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-1 299.5787 35.2024 299.108699 35.065978 313.648056 54.25343 71.3307159 3.0753508 59.5691 56419.0925578704 2013-05-07 02:13:17 56419.6071643518 2013-05-07 14:34:19 407015020 1.5124 20 3.2442 1.5124 0 21.48 2 2 0 1 1 0 0 20.9258 20.9258 44.458 0 PROCESSED 57611.2625347222 2016-08-11 06:18:03 56808 2014-05-31 00:00:00 56442.9715509259 2013-05-30 23:19:02 3.0.22.44 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070030 We propose to observe Cyg X-1 for 85 ks, utilizing P-sum mode for XIS3. Our aim is to perform shot analysis, which is originally invented by Negoro et al. 1995 with Ginga, and obtain high-quality wide-band spectra for several phases in less than 1 sec; for example, 0.1 sec before the peak, +/- 0.05 sec at the peak, and after the peak. With these spectra, we will quantify changes in five spectral components: hard Comptonization, soft Comptonization, disk emission, Fe-K lines, and reflection. This will be a clue to know long-standing mystery on rapid variability in black holes. GALACTIC POINT SOURCES 4 A SHINYA YAMADA JAP 7 AO7 INVESTIGATION OF DYNAMICAL SPECTRAL CHANGE IN CYG X-1 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407015020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '407015020'

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