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 CYG X-1 299.5916 35.1745 299.121401 35.038023 313.64901 54.223609 71.31236822 3.05181611 279.5001 55839.9245023148 2011-10-05 22:11:17 55840.9169328704 2011-10-06 22:00:23 406013010 3.7027 40 3.832 3.7027 0 40.2718 1 1 0 1 1 0 0 32.9625 32.9625 85.7339 1 PROCESSED 57603.3954166667 2016-08-03 09:29:24 56582 2013-10-17 00:00:00 56212.7247916667 2012-10-12 17:23:42 3.0.22.44 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 060057 We achieved 0.1 s time resolution with enough statistics on accumulating profiles of source brightening and made clear that electron temperature decreases and optical depth increases at the peak of brightness by using the XIS data of Psum mode. Progress to understanding the nature of fast time variability, which has been a mystery for 40 years since its discovery, connected with spectral properties is being made now. However, this property is not confirmed yet in other observations having different time scales of variability and spectral shapes, lacking the XIS data in Psum mode. We propose here another observation of Cyg X-1 with XIS0 1/8 window no burst, XIS1 1/4 window 0.5 s burst,and XIS3 Psum mode for a exposure of 40 ks. GALACTIC POINT SOURCES 4 A SHIN'YA YAMADA JAP 6 AO6 REVEALING THE NATURE OF FAST TIME VARIABILITY OF CYG X-1 WITH SHOT ANALYSIS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406013010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '406013010'

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