DARTS/Astro Query System - SQL Search -

All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".

total 1

No.
object_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
observation_id
exposure
awarded_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
quantity_of_hxd_burst
processing_status
processing_date_mjd
processing_date
public_date_mjd
public_date
distribution_date_mjd
distribution_date
processing_version
processing_count
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
observation_type
proposal_title
main_instrument
has_xis_injection
data_access_url
ql_access_url
ql_image_url
1 ASO0449 299.6429 28.7759 299.134977 28.639283 310.497072 48.135601 65.87759933 -0.32938525 56.1427 54974.6386921296 2009-05-23 15:19:43 54975.5786342593 2009-05-24 13:53:14 504044010 38.7337 20 38.7337 38.7417 0 38.7417 1 1 0 1 1 0 0 35.22 35.22 81.1999 2 PROCESSED 57546.6654050926 2016-06-07 15:58:11 55356 2010-06-09 00:00:00 54987.4424652778 2009-06-05 10:37:09 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 040101 Fermi Gamma-Ray Space Telescope has detected 29 gamma-ray pulsars in its first three month operation. We propose Suzaku observation of 10 new pulsars among them that have little previous coverage in X-ray band. We search for X-ray emission originating from (1) pulsar magnetosphere, (2) neutron star surface, (3) pulsar wind nebula, or (4) associated supernova remnant, with which we investigate the distance, environment, age and wind properties of these pulsars. Based on this information we aim to study the emission mechanism and particle acceleration in pulsars. GALACTIC DIFFUSE EMISSION 5 A NOBUYUKI KAWAI JAP 4 AO4 X-RAY COUNTERPARTS OF NEW FERMI GAMMA-RAY PULSARS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/504044010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '504044010'

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