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 AXP 4U 0142+614 26.5682 61.7591 25.700455 61.509234 52.151654 46.394786 129.37061357 -0.42523158 40.384 55811.6552314815 2011-09-07 15:43:32 55812.5731134259 2011-09-08 13:45:17 406031010 38.6497 60 38.6497 38.6497 0 38.6825 2 2 0 2 1 0 0 42.1964 42.1964 79.292 0 PROCESSED 57603.1220138889 2016-08-03 02:55:42 56218 2012-10-18 00:00:00 55851.4406828704 2011-10-17 10:34:35 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 060092 We propose a broad-band spectral study of magnetars in active phases in order to derive a unified interpretation of burst and persistent emissions. Magnetars are known for their unusually strong surface magnetic fields, up to 10^15 G. This proposal has two main observational goals. The first objective is to detect hard X-ray emission in magnetar burst spectra as seen in a previous SGR 0501+4516 burst spectrum. The second goal is to detect persistent emission in active phases. It is important to compare spectral characteristics in active phases with those in non-active phases. We will trigger ToO observations when one of the five magnetars exhibit high bursting activity and/or brightening of their persistent emission as observed by very sensitive monitoring observations with MAXI. GALACTIC POINT SOURCES 4 A YUJIN NAKAGAWA JAP 6 AO6-TOO A SYSTEMATIC STUDY TO SUPPORT A UNIFIED INTERPRETATION OF MAGNETAR EMISSIONS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406031010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '406031010'

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