mJy
• S1400 = 36.00 mJy
from these values, the spectral index of PSR B1749-28 isestimated to be −2.676 and by extrapolating this, we estimatethat
• S326.5 = 1894 mJy
![Page 7: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/7.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Pulsar Spectrum
the strength of the pulsar is known at 3 different frequencies -
• S400 = 1100.00 mJy
• S600 = 335.00 mJy
• S1400 = 36.00 mJy
from these values, the spectral index of PSR B1749-28 isestimated to be −2.676 and by extrapolating this, we estimatethat
• S326.5 = 1894 mJy
![Page 8: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/8.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Pulsar Spectrum
the strength of the pulsar is known at 3 different frequencies -
• S400 = 1100.00 mJy
• S600 = 335.00 mJy
• S1400 = 36.00 mJy
from these values, the spectral index of PSR B1749-28 isestimated to be −2.676 and by extrapolating this, we estimatethat
• S326.5 = 1894 mJy
![Page 9: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/9.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Calibrator - 2053-201
The Calibrator - 2053-201 is a galaxy at a redshift of 0.1566224
The strength of the calibrator is known at 6 differentfrequencies5 -
• S80 = 16Jy
• S408 = 6.2Jy
• S1410 = 2.6Jy
• S2700 = 1.6Jy
• S5000 = 0.99Jy
• S8400 = 0.6Jy
from these values, we estimate that
• S326.5 = 7.058Jy
4http://goo.gl/l3qoR5http://goo.gl/1d6OZ
![Page 10: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/10.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Calibrator - 2053-201
The Calibrator - 2053-201 is a galaxy at a redshift of 0.1566224
The strength of the calibrator is known at 6 differentfrequencies5 -
• S80 = 16Jy
• S408 = 6.2Jy
• S1410 = 2.6Jy
• S2700 = 1.6Jy
• S5000 = 0.99Jy
• S8400 = 0.6Jy
from these values, we estimate that
• S326.5 = 7.058Jy
4http://goo.gl/l3qoR5http://goo.gl/1d6OZ
![Page 11: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/11.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Calibrator - 2053-201
The Calibrator - 2053-201 is a galaxy at a redshift of 0.1566224
The strength of the calibrator is known at 6 differentfrequencies5 -
• S80 = 16Jy
• S408 = 6.2Jy
• S1410 = 2.6Jy
• S2700 = 1.6Jy
• S5000 = 0.99Jy
• S8400 = 0.6Jy
from these values, we estimate that
• S326.5 = 7.058Jy
4http://goo.gl/l3qoR5http://goo.gl/1d6OZ
![Page 12: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/12.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Observations
• Observations of the pulsar took place on Jul 13 from23:28:27 to 23:49:59 IST for a total of 1200s.
• The calibrator source for this specific pulsar is 2053-201,observed for 300s.
• the off source RA is 20 minutes east from the calibratorand was observed for 300s.
![Page 13: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/13.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Observations
• Observations of the pulsar took place on Jul 13 from23:28:27 to 23:49:59 IST for a total of 1200s.
• The calibrator source for this specific pulsar is 2053-201,observed for 300s.
• the off source RA is 20 minutes east from the calibratorand was observed for 300s.
![Page 14: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/14.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Observations
• Observations of the pulsar took place on Jul 13 from23:28:27 to 23:49:59 IST for a total of 1200s.
• The calibrator source for this specific pulsar is 2053-201,observed for 300s.
• the off source RA is 20 minutes east from the calibratorand was observed for 300s.
![Page 15: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/15.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Data Analysis Pipeline
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PSRB1749-28 -POS 2013
Poruri SaiRahul
Data Analysis Pipeline
The pulsar’s properties studied are
• Dispersion Measure
• Period of Pulsar
• Flux Density
in that particular order.
![Page 17: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/17.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Data Analysis Pipeline
The pulsar’s properties studied are
• Dispersion Measure
• Period of Pulsar
• Flux Density
in that particular order.
![Page 18: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/18.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Data Analysis Pipeline
The pulsar’s properties studied are
• Dispersion Measure
• Period of Pulsar
• Flux Density
in that particular order.
![Page 19: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/19.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Results
The pulsar’s properties have been determined to be
• Dispersion Measure - 50.733 ± 1.764pc/cm3 against theactual value of 50.88pc/cm3
• Period of Pulsar - 562.587ms against the actual value of562.55785783400ms
• Distance - 1.2683 ± 0.0441kpc against the actual value of1.53kpc - estimated from the DM and an average galacticelectron density n(e)6 of 4 × 10−2cm−3
• Flux Density - 1827.7 ± 59.8mJy against an estimatedvalue of 1894mJy
6http://adsabs.harvard.edu/abs/1969ApJ...157.1137J
![Page 20: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/20.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Results
The pulsar’s properties have been determined to be
• Dispersion Measure - 50.733 ± 1.764pc/cm3 against theactual value of 50.88pc/cm3
• Period of Pulsar - 562.587ms against the actual value of562.55785783400ms
• Distance - 1.2683 ± 0.0441kpc against the actual value of1.53kpc - estimated from the DM and an average galacticelectron density n(e)6 of 4 × 10−2cm−3
• Flux Density - 1827.7 ± 59.8mJy against an estimatedvalue of 1894mJy
6http://adsabs.harvard.edu/abs/1969ApJ...157.1137J
![Page 21: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/21.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Results
The pulsar’s properties have been determined to be
• Dispersion Measure - 50.733 ± 1.764pc/cm3 against theactual value of 50.88pc/cm3
• Period of Pulsar - 562.587ms against the actual value of562.55785783400ms
• Distance - 1.2683 ± 0.0441kpc against the actual value of1.53kpc - estimated from the DM and an average galacticelectron density n(e)6 of 4 × 10−2cm−3
• Flux Density - 1827.7 ± 59.8mJy against an estimatedvalue of 1894mJy
6http://adsabs.harvard.edu/abs/1969ApJ...157.1137J
![Page 22: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/22.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Results
The pulsar’s properties have been determined to be
• Dispersion Measure - 50.733 ± 1.764pc/cm3 against theactual value of 50.88pc/cm3
• Period of Pulsar - 562.587ms against the actual value of562.55785783400ms
• Distance - 1.2683 ± 0.0441kpc against the actual value of1.53kpc - estimated from the DM and an average galacticelectron density n(e)6 of 4 × 10−2cm−3
• Flux Density - 1827.7 ± 59.8mJy against an estimatedvalue of 1894mJy
6http://adsabs.harvard.edu/abs/1969ApJ...157.1137J
![Page 23: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/23.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Results
The pulsar’s properties have been determined to be
• Dispersion Measure - 50.733 ± 1.764pc/cm3 against theactual value of 50.88pc/cm3
• Period of Pulsar - 562.587ms against the actual value of562.55785783400ms
• Distance - 1.2683 ± 0.0441kpc against the actual value of1.53kpc - estimated from the DM and an average galacticelectron density n(e)6 of 4 × 10−2cm−3
• Flux Density - 1827.7 ± 59.8mJy against an estimatedvalue of 1894mJy
6http://adsabs.harvard.edu/abs/1969ApJ...157.1137J
![Page 24: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/24.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Band response - Offsource
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PSRB1749-28 -POS 2013
Poruri SaiRahul
Band response - Calibrator
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PSRB1749-28 -POS 2013
Poruri SaiRahul
Band response - Offsource
![Page 27: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/27.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Band response - Calibrator
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PSRB1749-28 -POS 2013
Poruri SaiRahul
Resources
Information regarding the pulsar and the calibrator wereobtained from the following sources -
• Australia Telescope National Facility- ATNF Pulsar Catalogue7,
• NASA/IPAC Extra Galactic Database - NED8,
• SIMBAD9,
• VizieR10.
7http://goo.gl/Xuo4c8http://goo.gl/CAjoH9http://goo.gl/jw2Sg
10http://goo.gl/maeGC
![Page 29: Observing PSR B1749-28](https://reader033.vdocuments.us/reader033/viewer/2022052911/559f61c11a28ab63528b4814/html5/thumbnails/29.jpg)
PSRB1749-28 -POS 2013
Poruri SaiRahul
Resources
Information regarding the pulsar and the calibrator wereobtained from the following sources -
• Australia Telescope National Facility- ATNF Pulsar Catalogue7,
• NASA/IPAC Extra Galactic Database - NED8,
• SIMBAD9,
• VizieR10.
7http://goo.gl/Xuo4c8http://goo.gl/CAjoH9http://goo.gl/jw2Sg
10http://goo.gl/maeGC