TY - JOUR
T1 - Plucking the Web: Searching Unidentified Gamma-ray Sources for Spider Pulsars using Jerksearch Algorithm
AU - Tabassum, S.
AU - Roberts, M.
AU - Ransom, S.
AU - Ray, P.
AU - Ferrara, E.
AU - Cromartie, H.
AU - Al Noori, H.
AU - Fermi Pulsar Search Consortium, null
AU - Camilo, F.
PY - 2020/1/1
Y1 - 2020/1/1
N2 - Binary millisecond pulsars (MSPs) can be used to study a wide variety of
scientific phenomenon including the testing and constraining of General
Relativity, Equation of State of nuclear matter, and properties of
matter at extreme densities. Finding new MSPs is one of the main science
drivers of current pulsar surveys. In the past decade, the most
successful approach to search for MSPs has been to use acceleration
searches to look for radio pulsations in the error bars of Gamma-ray
sources identified by the Large Area Telescope (LAT) aboard the Fermi
Satellite. However, 1000s of gamma-ray sources found by LAT still remain
unassociated with any astrophysical object. It is believed that many of
these could be MSPs. One of the reasons for their non-detection is the
use of acceleration searches to account for the orbital motion of the
pulsar. This method is ineffective when the observation time is longer
than 1/10th of the orbital period. Due to the fact that sensitivity to
pulses is directly proportional to the observation time, fainter systems
in very tight orbits have remained outside the parameter space of such
searches.We have been using the novel jerksearch algorithm implemented
in the PRESTO software package to re-search Fermi sources that remain
unidentified. Jerksearch is sensitive to changes in the period of the
pulsed signal caused by the second derivative of the orbital period,
resulting in increased sensitivity to tight binary systems. Hence, we
are searching in a parameter space which has scarcely been searched till
now without making a compromise on sensitivity. We are using radio data
gathered from the Robert C. Byrd Green Bank Telescope (GBT) at 820 MHz
for unassociated sources from Fermi LAT catalogs as part of the Fermi
Pulsar Search Collaboratory. We expect to find multiple millisecond
pulsar binaries, including spider systems and maybe even a black
hole-pulsar binary system. We are using the Dalma High Performance
Computing (HPC) cluster of NYUAD to run the computationally expensive
jerksearches. Here we present preliminary results of these searches,
showing several promising candidates which will potentially be followed
up using the GBT.
AB - Binary millisecond pulsars (MSPs) can be used to study a wide variety of
scientific phenomenon including the testing and constraining of General
Relativity, Equation of State of nuclear matter, and properties of
matter at extreme densities. Finding new MSPs is one of the main science
drivers of current pulsar surveys. In the past decade, the most
successful approach to search for MSPs has been to use acceleration
searches to look for radio pulsations in the error bars of Gamma-ray
sources identified by the Large Area Telescope (LAT) aboard the Fermi
Satellite. However, 1000s of gamma-ray sources found by LAT still remain
unassociated with any astrophysical object. It is believed that many of
these could be MSPs. One of the reasons for their non-detection is the
use of acceleration searches to account for the orbital motion of the
pulsar. This method is ineffective when the observation time is longer
than 1/10th of the orbital period. Due to the fact that sensitivity to
pulses is directly proportional to the observation time, fainter systems
in very tight orbits have remained outside the parameter space of such
searches.We have been using the novel jerksearch algorithm implemented
in the PRESTO software package to re-search Fermi sources that remain
unidentified. Jerksearch is sensitive to changes in the period of the
pulsed signal caused by the second derivative of the orbital period,
resulting in increased sensitivity to tight binary systems. Hence, we
are searching in a parameter space which has scarcely been searched till
now without making a compromise on sensitivity. We are using radio data
gathered from the Robert C. Byrd Green Bank Telescope (GBT) at 820 MHz
for unassociated sources from Fermi LAT catalogs as part of the Fermi
Pulsar Search Collaboratory. We expect to find multiple millisecond
pulsar binaries, including spider systems and maybe even a black
hole-pulsar binary system. We are using the Dalma High Performance
Computing (HPC) cluster of NYUAD to run the computationally expensive
jerksearches. Here we present preliminary results of these searches,
showing several promising candidates which will potentially be followed
up using the GBT.
M3 - Article
VL - 235
JO - American Astronomical Society meeting #235
JF - American Astronomical Society meeting #235
ER -