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 SGR 1806-20 272.1687 -20.4711 271.424026 -20.47983 272.024767 2.954425 9.94559743 -0.27498509 268.1397 54387.2332060185 2007-10-14 05:35:49 54388.333599537 2007-10-15 08:00:23 402094010 52.2477 50 52.2477 52.2717 0 52.2637 2 2 0 2 1 0 0 50.0895 50.0895 95.0599 1 PROCESSED 57540.2839583333 2016-06-01 06:48:54 54771 2008-11-01 00:00:00 54403.9548611111 2007-10-30 22:55:00 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 022016 Among magnetars, SGR 1806-20 is particularly interesting since it emitted two years ago the most powerful giant flare ever observed. We are performing a long term monitoring in the soft X-rays with XMM-Newton and hard X-rays with INTEGRAL to study how the source evolves back to quiescence. We obtained in AO-1 a Suzaku observation that was carried out simultaneously with XMM-Newton and provided for the first time a broad band spectrum of SGR 1806-20 on a short timescale. A new observation is required to study the spectral variability in the hard X-ray range and possibly the properties of bursts. GALACTIC POINT SOURCES 4 C SANDRO MEREGHETTI EUR 2 AO2 CONTINUED MONITORING OF SGR 1806-20 AFTER THE GIANT FLARE WITH SUZAKU AND XMM-NEWTON HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402094010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402094010'

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