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
|
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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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