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 | 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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