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 | CYGNUS X-1 | 299.5337 | 35.2545 | 299.064105 | 35.118267 | 313.618737 | 54.314854 | 71.35609035 | 3.13386262 | 50.0944 | 54980.4956712963 | 2009-05-29 11:53:46 | 54981.0586226852 | 2009-05-30 01:24:25 | 404075100 | 28.7845 | 300 | 28.7845 | 28.7845 | 0 | 28.7845 | 1 | 1 | 0 | 1 | 1 | 0 | 0 | 25.7389 | 25.7389 | 48.6319 | 1 | PROCESSED | 57546.7292476852 | 2016-06-07 17:30:07 | 54922 | 2009-04-01 00:00:00 | 54994.3872800926 | 2009-06-12 09:17:41 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 044131 | In both stellar-mass and supermassive black holes, connections between X-ray flux and radio flux hint at disk-jet connections expected theoretically. The next step in this work is to move beyond fluxes, and tie the physical parameters of the disk to radio jet emission. Cygnus X-1 is bright and highly variable in both X-rays and radio bands; moreover, it is the only black hole that always permits two measurements of the disk (through disk continuum and broad Fe K disk line/reflection). We propose to observe Cygnus X-1 on 20 occasions for 15 ksec (each) during AO-4, simultaneously with the updated Ryle radio telescope. This will form a modest Large Program with public data access, and an important legacy dataset for Suzaku. This project addresses NASA Beyond Einstein science goals. | GALACTIC POINT SOURCES | 4 | A | JON MILLER | SHIN YAMADA | USJ | 4 | AO4 | A STRONG TEST OF DISK-JET CONNECTIONS IN AN ACCRETING BLACK HOLE | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/404075100/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '404075100'
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