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 WR140 305.1374 43.8475 304.71526 43.688126 327.381123 60.483368 80.93293792 4.16074264 212.5272 56283.3528356482 2012-12-22 08:28:05 56284.2085300926 2012-12-23 05:00:17 407041010 54.7802 50 54.7962 54.7802 0 54.8042 3 2 0 3 1 0 0 52.3811 52.3811 73.92 0 PROCESSED 57608.3396990741 2016-08-08 08:09:10 56710 2014-02-22 00:00:00 56344.6961689815 2013-02-21 16:42:29 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 071203 In the campaign observations of the prototypical colliding wind binary system WR 140 at its last periastron passage in 2009, Suzaku discovered an extremely hard and variable X-ray component. The current best explanation of its origin is inverse-Compton cooling of particles accelerated in the wind-wind collision shock, and if so this would be the first detection of non-thermal X-ray emission from any Wolf-Rayet system. However, other mechanisms cannot be excluded because the observed intensity was stronger than expected from the observed radio luminosity. We propose to re-observe WR 140 near apastron in 2012 with Suzaku to identify the emission mechanism which produces the hard component. GALACTIC POINT SOURCES 4 C KENJI HAMAGUCHI USA 7 AO7 MEASURING EXTREMELY HARD X-RAY EMISSION FROM WR140 AT APASTRON XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407041010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '407041010'

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