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 1E 1841-045 280.3141 -4.8735 279.649841 -4.921767 280.812771 18.180712 27.4352849 0.03686802 77.3227 53844.4525462963 2006-04-19 10:51:40 53847.1328009259 2006-04-22 03:11:14 401100010 97.9622 100 97.9622 97.9702 97.9709 97.9709 2 2 2 2 1 0 0 63.474 63.474 231.5399 2 PROCESSED 57533.5748032407 2016-05-25 13:47:43 54401 2007-10-28 00:00:00 53907.2806597222 2006-06-21 06:44:09 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 014204 Anomalous X-ray Pulsars are young radio-quiet pulsars with unconventional properties challenging conventional wisdom on neutron star formation and evolution. Their slow rotation periods, unprecedented for their apparent youth, point to enormous surface magnetic fields, a thousand times stronger than the typical inferred radio-pulsar field. The origin of the X-ray emission from these pulsars is still being debated. The recent discovery of a hard nonthermal pulsed X-ray emission from 1E 1841-045 with RXTE well beyond 10keV, can probably be explain by a magnetospheric origin and should extend above 100keV. The HXD onboard Suzaku gives us a unique opportunity to characterize the high-energy part of the emission with the added advantage to use the XIS to characterize the lower energy data. GALACTIC POINT SOURCES 4 A ILANA HARRUS MIKIO NORII USJ 1 AO1 SUZAKU OBSERVATIONS OF THE ANOMALOUS X-RAY PULSAR 1E~1841-045 IN THE SNR KES 73 HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/401100010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401100010'

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