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 V4641 SGR 274.8371 -25.4052 274.064433 -25.426808 274.361493 -2.037678 6.77442002 -4.78571714 84.0004 56741.9737152778 2014-03-25 23:22:09 56744.8959722222 2014-03-28 21:30:12 408002010 49.2237 100 49.2237 49.2706 0 49.2242 3 3 0 3 1 0 0 89.7439 89.7439 252.4556 1 PROCESSED 57614.1632291667 2016-08-14 03:55:03 57190 2015-06-17 00:00:00 56821.8685532407 2014-06-13 20:50:43 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 080009 We propose a 100 ksec Suzaku observation of the Galactic microquasar V4641 Sgr in an outburst. V4641 Sgr has many unique charactersitics: 1)giant X-ray outbursts with fast rise and decay times, 2)violent variability in X-ray and optical bands, and 3)remarkable iron-K disk-line profiles in the X-ray spectrum. However, it is hardly understood due to the poor X-ray coverage which results from its short outburst duration and rapid intensity variations. Hence, we collaborate closely with VSNET, MAXI/GSC, Swift/XRT and Swift/BAT team for a rapid trigger. The moderate energy resolution and wideband energy coverage of Suzaku enable us to clarify the radiation mechanisms of V4641 Sgr. This observation is now planned simultaneously with Swift, many radio and optical/NIR observatories. GALACTIC POINT SOURCES 4 A KAZUTAKA YAMAOKA JAP 8 AO8-TOO THE LARGEST-EVER CAMPAIGN OF THE GALACTIC MICROQUASAR V4641 SGR XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/408002010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '408002010'

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