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 | 299.5875 | 35.2031 | 299.117489 | 35.06664 | 313.660052 | 54.251673 | 71.33506579 | 3.06957776 | 88.7802 | 56390.0953472222 | 2013-04-08 02:17:18 | 56391.9585532407 | 2013-04-09 23:00:19 | 407015010 | 4.1499 | 85 | 8.503 | 4.1499 | 0 | 66.4751 | 2 | 1 | 0 | 1 | 1 | 0 | 0 | 71.7128 | 71.7128 | 160.9658 | 3 | PROCESSED | 57611.2046875 | 2016-08-11 04:54:45 | 56808 | 2014-05-31 00:00:00 | 56402.1391087963 | 2013-04-20 03:20:19 | 3.0.22.44 | 2 | 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/ver3.0/407015010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '407015010'
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